{
"metadata": {
"description": "The content of this database is based on SPASE records from hpde.io, which are determined from SPASE IDs referenced by spase_DatasetResourceID in CDF Master metadata",
"creationDate": "2026-04-20T15:31:13Z",
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}
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[
"A1_K0_MPA",
"spase://NASA/NumericalData/LANL/2001/MPA/PT87S",
"spase://SMWG/Instrument/LANL/2001/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"87 sec",
"Geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/6jar-ra45",
"LANL 2001 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 01A MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"2001-08-31T00:00:00",
"2008-01-03T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"A2_K0_MPA",
"spase://NASA/NumericalData/LANL/2002/MPA/PT87S",
"spase://SMWG/Instrument/LANL/2002/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"87 sec",
"geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-28T12:34:56.789",
"https://doi.org/10.48322/z6y7-r007",
"LANL 2002 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 02A MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"2003-10-29T00:00:00",
"2008-01-03T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"AC_AT_DEF",
"spase://NASA/NumericalData/ACE/Attitude/Definitive/PT1H",
"spase://SMWG/Instrument/ACE/Ephemeris",
"Ephemeris",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/f2a8-nm36",
"ACE Definitive Attitude, Hourly Values, Direction Cosines in RTN, GSE, and J2000 GCI Coordinates",
"",
"E.C. Stone, Please acknowledge the Principal Investigator, E. C. Stone, California Institute of Technology, Pasadena, USA. See the Rules of Use available from the ACE Science Center, ASC, at: http://www.srl.caltech.edu/ACE/ASC/level2/policy_lvl2.html.",
"PT1H",
"1997-08-26T00:00:00.000",
"",
"",
"2.4.1"
],
[
"AC_H0_MFI",
"spase://NASA/NumericalData/ACE/MAG/L2/PT16S",
"spase://SMWG/Instrument/ACE/MAG",
"MagneticField",
"Heliosphere.NearEarth",
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data. The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/e0dc-0h53",
"ACE Magnetic Field 16-Second Level 2 Data",
"",
"Please acknowledge the ACE/MAG instrument team and the ACE Science Center",
"PT16S",
"1997-09-02T00:00:12Z",
"",
"",
"2.4.1"
],
[
"AC_H0_SWE",
"spase://NASA/NumericalData/ACE/SWEPAM/L2/PT64S",
"spase://SMWG/Instrument/ACE/SWEPAM",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data. The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/tsfn-6v47",
"ACE Solar Wind Electron Proton Alpha Monitor (SWEPAM) 64-Second Level 2 Data",
"",
"Please acknowledge the ACE/SWEPAM instrument team and the ACE Science Center",
"PT64S",
"1998-02-04T00:00:12Z",
"",
"",
"2.4.0"
],
[
"AC_H1_EPM",
"spase://NASA/NumericalData/ACE/EPAM/L2/PT5M",
"spase://SMWG/Instrument/ACE/EPAM",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-07-25T12:34:56.789",
"https://doi.org/10.48322/w4wv-rj18",
"ACE Electron Proton Alpha Monitor (EPAM) 5-min Level 2 Data",
"",
"Please acknowledge the ACE/EPAM instrument team and the ACE Science Center",
"PT5M",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.1"
],
[
"AC_H1_MFI",
"spase://NASA/NumericalData/ACE/MAG/L2/PT4M",
[
"spase://SMWG/Instrument/ACE/Ephemeris",
"spase://SMWG/Instrument/ACE/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/brf1-g493",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSM, Coordinates, Level 2 (H1), 4 min Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT4M",
"1997-09-02T00:00:00.000",
"",
"The Data become available about five Months after Observation",
"2.4.1"
],
[
"AC_H1_SIS",
"spase://NASA/NumericalData/ACE/SIS/L2/PT256S",
"spase://SMWG/Instrument/ACE/SIS",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/9kmb-8280",
"ACE Solar Isotope Spectrometer (SIS) 256-sec Level 2 Data",
"",
"Please acknowledge the ACE/SIS instrument team and the ACE Science Center",
"PT256S",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.0"
],
[
"AC_H2_CRIS",
"spase://NASA/NumericalData/ACE/CRIS/L2/PT1H",
"spase://SMWG/Instrument/ACE/CRIS",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"Level 2",
"",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/g72t-0814",
"ACE Cosmic Ray Isotope Spectrometer (CRIS) 1-Hour Level 2 Data",
"",
"Please acknowledgethe ACE/CRIS instrument team and the ACE Science Center",
"PT1H",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.0"
],
[
"AC_H2_EPM",
"spase://NASA/NumericalData/ACE/EPAM/L2/PT1H",
"spase://SMWG/Instrument/ACE/EPAM",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-07-25T12:34:56.789",
"https://doi.org/10.48322/pn1t-zx03",
"ACE Electron Proton Alpha Monitor (EPAM) 1-Hour Level 2 Data",
"",
"Please acknowledge the ACE/EPAM instrument team and the ACE Science Center",
"PT1H",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.1"
],
[
"AC_H2_MFI",
"spase://NASA/NumericalData/ACE/MAG/L2/PT1H",
[
"spase://SMWG/Instrument/ACE/Ephemeris",
"spase://SMWG/Instrument/ACE/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/fh85-fj47",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSM, Coordinates, Level 2 (H2), 1 h Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1H",
"1997-09-02T00:00:00.000",
"",
"The Data become available about five Months after Observation",
"2.4.1"
],
[
"AC_H2_SEP",
"spase://NASA/NumericalData/ACE/SEPICA/L2/PT1H",
"spase://SMWG/Instrument/ACE/SEPICA",
[
"EnergeticParticles",
"IonComposition"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"Level 2 Files produced prior to the Production of Version 4 Data used SEPICA Matrix and Sectored Rates alone. The Problem with this, is that the Matrix and Sectored Rates alone cannot be used to take into account the Results of Trails moving out of the Box Definitions in the Data Processing Unit (DPU). The Version 4 SEPICA Data are the first Version of the Level 2 Files created by using the more advanced Pulse Height Analysis/Basic Rate Normalization Method. The Software producing these Files could not reliably track Large-Scale Pressure Changes and it was possible for Trail Contamination across Boxes to occur. Version 5 takes into account Changes in Pressure and reliably keeps the proper Trails in the proper Boxes, but a Bug introduced in Version 5 Generation Code caused the Boxes to give improper Flux Readings for He5, He6, He7, and He8. The Version 6 SEPICA Data are virtually identical to the Version 5 SEPICA Data except for the Removal of the aforementioned Bug. Helium Rates: Two Helium Rates have special Significance because they include the Ions from the internal Americium 241 (Am241) Calibration Source in SEPICA. These are the Helium 4 Calibration (He4cal) Rate and the Helium Calibration Alpha Particle Check (HeCAck) Rate. The Difference between them is that HeCAck bounds the Alpha Particle Peak much more closely than He4cal. On Quiet Days, Alpha Particles from the Am241 Calibration Source dominate the Instrument Counting Rate. Excluding the He4cal Rate from a Spectrum substantially eliminates Contamination by the Calibration Alpha Particles. Alternatively, the external Helium Rate in He4cal may be calculated by subtracting an average Value of He4cal obtained on Quiet Days. Also beware that the He8 Data spans the Energy per Nucleon Ranges He3, He4cal and He5 Channels to provide a Helium Flux with a Mean Energy of 1.4 MeV/n. He8 also includes the Contribution from the Calibration Alpha Particle Rate. Heavy Ion Rates in the Solid State Detector (SSD) High-Gain Mode: When the Solid State Detectors are in High-Gain Mode instead of Low-Gain Mode, the maximum measurable Energy decreases. This enhances Detection of Helium at the Expense of High Energy Heavy Ions. The following Rates are available when the SSDs are in High-Gain Mode: Hydrogen - H1, H2, H3, Carbon - ClowE, C1, C2, Helium - He1, He2, He3, He4cal, He5, He6, He8, HeCAck, Oxygen - O1, O2, Neon - Ne1, Magnesium - Mg1, Iron - Fe1. In the Period from Year 2000, Day 070 to Year 2000, Day 318, the Instrument was in High-Gain Mode. Low Energy (lowE) Rates: The Rates with the lowE Designation should always be used with Caution. These Rates may be contaminated by other Ions, and the Level of Contamination may depend on the Pressure in the Proportional Counter. The Reason for this is as follows. The Instrument consists of a Proportional Counter/Solid State Detector Telescope. Ion Species are identified by the Energy they deposit in each Detector. At certain low Energies, the Ion Species are difficult to distinguish from one another. The lowE Rates extend as far as possible into this Energy Range. As the Pressure Changes, the Limiting Energy for Species Identification changes somewhat and the Automatic Flux Calculation Algorithm may improperly include other Species.",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/3086-yq22",
"ACE Solar Energetic Particle Ionic Charge Analyzer (SEPICA) Energetic Ion Flux Intensities Values and Uncertainties, Level 2 (H2), 1 h Data",
"",
"E.S. Moebius, Please acknowledge the Principal Investigator, E.S. Moebius, University of New Hampshire See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1H",
"1997-10-08T00:00:00.000",
"",
"The Data become available about two Weeks after Observation",
"2.4.1"
],
[
"AC_H2_SIS",
"spase://NASA/NumericalData/ACE/SIS/L2/PT1H",
"spase://SMWG/Instrument/ACE/SIS",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/eq1k-gs80",
"ACE Solar Isotope Spectrometer (SIS) 1-Hour Level 2 Data",
"",
"Please acknowledge the ACE/SIS instrument team and the ACE Science Center",
"PT1H",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.0"
],
[
"AC_H2_SWE",
"spase://NASA/NumericalData/ACE/SWEPAM/L2/PT1H",
[
"spase://SMWG/Instrument/ACE/Ephemeris",
"spase://SMWG/Instrument/ACE/SWEPAM"
],
[
"Ephemeris",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calculated",
"",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/9w01-2555",
"ACE Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM) Plasma Moments, Level 2 (H2), 1 h Data",
"",
"D.J. McComas, Please acknowledge the Principal Investigator, D.J. McComas, Southwest Research Institute. See the Rules Of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1H",
"1998-02-04T00:00:00.000",
"",
"The Data become available about three Months after Observation",
"2.4.0"
],
[
"AC_H2_SWI",
"spase://NASA/NumericalData/ACE/SWICS_SWIMS/L2/PT1H",
[
"spase://SMWG/Instrument/ACE/SWICS",
"spase://SMWG/Instrument/ACE/SWIMS"
],
[
"EnergeticParticles",
"IonComposition",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/p7gt-yh33",
"ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental and Isotopic Density, Speed, Thermal Speed, Charge State, and Ratio Parameters, Level 2 (L2), 1 h Data",
"",
"G. Gloeckler, Please acknowledge the Principal Investigator, G. Gloeckler of University of Maryland See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1H",
"1998-02-04T00:00:00.000Z",
"2011-08-21T22:40:54.000Z",
"",
"2.6.0"
],
[
"AC_H2_ULE",
"spase://NASA/NumericalData/ACE/ULEIS/Ion/Fluxes/L2/PT1H",
"spase://SMWG/Instrument/ACE/ULEIS",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"Level 2",
"The Quality of ACE Level 2 Data is such that it is suitable for serious Scientific Study. However, to avoid Confusion and Misunderstanding, it is recommended that Users consult with the appropriate ACE Team Members before publishing Work derived from the Data. The ACE Team has worked hard to ensure that the Level 2 Data are free from Errors, but the Team cannot accept Responsibility for Erroneous Data, or for Misunderstandings about how the Data may be used. This is especially true if the appropriate ACE Team Members are not consulted before Publication. At the very least, Preprints should be forwarded to the ACE Team before Publication.",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/agmq-ex61",
"ACE Ultra Low Energy Isotope Spectrometer (ULEIS) Ion Fluxes, Level 2, Hourly Data",
"",
"Please acknowledge the ACE ULEIS Instrument Team and the Principal Investigator Glenn Mason of JHU/APL.",
"PT1H",
"1998-02-20T00:00:00",
"",
"",
"2.4.0"
],
[
"AC_H3_CRIS",
"spase://NASA/NumericalData/ACE/CRIS/L2/P1D",
"spase://SMWG/Instrument/ACE/CRIS",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"",
"",
"2025-09-18T11:27:06Z",
"https://doi.org/10.48322/wbmv-4z80",
"ACE Cosmic Ray Isotope Spectrometer (CRIS) Daily Level 2 Data",
"",
"Please acknowledgethe ACE/CRIS instrument team and the ACE Science Center",
"PT24H",
"1997-08-29T00:00:00Z",
"",
"Data are presently ~2-3 weeks delayed",
"2.7.0"
],
[
"AC_H3_EPM",
"spase://NASA/NumericalData/ACE/EPAM/L2/PT12S",
"spase://SMWG/Instrument/ACE/EPAM",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2023-08-26T12:34:56.789",
"https://doi.org/10.48322/jqj0-vn49",
"ACE Electron Proton Alpha Monitor (EPAM) 12-sec Level 2 Data",
"",
"Please acknowledge the ACE/EPAM instrument team and the ACE Science Center",
"PT12S",
"1997-08-31T00:00:00Z",
"",
"",
"2.6.0"
],
[
"AC_H3_MFI",
"spase://NASA/NumericalData/ACE/MAG/L2/PT1S",
"spase://SMWG/Instrument/ACE/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/7xyh-4z44",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, and Geocentric Solar Magnetospheric, GSM, Coordinates, Level 2 (H3), 1 s Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1S",
"1998-01-01T00:00:00.000",
"",
"The Data become available about five Months after Observation",
"2.4.1"
],
[
"AC_H3_SW2",
"spase://NASA/NumericalData/ACE/SWICS/L2/PT2H",
"spase://SMWG/Instrument/ACE/SWICS",
[
"ThermalPlasma",
"IonComposition"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/xcsn-8w62",
"ACE SWICS 2.0 Solar Wind 2-Hour Data",
"",
"",
"PT2H",
"2012-06-01T00:00:00",
"",
"",
"2.6.0"
],
[
"AC_H3_SWI",
"spase://NASA/NumericalData/ACE/SWICS_SWIMS/L2/PT2H",
[
"spase://SMWG/Instrument/ACE/SWICS",
"spase://SMWG/Instrument/ACE/SWIMS"
],
[
"EnergeticParticles",
"IonComposition",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/mvcn-0276",
"ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental and Isotopic Density, Speed, Thermal Speed, Charge State, and Ratio Parameters, Level 2 (L2), 2 h Data",
"",
"G. Gloeckler, Please acknowledge the Principal Investigator, G. Gloeckler of University of Maryland See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT2H",
"1998-02-04T00:00:00.000Z",
"2011-08-21T21:40:53.000Z",
"",
"2.6.0"
],
[
"AC_H4_SWI",
"spase://NASA/NumericalData/ACE/SWICS_SWIMS/L2/P1D",
[
"spase://SMWG/Instrument/ACE/SWICS",
"spase://SMWG/Instrument/ACE/SWIMS"
],
[
"EnergeticParticles",
"IonComposition",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vpnc-ym91",
"ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental and Isotopic Density, Speed, Thermal Speed, Charge State, and Ratio Parameters, Level 2 (L2), Daily Data",
"",
"G. Gloeckler, Please acknowledge the Principal Investigator, G. Gloeckler of University of Maryland See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"P1D",
"1998-02-04T00:00:00.000Z",
"2011-08-21T02:28:39.999Z",
"",
"2.6.0"
],
[
"AC_H5_SWI",
"spase://NASA/NumericalData/ACE/SWICS_SWIMS/L2/ChargeState/PT2H",
[
"spase://SMWG/Instrument/ACE/SWICS",
"spase://SMWG/Instrument/ACE/SWIMS"
],
[
"EnergeticParticles",
"IonComposition"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/2c38-0s43",
"ACE Solar Wind Ion Composition Spectrometer (SWICS) Solar Wind Plasma Elemental Charge State Distributions with Statistical Uncertainties and Data Quality Flags, Level 2 (L2), 2 h Data",
"",
"G. Gloeckler, Please acknowledge the Principal Investigator, G. Gloeckler of University of Maryland See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT2H",
"1998-02-04T00:00:00.000",
"2011-08-21T23:59:59.999",
"",
"2.6.0"
],
[
"AC_H6_SWI",
"spase://NASA/NumericalData/ACE/SWICS/L2/PT12M",
"spase://SMWG/Instrument/ACE/SWICS",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/mfxn-cw77",
"ACE SWICS 2.0 Solar Wind Protons 12-min Data",
"",
"",
"PT12M",
"1998-01-29T00:07:03",
"",
"",
"2.6.0"
],
[
"AC_K0_EPM",
"spase://NASA/NumericalData/ACE/EPAM/KeyParameter/PT5M",
"spase://SMWG/Instrument/ACE/EPAM",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-07-25T12:34:56.789",
"https://doi.org/10.48322/ghbm-qj24",
"ACE Electron, Proton, and Alpha Monitor (EPAM) Solar Wind Plasma Energetic Particle Fluxes, Key Parameter (K0), 5 min Data",
"",
"R. Gold, Please acknowledge the Principal Investigator, R. Gold of JHU Applied Physics Laboratory See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/.",
"PT5M",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.1"
],
[
"AC_K0_MFI",
"spase://NASA/NumericalData/ACE/MAG/KeyParameter/PT5M",
"spase://SMWG/Instrument/ACE/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/cs7n-7c62",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, Coordinates, Preliminary Values, Key Parameter (K0), 5 min Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT5M",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.1"
],
[
"AC_K0_SIS",
"spase://NASA/NumericalData/ACE/SIS/L2/KP/PT1H",
"spase://SMWG/Instrument/ACE/SIS",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"The quality of ACE level 2 data is such that it is suitable for serious scientific study. However, to avoid confusion and misunderstanding, it is recommended that users consult with the appropriate ACE team members before publishing work derived from the data. The ACE team has worked hard to ensure that the level 2 data are free from errors, but the team cannot accept responsibility for erroneous data, or for misunderstandings about how the data may be used. This is especially true if the appropriate ACE team members are not consulted before publication. At the very least, preprints should be forwarded to the ACE team before publication.",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/1fgf-zm82",
"ACE Solar Isotope Spectrometer (SIS) 1-Hour Level 2 Key Parameter Data",
"",
"Please acknowledge the ACE/SIS instrument team and the ACE Science Center",
"PT1H",
"1997-08-29T00:00:00Z",
"",
"",
"2.4.0"
],
[
"AC_K0_SWE",
"spase://NASA/NumericalData/ACE/SWEPAM/KeyParameter/PT5M",
"spase://SMWG/Instrument/ACE/SWEPAM",
"ThermalPlasma",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calculated",
"",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/pfr6-fg57",
"ACE Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM) Plasma Moments, Preliminary Values, Key Parameter (K0), 5 min Data",
"",
"D.J. McComas, Please acknowledge the Principal Investigator, D.J. McComas, Southwest Research Institute.",
"PT5M",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.0"
],
[
"AC_K1_EPM",
"spase://NASA/NumericalData/ACE/EPAM/KeyParameter/PT1H",
"spase://SMWG/Instrument/ACE/EPAM",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-07-25T12:34:56.789",
"https://doi.org/10.48322/qgh8-2q85",
"ACE Electron, Proton, and Alpha Monitor (EPAM) Solar Wind Plasma Energetic Particle Fluxes, Key Parameter (K1), 1 h Data",
"",
"R. Gold, Please acknowledge the Principal Investigator, R. Gold of JHU Applied Physics Laboratory See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ace/.",
"PT1H",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.1"
],
[
"AC_K1_MFI",
"spase://NASA/NumericalData/ACE/MAG/KeyParameter/PT16S",
"spase://SMWG/Instrument/ACE/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/av87-m833",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, Coordinates, Preliminary Values, Key Parameter (K1), 16 s Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT16S",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.1"
],
[
"AC_K1_SWE",
"spase://NASA/NumericalData/ACE/SWEPAM/KeyParameter/K1/PT1H",
"spase://SMWG/Instrument/ACE/SWEPAM",
"ThermalPlasma",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2022-05-17T12:34:56.789",
"https://doi.org/10.48322/0n2v-es49",
"ACE Solar Wind Electron, Proton, and Alpha Monitor (SWEPAM), Key Parameter, K1, Preliminary Browse Data",
"",
"D.J. McComas",
"PT1H",
"2017-01-01T00:00:00",
"",
"Data are current to within about 1 week",
"2.4.0"
],
[
"AC_K2_MFI",
"spase://NASA/NumericalData/ACE/MAG/KeyParameter/PT1H",
"spase://SMWG/Instrument/ACE/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/pf44-ys65",
"ACE Magnetic Field (MAG) Geocentric Solar Ecliptic, GSE, Coordinates, Preliminary Values, Key Parameter (K2), 1 h Data",
"",
"N.F. Ness, Please acknowledge the Principal Investigator, N.F. Ness, Bartol Research Institute. See the Rules of Use available from the ACE Science Center at http://www.srl.caltech.edu/ace/asc/level2/policy_lvl2.html.",
"PT1H",
"2017-01-01T00:00:00.000",
"",
"The Data become available about one Week after Observation",
"2.4.1"
],
[
"AC_OR_DEF",
"spase://NASA/NumericalData/ACE/Ephemeris/Definitive/P1D",
"spase://SMWG/Instrument/ACE/Ephemeris",
"Ephemeris",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2022-08-19T12:34:56.789",
"https://doi.org/10.48322/mh1w-x115",
"ACE Definitive Orbit, Daily Values, in GSE and J2000 GCI Coordinates",
"",
"E.C. Stone, Please acknowledge the Principal Investigator, E. C. Stone, California Institute of Technology, Pasadena, USA. See the Rules of Use available from the ACE Science Center at: http://www.srl.caltech.edu/ACE/ASC/level2/policy_lvl2.html.",
"P1D",
"1997-08-26T00:00:00.000",
"",
"",
"2.4.1"
],
[
"AC_OR_SSC",
"spase://NASA/NumericalData/ACE/Ephemeris/PT12M",
"spase://SMWG/Instrument/ACE/Ephemeris",
"Ephemeris",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-05-01T12:34:56.789",
"https://doi.org/10.48322/by5e-zs07",
"ACE GSE 12-min Position Data",
"",
"",
"PT12M",
"1997-08-26T00:00:00Z",
"",
"",
"2.4.1"
],
[
"AEROCUBE-6-A_DOSIMETER_L2",
"spase://NASA/NumericalData/AeroCube-6/A/Dosimeter/PT1S",
"spase://NASA/Instrument/AeroCube-6/A/Dosimeter",
"EnergeticParticles",
[
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere.FRegion"
],
"",
"",
"",
"",
"2025-08-05T13:13:00Z",
"https://doi.org/10.48322/gn8x-mj75",
"AeroCube-6A Dosimeter Data, 1 s and 0.1 s Data",
"",
"The AC6 Principal Investigator is Dr. T.P. O Brien. Aerospace and government personnel who contributed to the AeroCube-6 mission: J. Bern Blake, D. Hinkley, C. Venturini, J. Avrett, D. Mabry, W. Crain, C. Nguyen, B. Hardy, J. Lee, D. Turner, D. Rowen, C. Coffman, B. Barney, P. Doyle, J. Fuller, D. Pedrino, G. Maul, D. Rumsey, A. Chin, R. Stevens, A Schutte, D. Arndt, and E. Mazur. Those wishing to use AC6 data are strongly urged to notify the PI of the topic of their work. This will enable the AC6 team to assist in use of the data and to track the instruments utility to the broader community.",
"PT1S",
"2014-06-21T00:00:00.000",
"2019-04-12T23:59:59.000",
"",
"2.7.0"
],
[
"AEROCUBE-6-B_DOSIMETER_L2",
"spase://NASA/NumericalData/AeroCube-6/B/Dosimeter/PT1S",
"spase://NASA/Instrument/AeroCube-6/B/Dosimeter",
"EnergeticParticles",
[
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere.FRegion"
],
"",
"",
"",
"",
"2025-08-05T13:13:00Z",
"https://doi.org/10.48322/49dd-na02",
"AeroCube-6B Dosimeter Data, 1 s and 0.1 s Data",
"",
"The AC6 Principal Investigator is Dr. T.P. O Brien. Aerospace and government personnel who contributed to the AeroCube-6 mission: J. Bern Blake, D. Hinkley, C. Venturini, J. Avrett, D. Mabry, W. Crain, C. Nguyen, B. Hardy, J. Lee, D. Turner, D. Rowen, C. Coffman, B. Barney, P. Doyle, J. Fuller, D. Pedrino, G. Maul, D. Rumsey, A. Chin, R. Stevens, A Schutte, D. Arndt, and E. Mazur. Those wishing to use AC6 data are strongly urged to notify the PI of the topic of their work. This will enable the AC6 team to assist in use of the data and to track the instruments utility to the broader community.",
"PT1S",
"2014-06-21T00:00:00.000",
"2017-06-30T23:59:59.000",
"",
"2.7.0"
],
[
"ALOUETTE2_AV_LIM",
"spase://NASA/NumericalData/Alouette2/SFS/AverageIonogram/Lima/PT31S",
"spase://SMWG/Instrument/Alouette2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"Alouette-2 Topside Sounder Average Ionogram over Lima, Peru: LIM, Latitude -12, Longitude 283",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT31S",
"1966-11-11T20:34:08",
"1967-01-15T12:59:00",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"ALOUETTE2_AV_QUI",
"spase://NASA/NumericalData/Alouette2/SFS/AverageIonogram/Quito/PT31S",
"spase://SMWG/Instrument/Alouette2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"Alouette-2 Topside Sounder Average Ionogram over Quito, Equador: QUI, Latitude -1, Longitude 281",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT31S",
"1965-11-29T13:47:39",
"1968-01-01T04:12:17",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"ALOUETTE2_AV_SNT",
"spase://NASA/NumericalData/Alouette2/SFS/AverageIonogram/Santiago/PT31S",
"spase://SMWG/Instrument/Alouette2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"Alouette-2 Topside Sounder Average Ionogram over Santiago, Chile: SNT, Latitude -33, Longitude 298",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT31S",
"1965-11-29T13:42:37",
"1967-01-01T04:19:41",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"ALOUETTE2_AV_SOL",
"spase://NASA/NumericalData/Alouette2/SFS/AverageIonogram/FalklandIslands/PT31S",
"spase://SMWG/Instrument/Alouette2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"Alouette-2 Topside Sounder Average Ionogram over Falkland Island, United Kingdom: SOL, Latitude -52, Longitude 302",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT31S",
"1965-12-01T01:31:39",
"1966-12-28T03:00:28",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"ALOUETTE2_AV_ULA",
"spase://NASA/NumericalData/Alouette2/SFS/AverageIonogram/Fairbanks/PT31S",
"spase://SMWG/Instrument/Alouette2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"Alouette-2 Topside Sounder Average Ionogram over Fairbanks, AK: ULA, Latitude 65, Longitude 212",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT31S",
"1965-11-29T06:20:12",
"1965-11-29T06:32:42",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
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[
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"",
"",
"",
[
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"Swept Frequency Sounder",
"Topside Ionosphere",
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"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
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"Plasma Resonance",
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],
"2021-04-27T15:38:11Z",
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"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the Alouette 2 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
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"1966-03-30T05:48:19",
"1966-04-06T06:01:10",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
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"",
"PT32S",
"1965-12-15T09:40:15",
"1972-07-10T22:37:22",
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"PT0.1875S",
"1984-08-29T00:00:00.000",
"1989-01-10T23:59:59.999",
"",
"2.6.0"
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"https://doi.org/10.48322/vars-pj10",
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"Please acknowledge NASA Space Physics Data Facility, National Space Science Data Center and the Principal Investigator for data usage.",
"PT60M",
"1969-11-19T19:30:00",
"1976-03-25T08:30:00",
"",
"2.6.0"
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"1976-03-25T08:35:57",
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"https://doi.org/10.48322/70qp-jj13",
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"1972-06-30T17:30:00",
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"1972-06-30T18:14:35",
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"https://doi.org/10.48322/6z4h-nc30",
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"PT0.05S",
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"https://doi.org/10.48322/w6hk-sg12",
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"Please acknowledge the Principal Investigator R. Millan for use of the Data. \n\nBARREL will make all its scientific data products quickly and publicly available but all users are expected to read and follow the \"BARREL Mission Data Usage Policy\" which can be found here: http://www.dartmouth.edu/~barrel/documents/data.use.policy.pdf.",
"PT0.25S",
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"2013-02-14T01:43:49",
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"PT4S",
"2013-01-28T13:25:51",
"2013-02-14T01:43:46",
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"Please acknowledge the Principal Investigator R. Millan for use of the Data. \n\nBARREL will make all its scientific data products quickly and publicly available but all users are expected to read and follow the \"BARREL Mission Data Usage Policy\" which can be found here: http://www.dartmouth.edu/~barrel/documents/data.use.policy.pdf.",
"PT32S",
"2013-01-28T13:27:51",
"2013-02-14T01:43:26",
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],
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"PT4S",
"2013-01-02T10:26:04",
"2013-01-09T20:16:59",
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],
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"https://doi.org/10.48322/zwpb-gd36",
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"Please acknowledge the Principal Investigator R. Millan for use of the Data. \n\nBARREL will make all its scientific data products quickly and publicly available but all users are expected to read and follow the \"BARREL Mission Data Usage Policy\" which can be found here: http://www.dartmouth.edu/~barrel/documents/data.use.policy.pdf.",
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"PT40S",
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"Please acknowledge the Principal Investigator R. Millan for use of the Data. \n\nBARREL will make all its scientific data products quickly and publicly available but all users are expected to read and follow the \"BARREL Mission Data Usage Policy\" which can be found here: http://www.dartmouth.edu/~barrel/documents/data.use.policy.pdf.",
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"https://doi.org/10.48322/xsac-gy90",
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"2022-05-11T12:34:56.789",
"https://doi.org/10.48322/drbp-w973",
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"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
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"",
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"cluster",
"magnetotail",
"lobe"
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"2021-04-27T17:52:14Z",
"",
"Cluster-Samba Prime Parameter Active Spacecraft Potential Control (ASPOC) Data",
"Cluster II Samba Prime Parameter ASPOC data",
"NASA, Willi W. Riedler",
"PT4S",
"2001-01-30T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.3.0"
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"C3_PP_CIS",
"spase://ESA/NumericalData/Cluster-Samba/CIS/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Samba/CIS",
"IonComposition",
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"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
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"",
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"2021-04-27T17:52:14Z",
"",
"Cluster-Samba Prime Parameter Cluster Ion Spectrometry (CIS) Data",
"Cluster 3 Prime Parameter CIS data",
"NASA, Prof. Henri Reme, European Space Agency",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C3_PP_EDI",
"spase://NASA/NumericalData/Cluster-Samba/EDI/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Samba/EDI",
"ElectricField",
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"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
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"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
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"Heliosphere.NearEarth"
],
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"",
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"magnetotail",
"lobe"
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"",
"Cluster-Samba Prime Parameter Electron Drift Instrument (EDI) Data",
"Cluster 3 Prime Parameter EDI data",
"NASA, Dr. Goetz Paschmann, European Space Agency",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
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[
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"spase://ESA/NumericalData/Cluster-Samba/EFW/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Samba/EFW",
[
"ElectricField",
"Waves.Passive"
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[
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"Calibrated",
"",
[
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"Cluster",
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"lobe"
],
"2021-03-29T17:14:50Z",
"",
"Cluster-Samba Prime Parameter Electric Field and Waves (EFW) Data",
"Cluster 3 Prime Parameter EFW Data",
"NASA, Georg Gustafsson",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C3_PP_PEA",
"spase://ESA/NumericalData/Cluster-Samba/PEACE/PrimeParameter/PT4S",
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"",
"Cluster-Samba Prime Parameter Plasma Electron and Current Experiment (PEACE) Data",
"Cluster 3 Prime Parameter PEACE Data",
"NASA, Dr. Andrew N. Fazakerley, European Space Agency",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C3_PP_RAP",
"spase://ESA/NumericalData/Cluster-Samba/RAPID/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Samba/RAPID",
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"",
"Cluster-Samba Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data",
"Cluster 3 Prime Parameter RAPID Data",
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"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
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[
"C3_PP_STA",
"spase://ESA/NumericalData/Cluster-Samba/STAFF/PrimeParameter/PT4S",
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"",
"Cluster-Samba Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Data",
"Cluster 3 Prime Parameter STAFF Data",
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"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
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"spase://ESA/NumericalData/Cluster-Samba/WHISPER/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Samba/WHISPER",
[
"ElectricField",
"ThermalPlasma",
"Waves.Passive"
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[
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"",
[
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"",
"Cluster-Samba Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation (WHISPER) Data",
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"2000-12-10T00:00:00.000",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
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"spase://ESA/NumericalData/Cluster-Samba/FGM/UnvalidatedParameter/PT4S",
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"",
"Cluster-Samba Unvalidated Prime Parameter Fluxgate Magnetometer (FGM) Data",
"Cluster 3 Unvalidated Prime Parameter FGM data",
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"PT4S",
"2006-01-01T00:00:00.000",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
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"spase://SMWG/Instrument/Cluster-Samba/WBD",
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"ElectricField",
"MagneticField"
],
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"Earth.NearSurface.AuroralRegion",
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"",
"See the Cluster WBD WBD data Interpretation Issues and Caveats documents at the web site http://www-pw.physics.uiowa.edu/cluster/ , and clicking on the links next to the \"Caution\" symbol in the listing on the left hand side of the page. The documents can also be retrieved from the Documentation section of the CSA.",
[
"Time Series",
"Waveform",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Kilometric Continuum radiation",
"Plasmaspheric Hiss",
"Terrestrial Kilometric Radiation",
"TKR",
"Very Long Baseline Interferometry",
"VLBI",
"Langmuir Waves",
"Type III Solar Bursts",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/y123-4274",
"Cluster-Samba Wideband Data (WBD) Plasma Wave Receiver/High Time Resolution Waveform Data",
[
"Cluster Samba Wideband Data Plasma Wave Receiver/High Time Resolution Waveform Data",
"C3_CE_Waveform_WBD_CDF",
"C3_CP_Waveform_WBD"
],
"Users of the Cluster WBD data are encouraged to acknowledge Jolene S. Pickett, PI and Donald A. Gurnett, Co-I University of Iowa and the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center, or the Cluster Science Archive, as appropriate, as the source of the data in any publication.",
"PT0.0000046S",
"2001-02-03T05:26:00Z",
"2016-06-19T15:20:00Z",
"",
"2.6.0"
],
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[
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"ElectricField",
"MagneticField"
],
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"Earth.NearSurface.AuroralRegion",
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],
"",
"",
"See the Cluster WBD WBD data Interpretation Issues and Caveats documents at the web site http://www-pw.physics.uiowa.edu/cluster/ , and clicking on the links next to the \"Caution\" symbol in the listing on the left hand side of the page. The documents can also be retrieved from the Documentation section of the CSA.",
[
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"Waveform",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
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"Plasmaspheric Hiss",
"Terrestrial Kilometric Radiation",
"TKR",
"Very Long Baseline Interferometry",
"VLBI",
"Langmuir Waves",
"Type III Solar Bursts",
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"Whistlers",
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],
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"",
"Cluster-Samba Wideband (WBD) Data Plasma Wave Receiver/High Time Resolution Electric and Magnetic Waveform Data Returned via BM2",
[
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"C3_CE_WBD_WAVEFORM_BM2_CDF",
"C3_WAVEFORM_WBD_BM2"
],
"Users of the Cluster WBD data are encouraged to acknowledge Jolene S. Pickett, PI and Donald A. Gurnett, Co-I University of Iowa and the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center, or the Cluster Science Archive, as appropriate, as the source of the data in any publication.",
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"",
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"2001-01-30T00:00:00.000",
"",
"",
"2.3.0"
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[
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"",
"Cluster-Tango Predicted Magnetic Positions (PMP), JSOC Parameter (JP), 5 min Data",
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"PT5M",
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"",
"",
"2.3.0"
],
[
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"",
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"M.A. Hapgood. Refer to Cluster Science Data System (CSDS) for Rules of Acknowledgement Refer to Cluster Science Data System (CSDS) for Rules of Use.",
"PT0.016S",
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"",
"2.3.0"
],
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"",
"Cluster-Tango Prime Parameter Active Spacecraft Potential Control (ASPOC) Data",
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"PT4S",
"2001-01-30T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
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"",
"Cluster-Tango Prime Parameter Cluster Ion Spectrometry (CIS) Data",
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"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
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],
[
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[
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"",
"Cluster-Tango Digital Wave Processor (DWP) prime parameter data at about 4 sec resolution (spin averaged) in GSE Coordinates",
"Cluster Tango DWP data",
"NASA; ESA; Dr. Hugo Alleyne",
"PT4S",
"2000-11-01T00:00:00",
"2009-12-30T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.3.0"
],
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"2021-04-27T15:38:11Z",
"",
"Cluster-Tango Prime Parameter Electron Drift Instrument (EDI) Data",
"Cluster 4 Prime Parameter EDI data",
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"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
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[
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"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Prime Parameter Electric Field and Waves (EFW) Data",
"Cluster 4 Prime Parameter EFW Data",
"NASA, Georg Gustafsson",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_PP_PEA",
"spase://ESA/NumericalData/Cluster-Tango/PEACE/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Tango/PEACE",
"ThermalPlasma",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
[
"4 second",
"magnetosphere",
"auroral region",
"polar cap",
"cusp",
"bow shock",
"solar wind",
"magnetosheath",
"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Prime Parameter Plasma Electron and Current Experiment (PEACE) Data",
"Cluster 4 Prime Parameter PEACE Data",
"NASA, Dr. Andrew N. Fazakerley, European Space Agency",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_PP_RAP",
"spase://ESA/NumericalData/Cluster-Tango/RAPID/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Tango/RAPID",
"EnergeticParticles",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
[
"4 second",
"magnetosphere",
"auroral region",
"polar cap",
"cusp",
"bow shock",
"solar wind",
"magnetosheath",
"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Prime Parameter Research with Adaptive Particle Imaging Detectors (RAPID) Data",
"Cluster 4 Prime Parameter RAPID Data",
"NASA, Dr. Berend Wilken, European Space Agency",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_PP_STA",
"spase://ESA/NumericalData/Cluster-Tango/STAFF/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Tango/STAFF",
[
"ElectricField",
"MagneticField",
"Waves.Passive"
],
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
[
"4 second",
"magnetosphere",
"auroral region",
"polar cap",
"cusp",
"bow shock",
"solar wind",
"magnetosheath",
"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Prime Parameter Spatio-Temporal Analysis of Magnetic Field Fluctuations (STAFF) Data",
"Cluster 4 Prime Parameter STAFF Data",
"NASA, Nicole Cornilleau-Wehrlin",
"PT4S",
"2000-12-09T00:00:00",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_PP_WHI",
"spase://ESA/NumericalData/Cluster-Tango/WHISPER/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Tango/WHISPER",
[
"ElectricField",
"ThermalPlasma",
"Waves.Passive"
],
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
[
"4 second",
"magnetosphere",
"auroral region",
"polar cap",
"cusp",
"bow shock",
"solar wind",
"magnetosheath",
"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Prime Parameter Waves of HF and Sounder for Probing Electron Density by Relaxation (WHISPER) Data",
"Cluster 4 Prime Parameter WHISPER Data",
"NASA, Pierrette Decreau",
"PT4S",
"2000-12-10T00:00:00.000",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_UP_FGM",
"spase://ESA/NumericalData/Cluster-Tango/FGM/UnvalidatedParameter/PT4S",
"spase://SMWG/Instrument/Cluster-Tango/FGM",
"MagneticField",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
[
"4 second",
"magnetosphere",
"auroral region",
"polar cap",
"cusp",
"bow shock",
"solar wind",
"magnetosheath",
"Cluster",
"magnetotail",
"lobe"
],
"2021-04-27T17:52:14Z",
"",
"Cluster-Tango Unvalidated Prime Parameter Fluxgate Magnetometer (FGM) Data",
"Cluster 4 Unvalidated Prime Parameter FGM data",
"NASA, Andre Balogh, Elizabeth E. Lucek",
"PT4S",
"2006-01-01T00:00:00.000",
"",
"Time format in data files is: day, month, year hour, min, seconds. Ex: 01-Jan-1981 00:00:00.000",
"2.3.0"
],
[
"C4_WAVEFORM_WBD",
"spase://NASA/NumericalData/Cluster-Tango/WBD/PT0.0000046S",
"spase://SMWG/Instrument/Cluster-Tango/WBD",
[
"Waves.Passive",
"ElectricField",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere",
"Heliosphere.Inner"
],
"",
"",
"See the Cluster WBD WBD data Interpretation Issues and Caveats documents at the web site http://www-pw.physics.uiowa.edu/cluster/ , and clicking on the links next to the \"Caution\" symbol in the listing on the left hand side of the page. The documents can also be retrieved from the Documentation section of the CSA.",
[
"Time Series",
"Waveform",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Kilometric Continuum radiation",
"Plasmaspheric Hiss",
"Terrestrial Kilometric Radiation",
"TKR",
"Very Long Baseline Interferometry",
"VLBI",
"Langmuir Waves",
"Type III Solar Bursts",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/nepa-q824",
"Cluster Tango Wideband Data (WBD) Plasma Wave Receiver/High Time Resolution Waveform Data",
[
"Cluster Tango Wideband Data Plasma Wave Receiver/High Time Resolution Waveform Data",
"C4_CE_Waveform_WBD_CDF",
"C4_CP_Waveform_WBD"
],
"Users of the Cluster WBD data are encouraged to acknowledge Jolene S. Pickett, PI and Donald A. Gurnett, Co-I University of Iowa and the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center, or the Cluster Science Archive, as appropriate, as the source of the data in any publication.",
"PT0.0000046S",
"2001-02-03T05:26:00Z",
"2016-06-28T15:30:00Z",
"",
"2.6.0"
],
[
"C4_WAVEFORM_WBD_BM2",
"spase://NASA/NumericalData/Cluster-Tango/WBD/BM2/PT0.0000046S",
"spase://SMWG/Instrument/Cluster-Tango/WBD",
[
"Waves.Passive",
"ElectricField",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere",
"Heliosphere.Inner"
],
"",
"",
"See the Cluster WBD WBD data Interpretation Issues and Caveats documents at the web site http://www-pw.physics.uiowa.edu/cluster/ , and clicking on the links next to the \"Caution\" symbol in the listing on the left hand side of the page. The documents can also be retrieved from the Documentation section of the CSA.",
[
"Time Series",
"Waveform",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Kilometric Continuum radiation",
"Plasmaspheric Hiss",
"Terrestrial Kilometric Radiation",
"TKR",
"Very Long Baseline Interferometry",
"VLBI",
"Langmuir Waves",
"Type III Solar Bursts",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2021-04-27T15:38:11Z",
"",
"Cluster-Tango Wideband (WBD) Data Plasma Wave Receiver/High Time Resolution Electric and Magnetic Waveform Data Returned via BM2",
[
"Cluster Tango Wideband (WBD) Data Plasma Wave Receiver/High Time Resolution Waveform Data Returned via BM2",
"C4_CE_WBD_WAVEFORM_BM2_CDF",
"C4_WAVEFORM_WBD_BM2"
],
"Users of the Cluster WBD data are encouraged to acknowledge Jolene S. Pickett, PI and Donald A. Gurnett, Co-I University of Iowa and the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center, or the Cluster Science Archive, as appropriate, as the source of the data in any publication.",
"PT0.0000046S",
"2010-07-28T14:00:00Z",
"",
"",
"2.3.2"
],
[
"CASSINI_MAG_1MIN_MAGNETIC_FIELD",
"spase://NASA/NumericalData/Cassini/MAG/CDF/PT1M",
"spase://SMWG/Instrument/Cassini/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Cassini 1-min cruise phase magnetic field data in CDF Format",
"",
"M. Dougherty",
"PT1M",
"2000-01-01T00:00:00.000",
"2004-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"CL_JP_PCY",
"spase://ESA/NumericalData/Cluster/JSOC/Predicted/SolarCycle/P1M",
"spase://SMWG/Instrument/Cluster/JSOC",
[
"MagneticField",
"ThermalPlasma"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"JSOC predicted Solar cycle trends.",
"",
"2021-04-27T17:52:14Z",
"",
"Cluster Joint Science Operations Centre (JSOC), Predicted Solar Cycle Trends, 1 month Data",
"",
"M. Hapgood, Refer to CSDS for Rules of Acknowledgement Refer to CSDS for Rules of Use.",
"P1M",
"1999-01-01T00:00:00",
"1999-02-01T23:59:59.999",
"",
"2.3.0"
],
[
"CL_JP_PGP",
"spase://ESA/NumericalData/Cluster/Ephemeris/JP/PredictedGeometricPosition/PT5M",
"spase://SMWG/Instrument/Cluster/JSOC",
[
"Ephemeris",
"InstrumentStatus"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"JSOC Predicted Orbits, calculated by using Cluster-Samba, C3, as the Reference Spacecraft",
"",
"2021-04-27T17:52:14Z",
"",
"Cluster Predicted Geometric Positions (PGP) Spacecraft Tetrahedron, JSOC Parameter (JP), 5 min Data",
"",
"M.A. Hapgood. Refer to Cluster Science Data System, CSDS, for Rules of Acknowledgement",
"PT5M",
"2000-08-14T20:35:00.000",
"",
"",
"2.3.0"
],
[
"CL_SP_AUX",
"spase://ESA/NumericalData/Cluster/Ephemeris/SummaryParameter/PT60S",
[
"spase://SMWG/Instrument/Cluster-Rumba/Ephemeris",
"spase://SMWG/Instrument/Cluster-Salsa/Ephemeris",
"spase://SMWG/Instrument/Cluster-Samba/Ephemeris",
"spase://SMWG/Instrument/Cluster-Tango/Ephemeris"
],
"Ephemeris",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"Cluster Auxiliary Data",
"",
"",
"PT1M",
"2000-08-22T00:00:30",
"",
"",
"2.3.0"
],
[
"CNOFS_CINDI_IVM_500MS",
"spase://NASA/NumericalData/CNOFS/CINDI/IVM/PT0.5S",
"spase://SMWG/Instrument/CNOFS/CINDI/IVM",
"ThermalPlasma",
"Earth.NearSurface",
"",
"CALIBRATED",
"In general the ion temperature and densities can be trusted to be valid throughout the entire orbit and at all altitudes. However the flow data can only be trusted at lower altitudes. The analysis of the ram velocity becomes more uncertain as the percentage of the light ions becomes predominate. Under those conditions, the analysis routine sets Vx to zero and solves for the other parameters. Note that the Vy or Vz data are also removed here since the drift meter does not produce usable data under these conditions. Likewise the crosstrack ion drift meter only works reliably when the percentage of O+ is very high and since the percentage of O+ decreases with increasing altitude, therefore the best crosstrack data come in the region near perigee and on the dayside. However, data from perigee on the nightside or near apogee on the dayside can also be acceptable, depending on the ambient O+ densities. Be certain to read the CINDI Quality Flag Description document and check the individual RPA and DM quality flags for each record before using the data. Also, please do not use these data in a presentation or publication without first checking with one of the CINDI researchers.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/r9x4-x639",
"CNOFS CINDI IVM 500 ms Ion Drift Data",
"",
"Please acknowledge NASA SPDF and the CINDI team at the University of Texas at Dallas that is supported by NASA grant NAS5-01068",
"PT0.5S",
"2008-08-01T00:00:00",
"",
"Data are presently ~6 months delayed",
"2.6.0"
],
[
"CNOFS_PLP_PLASMA_1SEC",
"spase://NASA/NumericalData/CNOFS/PLP/PT1S",
"spase://SMWG/Instrument/CNOFS/PLP",
"ThermalPlasma",
"Earth.NearSurface.Ionosphere",
"",
"Preliminary Calibrated",
"The data are PRELIMINARY, and as such, are intended for BROWSE PURPOSES ONLY. Continuous coverage not guaranteed; check the inventory graph for coverage.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/xnnr-w563",
"CNOFS PLP 1-sec plasma preliminary data",
"",
"the GSFC SPDF Team",
"PT1S",
"2008-05-09T00:00:00.000Z",
"2008-09-14T18:34:58.000Z",
"",
"2.6.0"
],
[
"CNOFS_VEFI_BFIELD_1SEC",
"spase://NASA/NumericalData/CNOFS/VEFI/BField/PT1S",
"spase://SMWG/Instrument/CNOFS/VEFI",
"MagneticField",
"Earth.NearSurface.Ionosphere",
"",
"Preliminary Calibrated",
"The data are PRELIMINARY, and as such, are intended for BROWSE PURPOSES ONLY. Continuous coverage is not guaranteed; check the inventory graph for coverage.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vbt7-gj03",
"CNOFS VEFI 1-sec Magnetic Field preliminary data",
"",
"the GSFC SPDF Team",
"PT1S",
"2008-05-09T00:00:00.000Z",
"2009-04-30T23:59:59.000Z",
"",
"2.6.0"
],
[
"CNOFS_VEFI_EFIELD_1SEC",
"spase://NASA/NumericalData/CNOFS/VEFI/EField/PT1S",
"spase://SMWG/Instrument/CNOFS/VEFI",
"ElectricField",
"Earth.NearSurface.Ionosphere",
"",
"Preliminary Calibrated",
"The data are PRELIMINARY, and as such, are intended for BROWSE PURPOSES ONLY. Continuous coverage not guaranteed; check the inventory graph for coverage.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1dcn-xp86",
"CNOFS VEFI 1-sec Electric Field preliminary data",
"",
"the GSFC SPDF Team",
"PT1S",
"2008-05-09T00:00:00.000Z",
"2008-09-14T18:34:58.000Z",
"",
"2.6.0"
],
[
"CNOFS_VEFI_LD_500MS",
"spase://NASA/NumericalData/CNOFS/VEFI/Lightning/PT0.5S",
"spase://SMWG/Instrument/CNOFS/VEFI",
"ElectricField",
"Earth.NearSurface.Ionosphere",
"",
"Preliminary Calibrated",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/pv2n-aj92",
"CNOFS VEFI 500-msec Optical Lightning Data",
"",
"the GSFC SPDF Team",
"PT0.5S",
"2008-04-23T00:00:00.000Z",
"2011-12-31T23:46:00.000Z",
"",
"2.6.0"
],
[
"CN_K0_ASI",
"spase://GBO/NumericalData/CANOPUS/ASI/KeyParameter/K0/PT1M",
"spase://SMWG/Instrument/CANOPUS/ASI",
"ImageIntensity",
[
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere"
],
"",
"",
"",
"",
"2022-07-25T12:34:56.789",
"",
"CANOPUS All Sky Imager (ASI), Key Parameters, K0, 1 min Data",
"",
"J.C. Samson, E.F. Donovan",
"PT1M",
"1993-02-13T05:10:01",
"1999-12-30T23:55:05",
"",
"2.4.1"
],
[
"CN_K0_BARS",
"spase://GBO/NumericalData/CANOPUS/BARS/KeyParameter/K0/PT1M",
"spase://SMWG/Instrument/CANOPUS/BARS",
"Irradiance",
[
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere"
],
"",
"",
"",
"",
"2022-07-25T12:34:56.789",
"",
"CANOPUS Bistatic Auroral Radar System (BARS), Key Parameters, K0, 1 min Data",
"",
"J.C. Samson, E.F. Donovan",
"PT1M",
"1992-07-20T03:50:30",
"1994-09-30T23:59:30",
"",
"2.4.1"
],
[
"CN_K0_MARI",
"spase://GBO/NumericalData/CANOPUS/MARI/PT60S",
"spase://SMWG/Instrument/CANOPUS/MARI",
"ActivityIndex",
"Earth.Surface",
"",
"CALCULATED",
"",
"",
"2021-07-19T14:39:57Z",
"",
"CANOPUS MARI Key Parameters",
"",
"",
"PT60S",
"1992-09-01T00:00:00",
"1999-12-30T00:00:00",
"",
"2.3.1"
],
[
"CN_K0_MPA",
"spase://GBO/NumericalData/CANOPUS/MPA/KeyParameter/K0/PT1M",
"spase://SMWG/Instrument/CANOPUS/MPA",
"ImageIntensity",
[
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere"
],
"",
"",
"",
"",
"2022-07-25T12:34:56.789",
"",
"CANOPUS Meridian Scanning Photometer Array (MPA), Key Parameters, K0, 1 min Data",
"",
"J.C. Samson, E.F. Donovan",
"PT1M",
"1992-09-01T01:42:00",
"1999-12-30T23:59:00",
"",
"2.4.1"
],
[
"CN_K1_MARI",
"spase://GBO/NumericalData/CANOPUS/MARI/KeyParameter/K1/PT1M",
"spase://SMWG/Instrument/CANOPUS/MARI",
"Waves.Passive",
[
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Ionosphere"
],
"",
"",
"",
"",
"2022-07-25T12:34:56.789",
"",
"CANOPUS Middle Atmosphere Research Initiative (MARI), Riometer Key Parameters, K1, 1 min Data",
"",
"J.C. Samson, E.F. Donovan",
"PT1M",
"1992-09-01T00:00:00",
"1999-12-30T23:59:00",
"",
"2.4.1"
],
[
"CRRES_H0_MEA",
"spase://NASA/NumericalData/CRRES/MEA/PT1M",
"spase://SMWG/Instrument/CRRES/MEA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/8e23-cz17",
"CRRES MEA 1-min electron distribution functions",
"",
"Please acknowledge A. Vampola at AFRL and the Space Phyics Data Facility at NASA/Goddard.",
"PT1M",
"1990-07-28T00:00:00",
"1991-10-09T00:00:00",
"",
"2.6.0"
],
[
"CSSWE_REPTILE_6SEC-COUNTS-L1",
"spase://NASA/NumericalData/CubeSat/CSSWE/REPTile/L1/Counts/PT6S",
"spase://SMWG/Instrument/CubeSat/CSSWE/REPTile",
"EnergeticParticles",
"Earth.Magnetosphere.RadiationBelt",
"",
"",
"Please contact the PI, Xinlin Li (xinlin.li@lasp.colorado.edu) before using these data for publication.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/dy3g-xz52",
"CSSWE REPTile Level 1 6-s Counts and Position",
"",
"Please acknowledge the PI and NASA SPDF for the CSSWE REPTile data.",
"PT6S",
"2012-09-14T00:28:03.000Z",
"2013-12-10T08:10:31.000Z",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/CubeSat/CSSWE/REPTile/L2/Flux/PT6S",
"spase://SMWG/Instrument/CubeSat/CSSWE/REPTile",
"EnergeticParticles",
"Earth.Magnetosphere.RadiationBelt",
"",
"",
"Please contact the PI, Xinlin Li (xinlin.li@lasp.colorado.edu) before using these data for publication.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/brd0-ak96",
"CSSWE REPTile Level 2 6-s Flux",
"",
"Please acknowledge the PI and NASA SPDF for the CSSWE REPTile data.",
"PT6S",
"2012-09-14T00:28:03.000Z",
"2013-12-10T08:10:31.000Z",
"",
"2.6.0"
],
[
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"spase://ESA/NumericalData/Cluster/Ephemeris/JP/PredictedScientificEvent/PT5M",
"spase://SMWG/Instrument/Cluster/JSOC",
[
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"InstrumentStatus"
],
"",
"",
"",
"JSOC Predicted Scientific Events",
"",
"2021-04-27T17:52:14Z",
"",
"Cluster Predicted Scientific Events (PSE), JSOC Parameter (JP), 5 min Data",
"",
"M.A. Hapgood. Refer to Cluster Science Data System, CSDS, for Rules of Acknowledgement Refer to Cluster Science Data System, CSDS, for Rules of Use.",
"PT5M",
"2000-08-01T00:00:00.000",
"",
"",
"2.3.0"
],
[
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"spase://NASA/NumericalData/DE1/RIMS/PT1M",
[
"spase://SMWG/Instrument/DynamicsExplorer1/Ephemeris",
"spase://SMWG/Instrument/DynamicsExplorer1/MAGA",
"spase://SMWG/Instrument/DynamicsExplorer1/RIMS"
],
[
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"ElectricField",
"Ephemeris",
"Irradiance",
"ThermalPlasma"
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[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/4e3s-bm07",
"DE 1 Retarding Ion Mass Spectrometer (RIMS) Low Channel, H+ and He++, and High Channel, He+, O+, and O++, Density, Temperature, and Electric Potential, 1 min Data",
"",
"Please acknowledge the Principal Investigator, C.R. Chappell, from NASA MSFC for providing the Data.",
"PT1M",
"1981-10-07T00:00:00.000",
"1984-12-02T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://SMWG/Instrument/DynamicsExplorer1/MAGA",
"MagneticField",
[
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"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.Polar"
],
"",
"Level-2",
"",
[
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"Magnetosphere",
"Auroral region",
"Polar Cap",
"Cusp",
"Radiation Belt",
"Plasmasphere",
"solar wind",
"Dynamics Explorer 1",
"Dynamics Explorer",
"magnetic fields",
"magnetometer"
],
"2025-05-02T15:38:11Z",
"10.48322/ps14-8x77",
"DE 1 Magnetic Field Observations Triaxial Fluxgate Magnetometer (MAG-A)",
[
"Dynamics Explorer 1 MAG-A data",
"DE-A MAG-A data"
],
"NASA; Masahisa Sugiura",
"PT6S",
"1981-09-15T00:00:00",
"1991-02-18T00:00:00",
"Time format in data files is: Year, Day of Year, Milliseconds of the Day",
"2.7.0"
],
[
"DE1_PWI_LFC-SPECTRA",
"spase://NASA/NumericalData/DE1/PWI/LFC/PT0.25S",
"spase://SMWG/Instrument/DynamicsExplorer1/PWI",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.NearSurface.Ionosphere",
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.Polar"
],
"",
"",
"",
"",
"2025-05-02T12:34:56.789",
"https://doi.org/10.48322/hx4p-3v35",
"DE 1 Plasma Wave Instrument (PWI) Low Frequency Correlator Electric and Magnetic Field Spectral Density",
[
"Dynamics Explorer 1 PWI LFC Spectra",
"DE-A PWI LFC Spectra"
],
"Users of the DE-1 PWI LFC data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication.",
"PT0.25S",
"1981-09-16T05:21:48",
"1984-06-28T05:53:31",
"\n ",
"2.6.0"
],
[
"DE1_PWI_OR-AT",
"spase://NASA/NumericalData/DE1/Ephemeris/PT8S",
"spase://SMWG/Instrument/DynamicsExplorer1/Ephemeris",
"Ephemeris",
[
"Earth.NearSurface.Ionosphere",
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.Polar"
],
"",
"",
"",
"",
"2025-05-02T12:34:56.789",
"https://doi.org/10.48322/wma0-gq05",
"DE 1 8-sec Position Data",
[
"Dynamics Explorer 1 8 Second Orbit and Attitude Data",
"DE-A 8 Second Orbit and Attitude Data"
],
"Users of the DE-1 PWI data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication.",
"PT8S",
"1981-09-16T05:21:48",
"1984-06-28T20:35:55",
"\n ",
"2.6.0"
],
[
"DE1_PWI_SFC-SPECTRA",
"spase://NASA/NumericalData/DE1/PWI/SFC/PT0.25S",
"spase://SMWG/Instrument/DynamicsExplorer1/PWI",
[
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"Spectrum"
],
[
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"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.Polar"
],
"",
"",
"",
"",
"2025-05-02T12:34:56.789",
"https://doi.org/10.48322/cb14-a164",
"DE 1 Plasma Wave Instrument (PWI) Step Frequency Correlator Electric and Magnetic Field Spectral Density",
[
"Dynamics Explorer 1 PWI SFC Spectra",
"DE-A PWI SFC Spectra"
],
"Users of the DE-1 PWI SFC data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication.",
"PT0.25S",
"1981-09-16T05:21:48",
"1984-06-28T20:35:55",
"\n ",
"2.6.0"
],
[
"DE2_62MS_VEFIMAGB",
"spase://NASA/NumericalData/DE2/MAGB-VEFI/CDF/PT0.062S",
[
"spase://SMWG/Instrument/DynamicsExplorer2/Ephemeris",
"spase://SMWG/Instrument/DynamicsExplorer2/MAGB",
"spase://SMWG/Instrument/DynamicsExplorer2/VEFI"
],
[
"ElectricField",
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2024-02-22T12:34:56.789",
"https://doi.org/10.48322/ha70-4305",
"DE 2 Vector Electric Field Instrument, VEFI, Magnetometer, MAG-B, Merged Magnetic and Electric Field Parameters, 62 ms Data",
"",
"Please acknowledge the Principal Investigator J.A. Slavin for use of the Data",
"PT0.062S",
"1981-08-15T00:00:00.000",
"1983-02-16T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/DE2/VEFI/AC/CDF/PT0.5S",
"spase://SMWG/Instrument/DynamicsExplorer2/VEFI",
[
"ElectricField",
"Ephemeris",
"InstrumentStatus"
],
[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2024-02-22T12:34:56.789",
"https://doi.org/10.48322/x1km-9q17",
"DE 2 Vector Electric Field Instrument (VEFI) AC Electric Field Spectrometers, A, B, and C, all frequency channels, Spacecraft, SC, coordinates, PT0.5S Data",
"",
"Please acknowledge the Principal Investigator N.C. Maynard and R.F. Pfaff for use of the Data",
"PT0.5S",
"1981-08-10T00:00:00.000",
"1983-02-16T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/DE2/VEFI/DC/CDF/PT0.5S",
"spase://SMWG/Instrument/DynamicsExplorer2/VEFI",
[
"ElectricField",
"Ephemeris"
],
[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2024-02-22T12:34:56.789",
"https://doi.org/10.48322/0s61-a111",
"DE 2 Vector Electric Field Instrument (VEFI) DC Electric Field X and Y components, Spacecraft, SC, coordinates, PT0.5S Data",
"",
"Please acknowledge the Principal Investigator N.C. Maynard for use of the Data",
"PT0.5S",
"1981-08-10T00:00:00.000",
"1983-02-16T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/DE2/RPA/PT0.016S",
"spase://SMWG/Instrument/DynamicsExplorer2/RPA",
"ThermalPlasma",
"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/aab6-jj49",
"DE 2 16ms Retarding Potential Analyzer (RPA) Ion Densities",
[
"Dynamics Explorer 2 RPA Ion Density",
"DE-B RPA Ion Density"
],
"Please acknowledge the RPA Principal Investigators, Drs. W.B. Hanson (original P.I.) and R.A. Heelis",
"PT0.016S",
"1981-08-03T00:00:00",
"1983-02-17T00:00:00",
"",
"2.6.0"
],
[
"DE2_ION2S_RPA",
"spase://NASA/NumericalData/DE2/RPA/PT2S",
"spase://SMWG/Instrument/DynamicsExplorer2/RPA",
"ThermalPlasma",
"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/41b3-kz41",
"DE 2 2s Retarding Potential Analyzer (RPA) Ion Plasma Parameters",
[
"Dynamics Explorer 2 RPA Ion Plasma",
"DE-B RPA Ion Plasma"
],
"Please acknowledge the RPA Principal Investigators, Drs. W.B. Hanson (original P.I.) and R.A. Heelis",
"PT2S",
"1981-08-06T00:00:00",
"1983-02-16T00:00:00",
"",
"2.6.0"
],
[
"DE2_NEUTRAL1S_NACS",
"spase://NASA/NumericalData/DE2/NACS/PT1S",
"spase://SMWG/Instrument/DynamicsExplorer2/NACS",
"NeutralGas",
[
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"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/j8kp-5y58",
"DE 2 1-sec NACS Temperature and Composition data",
[
"Dynamics Explorer 2 NACS data",
"DE-B NACS data"
],
"Please acknowledge the NACS Principal Investigator, Dr. George Carignan",
"PT1S",
"1981-08-08T00:00:00",
"1983-02-15T00:00:00",
"",
"2.6.0"
],
[
"DE2_NEUTRAL8S_FPI",
"spase://NASA/NumericalData/DE2/FPI/Neutral/PT8S",
"spase://SMWG/Instrument/DynamicsExplorer2/FPI",
"EnergeticParticles",
[
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Thermosphere"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/22v6-0p09",
"DE 2 Fabry-Perot Interferometer (FPI), Thermospheric Neutral Gas Density, Meridional Wind, and Temperature, 8-sec data",
[
"Dynamics Explorer 2 FPI Neutral 8s Data",
"DE-B FPI Neutral 8s Data"
],
"R.J. Niciejewski",
"PT8S",
"1981-08-09T00:00:00.000",
"1983-02-16T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/DE2/LANG/PT0.5S",
"spase://SMWG/Instrument/DynamicsExplorer2/LANG",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Earth.NearSurface.EquatorialRegion",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.Thermosphere",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/yq6h-5g10",
"DE 2 500ms Langmuir Probe (LANG) Te and Ni data",
[
"Dynamics Explorer 2 LANG data",
"DE-B LANG data"
],
"Please acknowledge the IDM Principal Investigator, Dr. Larry Brace",
"PT0.5S",
"1981-08-05T00:00:00",
"1983-02-16T00:00:00",
"",
"2.6.0"
],
[
"DE2_UA16S_ALL",
"spase://NASA/NumericalData/DE2/PT16S",
[
"spase://SMWG/Instrument/DynamicsExplorer2/RPA",
"spase://SMWG/Instrument/DynamicsExplorer2/IDM",
"spase://SMWG/Instrument/DynamicsExplorer2/WATS",
"spase://SMWG/Instrument/DynamicsExplorer2/LANG",
"spase://SMWG/Instrument/DynamicsExplorer2/FPI",
"spase://SMWG/Instrument/DynamicsExplorer2/NACS"
],
[
"ThermalPlasma",
"NeutralGas"
],
[
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"Earth.NearSurface.Atmosphere"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"DE 2 16-s Unified Abstract data",
[
"Dynamics Explorer 2 UA data",
"DE-B UAdata"
],
"",
"PT16S",
"1981-08-06T00:00:00",
"1983-02-15T00:00:00",
"",
"2.3.2"
],
[
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"spase://NASA/NumericalData/DE2/IDM/PT0.25S",
"spase://SMWG/Instrument/DynamicsExplorer2/IDM",
"ThermalPlasma",
"Earth.NearSurface.Ionosphere",
"",
"Level-2",
"The time format is variable",
[
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"Auroral region",
"Polar Cap",
"Cusp",
"Radiation Belt",
"Plasmasphere",
"Dynamics Explorer 2",
"Dynamics Explorer",
"ion drift speed"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/reef-jt02",
"DE 2 250ms IDM Ion Drift Velocities",
[
"Dynamics Explorer 2 IDM Ion Drift Velocities",
"DE-B IDM Ion Drift Velocities"
],
"Please acknowledge the IDM Principal Investigator, Dr. R.A. Heelis",
"PT0.25S",
"1981-08-15T00:00:00",
"1983-02-16T00:00:00",
"",
"2.6.0"
],
[
"DE2_WIND2S_WATS",
"spase://NASA/NumericalData/DE2/WATS/PT2S",
"spase://SMWG/Instrument/DynamicsExplorer2/NACS",
"NeutralGas",
[
"Earth.NearSurface.Thermosphere",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/z50y-hd65",
"DE 2 2s WATS Wind Velocity, Density and Temperature data",
[
"Dynamics Explorer 2 WATS data",
"DE-B WATS data"
],
"Please acknowledge the WATS Principal Investigator, the late Dr. Nelson Spencer",
"PT2S",
"1981-08-08T00:00:00",
"1983-02-17T00:00:00",
"",
"2.6.0"
],
[
"DE_UV_SAI",
"spase://NASA/NumericalData/DE1/SAI/PT3M",
"spase://SMWG/Instrument/DynamicsExplorer1/SAI",
"ImageIntensity",
"Earth.NearSurface.Atmosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/t7ya-6231",
"DE 1 Spin-Scan Auroral Imager UV Images",
[
"Dynamics Explorer 1 Spin-Scan Auroral Imager UV Images",
"DE-A Spin-Scan Auroral Imager UV Images"
],
"Please acknowledge the SAI Principal Investigator, Dr. Louis A. Frank at the University of Iowa, and the Space Physics Data Facility at NASA/GSFC",
"PT3M",
"1981-09-23T00:00:00",
"1991-02-18T00:00:00",
"",
"2.6.0"
],
[
"DE_VS_EICS",
"spase://NASA/NumericalData/DE1/EICS/PT96S",
"spase://SMWG/Instrument/DynamicsExplorer1/EICS",
"EnergeticParticles",
[
"Earth.NearSurface.Ionosphere",
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.Polar"
],
"",
"",
"",
"",
"2025-05-02T12:34:56.789",
"https://doi.org/10.48322/1gca-r323",
"DE 1 Energetic Ion Composition Spectrometer (EICS) Validated Summary Data",
[
"Dynamics Explorer 1 EICS Validated Summary Data",
"DE-A EICS Validated Summary Data"
],
"Please acknowledge the EICS Principal Investigator, Dr. E. G. Shelley",
"PT96S",
"1981-09-16T00:00:00",
"1991-02-18T00:00:00",
"",
"2.6.0"
],
[
"DMSP-F16_SSIES-3_THERMAL-PLASMA",
"spase://NASA/NumericalData/DMSP_5D-3/F16/SESS/SSIES-3/ThermalPlasma/CDF/PT1S",
"spase://SMWG/Instrument/DMSP_5D-3/F16/SESS/SSI/ES-3",
[
"ThermalPlasma",
"IonComposition"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2024-05-03T00:00:00.00",
"https://doi.org/10.48322/hcdm-vz96",
"DMSP F16 Special Sensors-Ions, Electrons, and Scintillation (SSIES) Thermal Plasma Analysis Package, Level 2 (L2), 1 s Data in CDF Format",
"",
"We gratefully acknowledge the University of Texas Dallas, Center for Space Sciences and the US Air Force for providing the DMSP thermal plasma data",
"PT1S",
"2006-01-01T00:48:39",
"",
"",
"2.6.0"
],
[
"DMSP-F16_SSJ_PRECIPITATING-ELECTRONS-IONS",
"spase://NASA/NumericalData/DMSP_5D-3/F16/SESS/SSJ5/PT1S",
"spase://SMWG/Instrument/DMSP_5D-3/F16/SESS/SSJ5",
"EnergeticParticles",
[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1rnz-f067",
"DMSP F16 Special Sensor J, SESS/SSJ5, Precipitating Electrons and Ions Observed at 850 km, 1 s Data",
"",
"R.J. Redmon, L.M. Kilcommons, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
"PT1S",
"2010-01-01T00:00:00.000",
"2014-12-31T23:59:59.999",
"",
"2.6.0"
],
[
"DMSP-F16_SSM_MAGNETOMETER",
"spase://NASA/NumericalData/DMSP_5D-3/F16/SESS/SSM-Boom/PT1S",
"spase://SMWG/Instrument/DMSP_5D-3/F16/SESS/SSM-Boom",
"MagneticField",
[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/bh8f-yy31",
"DMSP F16 Special Sensor Magnetometer, SESS/SSM-Boom, Magnetic Field Measurements taken at 850 km, 1 s Data",
"",
"R.J. Redmon, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
"PT1S",
"2010-01-01T00:00:00.000",
"2014-12-30T23:59:59.999",
"",
"2.6.0"
],
[
"DMSP-F17_SSIES-3_THERMAL-PLASMA",
"spase://NASA/NumericalData/DMSP_5D-3/F17/SESS/SSIES-3/ThermalPlasma/CDF/PT1S",
"spase://SMWG/Instrument/DMSP_5D-3/F17/SESS/SSI/ES-3",
[
"ThermalPlasma",
"IonComposition"
],
[
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"Earth.Magnetosphere.Polar",
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"R.J. Redmon, L.M. Kilcommons, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
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"2010-01-01T00:00:00.000",
"2014-12-31T23:59:59.999",
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"R.J. Redmon, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
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"2014-12-30T23:59:59.999",
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"2024-05-03T00:00:00.00",
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"We gratefully acknowledge the University of Texas Dallas, Center for Space Sciences and the US Air Force for providing the DMSP thermal plasma data",
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"",
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"",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/34mn-w272",
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"",
"R.J. Redmon, L.M. Kilcommons, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
"PT1S",
"2010-01-01T00:00:00.000",
"2014-12-31T23:59:59.999",
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"spase://SMWG/Instrument/DMSP_5D-3/F18/SESS/SSM-Boom",
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"Earth.Magnetosphere.Polar",
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"",
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"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/cj1v-6g43",
"DMSP F18 Special Sensor Magnetometer, SESS/SSM-Boom, Magnetic Field Measurements taken at 850 km, 1 s Data",
"",
"R.J. Redmon, Data Access provided by NGDC in Coordination with AFRL and the University of Colorado, Boulder. Please acknowledge the Data Providers. If you find Problems, please report them.",
"PT1S",
"2010-01-01T00:00:00.000",
"2014-12-30T23:59:59.999",
"",
"2.6.0"
],
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"Earth.NearSurface.Ionosphere",
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"",
"",
"",
"2021-04-27T17:51:40Z",
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"1999-11-04T23:55:00",
"",
"2.3.0"
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[
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"",
"",
"",
"2021-04-27T17:51:40Z",
"",
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"2001-08-05T23:58:56",
"",
"2.3.0"
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[
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"",
"",
"",
"2021-04-27T17:51:40Z",
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"",
"R. Greenwald",
"PT2M",
"1994-08-28T00:02:02",
"1999-11-03T23:55:00",
"",
"2.3.0"
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[
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"Earth.NearSurface.Ionosphere",
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"",
"",
"",
"2021-04-27T17:51:40Z",
"",
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"",
"R. Greenwald",
"PT2M",
"1994-08-28T00:02:10",
"1999-11-04T23:55:00",
"",
"2.3.0"
],
[
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"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2021-04-27T17:51:40Z",
"",
"SuperDARN Polar Anglo-American Conjugate Experiment (PACE), Ionospheric Convection Velocity",
"",
"R. Greenwald",
"PT2M",
"1992-12-04T00:01:06",
"2001-09-20T09:14:02",
"",
"2.3.0"
],
[
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"spase://GBO/NumericalData/DARN/Pykkvibaer/PT2M",
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"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2021-04-27T17:51:40Z",
"",
"SuperDARN Pykkvibaer (PYK), Ionospheric Convection Velocity",
"",
"R. Greenwald",
"PT2M",
"1996-07-01T00:00:48",
"2001-05-16T09:16:58",
"",
"2.3.0"
],
[
"DN_K0_SASK",
"spase://GBO/NumericalData/DARN/Saskatoon/PT2M",
"spase://SMWG/Instrument/SuperDARN/Radars",
"Irradiance",
"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2021-04-27T17:51:40Z",
"",
"SuperDARN Saskatoon (SAS), Ionospheric Convection Velocity",
"",
"R. Greenwald",
"PT2M",
"1994-07-02T12:00:52",
"1999-11-04T23:55:00",
"",
"2.3.0"
],
[
"DSCOVR_AT_DEF",
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"spase://SMWG/Instrument/DSCOVR/Ephemeris",
"Ephemeris",
[
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"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2024-06-20T12:34:56.789",
"",
"DSCOVR 3-Axis Stabilized Attitude (Ephemeris) Definitive Data",
"",
"A. Szabo",
"PT5S",
"2015-02-11T00:00:00.000",
"",
"",
"2.6.0"
],
[
"DSCOVR_AT_PRE",
"spase://NOAA/NumericalData/DSCOVR/Ephemeris/Attitude/Preliminary/PT10S",
"spase://SMWG/Instrument/DSCOVR/Ephemeris",
"Ephemeris",
[
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"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"DSCOVR 3-Axis Stabilized Attitude (Ephemeris) Preliminary Data",
"",
"A. Szabo",
"PT10S",
"2015-02-11T00:00:00.000",
"2017-05-31T23:59:59.999",
"",
"2.3.0"
],
[
"DSCOVR_H0_MAG",
"spase://NOAA/NumericalData/DSCOVR/PlasMag/FluxgateMagnetometer/CDF/PT1S",
"spase://SMWG/Instrument/DSCOVR/PlasMag/FluxgateMagnetometer",
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"Heliosphere.NearEarth",
"Heliosphere.Inner"
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"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"DSCOVR Fluxgate Magnetometer (MAG) Definitive Magnetic Field, 1 second data",
"",
"A. Koval",
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"2015-06-08T00:00:00.000",
"",
"",
"2.3.0"
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[
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"spase://SMWG/Instrument/DSCOVR/PlasMag/FaradayCup",
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"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"DSCOVR Faraday Cup (FC) Isotropic Maxwellian Parameters for Solar Wind Protons 1 minute averages",
"",
"J.C. Kasper, M.L. Stevens, A.W. Case, This Research has made use of Deep Space Climate Observatory (DSCOVR) Faraday Cup Experiment Science Data. These Data are provided by the Space Plasma Group at the Smithsonian Astrophysical Observatory under NASA Grant NNX17AC98G. The DSCOVR Mission is a Project of the U.S. National Oceanic and Atmospheric Administration.",
"PT1M",
"2016-06-03T00:00:00.000",
"",
"",
"2.3.0"
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[
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"spase://NOAA/NumericalData/DSCOVR/Ephemeris/Orbit/Preliminary/PT1M",
[
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"spase://SMWG/Instrument/DSCOVR/PlasMag/FaradayCup",
"spase://SMWG/Instrument/DSCOVR/PlasMag/FluxgateMagnetometer"
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"",
"",
"",
"",
"2024-06-20T12:34:56.789",
"",
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"",
"A. Szabo",
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"2015-02-11T00:00:00.000",
"",
"",
"2.6.0"
],
[
"ELA_L1_EPDEF",
"spase://NASA/NumericalData/ELFIN/A/EPD/L1/electron/PT0.2S",
"spase://NASA/Instrument/ELFIN/A/EPD",
"EnergeticParticles",
[
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-03-03T13:45:36Z",
"https://doi.org/10.48322/jyaq-cq12",
"ELFIN A Energetic Particle Detectors for Electrons (EPD-E) 0.2 s Data",
"",
"Please acknowledge the Principal Investigator, V. Angelopoulos, NASA, and NSF for providing the Data. Open Data for Scientific Use.",
"PT0.2S",
"2018-12-01T00:00:00.000",
"2022-09-11T23:59:59.999",
"",
"2.6.0"
],
[
"ELA_L1_EPDIF",
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"spase://NASA/Instrument/ELFIN/A/EPD",
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-03-03T13:45:36Z",
"https://doi.org/10.48322/csjm-bk25",
"ELFIN A Energetic Particle Detectors for Ions (EPD-I) 0.264 s Data",
"",
"Please acknowledge the Principal Investigator, V. Angelopoulos, NASA, and NSF for providing the Data. Open Data for Scientific Use.",
"PT0.264S",
"2018-12-04T00:00:00.000",
"2022-09-11T23:59:59.999",
"",
"2.6.0"
],
[
"ELB_L1_EPDEF",
"spase://NASA/NumericalData/ELFIN/B/EPD/L1/electron/PT0.2S",
"spase://NASA/Instrument/ELFIN/B/EPD",
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-03-03T13:45:36Z",
"https://doi.org/10.48322/w4ac-2h02",
"ELFIN B Energetic Particle Detectors for Electrons (EPD-E) 0.2 s Data",
"",
"Please acknowledge the Principal Investigator, V. Angelopoulos, NASA, and NSF for providing the Data. Open Data for Scientific Use.",
"PT0.2S",
"2019-05-22T00:00:00.000",
"2022-09-24T23:59:59.999",
"",
"2.6.0"
],
[
"ELB_L1_EPDIF",
"spase://NASA/NumericalData/ELFIN/B/EPD/L1/ion/PT0.264S",
"spase://NASA/Instrument/ELFIN/B/EPD",
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Atmosphere",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-03-03T13:45:36Z",
"https://doi.org/10.48322/0etj-j292",
"ELFIN B Energetic Particle Detectors for Ions (EPD-I) 0.264 s Data",
"",
"Please acknowledge the Principal Investigator, V. Angelopoulos, NASA, and NSF for providing the Data. Open Data for Scientific Use.",
"PT0.264S",
"2019-05-22T00:00:00.000",
"2022-09-19T23:59:59.999",
"",
"2.6.0"
],
[
"EQ_PP_AUX",
"spase://ESA/NumericalData/Equator-S/Ephemeris/PrimeParameter/PT4S",
"spase://SMWG/Instrument/Equator-S/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.EquatorialRegion"
],
"",
"",
"See also the TEXT Global Attribute for the Caveats File Location",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Epheneris and Auxiliary Prime Parameter 4 s Data",
"",
"G. Paschmann, Refer to ESDS for Rules of Acknowledgement Refer to EQS-MPE-EDC-01.",
"PT4S",
"1997-12-16T11:25:00",
"1998-04-30T01:52:44",
"",
"2.3.0"
],
[
"EQ_PP_EDI",
"spase://ESA/NumericalData/Equator-S/EDI/PP/PT60s",
"spase://SMWG/Instrument/Equator-S/EDI",
[
"ThermalPlasma",
"ElectricField"
],
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Electron Drift Instrument (EDI) 1-min Prime Parameters",
"",
"",
"PT60S",
"1998-03-25T21:53:13",
"1998-04-26T09:25:25",
"",
"2.3.0"
],
[
"EQ_PP_EPI",
"spase://ESA/NumericalData/Equator-S/EPI/PP/PT60S",
"spase://SMWG/Instrument/Equator-S/EPI",
"EnergeticParticles",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Energetic Particle Instrument (EPI) 1-min Prime Parameters",
"",
"",
"PT60S",
"1997-01-01T00:00:01",
"1998-04-30T01:56:05",
"",
"2.3.0"
],
[
"EQ_PP_ICI",
"spase://ESA/NumericalData/Equator-S/ICI/PP/PT60S",
"spase://SMWG/Instrument/Equator-S/ICI",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Ion Composition Instrument (ICI) Prime Parameters",
"",
"",
"PT60S",
"1997-12-16T00:00:01",
"1998-04-30T01:56:05",
"",
"2.3.0"
],
[
"EQ_PP_MAM",
"spase://ESA/NumericalData/Equator-S/MAM/PP/PT60S",
"spase://SMWG/Instrument/Equator-S/MAM",
"MagneticField",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Magnetic Field Instrument (MAM) 1-min Prime Parameters",
"",
"",
"PT60S",
"1997-12-16T00:00:01",
"1998-04-30T01:56:05",
"",
"2.3.0"
],
[
"EQ_PP_PCD",
"spase://ESA/NumericalData/Equator-S/PCD/PP/PT60S",
"spase://SMWG/Instrument/Equator-S/PCD",
"ThermalPlasma",
[
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"Earth.NearSurface.Ionosphere"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Potential Control Device (PDC) 1-min Prime Parameters",
"",
"Please acknowledge NASA Space Physics Data Facility, National Space Science Data Center and the Principal Investigator for data usage.",
"PT60S",
"1997-12-16T00:00:00",
"1998-04-30T01:56:09",
"",
"2.3.0"
],
[
"EQ_SP_SFD",
"spase://ESA/NumericalData/Equator-S/SFD/PP/PT60S",
"spase://SMWG/Instrument/Equator-S/SFD",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:14Z",
"",
"Equator-S Scintillating Fibre Detector (SFD) 1-min Prime Parameters",
"",
"",
"PT60S",
"1997-12-16T00:00:01",
"1998-04-30T01:56:05",
"",
"2.3.0"
],
[
"FAST_HR_DCB",
"spase://NASA/NumericalData/FAST/MAG/Fluxgate/PT7.8125MS",
[
"spase://SMWG/Instrument/FAST/Ephemeris",
"spase://SMWG/Instrument/FAST/MAG"
],
[
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"Continuous coverage not guaranteed. Check the inventory graph for coverage.",
"",
"2025-05-06T15:38:11Z",
"https://doi.org/10.48322/86pq-hb06",
"FAST Fluxgate Magnetometer High-Resolution 7.8125 ms Data",
"",
"C.W. Carlson, R.J. Strangeway Include Acknowledgement in any publication.",
"PT0.0078125S",
"1996-09-28T00:45:21.000",
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"",
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"https://doi.org/10.48322/23b9-6g23",
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"",
"",
"Continuous coverage not guaranteed. Check the inventory graph for coverage.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/78b7-gk94",
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"",
"GOES 10 high resolution magnetometer data",
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"",
"Note that magnetic field values have been replaced with missing data values during calibration periods. Also, note that there can be small jumps in the data (typically <1 nT) when the torquer counts go through zero. The magnitude of the effect can be different for different spacecraft.\n\nThe GOES 8 to GOES 12 spacecraft are 3-axis stabilized and there is only one opportunity for a spin maneuver at the beginning of the mission to determine on-orbit offsets. There are additional complications that result from needing to know the changing offsets introduced by torquer coils on the satellites. Though comparisons of data to model fields during quiet times, we are doing rather well with the offsets, but it is not possible to give an exact number for the accuracy. We continue to look at comparisons of data and models, and data to other nearby spacecraft encounters. We are interested in anything learned by the user, or working with the user to help interpret the data, or to answer questions. While we have put in a significant effort to remove the effects of torquer coil interference, in the 0.512 s data there can be small, typically less than 1 nT spikes in the data at the time of torquer current changes. More information on this topic is included the more extensive \"readme file\". This file is a living document that will be updated periodically.",
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"",
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"1994-11-25T23:57:30",
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"",
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"",
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[
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"",
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],
"NOAA Environmental Research Laboratories, Terry G. Onsager",
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"1995-01-01T00:00:00",
"2003-06-30T23:59:59",
"Time format in data files is year-month-day hour:minute:seconds.",
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],
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[
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"",
"GOES 8 Triaxial Fluxgate Magnetometer (FGM), Magnetic Field and Ephemeris, Multiple Coordinate Systems, 1.0 min Data",
"",
"Users should acknowledge the CDAWeb for providing access to the data as well as the P.I. H. Singer and originating institution NOAA Space Environment Center",
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"1995-12-01T00:00:30",
"2003-04-08T23:59:30",
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[
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"GOES",
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"",
"GOES 9 Energetic Particle Monitor Data at 5 min Time Resolution",
[
"GOES 9 EPS data",
"GOES 9 EP8 data"
],
"NOAA Environmental Research Laboratories, Terry G. Onsager",
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"1996-04-01T00:00:00",
"1998-07-31T23:59:59",
"Time format in data files is year-month-day hour:minute:seconds.",
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],
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"",
"Users should acknowledge the CDAWeb for providing access to the data as well as the P.I. H. Singer and originating institution NOAA Space Environment Center",
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],
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"",
"",
"2025-05-05T15:38:11Z",
"https://doi.org/10.48322/wdvm-s118",
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"",
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"",
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"2005-12-30T23:59:59",
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"",
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],
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],
"",
"",
"Please use the Editor-A LEP dataset prior to the Editor-B LEP dataset since plasma moments in the Editor-A data are more reliable. (Plasma moments inthe Editor-B are calculated onboard.)\n\n The ion moment data of the solar wind analyzer (LEP-SW) should be used only qualitatively.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Editor-A 12 second Low-Energy Particles",
"",
"In any publications, the use of the Geotail data should be acknowledged, for example, as \"Geotail magnetic field data were provided by Y. Saito, JAXA in Japan.\"",
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"2006-12-30T13:30:52",
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],
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"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Editor-A 3-second Magnetic Field Data",
"",
"In any publications, the use of the Geotail data should be acknowledged, for example, as \"Geotail magnetic field data were provided by T. Nagai, JAXA in Japan.\"",
"PT3S",
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"",
"",
"2.3.0"
],
[
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"spase://JAXA/NumericalData/Geotail/LEP/EDB/PT12S",
"spase://SMWG/Instrument/Geotail/LEP",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"Please use the Editor-A LEP dataset prior to the Editor-B LEP dataset since plasma moments in the Editor-A data are more reliable. (Plasma moments inthe Editor-B are calculated onboard.)\n\n The ion moment data of the solar wind analyzer (LEP-SW) should be used only qualitatively.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Editor-B 12 second Low-Energy Particles",
"",
"In any publications, the use of the Geotail data should be acknowledged, for example, as \"Geotail magnetic field data were provided by Y. Saito, JAXA in Japan.\"",
"PT12S",
"1993-10-05T10:09:45",
"2006-12-31T23:59:17",
"",
"2.3.0"
],
[
"GE_EDB3SEC_MGF",
"spase://JAXA/NumericalData/Geotail/MGF/EDB.PT3S",
"spase://SMWG/Instrument/Geotail/MGF",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Editor-B 3-second Magnetic Field Data",
"",
"In any publications, the use of the Geotail data should be acknowledged, for example, as \"Geotail magnetic field data were provided by T. Nagai, JAXA in Japan.\"",
"PT3S",
"1993-09-01T00:00:02",
"",
"",
"2.3.0"
],
[
"GE_H0_CPI",
"spase://JAXA/NumericalData/Geotail/CPI/SWA/PT48S",
"spase://SMWG/Instrument/Geotail/CPI/SWA",
[
"ThermalPlasma",
"IonComposition"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath"
],
"",
"",
"The CPI solar wind ion analyzer is an E/Q analyzer and the initial distribution functions were calculated assuming that the plasma is H+. Care must be taken when multi-component plasmas are present. If He++ is present and is flowing with the same speed as the H+ component, it will contribute to the distribution function at twice the velocity (four times the energy) of the H+. To facilitate the automated processing of the data the integral was evaluated between vmin = 171 km/s and vmax = 1.35 × u . The resulting temperatures produce excellent fits to the observations. When He++ is present the distribution functions are consistent with an He++ temperature, THe++ = 4 × TH+, i.e., the H+ and He++ have similar thermal velocities.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail CPI Definitive Solar Wind Moments",
"",
"",
"PT48S",
"1992-09-28T00:00:33",
"",
"",
"2.3.0"
],
[
"GE_HPAMOM_CPI",
"spase://JAXA/NumericalData/Geotail/CPI/HPA/PT64S",
"spase://SMWG/Instrument/Geotail/CPI/HPA",
"ThermalPlasma",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"The electron sensors for the CPI HP analyzer require regular intercalibration. Also, their sensitivity declined over time. A detrending factor is applied so that average electron densities are consistent with ion densities. The HP ion data and the electron data are good through a the end of 2005. The sensitivity decline had been linear until the end of 2005, but hasn't been checked for 2006 or 2007. That may affect the HP electron parameters for 2006 and 2007, but not the HP ion parameters.\n\n In June of 2007, the HP sensor bias voltage was raised to improve the electron gain, which over the course of 15 years had dropped by about half. This requires recalibration of both the HP ion sensors and the HP electron sensors.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail CPI Hot Plasma Moments",
"Geotail CPI HPA High Time Resolution Plasma Moments",
"",
"PT64S",
"1992-10-06T00:00:28",
"",
"",
"2.3.0"
],
[
"GE_K0_CPI",
"spase://JAXA/NumericalData/Geotail/CPI/KeyParameter/PT64S",
[
"spase://SMWG/Instrument/Geotail/CPI/HPA",
"spase://SMWG/Instrument/Geotail/CPI/SWA"
],
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"The CPI solar wind ion analyzer is an E/Q analyzer and the initial distribution functions were calculated assuming that the plasma is H+. Care must be taken when multi-component plasmas are present. If He++ is present and is flowing with the same speed as the H+ component, it will contribute to the distribution function at twice the velocity (four times the energy) of the H+. To facilitate the automated processing of the data the integral was evaluated between vmin = 171 km/s and vmax = 1.35 × u . The resulting temperatures produce excellent fits to the observations. When He++ is present the distribution functions are consistent with an He++ temperature, THe++ = 4 × TH+, i.e., the H+ and He++ have similar thermal velocities.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail CPI Plasma Key Parameters (64s)",
"",
"",
"PT64S",
"1992-09-08T07:30:40",
"",
"",
"2.3.0"
],
[
"GE_K0_EFD",
"spase://JAXA/NumericalData/Geotail/EFD/PT64S",
"spase://SMWG/Instrument/Geotail/EFD",
"ElectricField",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail EFD 64-sec Key Parameters",
"",
"",
"PT64S",
"1992-09-08T00:00:00",
"",
"Data are current to within days or weeks.",
"2.3.0"
],
[
"GE_K0_EPI",
"spase://JAXA/NumericalData/Geotail/EPIC/PT96S",
"spase://SMWG/Instrument/Geotail/EPIC",
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail EPIC 96-sec Key Parameters",
"",
"",
"PT96S",
"1992-09-08T00:00:00",
"",
"Data are current to within days or weeks.",
"2.3.0"
],
[
"GE_K0_LEP",
"spase://JAXA/NumericalData/Geotail/LEP/PT64S",
"spase://SMWG/Instrument/Geotail/LEP",
[
"EnergeticParticles",
"ThermalPlasma"
],
"Heliosphere.NearEarth",
"",
"CALIBRATED",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail LEP 64-sec Key Parameters",
"",
"",
"PT64S",
"1992-01-01T00:00:00",
"",
"Data are current to within days or weeks.",
"2.3.0"
],
[
"GE_K0_MGF",
"spase://JAXA/NumericalData/Geotail/MGF/PT64S",
"spase://SMWG/Instrument/Geotail/MGF",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"Switched from outer magnetometer to inner in January 2007. This data is computed with a preliminary algorithm and is not necessarily complete nor is it certified by the experimenters or considered publishable.",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail KP Magnetic Field Data (64s)",
"",
"Data were provided by T. Nagai at Institute of Space and Astronautical Science, JAXA in Japan.",
"PT64S",
"1992-09-04T19:14:06",
"",
"",
"2.3.0"
],
[
"GE_K0_PWI",
"spase://JAXA/NumericalData/Geotail/PWI/KP/PT64S",
"spase://SMWG/Instrument/Geotail/PWI",
[
"MagneticField",
"ThermalPlasma"
],
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail PWI 64-sec Key Parameters",
"",
"",
"PT64S",
"1992-09-08T07:30:05",
"",
"",
"2.3.0"
],
[
"GE_K0_SPHA",
"spase://JAXA/NumericalData/Geotail/Ephemeris/Spin_Phase_KP/PT10M",
"spase://SMWG/Instrument/Geotail/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Spin Phase Key Parameters",
"",
"",
"PT10M",
"1992-09-08T07:29:57",
"",
"",
"2.3.0"
],
[
"GE_OR_DEF",
"spase://JAXA/NumericalData/Geotail/Ephemeris/PT10M",
"spase://SMWG/Instrument/Geotail/Ephemeris",
"Ephemeris",
"",
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Spacecraft Definitive Positions",
"",
"",
"PT10M",
"1992-07-27T16:00:00",
"",
"",
"2.3.0"
],
[
"GE_OR_PRE",
"spase://JAXA/NumericalData/Geotail/Ephemeris/PT600S",
"spase://SMWG/Instrument/Geotail/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail Predicted Orbit",
"",
"",
"PT600S",
"1992-09-08T00:00:00",
"",
"Predicted data are given to about a month into the future.",
"2.3.0"
],
[
"GE_SW_CPI",
"spase://JAXA/NumericalData/Geotail/CPI/SWMD/PT48S",
"spase://SMWG/Instrument/Geotail/CPI/SWA",
[
"ThermalPlasma",
"IonComposition"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2021-04-27T17:52:35Z",
"",
"Geotail CPI Definitive Solar Wind Moments and three-dimensional velocity distribution function",
"",
"Principle Investigator Louis.A.Frank,the radio and plasma wave research group at The University of Iowa, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT48S",
"1992-10-06T00:00:55.000Z",
"1994-10-01T00:00:00.000Z",
"",
"2.3.0"
],
[
"GOES10_EPHEMERIS_SSC",
"spase://NOAA/NumericalData/GOES/10/Ephemeris/PT1M",
[
"spase://SMWG/Instrument/GOES/10/Ephemeris",
"spase://SMWG/Instrument/GOES/10/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 10 Ephemeris, Orbital Positions generated via Satellite Situation Center, SSC, Services, 1 min Data",
"",
"Please acknowledge R. M. Candey, the NASA GSFC Satellite Situation Center, SSC, and the National Oceanic and Atmospheric Administration.",
"PT1M",
"1997-04-25T00:06:00.000Z",
"1997-04-25T00:06:00.000Z",
"",
"2.3.0"
],
[
"GOES11_EPHEMERIS_SSC",
"spase://NOAA/NumericalData/GOES/11/Ephemeris/PT3M",
[
"spase://SMWG/Instrument/GOES/11/Ephemeris",
"spase://SMWG/Instrument/GOES/11/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 11 Ephemeris, Orbital Positions generated via Satellite Situation Center, SSC, Services, 3 min Data",
"",
"Please acknowledge R. M. Candey, the NASA GSFC Satellite Situation Center, SSC, and the National Oceanic and Atmospheric Administration.",
"PT3M",
"2000-05-17T00:00:00.000Z",
"2000-05-17T00:00:00.000Z",
"",
"2.3.0"
],
[
"GOES11_K0_EP8",
"spase://NOAA/NumericalData/GOES/11/EPS/PT5M",
"spase://SMWG/Instrument/GOES/11/SEM",
"EnergeticParticles",
"",
"",
"Level-0",
"",
[
"5 min",
"geosynchronous",
"GOES",
"energetic particle monitor",
"energetic particles"
],
"2021-04-27T17:52:57Z",
"",
"GOES 11 Energetic Particle Sensor Data at 5 min Time Resolution",
"GOES 11 EPS data",
"NOAA Environmental Research Laboratories, Terry G. Onsager",
"PT5M",
"2000-07-01T00:00:00",
"2011-02-28T23:59:59",
"Time format in data files is year-month-day hour:minute:seconds.",
"2.3.0"
],
[
"GOES11_K0_MAG",
"spase://NOAA/NumericalData/GOES/11/MAG/PT1M",
"spase://SMWG/Instrument/GOES/11/MAG",
"MagneticField",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"1 min",
"geosynchronous",
"GOES",
"magnetic field",
"magnetometer",
"Magnetic Field Monitor"
],
"2021-04-27T17:52:57Z",
"",
"GOES 11 Magnetic Field Sensor data at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 11 MFS data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Howard J. Singer",
"PT1M",
"2003-06-01T00:00:00",
"2011-02-28T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.0"
],
[
"GOES12_EPHEMERIS_SSC",
"spase://NOAA/NumericalData/GOES/12/Ephemeris/PT1M",
[
"spase://SMWG/Instrument/GOES/12/Ephemeris",
"spase://SMWG/Instrument/GOES/12/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 12 Ephemeris, Orbital Positions generated via Satellite Situation Center, SSC, Services, 1 min Data",
"",
"Please acknowledge R. M. Candey, the NASA GSFC Satellite Situation Center, SSC, and the National Oceanic and Atmospheric Administration.",
"PT1M",
"2006-01-01T00:00:00.000Z",
"2016-01-01T00:00:00.000Z",
"",
"2.3.0"
],
[
"GOES12_K0_MAG",
"spase://NOAA/NumericalData/GOES/12/MAG/PT1M",
"spase://SMWG/Instrument/GOES/12/MAG",
"MagneticField",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"1 min",
"geosynchronous",
"GOES",
"magnetic field",
"magnetometer",
"Magnetic Field Monitor"
],
"2021-04-27T17:52:57Z",
"",
"GOES 12 Magnetic Field Sensor data at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 12 MFS data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Howard J. Singer",
"PT1M",
"2003-01-01T00:00:00",
"2010-08-31T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.0"
],
[
"GOES13_EPEAD-SCIENCE-ELECTRONS-E13EW_1MIN",
"spase://NOAA/NumericalData/GOES/13/EPS/EPEAD/E13EW/PT1M",
"spase://SMWG/Instrument/GOES/13/EPS",
"EnergeticParticles",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"60 s",
"geosynchronous",
"GOES",
"Energetic Proton, Electron and Alpha Detectors"
],
"2021-04-27T17:52:57Z",
"",
"GOES 13 Energetic Proton, Electron and Alpha Detector (EPEAD) electron fluxes data at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 13 EPEAD E13EW data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Terry G. Onsager",
"PT1M",
"2010-05-01T00:00:00",
"2017-06-04T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.1"
],
[
"GOES13_EPHEMERIS_SSC",
"spase://NOAA/NumericalData/GOES/13/Ephemeris/PT3M",
[
"spase://SMWG/Instrument/GOES/13/Ephemeris",
"spase://SMWG/Instrument/GOES/13/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 13 Ephemeris, Orbital Positions generated via Satellite Situation Center, SSC, Services, 3 min Data",
"",
"Please acknowledge R. M. Candey, the NASA GSFC Satellite Situation Center, SSC, and the National Oceanic and Atmospheric Administration.",
"PT3M",
"2006-06-10T00:00:00.000Z",
"",
"",
"2.3.0"
],
[
"GOES13_EPS-MAGED_1MIN",
"spase://NOAA/NumericalData/GOES/13/EPS/MAGED/19ME15/PT1M",
"spase://SMWG/Instrument/GOES/13/EPS",
"EnergeticParticles",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"1 min",
"geosynchronous",
"GOES",
"Magnetospheric Electron Detector"
],
"2021-04-27T17:52:57Z",
"",
"GOES 13 Magnetospheric Electron Detector (MAGED) data with average flux of 40 keV at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 13 MAGED 19ME15 data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Terry G. Onsager",
"PT1M",
"2006-06-01T00:00:00",
"2017-06-11T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.1"
],
[
"GOES13_EPS-MAGED_5MIN",
"spase://NOAA/NumericalData/GOES/13/EPS/MAGED/19ME15/PT5M",
"spase://SMWG/Instrument/GOES/13/EPS",
"EnergeticParticles",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"5 min",
"geosynchronous",
"GOES",
"Magnetospheric Electron Detector"
],
"2021-04-27T17:52:57Z",
"",
"GOES 13 Magnetospheric Electron Detector (MAGED) data with average flux of 40 keV at 5 min Time Resolution in Spacecraft Coordinates",
"GOES 13 MAGED 19ME15 data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Terry G. Onsager",
"PT5M",
"2011-01-01T00:00:00",
"2017-06-11T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.1"
],
[
"GOES13_EPS-PITCH-ANGLES_1MIN",
"spase://NOAA/NumericalData/GOES/13/EPS/SEM/L2/PitchAngle/PT1M",
"spase://SMWG/Instrument/GOES/13/SEM",
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 13 Energetic Particle Sensor (EPS), MagED and MagPD Telescope Magnetic Field Dependent Pitch Angle Directions, 1 min Data",
"",
"J.V. Rodriguez, NOAA NGDC and SWPC",
"PT1M",
"2010-05-01T00:00:00.000",
"2017-08-16T23:59:59.999",
"",
"2.3.0"
],
[
"GOES14_EPEAD-SCIENCE-ELECTRONS-E13EW_1MIN",
"spase://NOAA/NumericalData/GOES/14/EPS/EPEAD/E13EW/PT1M",
"spase://SMWG/Instrument/GOES/14/EPS",
"EnergeticParticles",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"60 s",
"geosynchronous",
"GOES",
"Energetic Proton, Electron and Alpha Detectors"
],
"2021-04-27T17:52:57Z",
"",
"GOES 14 Energetic Proton, Electron and Alpha Detector (EPEAD) electron fluxes data at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 14 EPEAD E13EW data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Terry G. Onsager",
"PT1M",
"2012-10-01T00:00:00",
"2016-11-17T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.1"
],
[
"GOES14_EPHEMERIS_SSC",
"spase://NOAA/NumericalData/GOES/14/Ephemeris/PT3M",
[
"spase://SMWG/Instrument/GOES/14/Ephemeris",
"spase://SMWG/Instrument/GOES/14/MAG"
],
[
"Ephemeris",
"MagneticField"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"GOES 14 Ephemeris, Orbital Positions generated via Satellite Situation Center, SSC, Services, 3 min Data",
"",
"Please acknowledge R. M. Candey, the NASA GSFC Satellite Situation Center, SSC, and the National Oceanic and Atmospheric Administration.",
"PT3M",
"2009-07-09T00:00:00.000Z",
"",
"",
"2.3.0"
],
[
"GOES14_EPS-MAGED_1MIN",
"spase://NOAA/NumericalData/GOES/14/EPS/MAGED/19ME15/PT1M",
"spase://SMWG/Instrument/GOES/14/EPS",
"EnergeticParticles",
"",
"",
"Level-2",
"Flags=-99999.0",
[
"1 min",
"geosynchronous",
"GOES",
"Magnetospheric Electron Detector"
],
"2021-04-27T17:52:57Z",
"",
"GOES 14 Magnetospheric Electron Detector (MAGED) data with average flux of 40 keV at 1 min Time Resolution in Spacecraft Coordinates",
"GOES 14 MAGED 19ME15 data",
"NASA Office of Space Science Applications (United States), NOAA National Environmental Satellite Service (United States), Terry G. Onsager",
"PT1M",
"2009-07-01T00:00:00",
"2016-11-17T23:59:00",
"Time format in data files is year-month-day hour:minute:seconds. Data file may fill out the first month and last month with flags.",
"2.3.1"
],
[
"GOES14_EPS-MAGED_5MIN",
"spase://NOAA/NumericalData/GOES/14/EPS/MAGED/19ME15/PT5M",
"spase://SMWG/Instrument/GOES/14/EPS",
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],
[
"I1_AV2_OTT",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Version2/Ottawa/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Ottawa, QC, Canada, OTT, Version 2, Latitude 45°, Longitude 284°, 29 s Data",
"",
"Please acknowledge the Principal Investigator James H. Whitteker, Robert F. Benson, Dieter K. Bilitza, and Leonard N. Garcia for use of the Data",
"PT29S",
"1969-01-30T14:50:12",
"1983-12-17T13:07:34",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV2_QUI",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Version2/Quito/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Quito, Equador, QUI, Version 2, Latitude -1°, Longitude 281°, 29 s Data",
"",
"Please acknowledge the Principal Investigator James H. Whitteker, Robert F. Benson, Dieter K. Bilitza, and Leonard N. Garcia for use of the Data",
"PT29S",
"1969-01-31T04:20:04",
"1972-03-29T04:05:42",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV2_ULA",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Version2/Fairbanks/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Fairbanks, AK, ULA, Version 2, Latitude 65°, Longitude 212°, 29 s Data",
"",
"Please acknowledge the Principal Investigator James H. Whitteker, Robert F. Benson, Dieter K. Bilitza, and Leonard N. Garcia for use of the Data",
"PT29S",
"1975-01-04T18:15:50",
"1979-09-14T12:06:02",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_ALL",
"spase://NASA/NumericalData/ISIS1/SFS/Ionogram/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Waves.Active",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"topside sounder",
"fixed- and swept-frequency sounder",
"topside ionosphere",
"ionospheric reflections",
"ground reflections",
"ionospheric echoes",
"ground echoes",
"ducted echoes",
"wave scattering",
"field-aligned irregularities",
"FAI",
"plasma resonance",
"plasma waves",
"AKR",
"solar type III bursts",
"upper-hybrid noise band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS 1 Topside Sounder Ionograms",
"ISIS-1 Topside Sounder Ionogram CDFs at NASA's CDAWeb",
"Users please acknowledge the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center, ISIS-1 SFS instrument Principal Investigator J. H. Whitteker and ISIS Data-Restoration project lead Robert F. Benson.",
"PT24S",
"1969-01-30T14:50:12Z",
"1983-12-30T15:19:33Z",
"The cadence is 17 or 29 s for ionograms that have a swept-frequency portion from 0.1 to 10.0 MHz and 0.1 to 20 MHz, respectively. NOTE: for ISIS2 the appropriate values are 14 and 22.5 s, for 0.1 to 10.0 MHz and 0.1 to 20 MHz ionograms, respectively.",
"2.3.2"
],
[
"I1_AV_KER",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/KerguelenIsland/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Kerguelen Island, France: KER, Latitude -49, Longitude 70",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1983-08-24T15:21:21",
"1983-12-30T15:19:33",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_KSH",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Kashima/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Kashima, Japan: KSH, Latitude 36, Longitude 141",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1978-01-06T04:52:17",
"1981-12-30T16:22:49",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_KWA",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Kwajalein/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Kwajalein, Marshall Islands: KWA, Latitude 9, Longitude 168",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1978-01-03T04:13:25",
"1978-12-30T21:34:08",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_ODG",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Ouagadougou/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Ouagadougou, Burkina Faso: ODG, Latitude 14, Longitude 359",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-02-03T13:27:25",
"1976-06-28T17:19:36",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_ORR",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Orroral/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Orroral, Australia: ORR, Latitude -36, Longitude 149",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1970-01-28T09:47:09",
"1981-08-24T14:00:56",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_OTT",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Ottawa/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Ottawa, QC, Canada: OTT, Latitude 45, Longitude 284",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-01-30T14:50:12",
"1983-12-17T13:08:05",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_QUI",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Quito/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Quito, Equador: QUI, Latitude -1, Longitude 281",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-01-31T04:20:04",
"1978-06-22T04:44:35",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_RES",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/ResoluteBay/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Resolute Bay, NU, Canada: RES, Latitude 75, Longitude 265",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-01-30T21:18:14",
"1976-02-22T19:07:32",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_SNT",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Santiago/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Santiago, Chile: SNT, Latitude -33, Longitude 298",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-01-31T01:29:39",
"1972-12-25T07:01:13",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_SOD",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Sodankyla/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Sodankyla, Finland: SOD, Latitude 67, Longitude 27",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1977-12-14T22:30:46",
"1979-03-30T14:10:33",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_TRO",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Tromso/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Tromso, Norway: TRO, Latitude 70, Longitude 19",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-02-05T18:15:49",
"1969-12-28T15:12:00",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_ULA",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Fairbanks/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Fairbanks, AK: ULA, Latitude 65, Longitude 212",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1975-01-04T18:15:16",
"1979-09-14T12:06:35",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_AV_WNK",
"spase://NASA/NumericalData/ISIS1/SFS/AverageIonogram/Winkfield/PT29S",
"spase://SMWG/Instrument/ISIS1/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2025-09-10T15:38:11Z",
"",
"ISIS-1 Topside Sounder Average Ionogram over Winkfield, United Kingdom: WNK, Latitude 51, Longitude 359",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT29S",
"1969-02-03T01:02:10",
"1975-07-18T05:06:36",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I1_NEPROF_TOPS",
"spase://NASA/NumericalData/ISIS1/SFS/TOPS",
"spase://SMWG/Instrument/ISIS1/SFS",
"Profile",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionosphere",
"Topside",
"Sounder",
"Ionogram"
],
"2021-04-27T15:38:11Z",
"",
"ISIS 1 CRC Electron Density Profiles",
"",
"Please acknowledge the NASA Space Physics Data Facility and the instrument's Principal Investigator for data usage.",
"",
"1969-02-01T15:50:12",
"1980-05-30T02:41:08",
"",
"2.7.0"
],
[
"I2_AV_ACN",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/AscensionIsland/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Ascension Island, United Kingdom: ACN, Latitude -8, Longitude 346",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1975-01-09T01:22:59",
"1978-09-28T16:37:11",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_ADL",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/TerreAdelie/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Terre Adelie, Antarctica: ADL, Latitude -67, Longitude 140",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-01-12T10:18:21",
"1983-02-03T18:47:56",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_AME",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Ahmedabad/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Ahmedabad, India: AME, Latitude 23, Longitude 73",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-02-03T04:00:26",
"1978-01-23T07:28:43",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_BRZ",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Brazzaville/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Brazzavillle, Congo: BRZ, Latitude -4, Longitude 15",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-08-05T16:17:40",
"1975-09-25T16:12:59",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_BUR",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Johannesburg/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Johannesburg, South Africa: BUR, Latitude -26, Longitude 28",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-08-07T15:26:03",
"1976-01-16T19:18:39",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_CNA",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/LasPalmas/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Las Palmas, Canary Island, Spain: CNA, Latitude 28, Longitude 345",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1974-01-16T17:42:39",
"1976-02-01T11:15:40",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_KER",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/KerguelenIsland/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Kerguelen Island, France: KER, Latitude -49, Longitude 70",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1977-01-01T00:01:37",
"1984-01-27T18:16:53",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_KRU",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Kourou/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Kourou, French Guyana: KRU, Latitude 5, Longitude 307",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-02-06T01:16:08",
"1978-07-23T22:07:30",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_KSH",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Kashima/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Kashima, Japan: KSH, Latitude 36, Longitude 141",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-01-01T00:01:10",
"1984-01-06T14:08:01",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_KWA",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Kwajalein/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Kwajalein, Marshall Islands: KWA, Latitude 9, Longitude 168",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1978-01-10T08:46:53",
"1978-11-09T07:38:18",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_LAU",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Lauder/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Lauder, New Zealand: LAU, Latitude -45, Longitude 170",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-01-01T04:14:29",
"1981-01-18T15:47:50",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_ODG",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Ouagadougou/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Ouagadougou, Burkina Faso: ODG, Latitude 14, Longitude 359",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-08-06T05:36:37",
"1979-11-22T15:25:12",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_ORR",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Orroral/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Orroral, Australia: ORR, Latitude -36, Longitude 149",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-03-15T03:33:11",
"1981-07-20T20:42:22",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_OTT",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Ottawa/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Ottawa, QC, Canada: OTT, Latitude 45, Longitude 284",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1971-11-11T18:18:16",
"1984-01-04T05:16:00",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_QUI",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Quito/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Quito, Equador: QUI, Latitude -1, Longitude 281",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-01-03T02:22:10",
"1979-10-18T04:22:30",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_RES",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/ResoluteBay/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Resolute Bay, NU, Canada: RES, Latitude 75, Longitude 265",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1971-04-01T09:22:52",
"1983-01-13T11:06:43",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_SNT",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Santiago/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Santiago, Chile: SNT, Latitude -33, Longitude 298",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-06-15T09:48:17",
"1980-03-21T09:09:03",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_SOD",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Sodankyla/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Sodankyla, Finland: SOD, Latitude 67, Longitude 27",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1977-12-11T21:47:50",
"1978-09-13T21:01:48",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_SOL",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/FalklandIslands/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Falkland Island, United Kingdom: SOL, Latitude -52, Longitude 302",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-01-12T16:31:05",
"1972-12-10T00:57:02",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_SYO",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/SyowaBase/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Syowa Base, Antartica: SYO, Latitude -69, Longitude 40",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-02-03T05:49:37",
"1983-01-13T11:06:43",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_TRO",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Tromso/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Tromso, Norway: TRO, Latitude 70, Longitude 19",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-01-19T10:38:36",
"1977-10-06T20:20:00",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_ULA",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Fairbanks/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Fairbanks, AK: ULA, Latitude 65, Longitude 212",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1972-12-31T00:00:00",
"1979-07-30T02:17:45",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_AV_WNK",
"spase://NASA/NumericalData/ISIS2/SFS/AverageIonogram/Winkfield/PT22S",
"spase://SMWG/Instrument/ISIS2/SFS",
[
"Spectrum",
"Waves.Active"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
[
"Ionogram",
"Topside Sounder",
"Swept Frequency Sounder",
"Topside Ionosphere",
"Ionospheric Reflections",
"Ground Reflections",
"Ionospheric Echoes",
"Ground Echoes",
"Ducted Echoes",
"Wave Scattering",
"Field-Aligned Irregularities, FAI",
"Plasma Resonance",
"Plasma Waves",
"Auroral Kilometric Radiation, AKR",
"Solar Type III Bursts",
"Upper Hybrid Noise Band"
],
"2021-04-27T15:38:11Z",
"",
"ISIS-2 Topside Sounder Average Ionogram over Winkfield, United Kingdom: WNK, Latitude 51, Longitude 359",
"",
"James H. Whitteker, Robert F. Benson, Dieter K. Bilitza. Please thank James H. Whitteker, Principal Investigator for the ISIS 1 Swept Frequency Sounder, SFS, Instrument and Robert F. Benson, Project Scientist for the Alouette/ISIS Data-Restoration",
"PT22S",
"1973-03-14T11:55:35",
"1979-07-15T04:35:11",
"The Cadence is 31 s between Ionograms. The Alouette 2 Ionograms have the slowest Sweep Rate of any of the Alouette/ISIS Topside Sounders sweeping from 0.12 to 14.5 MHz in about 28 s with a Frequency Sweep Rate of 0.13 MHz/s below 2.0 MHz, providing the highest Frequency Resolution of any of the ISIS Program Sounders. The Alouette 2 Frequency Sweep Rate above 2 MHz was 1 MHz/s. Alouette 2 did not have a Fixed Frequency Operation.",
"2.3.2"
],
[
"I2_NEPROF_TOPIST",
"spase://NASA/NumericalData/ISIS2/SFS/TOPIST",
"spase://SMWG/Instrument/ISIS2/SFS",
"Profile",
"Earth.NearSurface.Ionosphere",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"ISIS 2 TOPIST Produced Electron Density Profiles",
"",
"",
"",
"1971-11-11T18:18:40",
"1984-01-04T05:15:38",
"",
"2.3.2"
],
[
"I2_NEPROF_TOPS",
"spase://NASA/NumericalData/ISIS2/SFS/TOPS",
"spase://SMWG/Instrument/ISIS2/SFS",
"Profile",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere.Topside"
],
"",
"",
"",
[
"Ionosphere",
"Topside",
"Sounder",
"Ionogram"
],
"2025-09-10T15:38:11Z",
"",
"ISIS 2 CRC Electron Density Profiles",
"",
"Please acknowledge the NASA Space Physics Data Facility and the instrument's Principal Investigator for data usage.",
"",
"1971-04-08T22:27:48",
"1979-08-27T17:52:25",
"",
"2.7.0"
],
[
"I8_15SEC_MAG",
"spase://NASA/NumericalData/IMP8/MAG/PT15.36S",
"spase://SMWG/Instrument/IMP8/MAG",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"Level 2",
"The time resolution (cadence) is not constant. The time tag corresponds to the last 1.28s measurement in the 15.36s average. Since the data is on average 70% complete, this is quite often different from 15.36 seconds from the previous time tag. On average, however, it should be about 15.36 seconds.",
"Magnetic field",
"2025-10-09T12:34:56.789",
"https://doi.org/10.48322/pxb6-h511",
"IMP 8 MAG 15.36s Magnetic Field Measurements",
"",
"User will acknowledge the IMP-8 magnetometer team, and the data access path used, in any publication resulting from the use of these data.",
"PT15.36S",
"1973-10-30T15:00:32Z",
"2000-06-10T15:09:18.720Z",
"Instrument stopped working on 2000-06-10.",
"2.6.0"
],
[
"I8_320MSEC_MAG",
"spase://NASA/NumericalData/IMP8/MAG/PT0.32S",
"spase://SMWG/Instrument/IMP8/MAG",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/k2cv-vy73",
"IMP 8 MAG 320 msec GSE magnetic field data",
"",
"Dr. Adam Szabo",
"PT0.32S",
"1973-10-30T00:00:00",
"2000-06-10T00:00:00",
"",
"2.6.0"
],
[
"I8_H0_GME",
"spase://NASA/NumericalData/IMP8/GME/PT30M",
"spase://SMWG/Instrument/IMP8/MCGUIRE",
"EnergeticParticles",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"",
"2025-09-10T12:34:56.789",
"https://doi.org/10.48322/m36p-0998",
"IMP 8 Goddard Medium Energy (GME) 30-min energetic particle rates and fluxes",
"",
"Acknowledge Robert E. McGuire, the PI.",
"PT30M",
"1973-11-01T00:00:00",
"2001-10-26T00:00:00",
"",
"2.6.0"
],
[
"I8_H0_MITPLASMA",
"spase://NASA/NumericalData/IMP8/PLS/PT01M",
"spase://SMWG/Instrument/IMP8/PLS",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath"
],
"",
"",
"The cadence varies slightly (by a few seconds) and is approximately 1 minute. The parameter values are derived from taking moments of the distributions and from fits to the distributions. As can be seen easily by eye, there is some discrepancy between moments and our best (fit) parameters; moments are definitely less accurate. Use moment values with caution, and PLEASE request assistance or clarification. For the moment parameters, changes in value are more trustworthy than absolute values, but nothing is guaranteed to be accurate. A value of 9999.0 means that we couldn't calculate that parameter. All parameters are based on a convected, isotropic Maxwellian model. The moment values, for angles and for the speed, do NOT have aberration corrections included. This means that the total speeds are slightly too low, and that the angles are not really correct. In particular, the azimuthal (E/W) angle is about 4 degrees too positive; this can clearly be seen where both nonlinear and moment angles are available. If good angles cannot be obtained, there won't be any velocity components; speeds are available in some such cases. Dr. Joseph King (NASA/GSFC) has looked at 27-day averages of OMNIWeb data from 1984-1994. He finds (and the MIT team agrees) that there is an offset of about +2 degrees (from the South) in the N/S angle and an annual variation of that angle with an amplitude of about 1 degree. The MIT team believes that the annual variation is due to a tilt of the s/c spin axis. He found the mean flow longitude in that study to be -0.3 degrees with no obvious annual variation.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/4dhv-w146",
"IMP 8 MIT Full Resolution Definitive Interplanetary Plasma Data",
"IMP 8 Solar Wind Plasma Faraday Cup Data",
"For papers and presentations using these data, please acknowledge the MIT Space Plasma Physics Group and the path through which you accessed the data.",
"PT01M",
"1973-10-31T20:10:26",
"2006-07-26T17:10:34",
"",
"2.6.0"
],
[
"I8_OR_SSC",
"spase://NASA/NumericalData/IMP8/Ephemeris/PT12M",
"spase://SMWG/Instrument/IMP8/Ephemeris",
"Ephemeris",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"IMP 8 Spacecraft Positions",
"",
"",
"PT12M",
"1973-10-30T00:00:00Z",
"",
"",
"2.3.2"
],
[
"IA_K0_ENF",
"spase://NASA/NumericalData/Interball-2/SK3/KP/PT120S",
"spase://SMWG/Instrument/Interball-2/SKA3",
"MagneticField",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Auroral Probe SKA-3 2-min Key Parameters ",
"",
"",
"PT120S",
"1996-09-20T01:03:00",
"1997-03-28T23:59:00",
"",
"2.3.2"
],
[
"IA_K0_EPI",
"spase://NASA/NumericalData/Interball-2/DOK2A/KP/PT120S",
"spase://SMWG/Instrument/Interball-2/DOK2A",
"EnergeticParticles",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Auroral Energetic Particle 2-min Key Parameters",
"",
"",
"PT120S",
"1996-09-03T09:39:00",
"1997-10-30T12:51:00",
"",
"2.3.2"
],
[
"IA_K0_ICD",
"spase://NASA/NumericalData/Interball-2/PROMICS3/KP/PT120S",
"spase://SMWG/Instrument/Interball-2/PROMICS3",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Auroral PROMICS H+ and O+ 2-min Key Parameters",
"",
"",
"PT120S",
"1996-09-18T09:23:36",
"1998-05-01T09:28:02",
"",
"2.3.2"
],
[
"IA_K0_MFI",
"spase://NASA/NumericalData/Interball-2/IMAP3/PT120S",
"spase://SMWG/Instrument/Interball-2/IMAP3",
"MagneticField",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Aurora MAG 2-min Key Parameters",
"",
"",
"PT120S",
"1996-09-01T00:00:00",
"1997-06-17T00:00:00",
"",
"2.3.2"
],
[
"IA_OR_DEF",
"spase://NASA/NumericalData/Interball-2/Ephemeris/PT120S",
"spase://SMWG/Instrument/Interball-2/Ephemeris",
"Ephemeris",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Auroral Ephemeris Data",
"",
"",
"PT120S",
"1996-09-19T00:00:00",
"1997-06-04T23:50:00",
"",
"2.3.2"
],
[
"IBEX_H3_ENA_HI_R02_CG_NOSP_OMNI_6MO",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release02/CG/NOSP/Omni/P6M",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/rcw2-kh18",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 02, Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P6M",
"2008-12-25T00:00:00.000",
"2009-06-25T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R02_NOCG_NOSP_OMNI_6MO",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release02/NOCG/NOSP/Omni/P6M",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/0vjh-ph32",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 02, not Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P6M",
"2008-12-25T00:00:00.000",
"2009-06-25T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_NOSP_ANTIRAM_1YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/NOSP/Antiram/P1Y",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
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"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/8m6t-z779",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, not Survival Probability corrected, Antiram direction, West Longitude Ecliptic Maps, Level H3 (H3), annually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P1Y",
"2008-12-25T00:00:00.000",
"2010-12-26T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_NOSP_OMNI_6MO",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/NOSP/Omni/P6M",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/bfkf-5y54",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P6M",
"2008-12-25T00:00:00.000",
"2011-06-25T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_NOSP_RAM_1YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/NOSP/Ram/P1Y",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/4ey3-fd10",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, not Survival Probability corrected, Ram direction, West Longitude Ecliptic Maps, Level H3 (H3), annually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P1Y",
"2008-12-25T00:00:00.000",
"2010-12-26T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_SP_ANTIRAM_1YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/SP/Antiram/P1Y",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/db3x-tq55",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, Survival Probability corrected, Antiram direction, West Longitude Ecliptic Maps, Level H3 (H3), annually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P1Y",
"2008-12-25T00:00:00.000",
"2010-12-26T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_SP_OMNI_6MO",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/SP/Omni/P6M",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
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"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/c9gv-sz19",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P6M",
"2008-12-25T00:00:00.000",
"2011-06-25T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_CG_SP_RAM_1YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/CG/SP/Ram/P1Y",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
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"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/55hv-vx14",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, Compton-Getting corrected, Survival Probability corrected, Ram direction, West Longitude Ecliptic Maps, Level H3 (H3), annually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P1Y",
"2008-12-25T00:00:00.000",
"2010-12-26T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_NOCG_NOSP_ANTIRAM_1YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/NOCG/NOSP/Antiram/P1Y",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
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"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/c3kb-p352",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, not Compton-Getting corrected, not Survival Probability corrected, Antiram direction, West Longitude Ecliptic Maps, Level H3 (H3), annually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P1Y",
"2008-12-25T00:00:00.000",
"2010-12-26T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_NOCG_NOSP_OMNI_3YR",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/NOCG/NOSP/Omni/P3Y",
"spase://SMWG/Instrument/IBEX/Hi",
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"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/qmwe-ve75",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, not Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), three year average Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 4 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P3Y",
"2008-12-25T00:00:00.000",
"2008-12-25T23:59:59.999",
"",
"2.6.0"
],
[
"IBEX_H3_ENA_HI_R04_NOCG_NOSP_OMNI_6MO",
"spase://NASA/NumericalData/IBEX/Hi/H3/Release04/NOCG/NOSP/Omni/P6M",
"spase://SMWG/Instrument/IBEX/Hi",
"NeutralAtomImages",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2024-02-13T12:34:56.789",
"https://doi.org/10.48322/kef0-gf62",
"IBEX High Energy Neutral Atom Imager (Hi) Data Release 04, not Compton-Getting corrected, not Survival Probability corrected, Omnidirectional, West Longitude Ecliptic Maps, Level H3 (H3), semiannually averaged Data",
"",
"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 16 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
"P6M",
"2008-12-25T00:00:00.000",
"2011-06-25T23:59:59.999",
"",
"2.6.0"
],
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"Please acknowledge the IBEX Mission Principal Investigator, David J. McComas, Princeton University. The IBEX Release 10 data are archived as fully citable data. Please consult the IBEX Science Team personnel and publications for further details on production, processing, and usage of these data.",
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"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 12 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
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"Please acknowledge the IBEX Mission Principal Investigator, David J. McComas, Princeton University. The IBEX Release 13 data are archived as fully citable data. Please consult the IBEX Science Team personnel and publications for further details on production, processing, and usage of these data.",
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"",
"Please acknowledge the IBEX Mission Principal Investigator, D.J. McComas of Princeton University.. The IBEX Release 14 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
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"Please acknowledge the IBEX Mission Principal Investigator, Dr. David J McComas of Princeton University.. The IBEX Release 16 data are archived as fully citable data. Please consult IBEX team publications and personnel for further details on production, processing, and usage of these data.",
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"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_HK_AST",
"spase://NASA/NumericalData/IMAGE/HK/CDAWeb/PT24H",
"spase://SMWG/Instrument/IMAGE/HK",
"InstrumentStatus",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_HK_COM",
"spase://NASA/NumericalData/IMAGE/HK/CDAWeb/PT24H",
"spase://SMWG/Instrument/IMAGE/HK",
"InstrumentStatus",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_HK_FSW",
"spase://NASA/NumericalData/IMAGE/HK/CDAWeb/PT24H",
"spase://SMWG/Instrument/IMAGE/HK",
"InstrumentStatus",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_HK_PWR",
"spase://NASA/NumericalData/IMAGE/HK/CDAWeb/PT24H",
"spase://SMWG/Instrument/IMAGE/HK",
"InstrumentStatus",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_HK_TML",
"spase://NASA/NumericalData/IMAGE/HK/CDAWeb/PT24H",
"spase://SMWG/Instrument/IMAGE/HK",
"InstrumentStatus",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"IMAGE Housekeeping Data via CDAWeb",
"",
"Please acknowledge the IMAGE PI and the NASA Space Physics Data Facility.",
"PT24H",
"2000-03-25T00:00:00.000Z",
"2005-12-18T07:38:17.000Z",
"",
"2.2.2"
],
[
"IM_K0_RPI",
"spase://NASA/NumericalData/IMAGE/RPI/PT24H",
"spase://SMWG/Instrument/IMAGE/RPI",
"Waves.Active",
[
"Heliosphere.Inner",
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/0kry-rn33",
"IMAGE RPI Plasmagram/Echogram Key Parameters",
"",
"Please acknowledge the instrument PI and NASA's Space Physics Data Facility.",
"PT24H",
"2000-03-26T00:00:00.000Z",
"2005-12-18T00:00:00.000Z",
"",
"2.6.0"
],
[
"IM_K1_RPI",
"spase://NASA/NumericalData/IMAGE/RPI/DS/PT5M",
"spase://SMWG/Instrument/IMAGE/RPI",
[
"Waves.Passive",
"Spectrum",
"ElectricField"
],
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Heliosphere.Inner"
],
"",
"Calibrated data in physical units. Spacecraft MET to UT is converted using history of IMAGE observatory clock drift. Added data items: Combined XY channel VSD value is obtained as the length of a vector formed by X and Y channel VSD components; spacecraft spin modulation is not seen in XY channel data. Data reduction from full resolution telemetry dataset to this Level-1 dataset: (1) Selection of one sample out of 8 available in TTD databin, (2) removal of cross-phase and cross-power terms available in TTD databin.",
"(A) Known artifacts of dynamic spectrograms are (1) a horizontal line at 20 kHz where the frequency stepping changes from linear to logarithmic, and (2) a variety of interference sources internal to the IMAGE observatory appear as horizontal lines on the dynamic spectrograms including, most prominently, 101 kHz; additional lines appear at 63 kHz and its 126 kHz 2nd harmonic (battery charger), at times a broad band is also present between 160 and 200 kHz due to the torque rod operation, and a narrow line appears at 75 kHz due to the S-band transponder. Other known intereferer lines are 150 kHz, 200 kHz, and 240 kHz (deck plate heaters and other onboard instruments), but these lines are usually not present in the measurement. (B) When the spectrogram is plotted, the pixel size is made wide enough to fill the gaps caused by the 5 minute cadence of the measurements. (C) Comparison of voltage spectral density with other space receiver data has to consider differences in the antenna configurations.",
[
"Dynamic Spectrogram",
"Spectrogram",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
"Continuum radiation",
"Myriametric radiation",
"Plasmaspheric Hiss",
"Solar radio burst",
"Terrestrial Kilometric Radiation",
"TKR",
"Type II Solar radio burst",
"Type III Solar radio burst",
"UHR",
"Upper hybrid resonance",
"VLF Station",
"VLF Transmitter",
"Whistler"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/tqpm-9804",
"IMAGE RPI Dynamic Spectrogram data in CDF at NASA CDAWeb",
"IM_K1_RPI",
"Users please acknowledge Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center and RPI Principal Investigator Prof. B. W. Reinisch of the University of Massachusetts Lowell for making these CDF files available.",
"PT5M",
"2000-04-21T20:24:42Z",
"2005-12-18T07:50:00Z",
"In Cadence below, the 5 minutes refers to the nominal interval between measurements. Actual cadence of passive measurement varied between 3 to 6 minutes depending on the RPI science plan and design of measurement schedules.",
"2.6.0"
],
[
"IM_OR_DEF",
"spase://NASA/NumericalData/IMAGE/Orbit/Definitive/PT120S",
"spase://SMWG/Instrument/IMAGE/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"IMAGE Definitive Orbit Data",
"",
"",
"PT120S",
"2000-03-27T00:00:00",
"2004-06-21T00:00:00",
"Data are current to within about a week.",
"2.3.2"
],
[
"IM_OR_PRE",
"spase://NASA/NumericalData/IMAGE/Orbit/Predict/PT120S",
"",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/gnrm-pd86",
"IMAGE Predicted Orbital Data",
"",
"",
"PT120S",
"2001-03-27T00:00:00",
"2006-06-21T00:00:00",
"Data are current to within about a week.",
"2.6.0"
],
[
"ISEE-3_MAGPLASMA_2MIN_MAGNETIC_FIELD_PLASMA",
"spase://NASA/NumericalData/ISEE3/Merged/MAG_SWP/CDF/PT2M",
[
"spase://SMWG/Instrument/ISEE3/MAG",
"spase://SMWG/Instrument/ISEE3/SWP"
],
[
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/nexz-5z17",
"ISEE 3 Merged Vector Helium Magnetometer (MAG), and Solar WInd Plasma (SWP), 2 min CDF Data",
"",
"E.J. Smith, Helium Vector Magnetometer, J.T. Gosling, Solar Wind Plasma",
"PT2M",
"1978-08-13T00:00:00.000",
"1982-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"ISEE-3_MAG_1MIN_MAGNETIC_FIELD",
"spase://NASA/NumericalData/ISEE3/MAG/CDF/PT1M",
"spase://SMWG/Instrument/ISEE3/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/t0jh-af86",
"ISEE 3 Vector Helium Magnetometer (MAG), Magnetic Field, 1 min CDF Data",
"",
"E.J. Smith",
"PT1M",
"1978-08-01T00:00:00.000",
"1990-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"ISEE1_4SEC_MFI",
"spase://NASA/NumericalData/ISEE1/MAG/PT4S",
"spase://SMWG/Instrument/ISEE1/MAG",
"MagneticField",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/nms1-t205",
"ISEE 1 magnetometer 4-sec data",
"",
"UCLA-IGPP ISEE Magnetometer Team, and the source used for accessing data.",
"PT4S",
"1977-10-22T21:04:19",
"1987-09-25T16:10:30",
"",
"2.6.0"
],
[
"ISEE1_60SEC_MFI",
"spase://NASA/NumericalData/ISEE1/MAG/PT1M",
"spase://SMWG/Instrument/ISEE1/MAG",
"MagneticField",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/6023-ss94",
"ISEE 1 magnetometer 1-min data",
"",
"ISEE Magnetometer Team at UCLA/IGPP and the CDAWeb team at NASA/GSFC",
"PT1M",
"1977-10-22T21:04:19",
"1987-09-25T16:10:30",
"",
"2.6.0"
],
[
"ISEE1_H0_FE",
"spase://NASA/NumericalData/ISEE1/VES/PT18S",
"spase://SMWG/Instrument/ISEE1/VES",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere"
],
"",
"",
"",
"",
"2025-10-09T12:34:56.789",
"https://doi.org/10.48322/w4js-dk79",
"ISEE 1 VES Electron Data at 9s or 18s",
"",
"Please acknowledge the VES PI, Dr. Keith Ogilvie",
"PT18S",
"1977-10-29T00:00:00",
"1979-06-03T00:00:00",
"",
"2.6.0"
],
[
"ISEE1_H1_FPE",
"spase://NASA/NumericalData/ISEE1/FPE/PT1M",
"spase://SMWG/Instrument/ISEE1/FPE",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/qt96-em12",
"ISEE 1 FPE plasma parameters, 6 Re to bow shock",
"",
"Please acknowledge the FPE PI, Dr. John Gosling",
"PT1M",
"1977-10-29T00:00:00",
"1979-01-19T00:00:00",
"",
"2.6.0"
],
[
"ISEE1_H2_FPE",
"spase://NASA/NumericalData/ISEE1/FPE/PT24S",
"spase://SMWG/Instrument/ISEE1/FPE",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/wvvd-c308",
"ISEE 1 Solar Wind Analyzer 24-s Plasma Parameters",
"",
"Please acknowledge the FPE PI, Dr. John Gosling",
"PT24S",
"1977-10-30T00:00:00",
"1984-01-30T00:00:00",
"",
"2.6.0"
],
[
"ISEE1_PWI_SA",
"spase://NASA/NumericalData/ISEE1/PWE/SA/PT1S",
"spase://SMWG/Instrument/ISEE1/PWE",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"Quality Note: This experiment showed no anomalies in its operation throughout the lifetime of the spacecraft. Interference from four sources were occasionally observed and flags to identify the possible presence of these sources are included in the 'E_Quality' and 'B_Quality' variables. The data from the search coil magnetometers have possible interference when the internal Z-measurement calibration operates and when the Energetic Electrons Instrument's scan platform (D. J. Williams) passes through certain positions. The data from the electric field sensors have possible interference when the Plasma Density Instrument (C. C. Harvey) applies signals to the antennas and when the Quasi-static Electric Fields Instrument (F. S. Mozer) performs bias sweeps. The Energetic Electrons Instrument's scan platform generates noise which shows up as bursts in the search coil data in the frequency range from 56.2 Hz to 562 Hz when the scan platform passes through the spin plane. When the scan platform is operating, the interference occurs approximately every six spins. When the SCAN flag is set in the 'B_Quality' variable, one needs to examine the data to determine whether or not the glitches exceed the naturally occurring signals in this frequency range. The Z-MEAS flag indicates when internally generated signals are applied to the search coil antennas. When the Z-MEAS flag is set in the 'B_Quality' variable, one needs to examine the data to determine whether or not the glitches exceed the naturally occurring signals in the search coil data. The MOZER flag identifies possible interference when the Quasi-static Electric Field's Instrument performs a bias sweep. In normal operations a bias sweep was performed in a two second period every 128 seconds. This resulted in spikes appearing in the electric field data. When the MOZER flag is set in the 'E_Quality' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. The HARVEY flag identifies possible interference when the Plasma Density Instrument injects signals on either of the long electric dipole antennas. When the HARVEY flag is set in the 'E_Quality' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. When the Plasma Density Instrument interference occurs, it frequently cycles on and off at periods of 128, 256, or 512 seconds. Interference noise generated by the solar array is frequently evident in the electric field data at low frequencies up to about 100 Hz. This particular source is NOT identified in the 'E_Quality' variable, thus data from lowest 6 frequency bins of the 'Ev_Spectra' and 'Eu_Spectra' variables are always suspect. Nominally the 20-channel spectrum analyzer was connected to one of the electric antennas and the 14-channel spectrum analyzer was connected to one of the magnetic search coils, but about 2.2 percent of the SA data were collected with the analyzers swapped. This arrangement was required because the SFR and the 20-channel analyzer were fed off the same antenna selection switch. So in order to send magnetic field signals to the Sweep Frequency Receiver (SFR) for high frequency resolution measurements, the 20-channel analyzer had to be connected to a magnetic antenna. In this state, the upper 6 channels of magnetic field data are collected above the search search coil's cutoff frequency. Archive users should be aware that low magnetic spectral density values above 10 kHz are not physically meaningful. For any type of survey study, it would be best to reject the respective data when an interference flag is set, and to reject all magnetic spectral densities above 10 kHz. For high-time resolution event studies, it would be appropriate to examine the data in detail to see whether or not the naturally occurring or the interference signals dominate.",
"",
"2025-05-15T15:38:11",
"https://doi.org/10.48322/zw5z-3r03",
"ISEE 1 Plasma wave experiment (PWE) Spectrum Analyzer",
"ISEE-A Gurnett PWI SA",
"Users of the ISEE-1 PWI SA data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication. ISEE-1 PWI SA data are open to everyone. However, users of these data are encouraged to contact the PI institute and the U of I ISEE website should questions arise.",
"PT1S",
"1977-10-22T19:13:20",
"1987-09-26T06:07:59",
"\n ",
"2.6.0"
],
[
"ISEE1_PWI_SA-RAPID-E",
"spase://NASA/NumericalData/ISEE1/PWE/SA/PT0.125S",
"spase://SMWG/Instrument/ISEE1/PWE",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"Quality note This experiment showed no anomalies in its operation throughout the lifetime of the spacecraft. Interference from four sources were occasionally observed and flags to identify the possible presence of these sources are included in the 'Quality_Flag' variable. The data from the electric field sensors have possible interference when the Plasma Density Instrument (C. C. Harvey) applies signals to the antennas and when the Quasi-static Electric Fields Instrument (F. S. Mozer) performs bias sweeps. Data in this file were obtained from the Ev long wire antenna and the Eu two-sphere antenna via the SFR receiver. Approximately 98.2% of all ESA measurements were made using the long-wire antenna, thus not much Eu data are present in this file series. ESA samples that came from the Eu antenna are marked with a value of 1 in the 'Eu_Sensor' variable. The Es antenna was utilized for less than 0.01% of all PWI measurements over the course of the ISEE mission. These data are typically of very low quality given the relative insensitivity of the short electric antenna and have been dropped from the dataset. The MOZER flag identifies possible interference when the Quasi-static Electric Field's Instrument performs a bias sweep. In normal operations a bias sweep was performed in a two second period every 128 seconds. This resulted in spikes appearing in the electric field data. When the MOZER flag is set in the 'Quality_Flag' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. The HARVEY flag identifies possible interference when the Plasma Density Instrument injects signals on either of the long electric dipole antennas. When the HARVEY flag is set in the 'Quality_Flag' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. When the Plasma Density Instrument interference occurs, it frequently cycles on and off at periods of 128, 256, or 512 seconds. Interference noise generated by the solar array is frequently evident in the electric field data at low frequencies up to about 100 Hz. This particular source is NOT identified in the 'Quality_Flag' variable, thus rapid sample data for frequencies less that or equal to 100 Hz are always suspect. For any type of survey study, it would be best to reject the respective data when an interference flag is set. For high-time resolution event studies, it would be appropriate to examine the data in detail to see whether or not the interference signals dominate the naturally occurring signals. .",
"",
"2025-05-15T15:38:11",
"https://doi.org/10.48322/9aeg-0y83",
"ISEE 1 Plasma wave experiment (PWE) Spectrum Analyzer - Rapid Sample",
"ISEE-A Gurnett PWI SA Rapid Sample",
"Users of the ISEE-1 PWI SA Rapid Sample data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication. ISEE-1 PWI SA Rapid Sample data are open to everyone. However, users of these data are encouraged to contact the PI institute and the U of I ISEE website should questions arise.",
"PT0.125S",
"1977-10-27T00:00:00",
"1987-09-26T06:07:59",
"\n ",
"2.6.0"
],
[
"ISEE1_PWI_SFR-E",
"spase://NASA/NumericalData/ISEE1/PWE/SFR/PT32S",
"spase://SMWG/Instrument/ISEE1/PWE",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"Quality Note: This experiment showed no anomalies in its operation throughout the lifetime of the spacecraft. Interference from four sources were occasionally observed and flags to identify the possible presence of these sources are included in the 'Quality_Flag' variable. The data from the electric field sensors have possible interference when the Plasma Density Instrument (C. C. Harvey) applies signals to the antennas and when the Quasi-static Electric Fields Instrument (F. S. Mozer) performs bias sweeps. Data in this file were obtained from the Ev long wire antenna and the Eu two-sphere antenna via the SFR receiver. Approximately 98.2% of all SFR measurements were made using the long-wire antenna, thus not much Eu data are present in this file series. SFR sweeps that contain at least one data point from the Eu antenna are marked with a value of 1 in the 'Eu_Sensor' variable. The Es antenna was utilized for less than 0.01% of all PWI measurements over the course of the ISEE mission. These data are typically of very low quality given the relative insensitivity of the short electric antenna and have been dropped from the dataset. The MOZER flag identifies possible interference when the Quasi-static Electric Field's Instrument performs a bias sweep. In normal operations a bias sweep was performed in a two second period every 128 seconds. This resulted in spikes appearing in the electric field data. When the MOZER flag is set in the 'Quality_Flag' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. The HARVEY flag identifies possible interference when the Plasma Density Instrument injects signals on either of the long electric dipole antennas. When the HARVEY flag is set in the 'Quality_Flag' variable, one needs to examine the data to determine whether or not the interference exceeds the naturally occurring signals in the electric field data. When the Plasma Density Instrument interference occurs, it frequently cycles on and off at periods of 128, 256, or 512 seconds. Interference noise generated by the solar array is frequently evident in the electric field data at low frequencies up to about 100 Hz. This particular source is NOT identified in the 'Quality_Flag' variable, thus data from lowest frequency bin of the 'E_Spectra' variable are always suspect. For any type of survey study, it would be best to reject the respective data when an interference flag is set. For high-time resolution event studies, it would be appropriate to examine the data in detail to see whether or not the naturally occurring or the interference signals dominate.",
"",
"2025-05-15T15:38:11",
"https://doi.org/10.48322/7e5f-4z64",
"ISEE 1 Plasma wave experiment (PWE) Sweep Frequency Receiver",
"ISEE-A Gurnett PWI SFR",
"Users of the ISEE-1 PWI SFR data are encouraged to acknowledge NASA CDAWeb and The University of Iowa as the source of the data in any publication. ISEE-1 PWI SFR data are open to everyone. However, users of these data are encouraged to contact the PI institute and the U of I ISEE website should questions arise.",
"PT32S",
"1977-10-22T21:40:38",
"1987-09-26T04:43:49",
"\n ",
"2.6.0"
],
[
"ISEE2_4SEC_MFI",
"spase://NASA/NumericalData/ISEE2/MAG/PT4S",
"spase://SMWG/Instrument/ISEE2/MAG",
"MagneticField",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-10-09T12:34:56.789",
"https://doi.org/10.21978/p8pg8v",
"ISEE 2 magnetometer 4-sec data",
"",
"UCLA-IGPP ISEE Magnetometer Team, and the source used for accessing data (see below).",
"PT4S",
"1977-10-22T14:49:19",
"1987-09-26T05:59:00",
"",
"2.3.2"
],
[
"ISEE2_60SEC_MFI",
"spase://NASA/NumericalData/ISEE2/MAG/PT1M",
"spase://SMWG/Instrument/ISEE2/MAG",
"MagneticField",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.21978/p8t923",
"ISEE 2 magnetometer 1-min data",
"",
"ISEE Magnetometer Team at UCLA/IGPP and the CDAWeb team at NASA/GSFC",
"PT1M",
"1977-10-22T21:04:19",
"1987-09-26T16:10:30",
"",
"2.3.2"
],
[
"ISEE2_H1_FPE",
"spase://NASA/NumericalData/ISEE2/FPE/PT1M",
"spase://SMWG/Instrument/ISEE2/FPE",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/ytnf-nz91",
"ISEE 2 FPE plasma parameters, 6 Re to bow shock",
"",
"Please acknowledge the FPE PI, Dr. John Gosling",
"PT1M",
"1977-10-27T00:00:00",
"1979-01-19T00:00:00",
"",
"2.6.0"
],
[
"ISS_27DAY-AVERAGES_AMS-02",
"spase://NASA/NumericalData/ISS/AMS-02/P27D",
"spase://SMWG/Instrument/ISS/AMS-02",
"EnergeticParticles",
[
"Earth.NearSurface.Ionosphere.FRegion",
"Earth.NearSurface.Thermosphere"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"ISS Alpha Magnetic Spectrometer-02 (AMS-02) Particle Fluxes and Flux Ratios, Bartel Rotation Averages, Modified Data 0 (M0), 27 Day Data",
"",
"V. Bindi, Please acknowledge the Principal Investigators and CDAWeb when using these Data.",
"P27D",
"2011-05-20T00:00:00.000",
"2017-04-18T23:59:59.999",
"",
"2.3.2"
],
[
"ISS_DOSANL_TEPC",
"spase://NASA/NumericalData/ISS/TEPC/PT10S",
"spase://SMWG/Instrument/ISS/TEPC",
"EnergeticParticles",
[
"Earth.NearSurface.Ionosphere.FRegion",
"Earth.NearSurface.Thermosphere"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"ISS Tissue-Equivalent Proportional Counter (TEPC), Dose Analyzer, 10 s Data",
"",
"E.N. Zapp, Space Radiation Analysis Group, NASA Johnson Space Center",
"PT10S",
"2000-11-09T15:11:03",
"2010-04-29T00:49:30",
"",
"2.3.2"
],
[
"ISS_SP_FPMU",
"spase://NASA/NumericalData/ISS/FPMU/PT1S",
"spase://SMWG/Instrument/ISS/FPMU",
"ThermalPlasma",
[
"Earth.NearSurface.Ionosphere.FRegion",
"Earth.NearSurface.Thermosphere"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"ISS Floating Potential Measurement Unit (FPMU), Summary Parameter 1 s Data",
"",
"R.M. Suggs, S.L. Koontz, NASA Johnson Space Center Contact Rob Suggs for support and use. Rob.Suggs@nasa.gov.",
"PT1S",
"2010-01-27T00:00:00.000",
"2016-10-02T23:59:59.999",
"",
"2.3.2"
],
[
"IT_H0_MFI",
"spase://NASA/NumericalData/Interball-1/MIFM/PT6S",
[
"spase://SMWG/Instrument/Interball-1/MIFM",
"spase://SMWG/Instrument/Interball-1/FM3I",
"spase://SMWG/Instrument/Interball-1/FGMI"
],
"MagneticField",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail 6-sec magnetic field data",
"",
"The Interball project, IZMIRAN and Space Research Institute RAS (SRI).",
"PT6S",
"1995-08-06T00:00:00",
"2000-10-15T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_AKR",
"spase://NASA/NumericalData/Interball-1/AKR2/KP/PT120S",
"spase://SMWG/Instrument/Interball-1/AKR2",
"Waves",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail Radio Emission 2-min Key Parameters",
"",
"",
"PT120S",
"1995-08-06T07:11:00",
"2000-10-16T01:17:00",
"",
"2.3.2"
],
[
"IT_K0_COR",
"spase://NASA/NumericalData/Interball-1/CORALL/PT120S",
"spase://SMWG/Instrument/Interball-1/CORALL",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALCULATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail CORALL Plasma 2-Min Key Parameters",
"",
"",
"PT120S",
"1995-09-02T00:00:00",
"1998-12-31T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_ELE",
"spase://CNES/NumericalData/Interball-1/ELECTRON/PT120S",
"spase://SMWG/Instrument/Interball-1/ELECTRON",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALCULATED",
"",
"",
"2021-06-01T00:00:00Z",
"",
"Interball Tail Plasma Electron 2-min Key Parameters",
"",
"",
"PT120S",
"1995-08-15T00:00:00",
"2000-10-16T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_EPI",
"spase://NASA/NumericalData/Interball-1/DOK2-SKA-2/PT2M",
[
"spase://SMWG/Instrument/Interball-1/DOK2",
"spase://SMWG/Instrument/Interball-1/SKA2"
],
"EnergeticParticles",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail energetic particle 2-min Key Parameters",
"",
"",
"PT2M",
"1995-08-04T00:00:00",
"2000-10-16T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_ICD",
"spase://NASA/NumericalData/Interball-1/PROMICS3/PT120S",
"spase://SMWG/Instrument/Interball-1/PROMICS3",
[
"EnergeticParticles",
"IonComposition"
],
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail PROMICS H+ and O+ 2-min Key Parameters",
"",
"",
"PT120S",
"1995-08-22T00:00:00",
"1996-06-07T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_MFI",
"spase://NASA/NumericalData/Interball-1/MIFM/PT120S",
[
"spase://SMWG/Instrument/Interball-1/MIFM",
"spase://SMWG/Instrument/Interball-1/FM3I",
"spase://SMWG/Instrument/Interball-1/FGMI"
],
"MagneticField",
[
"Earth.Magnetosphere",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail Magnetic Field 2-min Key Parameters",
"",
"",
"PT120S",
"1995-08-06T00:00:00",
"2000-10-16T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_VDP",
"spase://NASA/NumericalData/Interball-1/VDP/PT2M",
"spase://SMWG/Instrument/Interball-1/VDP",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail VDP ion flux 2-min Key Parameters",
"",
"",
"PT2M",
"1995-08-14T00:00:00",
"2000-10-16T00:00:00",
"",
"2.3.2"
],
[
"IT_K0_WAV",
"spase://NASA/NumericalData/Interball-1/MIFM/PT2M",
"spase://SMWG/Instrument/Interball-1/MIFM",
"Waves.Passive",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail wave data 2-min Key Parameters",
"",
"",
"PT2M",
"1998-01-01T00:00:00",
"2000-10-16T00:00:00",
"",
"2.3.2"
],
[
"IT_OR_DEF",
"spase://NASA/NumericalData/Interball-1/Ephemeris/PT2M",
[
"spase://SMWG/Instrument/Interball-1/Ephemeris",
"spase://SMWG/Instrument/Magion-4/Ephemeris"
],
"Ephemeris",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Polar"
],
"",
"",
"The data cadence varies.",
"",
"2021-04-27T15:38:11Z",
"",
"Interball Tail definitive orbital data",
"",
"The Interball project, Russian Space Research Institute (IKI) and Dr. Prokhorenko",
"PT2M",
"1995-08-07T00:00:00Z",
"2000-10-16T13:55:00.00Z",
"",
"2.3.2"
],
[
"L0_K0_MPA",
"spase://NASA/NumericalData/LANL/1990/MPA/PT86S",
"spase://SMWG/Instrument/LANL/1990/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"87 sec",
"geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/b3yv-mf47",
"LANL1990 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 095 MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"1992-12-16T00:00:00",
"2005-11-09T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L0_K0_SPA",
"spase://NASA/NumericalData/LANL/1990/SOPA/PT60S",
"spase://SMWG/Instrument/LANL/1990/SOPA",
"EnergeticParticles",
[
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"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31",
[
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"geosynchronous",
"LANL",
"Synchronous Orbit Particle Analyzer",
"SOPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/zzr5-dd89",
"LANL 1990 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates",
"LANL 095 SOPA data",
"Los Alamos National Laboratory; Dr. Reiner Friedel",
"PT60S",
"1992-12-16T00:00:00",
"2005-11-09T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L1_K0_MPA",
"spase://NASA/NumericalData/LANL/1991/MPA/PT86S",
"spase://SMWG/Instrument/LANL/1991/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
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"geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/5jaw-x105",
"LANL1991 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 080 MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"1993-10-27T00:00:00",
"2004-11-23T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L1_K0_SPA",
"spase://NASA/NumericalData/LANL/1991/SOPA/PT60S",
"spase://SMWG/Instrument/LANL/1991/SOPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"60 sec",
"Geosynchronous",
"LANL",
"Geosynchronous Orbit Particle Analyzer",
"SOPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/1jyx-5h51",
"LANL 1991 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates",
"LANL 095 SOPA data",
"Los Alamos National Laboratory; Dr. Reiner Friedel",
"PT60S",
"1992-08-01T00:00:00",
"2004-11-23T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L4_K0_MPA",
"spase://NASA/NumericalData/LANL/1994/MPA/PT86S",
"spase://SMWG/Instrument/LANL/1994/MPA",
"EnergeticParticles",
[
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"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
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"geosynchronosus",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/8y0b-0s77",
"LANL1994Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 084 MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"1996-01-01T00:00:00",
"2008-01-03T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L4_K0_SPA",
"spase://NASA/NumericalData/LANL/1994/SOPA/PT60S",
"spase://SMWG/Instrument/LANL/1994/SOPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"60 sec",
"geosynchronous",
"LANL",
"Synchronous Orbit Particle Analyzer",
"SOPA"
],
"2025-05-22T15:38:11",
"https://doi.org/10.48322/abg8-2403",
"LANL 1994 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates",
"LANL 095 SOPA data",
"Los Alamos National Laboratory; Dr. Reiner Friedel",
"PT60S",
"1996-02-16T00:00:00",
"2007-10-15T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L7_H0_MPA",
"spase://NASA/NumericalData/LANL/1997/MPA/PT1S",
"spase://SMWG/Instrument/LANL/1997/MPA",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"CALCULATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/2hyb-ms72",
"LANL1997 MPA High Resolution Data",
"",
"",
"PT1S",
"1998-04-29T00:00:00",
"1998-05-09T23:59:59",
"",
"2.6.0"
],
[
"L7_K0_MPA",
"spase://NASA/NumericalData/LANL/1997/MPA/PT86S",
"spase://SMWG/Instrument/LANL/1997/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31",
[
"87 sec",
"Geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/pb5s-re17",
"LANL1997 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 97A MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"1997-07-04T00:00:00",
"2008-01-03T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L7_K0_SPA",
"spase://NASA/NumericalData/LANL/1997/SOPA/PT60S",
"spase://SMWG/Instrument/LANL/1997/SOPA",
"EnergeticParticles",
[
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"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31",
[
"60 sec",
"geosynchronous",
"LANL",
"Geosynchronous Orbit Particle Analyzer",
"SOPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/51vv-e118",
"LANL 1997 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates",
"LANL 97A SOPA data",
"Los Alamos National Laboratory; Dr. Reiner Friedel",
"PT60S",
"1999-01-01T00:00:00",
"2007-10-15T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L9_H0_MPA",
"spase://NASA/NumericalData/LANL/1989/MPA/PT1S",
"spase://SMWG/Instrument/LANL/1989/MPA",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"CALCULATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/7d0a-cf96",
"LANL1989 MPA High Resolution",
"",
"",
"PT1S",
"1998-05-03T00:00:00",
"1998-05-03T23:59:59",
"",
"2.6.0"
],
[
"L9_K0_MPA",
"spase://NASA/NumericalData/LANL/1989/MPA/PT86S",
"spase://SMWG/Instrument/LANL/1989/MPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"87 sec",
"Geosynchronous",
"LANL",
"Magnetospheric Plasma Analyzer",
"MPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/jv8m-ra10",
"LANL 1989 Magnetospheric Plasma Analyzer (MPA) at 87 sec Resolution in Spacecraft Coordinates",
"LANL 046 MPA data",
"Los Alamos National Laboratory; Dr. Michelle Thomsen; Dr. Michael G. Henderson",
"PT87S",
"1998-05-03T00:00:00",
"2008-01-03T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"L9_K0_SPA",
"spase://NASA/NumericalData/LANL/1989/SOPA/PT60S",
"spase://SMWG/Instrument/LANL/1989/SOPA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere"
],
"",
"Numerical Data",
"Flags=-1.0e+31. The content of the LANL SOPA cdfs at CDAWeb has not been fully documented.",
[
"60 sec",
"Geosynchronous",
"LANL",
"Geosynchronous Orbit Particle Analyzer",
"SOPA"
],
"2023-12-24T12:34:56.789",
"https://doi.org/10.48322/7xdy-y825",
"LANL 1989 Geosynchronous Orbit Particle Analyzer (SOPA) at 60 sec Resolution in Spacecraft Coordinates",
"LANL 046 SOPA data",
"Los Alamos National Laboratory; Dr. Reiner Friedel",
"PT60S",
"1999-01-01T00:00:00",
"2007-10-15T23:59:59",
"Time format in data files is: day, month, year hour, min, seconds. Ex: '01-Jan-1981 00:00:00.000'",
"2.6.0"
],
[
"MESSENGER_MAG_RTN",
"spase://NASA/NumericalData/MESSENGER/MAG/PT0.05S",
[
"spase://SMWG/Instrument/MESSENGER/Ephemeris",
"spase://SMWG/Instrument/MESSENGER/Magnetometer"
],
[
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
[
"Mercury.Magnetosphere",
"Mercury.Magnetosphere.Magnetotail",
"Mercury.Magnetosphere.Main",
"Mercury.Magnetosphere.Polar"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/9wyq-j955",
"MESSENGER Magnetometer (MAG) Interplanetary Magnetic Field, Radial-Tangential-Normal, RTN, Coordinates, High Resolution, 1 s Data",
"",
"Please acknowledge the Principal Investigator S.C. Solomon and the instrument scientist, Brian Anderson for use of the Data",
"PT0.05S",
"2004-08-12T17:44:08.000",
"2011-05-18T00:00:09.000",
"",
"2.6.0"
],
[
"METOP1_POES-SEM2_FLUXES-2SEC",
"spase://NOAA/NumericalData/MetOp/B/SEM-2/CDF/PT2S",
"spase://SMWG/Instrument/MetOp/B/SEM-2",
"EnergeticParticles",
[
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"",
"",
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"",
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"Please acknowledge O. Le Contel, R.E. Ergun, R.B. Torbert, L. Mirioni, and J.L. Burch for use of these data",
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"Please acknowledge R.E. Ergun, P.-A. Lindqvist, R.B. Torbert, N. Ahmadi, D.B. Graham, and J.L. Burch for use of these data",
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[
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"Please acknowledge O. Le Contel, R.E. Ergun, R.B. Torbert, L. Mirioni, and J.L. Burch for use of these data",
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"Please acknowledge R.E. Ergun, P.-A. Lindqvist, R.B. Torbert, N. Ahmadi, D.B. Graham, and J.L. Burch for use of these data",
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"Please acknowledge R.B. Torbert, M.R. Argall, and J.L. Burch for use of these data",
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"Please acknowledge R.B. Torbert, M.R. Argall, and J.L. Burch for use of these data",
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"Please acknowledge R.B. Torbert, M.R. Argall, and J.L. Burch for use of these data",
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"PT5S",
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[
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"PT0.125S",
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"MMS 1 Electric Double Probe (EDP) Three-Dimensional Electric Field, Level 2 (L2), Burst Mode, 0.1220703125 ms Data",
"MMS1_EDP_BRST_L2_DCE",
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[
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[
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"Please acknowledge M.G. Henderson, S.K. Morley, and J.L. Burch for use of these data",
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[
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[
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"PT0.0000610151563S",
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[
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"Please acknowledge O. Le Contel, R.B. Torbert, L. Mirioni, M.R. Argall, and J.L. Burch for use of these data",
"PT0.03125S",
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[
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[
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"PT2S",
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[
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[
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"Please acknowledge R.E. Ergun, P.-A. Lindqvist, R.B. Torbert, N. Ahmadi, D.B. Graham, and J.L. Burch for use of these data",
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[
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"MMS4_DSP_SLOW_L2_BPSD",
"Please acknowledge O. Le Contel, R.E. Ergun, R.B. Torbert, L. Mirioni, and J.L. Burch for use of these data",
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"Please acknowledge R.E. Ergun, P.-A. Lindqvist, R.B. Torbert, N. Ahmadi, D.B. Graham, and J.L. Burch for use of these data",
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"Please acknowledge R.B. Torbert, M.R. Argall, and J.L. Burch for use of these data",
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"PT0.125S",
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[
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"2024-02-26T00:00:00",
"https://doi.org/10.17189/1414241",
"MAVEN SWIA Calibrated Fine Survey 3D Data Collection",
"MVN_SWI_L2_FINESVY3D",
"Please acknowledge the Principal Investigator J.S. Halekas for use of these data.",
"PT8S",
"2014-03-19T14:19:47",
"",
"",
"2.6.0"
],
[
"MVN_SWI_L2_ONBOARDSVYMOM",
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"spase://SMWG/Instrument/MAVEN/SWIA",
"ThermalPlasma",
"Mars",
"",
"",
"",
"",
"2024-02-26T00:00:00",
"https://doi.org/10.17189/1414246",
"MAVEN SWIA Calibrated Onboard Survey Moment Data Collection",
"MVN_SWI_L2_ONBOARDSVYMOM",
"Please acknowledge the Principal Investigator J.S. Halekas for use of these data.",
"PT4S",
"2014-03-19T14:19:43",
"",
"",
"2.6.0"
],
[
"MVN_SWI_L2_ONBOARDSVYSPEC",
"spase://NASA/NumericalData/MAVEN/SWIA/Level2/EnergySpectra/Survey/PT4S",
"spase://SMWG/Instrument/MAVEN/SWIA",
[
"EnergeticParticles",
"ThermalPlasma"
],
"Mars",
"",
"",
"",
"",
"2024-02-26T00:00:00",
"https://doi.org/10.17189/1414248",
"MAVEN SWIA Calibrated Onboard Survey Spectra Data Collection",
"MVN_SWI_L2_ONBOARDSVYSPEC",
"Please acknowledge the Principal Investigator J.S. Halekas for use of these data.",
"PT4S",
"2014-03-19T14:20:43",
"",
"",
"2.6.0"
],
[
"NEW_HORIZONS_SWAP_PICKUP-IONS",
"spase://NASA/NumericalData/NewHorizons/SWAP/PickupIon/ValidatedSummary/P1D",
"spase://SMWG/Instrument/NewHorizons/SWAP",
[
"EnergeticParticles",
"ThermalPlasma"
],
[
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"Heliosphere.NearEarth",
"Heliosphere.Outer"
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/d4g8-sm25",
"New Horizons Solar Wind Around Pluto (SWAP) Pick-Up Ions, Validated Summary Data (VS), Daily Data",
"",
"D.J. McComas",
"P1D",
"2008-11-16T00:00:00.000",
"",
"",
"2.6.0"
],
[
"NEW_HORIZONS_SWAP_PICKUP-IONS-HISTOGRAM",
"spase://NASA/NumericalData/NewHorizons/SWAP/PickupIonHistogram/ValidatedSummary/P1D",
"spase://SMWG/Instrument/NewHorizons/SWAP",
[
"EnergeticParticles",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"The Histogram Data Set was generated before the Culling described in McComas et al. (2017), for Times when the Solar Wind Speed varied over about a 24 hour Period by >1% (about 13% of the Samples) or when the Pickup Ion (PUI) Fitting Routine experienced a failing (see McComas et al., 2017 for more Details).",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/z274-yv24",
"New Horizons Solar Wind Around Pluto (SWAP) Pick-Up Ion Histograms, Validated Summary Data (VS), Daily Data",
"",
"D.J. McComas",
"P1D",
"2008-10-31T00:00:00.000",
"",
"",
"2.6.0"
],
[
"NOAA05_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/5/SPM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/5/SPM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 05 Solar Proton Monitor (SPM) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1978-11-02T14:43:00.000",
"1979-08-11T00:00:00.000",
"",
"2.3.0"
],
[
"NOAA06_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/6/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/6/SEM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 06 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1979-06-28T01:40:00.000",
"1986-11-18T02:51:00.000",
"",
"2.3.0"
],
[
"NOAA07_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/7/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/7/SEM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 07 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1981-07-11T00:00:00.000",
"1985-02-11T00:00:00.000",
"",
"2.3.0"
],
[
"NOAA08_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/8/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/8/SEM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 08 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1983-05-09T17:36:00.000",
"1985-10-14T12:18:00.000",
"",
"2.3.2"
],
[
"NOAA10_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/10/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/10/SEM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 10 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1986-10-11T00:00:00.000",
"1991-08-31T23:59:00.000",
"",
"2.3.0"
],
[
"NOAA12_MEPED1MIN_SEM",
"spase://NOAA/NumericalData/POES/12/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/12/SEM",
[
"EnergeticParticles",
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 12 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1991-06-01T00:00:00.000",
"1999-09-30T23:59:00.000",
"",
"2.3.0"
],
[
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"spase://NOAA/NumericalData/POES/14/SEM/MEPED/KeyParameter/PT1M",
"spase://SMWG/Instrument/NOAA/14/SEM",
[
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"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
"",
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 14 Space Environment Monitor-1 (SEM-1) Medium Energy Proton and Electron Detector (MEPED) Re-processed Particle Count Rates, Fluxes, and Model Fields, 1 min Data",
"",
"S.F. Fung, Please acknowledge NOAA/NGDC for providing the raw Data.",
"PT1M",
"1995-01-11T00:00:00.000",
"2004-12-31T23:59:00.000",
"",
"2.3.0"
],
[
"NOAA15_POES-SEM2_FLUXES-2SEC",
"spase://NOAA/NumericalData/POES/15/SEM-2/CDF/PT2S",
"spase://SMWG/Instrument/NOAA/15/SEM-2",
"EnergeticParticles",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 15 POES Space Environment Monitor-2 (SEM-2) 2-second Particle Precipitation Data",
"",
"NGDC, SWPC",
"PT2S",
"2013-01-01T00:00:00.000",
"",
"",
"2.3.2"
],
[
"NOAA16_POES-SEM2_FLUXES-2SEC",
"spase://NOAA/NumericalData/POES/16/SEM-2/CDF/PT2S",
"spase://SMWG/Instrument/NOAA/16/SEM-2",
"EnergeticParticles",
[
"Earth.Magnetosheath",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 16 POES Space Environment Monitor-2 (SEM-2) 2-second Particle Precipitation Data",
"",
"NGDC, SWPC",
"PT2S",
"2013-01-01T00:00:00.000",
"2014-06-06T23:59:59.999",
"",
"2.3.2"
],
[
"NOAA18_POES-SEM2_FLUXES-2SEC",
"spase://NOAA/NumericalData/POES/18/SEM-2/CDF/PT2S",
"spase://SMWG/Instrument/NOAA/18/SEM-2",
"EnergeticParticles",
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"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
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"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 18 POES Space Environment Monitor-2 (SEM-2) 2-second Particle Precipitation Data",
"",
"NGDC, SWPC",
"PT2S",
"2013-01-01T00:00:00.000",
"",
"",
"2.3.2"
],
[
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"spase://SMWG/Instrument/NOAA/19/SEM-2",
"EnergeticParticles",
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"Earth.Magnetosphere.Polar",
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"",
"",
"",
"",
"2021-04-27T17:52:57Z",
"",
"NOAA 19 POES Space Environment Monitor-2 (SEM-2) 2-second Particle Precipitation Data",
"",
"NGDC, SWPC",
"PT2S",
"2013-01-01T00:00:00.000",
"",
"",
"2.3.2"
],
[
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"spase://NASA/NumericalData/OMNI/PT1H",
"spase://SMWG/Instrument/OMNI",
[
"ThermalPlasma",
"MagneticField",
"EnergeticParticles",
"ActivityIndex"
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"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/1shr-ht18",
"OMNI Hourly Data Set",
"",
"We acknowledge the experiment teams that acquired, processed and provided the OMNI-included data, and J.H. King and N.E. Papitashvili of NASA/GSFC for creating the OMNI data set.",
"PT1H",
"1963-01-01T00:00:00",
"",
"Various parameters are held current to differing levels. Typical delay is about 1-2 months.",
"2.3.2"
],
[
"OMNI_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/OMNI/COHO/MergedMagPlasma/PT1H",
"spase://SMWG/Instrument/OMNI",
[
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/6ffx-3441",
"OMNI Combined Heliopheric Observations (COHO), Merged Magnetic Field, Plasma and Ephermeris, Definitive Hourly Data",
"",
"J.H. King, N.E. Papitashvili",
"PT1H",
"1963-01-01T00:00:00",
"2017-05-01T23:59:59.999",
"",
"2.6.1"
],
[
"OMNI_HRO2_1MIN",
"spase://NASA/NumericalData/OMNI/HighResolutionObservations/Version2/PT1M",
[
"spase://SMWG/Instrument/ACE/Ephemeris",
"spase://SMWG/Instrument/ACE/MAG",
"spase://SMWG/Instrument/ACE/SWEPAM",
"spase://SMWG/Instrument/Geotail/CPI",
"spase://SMWG/Instrument/Geotail/Ephemeris",
"spase://SMWG/Instrument/Geotail/MGF",
"spase://SMWG/Instrument/IMP8/Ephemeris",
"spase://SMWG/Instrument/IMP8/MAG",
"spase://SMWG/Instrument/IMP8/PLS",
"spase://SMWG/Instrument/Wind/Ephemeris",
"spase://SMWG/Instrument/Wind/MFI",
"spase://SMWG/Instrument/Wind/SWE"
],
[
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"ElectricField",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
[
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"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/mj0k-fq60",
"OMNI, Combined Solar Wind Plasma Moments and Interplanetary Magnetic Field (IMF) Time-Shifted to the Nose of the Earth's Bow Shock, plus Geomagnetic Indices, 1 min Data",
"",
"Please acknowledge the Principal Investigator J.H. King and N.E. Papitashvili for use of the Data",
"PT1M",
"1995-01-01T00:00:00.000",
"2020-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"OMNI_HRO2_5MIN",
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[
"spase://SMWG/Instrument/ACE/Ephemeris",
"spase://SMWG/Instrument/ACE/MAG",
"spase://SMWG/Instrument/ACE/SWEPAM",
"spase://SMWG/Instrument/Geotail/CPI",
"spase://SMWG/Instrument/Geotail/Ephemeris",
"spase://SMWG/Instrument/Geotail/MGF",
"spase://SMWG/Instrument/IMP8/Ephemeris",
"spase://SMWG/Instrument/IMP8/MAG",
"spase://SMWG/Instrument/IMP8/PLS",
"spase://SMWG/Instrument/Wind/Ephemeris",
"spase://SMWG/Instrument/Wind/MFI",
"spase://SMWG/Instrument/Wind/SWE"
],
[
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"ElectricField",
"EnergeticParticles",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/hkaw-ff03",
"OMNI, Combined Solar Wind Plasma Moments and Interplanetary Magnetic Field (IMF) Time-Shifted to the Nose of the Earth's Bow Shock, plus Geomagnetic Indices, 5 min Data",
"",
"Please acknowledge the Principal Investigator J.H. King and N.E. Papitashvili for use of the Data",
"PT5M",
"1995-01-01T00:00:00.000",
"2020-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"OMNI_HRO_1MIN",
"spase://NASA/NumericalData/OMNI/HighResolutionObservations/Version1/PT1M",
"spase://SMWG/Instrument/OMNI",
[
"ThermalPlasma",
"MagneticField",
"ActivityIndex"
],
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2022-03-09T12:34:56.789",
"https://doi.org/10.48322/45bb-8792",
"OMNI 1-min Data Set",
"",
"We acknowledge the experiment teams that acquired, processed and provided the OMNI-included data, and J.H. King and N.E. Papitashvili of NASA/GSFC for creating the OMNI data set.",
"PT1M",
"1995-01-01T00:00:00",
"",
"Various parameters are held current to differing levels. Typical delay is about 1-2 months.",
"2.4.0"
],
[
"OMNI_HRO_5MIN",
"spase://NASA/NumericalData/OMNI/HighResolutionObservations/Version1/PT5M",
"spase://SMWG/Instrument/OMNI",
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/gbpg-5r77",
"OMNI 5-min Data Set",
"HRO-5",
"We acknowledgement J.H. King and N.E. Papitashvili of NASA/SPDF and QSS and the original providers of the input ACE, Wind and IMP 8 data",
"PT5M",
"1995-01-01T00:00:00",
"",
"",
"2.3.2"
],
[
"PIONEER10_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/Pioneer10/MAGandPLS/PT1H",
[
"spase://SMWG/Instrument/Pioneer10/MAG",
"spase://SMWG/Instrument/Pioneer10/PLS"
],
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Outer",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/dn2j-fn46",
"Pioneer 10 hourly merged magnetic field and plasma data",
"",
"Please acknowledge the magnetic field and plasma Principal Investigators, Drs. E. Smith and P. Gazis, and NSSDC or GSFC-SPDF",
"PT1H",
"1972-03-06T00:00:00",
"1995-09-07T00:00:00",
"Plasma data do not start until day 108 of 1972. Magnetic field data end on day 321 of 1975. Plasma data become especially sparse after ~day 90 of 1994.",
"2.6.0"
],
[
"PIONEER10_MAG_1MIN_MAGNETIC_FIELD",
"spase://NASA/NumericalData/Pioneer10/MAG/CDF/PT1M",
"spase://SMWG/Instrument/Pioneer10/MAG",
"MagneticField",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/3np4-sz16",
"Pioneer 10 Helium Vector Magnetometer (MAG), Magnetic Field in RTN Coordinates and One Way Light Time Delays, Cruise Phase",
"",
"E.J. Smith, Acknowledgement: Use of these Data in Publications should be accompanied by at minimum Acknowledgements of the NSSDC and the responsible Principal Investigator defined in the Experiment Documentation provided here. Citation of the NSSDC Coordinated Heliospheric Observations, COHO, Data Base would also be appreciated, so that other potential Users will be made aware of this Service.",
"PT1M",
"1972-03-03T00:00:00.000",
"1975-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"PIONEER11_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/Pioneer11/MAGandPLS/PT1H",
[
"spase://SMWG/Instrument/Pioneer11/MAG1",
"spase://SMWG/Instrument/Pioneer11/PLS"
],
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Outer",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vb0s-0w02",
"Pioneer 11 hourly merged magnetic field and plasma data",
"",
"Please acknowledge the magnetic field and plasma Principal Investigators, Drs. E. Smith and P. Gazis, and NSSDC or GSFC-SPDF",
"PT1H",
"1973-04-06T00:00:00",
"1992-08-01T00:00:00",
"Plasma data do not start until day 111 of 1973. Plasma data end on day 150 of 1992. Field and plasma data become increasingly sparse after the early 1980's.",
"2.6.0"
],
[
"PIONEERVENUS_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/PioneerVenusOrbiter/MAGandPLS/PT1H",
[
"spase://SMWG/Instrument/PioneerVenusOrbiter/OMAG",
"spase://SMWG/Instrument/PioneerVenusOrbiter/ORPA"
],
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Inner",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/f172-0b94",
"Pioneer Venus Orbiter (PVO) hourly merged magnetic field and plasma data",
"",
"Please acknowledge the magnetic field and plasma Principal Investigators, Drs. C.T. Russell and P. Gazis, and NSSDC or GSFC-SPDF",
"PT1H",
"1978-12-05T00:00:00",
"1992-10-09T00:00:00",
"Plasma data end on Oct. 9, 1992. Magnetic field data end on Aug. 7, 1988.",
"2.6.0"
],
[
"PIONEERVENUS_MERGED_SOLAR-WIND_10M",
"spase://NASA/NumericalData/PioneerVenusOrbiter/Merged/OMAG_OPA/CDF/PT10M",
[
"spase://SMWG/Instrument/PioneerVenusOrbiter/Ephemeris",
"spase://SMWG/Instrument/PioneerVenusOrbiter/OMAG",
"spase://SMWG/Instrument/PioneerVenusOrbiter/OPA"
],
[
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
"Venus",
"",
"",
"",
"",
"2025-08-05T13:12:22Z",
"https://doi.org/10.48322/ey7t-8763",
"Pioneer Venus Orbiter (PVO) Magnetometer, OMAG, Plasma Analyzer, OPA, Merged Solar Wind Data, 10 min Data",
"",
"Please acknowledge the Principal Investigator C.T. Russell and A. Barnes for use of the Data",
"PT10M",
"1978-12-06T00:00:00.000",
"1988-08-07T10:50:00.000",
"",
"2.7.0"
],
[
"POLAR_HYDRA_MOMENTS-14SEC",
"spase://NASA/NumericalData/POLAR/HYDRA/Moments/PT14S",
"spase://SMWG/Instrument/POLAR/HYDRA",
"EnergeticParticles",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
"",
"2025-08-05T13:12:20Z",
"https://doi.org/10.48322/gvf7-x480",
"Polar HYDRA 14-sec Moments",
"",
"Please acknowledge the P.I. and NASA Space Physics Data Facility (SPDF) CDAWeb when using these data.",
"PT14S",
"1996-03-20T14:38:27.000Z",
"2008-04-15T21:00:18Z",
"",
"2.7.0"
],
[
"PO_10MINATT_EFI",
"spase://NASA/NumericalData/POLAR/EFI/SC/GSE/Attitude/PT600S",
"spase://SMWG/Instrument/POLAR/EFI",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"Important Warning: The Data described below is meant for Archival Purposes. It should not be considered as highly accurate Data. For example, Accurate Data requires a Correction in the Form of an Offset to the Sunward Component of the Electric Field. A Constant Offset of 1.2 mV/m has been used for all the Data this being an approximate Average Value. In fact, however, the Offset varies with Time and must be determined by Analysis of the particular Time of Interest. Users of these Data desiring more Information should get in touch with Dr. F.S. Mozer, at the Space Sciences Laboratory, University of California, Berkeley. The Electric Field Data is at Spin Period Time Resolution. This means that there is one Data Point about every 6 s. However, it should be noted that there can be longer Intervals between Data Points due to Missing Data. Data Gaps are not filled in. The Components of the Electric Field are given in a Coordinate System designated as Despun Spacecraft Coordinates, DSC. This is a Coordinate System for a rotating Spacecraft that is in an Orbit near the Earth. DSC is defined by the Spacecraft's Spin Plane and Spin Axis. However, as the Despun Part of the Name suggests, the Coordinate Axes do not participate in the Spacecraft's Rotation. The X-Axis and Y-Axis are on the Spacecraft's Spin Plane; the Z-Axis is along the Spacecraft's Spin Axis. The positive X, Y, and Z-Axes form an Orthogonal, Right-Handed Coordinate System. The positive Z-Axis points in the same Direction as the Spacecraft's Angular Momentum, or Spin or Attitude, Vector. The positive X-Axis points in the Direction in the Spin Plane that is closest to the Direction towards the Sun. In other Words, the positive X-Axis points in the Direction of the Projection on the Spin Plane of the Vector from the Spacecraft to the Sun. The positive Y-Axis is determined by the Requirement that the DSC XYZ System form an Orthogonal Right-Handed System. It follows that the positive Y-Axis points in the Direction on the Spin Plane that is 90 degrees ahead of the positive X-Axis in the Sense of the Spacecraft's Rotation. The Electric Field Data included in these Files consists of the two Electric Field Components in the Spin Plane. The Original Data used is V34L, which typically has a Time Resolution of about 40 Data Points per Second. A Least-Squares Spin Fit of V34L is performed and the Spin Fit Coefficients provide the Spin Plane Components of the Spin Period Electric Field. Time is a Real Double Precision Quantity. The Units for the Time are Seconds. The Time is the Time elapsed since the Epoch starting on May 24, 1968 at 00:00:00 UT. Each Time Tag indicates the Mid-Point of the Time Interval for the corresponding Spin Period. Data Gaps are not filled and each Time Tag corresponds to an Actual Data Point. X, Y, and Z are the three Components of the Attitude Vector in the Geocentric Solar Ecliptic, GSE, Coordinate System.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/a4sb-1d04",
"Polar Electric Fields Instrument (EFI), Spacecraft Attitude in GSE coordinates",
"",
"Please acknowledge the instrument PI, F.S. Mozer, and CDAWeb when using these data.",
"PT600S",
"1996-03-16T00:00:00",
"2008-04-13T24:00:00",
"",
"2.6.0"
],
[
"PO_6SECEDSC_EFI",
"spase://NASA/NumericalData/POLAR/EFI/Despun/PT6S",
"spase://SMWG/Instrument/POLAR/EFI",
"ElectricField",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"Accurate data requires a correction in the form of an offset to the Sunward component of the electric field. Users of this data desiring more information should get in touch with Dr. Forrest Mozer, at the Space Sciences Laboratory, University of California, Berkeley.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vkpj-6n73",
"Polar Electric Fields Instrument (EFI), 6-sec Electric Field in Despun Spacecraft Coordinates",
"",
"",
"PT6S",
"1996-03-16T00:00:00",
"2008-04-12T00:00:00",
"",
"2.6.0"
],
[
"PO_6SECPOTLDENS_EFI",
"spase://NASA/NumericalData/POLAR/EFI/SC/Potential_PlasmaDensity/Spin/PT6S",
"spase://SMWG/Instrument/POLAR/EFI",
[
"ElectricField",
"ThermalPlasma"
],
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
"",
"2025-08-05T13:12:20Z",
"https://doi.org/10.48322/ttha-dc31",
"Polar Electric Fields Instrument (EFI), Spacecraft Potential and Plasma Density, Spin Resolution",
"",
"The user will acknowledge, in any publication which uses POLAR EFI data, the instrument PI, as well as the instrument PI for the POLAR Hydra instrument, if the Plasma Density is used.",
"PT6S",
"1996-03-16T00:00:00",
"2008-04-12T24:00:00",
"",
"2.7.0"
],
[
"PO_AT_DEF",
"spase://NASA/NumericalData/POLAR/Attitude/Definitive/PT10M",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/r4rq-sq24",
"Polar Definitive Attitude, 10 min Data, Spin Axis Orientation Angles in GCI, GSE and GSM Coordinates",
"",
". Please acknowledge the data providers and CDAWeb when using these data.",
"PT10M",
"1996-02-24T00:00:00",
"1997-07-15T23:50:00",
"",
"2.6.0"
],
[
"PO_AT_PRE",
"spase://NASA/NumericalData/POLAR/Ephemeris/Attitude/PT10M",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-09-15T12:34:56.789",
"",
"Polar Attitude Data, 10 min Data",
"",
"",
"PT10M",
"1996-03-08T00:00:00",
"2008-06-14T23:50:00",
"",
"2.6.0"
],
[
"PO_H0_CAM",
"spase://NASA/NumericalData/POLAR/CAMMICE/Fluxes/PT204S",
"spase://SMWG/Instrument/POLAR/CAMMICE",
"EnergeticParticles",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/bdjc-7g81",
"Polar CAMMICE 3-Min Fluxes",
"",
"",
"PT204S",
"1996-03-18T00:00:00",
"2000-03-16T00:00:00",
"",
"2.6.0"
],
[
"PO_H0_HYD",
"spase://NASA/NumericalData/POLAR/HYDRA/PT13.8S",
"spase://SMWG/Instrument/POLAR/HYDRA",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/rpbf-wd36",
"Polar HYDRA 13.8 sec Ion and Electron Fluxes",
"",
"",
"PT13.8S",
"1996-04-01T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_H0_PWI",
"spase://NASA/NumericalData/POLAR/PWI/MCA/PT1.3S",
"spase://SMWG/Instrument/POLAR/PWI",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"",
"See the Polar Interpretation Issues web site at http://www-pw.physics.uiowa.edu/plasma-wave/istp/polar/interpretation.html",
[
"Dynamic Spectrogram",
"Spectrogram",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Banded emissions",
"Broadband Electrostatic Noise",
"BEN",
"Chorus",
"Continuum radiation",
"Electromagnetic Ion Cyclotron waves",
"EMIC",
"Electron Cyclotron Harmonics",
"Kilometric Continuum radiation",
"Myriametric radiation",
"Plasmaspheric Hiss",
"Solar radio burst",
"Terrestrial Kilometric Radiation",
"TKR",
"UHR",
"Upper hybrid resonance",
"Whistler mode",
"Whistlers"
],
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/879x-0r04",
"Polar Plasma Wave Instrument (PWI), Multichannel Analyzer - 1.3 sec resolution fields",
[
"PO_H0_PWI",
"Polar PWI MCA CDFs at NASA's CDAWeb"
],
"Users please acknowledge the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center and Polar PWI instrument Principal Investigator Don Gurnett.",
"PT1.3S",
"1996-03-25T00:00:00Z",
"1997-09-16T17:00:00Z",
"",
"2.6.0"
],
[
"PO_H0_TID",
"spase://NASA/NumericalData/POLAR/TIDE/H0_CDF",
"spase://SMWG/Instrument/POLAR/TIDE",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"Level 1",
"TIDE was originally designed to detect mass-resolved ions, H+, O+, He+, and NO+, for 32 energy steps (31 reported), 32 spin angle bins, and 7 polar angle channels. The detection of time-of-flight direct-events deteriorated rapidly early in the mission, reducing the ability to resolve ion masses and resulting in the lost of information in one axis (Z). After 09/30/96, the ion data is of poor quality and as a result, only Total Ions (Stops) are reported starting 12/08/96. Total Ions is the sum over the 7 polar angle channels of the particle counts detected by the Stop microchannel plate (MCP) detectors. The resolution in the 32 energy steps and in the 32 spin angle bins is retained. 1996 H+, O+, and He+ data are reported in the TIDE H0 CDFs. In order to avoid damage to the MCPs, starting 03/27/96 and continuing throughout the rest of the mission, the high voltage on the MCPs is reduced during radiation belt passes.",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/zkvp-5751",
"Polar TIDE 6-s H, He, O Data",
"",
"",
"PT6.00S",
"1996-03-27T00:00:00",
"1996-12-07T23:59:59",
"",
"2.6.0"
],
[
"PO_H0_TIM",
"spase://NASA/NumericalData/POLAR/TIMAS/H0/PT12S",
"spase://SMWG/Instrument/POLAR/TIMAS",
[
"EnergeticParticles",
"IonComposition",
"Spectrum",
"ThermalPlasma"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"Level 1",
"The Epoch_xx times are the center times of the accumulation interval over which the data were acquired. Depending on instrument mode, fluxes for each major species are accumulated for 2, 4, 8, 16, or 32 spins on-board. This corresponds to 12, 24, 48, 96, or 192 second resolution. The spin accumulation indicator shows the number of spins accumulated for each major ion species for each data record. Note that data with both high and medium resolution are combined in these files. This means that the energy, angle, and time resolution of some data are less than the resolution provided in the data file. Early in the mission, The TIMAS high energy limit was 22 keV/e. It was changed to 33 keV/e on June 26, 1996. The Energy_Range_ID flag indicates which energy range the TIMAS instrument was in at the time of data acquisition. Even energy steps (0, 2, ...) are acquired on even spin numbers and odd energy steps (1,3, ...) are acquired on odd spin numbers. High resolution data are included from two spins. To resolve timing uncertainties the Even/Odd indicator is set to indicate which set of energy steps were acquired in the first 6 seconds of the two spin accumulation interval. The quality of TIMAS data depends on the total number of counts processed by the detector. Some summary quality information is provided in the Quality Flags. The Quality Flags are derived from the fast event counter and other data sources. The TIMAS sensor responds to penetrating radiation that is particularly intense in the radiation belt part of each orbit. The Fluxes returned have been corrected for the background counting rate. Correction of TIMAS fluxes for high count rates increases the uncertainty in the flux values reported. The quality flag is provided as a convenient flag to use to select data that has been acquired in the linear response range of the instrument. Depending on instrument mode, fluxes for each major species are averaged or not averaged over energy ranges on-board. The energy resolution indicator provides a summary of the energy resolution of the data in each record for each ion species. Depending on instrument mode, fluxes for each major species are averaged with one of three angular resolutions on-board. The pitch angle resolution indicator provides a summary of the angular resolution of the data in each record for each ion species. On December 8, 1998 the TIMAS instrument had a high voltage breakdown that resulted in a loss of sensitivity at energies above 700 eV/q and non linear response to ion fluxes at energies below 700 eV/q. After this date the TIMAS K1 data product should be used instead.",
[
"Energetic Ion Mass-Energy Spectra",
"Three dimensional Angular Response"
],
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/khhg-8859",
"Polar TIMAS H0 High-resolution Level 1 Data",
"",
"",
"PT12S",
"1996-03-17T00:03:19",
"2004-04-03T09:04:47",
"",
"2.6.0"
],
[
"PO_H1_PWI",
"spase://NASA/NumericalData/POLAR/PWI/SFR/AB/PT2S",
"spase://SMWG/Instrument/POLAR/PWI",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Heliosphere.Inner"
],
"",
"",
"A full frequency sweep for the SFR takes about 33 seconds. From about 12.5 kHz to 800 kHz a full frequency spectrum can be obtained every 2.4 sec in the log mode. There are 224 SFR frequency bands, logarithmically spaced. When SFR_MODE is Linear, the 448 linear frequency bands are mapped to 224 logarithmic bands.",
[
"Dynamic Spectrogram",
"Spectrogram",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Banded emissions",
"Broadband Electrostatic Noise",
"BEN",
"Chorus",
"Continuum radiation",
"Electromagnetic Ion Cyclotron waves",
"EMIC",
"Electron Cyclotron Harmonics",
"Kilometric Continuum radiation",
"Myriametric radiation",
"Plasmaspheric Hiss",
"Solar radio burst",
"Terrestrial Kilometric Radiation",
"TKR",
"UHR",
"Upper hybrid resonance",
"Whistler mode",
"Whistlers"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/k1kt-d028",
"Polar Plasma Wave Instrument (PWI), Sweep Frequency Receivers A and B - 2 sec resolution fields",
[
"PO_H1_PWI",
"Polar PWI SFR A and B CDFs at NASA's CDAWeb"
],
"Users please acknowledge the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center and Polar PWI instrument Principal Investigator Don Gurnett.",
"PT2S",
"1996-03-25T00:00:00Z",
"1997-09-16T17:00:00Z",
"",
"2.6.0"
],
[
"PO_H1_TID",
"spase://NASA/NumericalData/POLAR/TIDE/H1_CDF",
"spase://SMWG/Instrument/POLAR/TIDE",
"ThermalPlasma",
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap"
],
"",
"Level 1",
"TIDE was originally designed to detect mass-resolved ions, H+, O+, He+, and NO+, for 32 energy steps (31 reported), 32 spin angle bins, and 7 polar angle channels. The detection of time-of-flight direct-events deteriorated rapidly early in the mission, reducing the ability to resolve ion masses and resulting in the lost of information in one axis (Z). After 09/30/96, the ion data is of poor quality and as a result, only Total Ions (Stops) are reported starting 12/08/96. Total Ions is the sum over the 7 polar angle channels of the particle counts detected by the Stop microchannel plate (MCP) detectors. The resolution in the 32 energy steps and in the 32 spin angle bins is retained. 1996 H+, O+, and He+ data are reported in the TIDE H0 CDFs. In order to avoid damage to the MCPs, starting 03/27/96 and continuing throughout the rest of the mission, the high voltage on the MCPs is reduced during radiation belt passes.",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/t5sd-r305",
"Polar TIDE 6-s Z-unresolved Data",
"",
"",
"PT6.00S",
"1996-12-08T00:00:00",
"2008-04-16T23:59:59",
"",
"2.6.0"
],
[
"PO_H2_PWI",
"spase://NASA/NumericalData/POLAR/PWI/LFWR/PT0.01S",
"spase://SMWG/Instrument/POLAR/PWI",
[
"Waves.Passive",
"Spectrum"
],
[
"Earth.Magnetosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Heliosphere.Inner"
],
"",
"",
"See the Polar Interpretation Issues web site at http://www-pw.physics.uiowa.edu/plasma-wave/istp/polar/interpretation.html",
[
"Dynamic Spectrogram",
"Spectrogram",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Banded emissions",
"Broadband Electrostatic Noise",
"BEN",
"Chorus",
"Continuum radiation",
"Electromagnetic Ion Cyclotron waves",
"EMIC",
"Electron Cyclotron Harmonics",
"Kilometric Continuum radiation",
"Myriametric radiation",
"Plasmaspheric Hiss",
"Solar radio burst",
"Terrestrial Kilometric Radiation",
"TKR",
"UHR",
"Upper hybrid resonance",
"Whistler mode",
"Whistlers"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/xbm6-4c53",
"Polar Plasma Wave Instrument (PWI), Low Frequency Waveform Receiver, ~0.01 sec resolution fields",
"PO_H2_PWI",
"Users please acknowledge the Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center and Polar PWI instrument Principal Investigator Don Gurnett of The University of Iowa.",
"PT0.01S",
"1996-03-25T00:00:16.000",
"1997-09-16T16:52:55.000",
"",
"2.6.0"
],
[
"PO_H2_TIM",
"spase://NASA/NumericalData/POLAR/TIMAS/H2/PT12S",
"spase://SMWG/Instrument/POLAR/TIMAS",
[
"EnergeticParticles",
"IonComposition",
"Spectrum",
"ThermalPlasma"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 1",
"Several compromises were made in assembling the data base. In particular background subtraction, short averaging intervals and the normally low count rates for minor ions (O+, He+, and He++) lead to many data intervals where the data values reported are not statistically significant. The data files therefore contain many diagnostic parameters and data quality flags.",
[
"Energetic Ion Mass-Energy Spectra",
"Net outflowing number flux"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/5hsz-5423",
"Polar TIMAS H2 Level 1 Ion Upflowing Fluxes Data",
"",
"",
"PT12S",
"1996-03-17T00:03:25",
"1998-12-08T22:55:45",
"",
"2.6.0"
],
[
"PO_H3_PWI",
"spase://NASA/NumericalData/POLAR/PWI/LHFWR/16kHz/PT0000028S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: POLAR PWI HFWR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Magnetospheric Data",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 3",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H3>LHFWR 16kHz (6 channels)",
"CDF Global Attribute ADID_REF: NSSD2001",
"CDF Global Attribute MODS: Created Mar 2021",
"Auroral hiss",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:21Z",
"https://doi.org/10.48322/zvyr-jh19",
"Polar Plasma Wave Instrument (PWI), High Frequency Waveform Receiver, 16 kHz bandwidth, 6-channel Fields",
"",
"UIowa, Donald A. Gurnett",
"PT0.000028S",
"1996-03-25T00:00:00.000",
"1997-09-17T00:00:00.000",
"The cadence value given here is computed from the inverse of the sampling rate (35712 Hz).",
"2.7.0"
],
[
"PO_H4_PWI",
"spase://NASA/NumericalData/POLAR/PWI/LHFWR/2kHz/PT0.000224S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: POLAR PWI HFWR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Magnetospheric Data",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 3",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H4>LHFWR 2KHz (6 channels)",
"CDF Global Attribute ADID_REF: NSSD0171",
"CDF Global Attribute MODS: Created Mar 2021",
"Auroral hiss",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:21Z",
"https://doi.org/10.48322/32d0-db83",
"Polar Plasma Wave Instrument, High Frequency Waveform Receiver, 2 kHz, Time Domain Fields",
"",
"U. Iowa, Donald. A. Gurnett",
"PT0.000224S",
"1996-03-26T00:00:00.000",
"1997-09-17T00:00:00.000",
"The cadence value given here is computed from the inverse of the sampling rate (4464 Hz).",
"2.7.0"
],
[
"PO_H5_PWI",
"spase://NASA/NumericalData/POLAR/PWI/LHFWR/16kHz/Interferometry/PT0.000028S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: POLAR PWI HFWR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Magnetospheric Data",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 1",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H5>High Resolution Data",
"CDF Global Attribute ADID_REF: NSSD2001",
"CDF Global Attribute MODS: Created Jan 2004",
"Auroral hiss",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:21Z",
"https://doi.org/10.48322/kvvt-2c42",
"Polar Plasma Wave Instrument (PWI), High Frequency Waveform Receiver, 16 kHz, Time Domain Fields.",
"",
"U. Iowa, Donald. A. Gurnett",
"PT0.000028S",
"1996-03-25T00:00:00.000",
"1997-09-15T00:00:00.000",
"The cadence value given here is computed from the inverse of the sampling rate (35.71 kHz).",
"2.7.0"
],
[
"PO_H7_PWI",
"spase://NASA/NumericalData/POLAR/PWI/HFWR/25kHz/PT0.000014S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: POLAR PWI HFWR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Magnetospheric Data",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 2",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H7>HFWR 6-channel, 14 usec",
"CDF Global Attribute ADID_REF: NSSD2001",
"CDF Global Attribute MODS: Created Feb 2012",
"Auroral hiss",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:21Z",
"https://doi.org/10.48322/7vp8-5w49",
"Polar Plasma Wave Instrument (PWI), High Frequency Waveform Receiver, 25kHz bandwidth, 6-channel fields",
"",
"UIowa, Donald A. Gurnett",
"PT0.000014S",
"1996-03-26T15:00:00.000",
"1997-09-16T17:00:00.000",
"The cadence value given here is computed from the inverse of the sampling rate (71.43 kHz).",
"2.7.0"
],
[
"PO_H8_PWI",
"spase://NASA/NumericalData/POLAR/PWI/HFWR/25kHz/Interferometry/PT0.000014S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: POLAR PWI HFWR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Magnetospheric Data",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 1",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H8>HFWR Interferometry, 14 usec",
"CDF Global Attribute ADID_REF: NSSD2001",
"CDF Global Attribute MODS: Created Jan 2004",
"Auroral hiss",
"Chorus",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:20Z",
"https://doi.org/10.48322/06zn-yc02",
"Polar Plasma Wave Instrument (PWI), High Frequency Waveform Receiver, 25kHz bandwidth interferometry fields",
"",
"UIowa, Donald A. Gurnett",
"PT0.000014S",
"1996-04-04T15:00:00.000",
"1997-09-14T19:00:00.000",
"The cadence value given here is computed from the inverse of the sampling rate (71.43 kHz).",
"2.7.0"
],
[
"PO_H9_PWI",
"spase://NASA/NumericalData/POLAR/PWI/WBR/PT0.000004016S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
[
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.AuroralRegion",
"Earth.Magnetosphere"
],
"",
"",
"",
[
"CDF Global Attribute TITLE: Polar PWI WBR",
"CDF Global Attribute MISSION_GROUP: Polar CDF Global Attribute MISSION_GROUP: Polar",
"CDF Global Attribute PROJECT: ISTP>International Solar-Terrestrial Physics",
"CDF Global Attribute DATA_VERSION: 1",
"CDF Global Attribute DISCIPLINE: Space Physics>Magnetospheric Science",
"CDF Global Attribute DATA_TYPE: H9>High Resolution Data",
"CDF Global Attribute ADID_REF: NSSD2001",
"CDF Global Attribute MODS: Created Jan 2004",
"Auroral hiss",
"Chorus",
"Auroral kilometric radiation",
"Continuum radiation",
"Equatorial Noise",
"Plasmaspheric Hiss",
"Langmuir Waves",
"Electostatic Solitary Waves",
"ESW",
"Whistlers",
"Ion Acoustic Waves",
"Bernstein Waves",
"Upper Hybrid Waves",
"Lower Hybrid Waves"
],
"2025-08-05T13:12:21Z",
"https://doi.org/10.48322/ybd2-7a47",
"Polar Plasma Wave Instrument (PWI), Wideband Receiver (WBR) 4.016 microsecond resolution",
"",
"UIowa, Donald A. Gurnett",
"PT0.000004016S",
"1996-03-25T10:00:00.000Z",
"1997-09-17T00:00:00.000Z",
"The cadence value given here is computed from the inverse of the sampling rate (249 kHz).",
"2.7.0"
],
[
"PO_K0_CAM",
"spase://NASA/NumericalData/POLAR/CAMMICE/KeyParameters/PT204S",
"spase://SMWG/Instrument/POLAR/CAMMICE-MICS",
"EnergeticParticles",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/88r3-b823",
"Polar (Charge and Mass Magnetospheric Ion Composition) CAMMICE 3-Min Key Parameters",
"",
"",
"PT204S",
"1996-02-26T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_K0_CEP",
"spase://NASA/NumericalData/POLAR/CEPPAD/PT100S",
"spase://SMWG/Instrument/POLAR/CEPPAD",
"EnergeticParticles",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/gav4-4v68",
"Polar CEPPAD Key Parameters, 100-sec Count Rates",
"",
"",
"PT100S",
"1996-02-26T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_K0_EFI",
"spase://NASA/NumericalData/POLAR/EFI/KeyParameters/PT6S",
"spase://SMWG/Instrument/POLAR/EFI",
"ElectricField",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/6n18-vn30",
"Polar Electric Fields Instrument (EFI), 6-sec Key Parameters",
"",
"",
"PT6S",
"1996-03-15T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_K0_HYD",
"spase://NASA/NumericalData/POLAR/HYDRA/PT55S",
"spase://SMWG/Instrument/POLAR/HYDRA",
"ThermalPlasma",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/8ksp-p425",
"Polar HYDRA 55-s Key Parameters",
"",
"",
"PT55S",
"1996-03-20T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_K0_MFE",
"spase://NASA/NumericalData/POLAR/MFE/PT55S",
"spase://SMWG/Instrument/POLAR/MFE",
"MagneticField",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"CALIBRATED",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vsfk-ph35",
"Polar Magnetic Field Key Parameters",
"",
"",
"PT55S",
"1996-03-16T00:00:00",
"2008-04-16T00:00:00",
"As of 8/27/04, coverage ended 12/31/03.",
"2.6.0"
],
[
"PO_K0_PWI",
"spase://NASA/NumericalData/POLAR/PWI/KeyParameters/PT300S",
"spase://SMWG/Instrument/POLAR/PWI",
"Waves.Passive",
"Earth.Magnetosphere",
"",
"CALIBRATED",
"Key parameter and survey data (labels K0, K1, K2) are preliminary browse data.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/0zmq-1b63",
"Polar PWI Key Parameters",
"",
"",
"PT300S",
"1996-02-27T12:20:27",
"1997-09-16T16:51:41",
"",
"2.6.0"
],
[
"PO_K0_SPHA",
"spase://NASA/NumericalData/POLAR/Ephemeris/KeyParameters/PT24H",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/f58f-3y50",
"Polar Spin Phase Key Parameter Data",
"",
"",
"PT24H",
"1996-03-08T00:00:00",
"2008-06-14T23:50:00",
"",
"2.6.0"
],
[
"PO_K0_UVI",
"spase://NASA/NumericalData/POLAR/UVI/K0_CDF",
"spase://SMWG/Instrument/POLAR/UVI",
"ImageIntensity",
"Earth.NearSurface.Ionosphere",
"",
"Level 1",
"UVI Key Parameters are summary data only. In some cases parameters such as pointing and calibration were not be adequate to support quantitative scientific analysis. They should not to be used for presentation, publication, or analysis. The UVI KP CDF files only contain output for normal instrument mode when the spacecraft is in 9.2 second science telemetry mode. No Key Parameters are produced when the spacecraft is in maneuver telemetry mode, when UVI is in star (fast) mode, and when the despun platform is pointed away from the earth.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1ac1-5c88",
"Polar Ultraviolet Imager, Key Parameters",
"",
"",
"",
"1996-03-23T15:56:15",
"2008-02-10T18:40:28",
"",
"2.6.0"
],
[
"PO_K1_TIM",
"spase://NASA/NumericalData/POLAR/TIMAS/K1/PT96S",
"spase://SMWG/Instrument/POLAR/TIMAS",
[
"EnergeticParticles",
"IonComposition",
"Spectrum",
"ThermalPlasma"
],
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 1",
"On December 8, 1998 the TIMAS instrument had a high voltage breakdown that resulted in a loss of sensitivity at energies above 700 eV/q and non linear response to ion fluxes at energies below 700 eV/q. The data from the two lowest energy channels in this data set (430 and 585 eV respectively) should be used with caution. Prior to the breakdown, the TIMAS H0 data product provides higher time resolution data in the full energy and angular range. The K1 data are averaged over time (96 seconds) and angle (nearly the full 4 pi), so narrow angular and/or temporal features are not shown. Higher temporal and angular resolution data can be interactively generated at http://lasp.colorado.edu/timas/mrdf",
[
"Energetic Ion Mass-Energy Spectra",
"Omni-directional Number Flux",
"Three dimensional Angular Response"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/qzm5-9r79",
"Polar TIMAS K1 Key Parameter data",
"",
"",
"PT96S",
"1999-06-07T00:09:31",
"2008-04-16T13:22:28",
"",
"2.6.0"
],
[
"PO_LEVEL1_UVI",
"spase://NASA/NumericalData/POLAR/UVI/L1_CDF",
"spase://SMWG/Instrument/POLAR/UVI",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Earth.NearSurface.Ionosphere"
],
"",
"Calibrated",
"",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/kchw-gw93",
"Polar UVI Imagery from CDAWeb",
"",
"",
"",
"1996-05-26T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_OR_DEF",
"spase://NASA/NumericalData/POLAR/Ephemeris/Definitive/PT1M",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/x2af-pn51",
"Polar Definitive Orbit, 1 min Data, Spacecraft Position and Velocity in GCI, GSE, GSM, and HEC Coordinates",
"",
". Please acknowledge the data providers and CDAWeb when using these data.",
"PT1M",
"1996-02-27T00:00:00",
"1997-07-15T23:59:00",
"",
"2.6.0"
],
[
"PO_OR_PRE",
"spase://NASA/NumericalData/POLAR/Ephemeris/PT60S",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/5tsm-w805",
"Polar Predicted Orbit, 1 min Data",
"",
"",
"PT60S",
"1996-02-27T00:00:00",
"2008-04-16T00:00:00",
"",
"2.6.0"
],
[
"PO_PA_DEF",
"spase://NASA/NumericalData/POLAR/Ephemeris/Attitude/PT24H",
"spase://SMWG/Instrument/POLAR/Ephemeris",
"Ephemeris",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/akgc-de65",
"Polar Platform Attitude, Daily Definitive Data",
"",
"",
"PT24H",
"1996-03-08T00:00:00",
"2008-06-14T23:50:00",
"",
"2.6.0"
],
[
"PO_VIS_EARTH-CAMERA-CALIBRATED",
"spase://NASA/NumericalData/POLAR/VIS/EarthCameraCalibrated/PT4M",
"spase://SMWG/Instrument/POLAR/VIS",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"",
"",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/ma2e-tm75",
"Polar Visible Imaging System (VIS) Earth Camera Images, Calibrated (E0), 4 min Data",
"",
"L.A. Frank",
"PT4M",
"1996-04-30T00:00:00.000",
"2008-04-16T07:59:59.999",
"",
"2.6.0"
],
[
"PO_VIS_VISIBLE-IMAGER-CALIBRATED",
"spase://NASA/NumericalData/POLAR/VIS/VisibleImagerCalibrated/PT24S",
"spase://SMWG/Instrument/POLAR/VIS",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Polar",
"Earth.NearSurface",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.EquatorialRegion",
"Earth.NearSurface.Ionosphere",
"Earth.NearSurface.PolarCap"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1mkd-p917",
"Polar Visible Imaging System (VIS) Low Resolution Camera Images, Calibrated, Level 0 (L0), 12 s Data",
"",
"L.A. Frank",
"PT24S",
"1996-11-12T00:00:00.000",
"2008-04-16T23:59:59.999",
"",
"2.6.0"
],
[
"PSP_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/ParkerSolarProbe/MAGandPLS/PT1H",
[
"spase://SMWG/Instrument/ParkerSolarProbe/Ephemeris",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/MAG",
"spase://SMWG/Instrument/ParkerSolarProbe/SWEAP/SPC"
],
[
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Sun.Corona"
],
"",
"",
"",
"",
"2024-07-02T00:00:00",
"https://doi.org/10.48322/19ed-kz70",
"Parker Solar Probe (PSP) Merged Magnetic Field, Plasma, and Ephemeris, Hourly Data",
"",
"Please acknowledge the Principal Investigator N.E. Papitashvili for use of the Data",
"PT1H",
"2018-01-01T00:00:00.000",
"2019-12-01T23:59:59.999",
"",
"2.6.1"
],
[
"PSP_FLD_L2_DFB_AC_BPF_DV12HG",
"spase://NASA/NumericalData/ParkerSolarProbe/FIELDS/DFB/Level2/AC/BandpassFilter/DV12/HighGain/PT0.873813S",
[
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/DFB",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/V1",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/V2"
],
[
"InstrumentStatus",
"Waves.Passive"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Sun.Corona"
],
"",
"",
"",
"",
"2022-05-25T12:34:56.789",
"https://doi.org/10.48322/y8gb-3n29",
"PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V1-V2 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data",
"",
"Please acknowledge the Principal Investigator S.D. Bale for use of the Data",
"PT0.873813S",
"2019-08-22T00:00:00.000",
"",
"",
"2.4.0"
],
[
"PSP_FLD_L2_DFB_AC_BPF_DV34HG",
"spase://NASA/NumericalData/ParkerSolarProbe/FIELDS/DFB/Level2/AC/BandpassFilter/DV34/HighGain/PT0.873813S",
[
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/DFB",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/V3",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/V4"
],
[
"InstrumentStatus",
"Waves.Passive"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Sun.Corona"
],
"",
"",
"",
"",
"2022-05-25T12:34:56.789",
"https://doi.org/10.48322/6nn3-ts64",
"PSP FIELDS Digital Fields Board (DFB) AC-coupled Differential Voltage, V3-V4 Antennae, Dipole Mode, Bandpass filtered, High Gain, Sensor coordinates, Level 2 (L2), 0.873813 s Data",
"",
"Please acknowledge the Principal Investigator S.D. Bale for use of the Data",
"PT0.873813S",
"2018-10-06T00:00:00.000",
"",
"",
"2.4.0"
],
[
"PSP_FLD_L2_DFB_AC_BPF_SCMULFHG",
"spase://NASA/NumericalData/ParkerSolarProbe/FIELDS/DFB/Level2/AC/BandpassFilter/SCM/U/LowFrequency/HighGain/PT0.873813S",
[
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/DFB",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/SCM"
],
[
"InstrumentStatus",
"Waves.Passive"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Sun.Corona"
],
"",
"",
"",
"",
"2022-05-25T12:34:56.789",
"https://doi.org/10.48322/6svt-vr86",
"PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer, SCM, Bandpass filtered, Low Frequency, High Gain, u-component, Sensor coordinates, Level 2 (L2), 0.873813 s Data",
"",
"Please acknowledge S.D. Bale for use of the Data",
"PT0.873813S",
"2018-10-06T00:00:00.000",
"",
"",
"2.4.0"
],
[
"PSP_FLD_L2_DFB_AC_BPF_SCMUMFHG",
"spase://NASA/NumericalData/ParkerSolarProbe/FIELDS/DFB/Level2/AC/BandpassFilter/SCM/MediumFrequency/HighGain/PT0.873813S",
[
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/DFB",
"spase://SMWG/Instrument/ParkerSolarProbe/FIELDS/SCM"
],
[
"InstrumentStatus",
"Waves.Passive"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Sun.Corona"
],
"",
"",
"",
"",
"2022-05-25T12:34:56.789",
"https://doi.org/10.48322/be3k-1d62",
"PSP FIELDS Digital Fields Board (DFB) AC-coupled Searchcoil Magnetometer, SCM, Bandpass filtered, Medium Frequency, High Gain, u-component, Sensor coordinates, Level 2 (L2), 0.873813 s Data",
"",
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"https://doi.org/10.48322/s8mc-9x35",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Fluxgate Magnetometer (MAG) Burst Mode, Magnetic Field Vector, Spacecraft (SC) Coordinates, Level 1 (L1), 31 ms Data",
"",
"Please acknowledge the STEREO IMPACT Principal Investigator J.G. Luhmann for use of the Data and the key IMPACT Magnetometer personnel: C.W. Smith and the late M.H. Acuna.",
"PT0.031S",
"2006-11-07T02:01:21.000",
"2018-12-01T00:00:00.000",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/L1/PT0.125S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/MAG",
"MagneticField",
"Heliosphere.Remote1AU",
"",
"1",
"Current version of the data include very fast (subsecond) glitches in the magnetometer's X sensor. Magnitude of these glitches are approximately 0.5 nT and occur at varying frequencies throughout the mission.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/200r-rj72",
"STEREO-A In-situ Measurements of Particles And CME Transients (IMPACT) Magnetic Field Vectors and Ancillary Data",
"STEREO-A IMPACT/MAG Level 1 Data",
"The STEREO IMPACT/MAG Team",
"PT0.125S",
"2006-11-08T00:00:00Z",
"",
"",
"2.6.0"
],
[
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"spase://SMWG/Instrument/STEREO-A/IMPACT/MAG",
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/a8eg-e811",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Fluxgate Magnetometer (MAG) Magnetic Field Vectors, in Spacecraft (SC) Coordinates",
"",
"J. Luhmann",
"PT0.125S",
"2006-11-07T00:00:00",
"",
"",
"2.6.0"
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[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/SEPT/L1/PT1M",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SEPT",
"EnergeticParticles",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/b6fb-a452",
"STEREO-A IMPACT (In-Situ Measurements of Particles and CME Transients) Solar Electron Proton Telescope (SEPT) 1-min Level 1 Electron and Proton Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT1M",
"2006-11-14T00:00:00",
"",
"",
"2.6.0"
],
[
"STA_L1_SIT",
"spase://NASA/NumericalData/STEREO-A/IMPACT/SIT/L1/PT1M",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SIT",
"EnergeticParticles",
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/sp7s-tp20",
"STEREO-A IMPACT (In-Situ Measurements of Particles and CME Transients) Suprathermal Ion Telescope (SIT) 1-min Level 1 Multi-Z Ion Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT1M",
"2007-03-15T00:00:00",
"",
"",
"2.6.0"
],
[
"STA_L1_STE",
"spase://NASA/NumericalData/STEREO-A/IMPACT/STE/L1/PT10S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/STE",
"EnergeticParticles",
"Heliosphere.Remote1AU",
"",
"",
"The four sensors labelled \"U\" and numbered 1-4 are saturated and should not be used. Sensors providing usable data are labelled \"D\" and are numbered 5-8.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/c1sh-f024",
"STEREO-A IMPACT (In-Situ Measurements of Particles and CME Transients) Suprathermal Electron Telescope (STE) 10-s Level 1 Electron Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT10S",
"2006-11-01T00:00:00",
"2009-08-04T00:00:00",
"Further extensions may be made",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/L1/PT2S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SWEA",
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus"
],
"Heliosphere.Remote1AU",
"",
"",
"Since commissioning, the SWEA instruments on both STEREO spacecraft have registered difficult to characterize degradations in the solar wind core electron energies, probably due to charging effects. The nature of the degradations are such that the data are not reliable for electron measurements below 45 eV. However, halo and higher energy electrons are unaffected. Versions 4 and higher of the SWEA 3D distribution data products have these lower energies removed. Similarly, Versions 4 and higher of the SWEA pitch angle distribution products also remove these energies. Use of the SWEA pitch angle distributions for most purposes, for example, higher energy heat flux pitch angle distribbutions, PADs, should be largely unaffected. For more information regarding these issues, please contact Peter Schroeder, peters@ssl.berkeley.edu. If you have downloaded Version 3 or earlier Files, those files contain unreliable data below 45 eV and should be replaced with Version 4 files. Note that if the interpretation of these data become a significant focus in your work, you should obtain explicit prior permission from the PI of the experiment before publication.",
"",
"2023-07-31T12:34:56.789",
"https://doi.org/10.48322/h0g4-j046",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) 3-Dimensional Electron Distributions, Burst Mode, Level 1 (L1), 2 s Data",
"",
"Please acknowledge the Principal Investigator J.G. Luhmann for use of the Data",
"PT2S",
"2006-10-28T15:35:39.000",
"2018-11-30T23:59:58.000",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/L1/PT30S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SWEA",
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus"
],
"Heliosphere.Remote1AU",
"",
"",
"Since commissioning, the SWEA instruments on both STEREO spacecraft have registered difficult to characterize degradations in the solar wind core electron energies, probably due to charging effects. The nature of the degradations are such that the data are not reliable for electron measurements below 45 eV. However, halo and higher energy electrons are unaffected. Versions 4 and higher of the SWEA 3D distribution data products have these lower energies removed. Similarly, Versions 4 and higher of the SWEA pitch angle distribution products also remove these energies. Use of the SWEA pitch angle distributions for most purposes, for example, higher energy heat flux pitch angle distribbutions, PADs, should be largely unaffected. For more information regarding these issues, please contact Peter Schroeder, peters@ssl.berkeley.edu. If you have downloaded Version 3 or earlier Files, those files contain unreliable data below 45 eV and should be replaced with Version 4 files. Note that if the interpretation of these data become a significant focus in your work, you should obtain explicit prior permission from the PI of the experiment before publication.",
"",
"2023-07-31T12:34:56.789",
"https://doi.org/10.48322/p3vt-z848",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) 3-Dimensional Electron Distributions, Level 1 (L1), 30 s Data",
"",
"Please acknowledge the Principal Investigator J.G. Luhmann for use of the Data",
"PT30S",
"2006-10-28T15:36:11.000",
"2018-11-30T23:59:53.000",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/Spectra/L1/PT10S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SWEA",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/fd9e-bg75",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) Spectra",
"",
"J. Luhmann",
"PT10S",
"2012-12-01T00:00:00.000",
"2013-12-31T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L2_MAGPLASMA_1M",
"spase://NASA/NumericalData/STEREO-A/MAGPLASMA/L2/PT1M",
[
"spase://SMWG/Instrument/STEREO-A/Ephemeris",
"spase://SMWG/Instrument/STEREO-A/IMPACT",
"spase://SMWG/Instrument/STEREO-A/PLASTIC"
],
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"Level 2",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/2qaz-wv11",
"STEREO-A In-Situ Measurements of Particles and CME Transients from the Magnetometer and the Plasma and Suprathermal Ion and Composition Instruments (IMPACT/MAG, PLASTIC) Solar Wind Plasma Data",
"",
"J. Luhmann",
"PT1M",
"2006-01-01T00:00:00.000",
"2014-01-01T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT10M",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
"ThermalPlasma",
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/ka9p-x087",
"STEREO-A Plasma and Suprathermal Ion Composition (PLASTIC) 10-min Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1H",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT1H",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/nax5-0024",
"STEREO-A Plasma and Suprathermal Ion Composition (PLASTIC) 1-hour Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1H",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
],
[
"STA_L2_PLA_1DMAX_1MIN",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/Protons/PT1M",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1kfn-q976",
"STEREO-A Plasma and Suprathermal Ion Composition (PLASTIC) 1-min Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1M",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
],
[
"STA_L2_PLA_IRON_Q_2HR",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/Fe-abundance/PT2H",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/8gb9-1w75",
"STEREO-A Plasma and Suprathermal Ion Composition (PLASTIC) 2-hour Iron Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT2H",
"2007-01-01T00:00:00",
"",
"",
"2.6.0"
],
[
"STA_L2_SWEA_PAD",
"spase://NASA/NumericalData/STEREO-A/IMPACT/SWEA/PAD/L2/PT30S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/SWEA",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"Level 2",
"",
"",
"2024-07-02T00:00:00",
"https://doi.org/10.48322/2y16-0t29",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) Pitch Angle Distribution, Level 2 (L2), 30 s Data in CDF format",
"",
"Please acknowledge the Principal Investigator J. Luhmann for use of the Data",
"PT30S",
"2006-10-31T00:00:39",
"",
"",
"2.6.1"
],
[
"STA_L3_PLA_HE2PL_F_VSW_01HR",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/AlphaParticle/PhaseSpaceDensities/PT1H",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"InstrumentStatus",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/kvfg-ca60",
"STEREO-A PLasma and Supra-Thermal Ion Composition (PLASTIC) He++ Phase Space Densities and Counts in 6 normailzed Velocity Ranges and Proton Plasma Moments, Level 3 (L3), 1 h Data",
"",
"Please acknowledge the Principal Investigator, Dr. Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132.. See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"PT1H",
"2007-01-01T00:00:00.000",
"2009-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L3_PLA_HEPLUS_24HR",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlusParameter/P1D",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/p8nz-hw11",
"STEREO-A PLasma and Supra-Thermal Ion Composition (PLASTIC) He⁺ Counts and Relative Energy Flux in four Velocity Ranges normalized by the Solar Wind Speed, Level 3 (L3), Daily Data",
"",
"Please acknowledge the Principal Investigator, Dr. Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132.. See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"P1D",
"2007-04-01T00:00:00.000",
"2017-07-31T00:00:00.000",
"",
"2.6.0"
],
[
"STA_L3_PLA_HEPLUS_F_VSW_01HR",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/L3/PT1H",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/f1zg-ac02",
"STEREO-A Plasma and Supra-Thermal Ion Composition (PLASTIC) He+ Hourly Phase Space Densities",
"",
"A.B. Galvin, Please acknowledge the Principal Investigator, Antoinette Galvin, University of New Hampshire, and NASA contract NAS5-00132. See the Rules Of Use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"P1D",
"2007-01-01T00:00:00.000",
"2014-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L3_PLA_HEPLUS_F_VSW_10MIN",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlus/PhaseSpaceDensities/PT10M",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"InstrumentStatus",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/gm12-v076",
"STEREO-A PLasma and Supra-Thermal Ion Composition (PLASTIC) He+ Phase Space Densities and Counts in 6 normailzed Velocity Ranges and Proton Plasma Moments, Level 3 (L3), 10 min Data",
"",
"Please acknowledge the Principal Investigator, Dr. Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132.. See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"PT10M",
"2007-01-01T00:00:00.000",
"2017-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L3_PLA_HEPLUS_F_VSW_24HR",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/L3/P1D",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/0svp-2j12",
"STEREO-A Plasma and Supra-Thermal Ion Composition (PLASTIC) He+ Daily Phase Space Densities",
"",
"A.B. Galvin, Please acknowledge the Principal Investigator, Antoinette Galvin, University of New Hampshire, and NASA contract NAS5-00132. See the Rules Of Use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"P1D",
"2007-01-01T00:00:00.000",
"2014-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L3_PLA_HEPLUS_SW_VELCTDIST_5MIN",
"spase://NASA/NumericalData/STEREO-A/PLASTIC/HeliumPlus/VelocityCountDistributions/PT5M",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
[
"EnergeticParticles",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/3sk0-f028",
"STEREO-A PLasma and Supra-Thermal Ion Composition (PLASTIC) He+ Pickup Ion (PUI) Solar Wind Frame Velocity Count Distributions and Proton Plasma Densities and Velocities, Level 3 (L3), 5 min Data",
"",
"Please acknowledge the Principal Investigator, Dr. Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132.. See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"PT5M",
"2007-01-01T00:00:00.000",
"2013-01-01T23:59:59.999",
"",
"2.6.0"
],
[
"STA_L3_WAV_HFR",
"spase://NASA/NumericalData/STEREO-B/SWAVES/stb_l3_wav_hfr/PT15S",
"spase://SMWG/Instrument/STEREO-A/SWAVES",
[
"ElectricField",
"Waves"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2025-09-18T12:12:35Z",
"https://doi.org/10.48322/5e9v-xg43",
"STEREO-B/WAVES High Frequency Receiver, Data",
"",
"Please acknowledge the STEREO/Waves team. Data provided are Publicly available. If used in presentations or publications, please acknowledge STEREO/Waves Investigation (M. Maksimovic and S. D. Bale, PIs). Please read carefully the caveats attached to the data. For reporting purposes, we request bibliography information for any publication, etc., using these data. Please send information on the use of this data to M. Maksimovic and S. D. Bale (PIs).",
"PT15S",
"2006-10-28T00:00:00.000",
"",
"",
"2.7.0"
],
[
"STA_L3_WAV_LFR",
"spase://NASA/NumericalData/STEREO-A/SWAVES/sta_l3_wav_lfr/PT15S",
"spase://SMWG/Instrument/STEREO-A/SWAVES",
[
"ElectricField",
"Waves"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2025-09-18T12:12:34Z",
"https://doi.org/10.48322/x8s7-j459",
"STEREO-A/WAVES Low Frequency Receiver, Data",
"",
"Please acknowledge the STEREO/Waves team. Data provided are Publicly available. If used in presentations or publications, please acknowledge STEREO/Waves Investigation (M. Maksimovic and S. D. Bale, PIs). Please read carefully the caveats attached to the data. For reporting purposes, we request bibliography information for any publication, etc., using these data. Please send information on the use of this data to M. Maksimovic and S. D. Bale (PIs).",
"PT15S",
"2006-10-28T00:00:00.000",
"",
"",
"2.7.0"
],
[
"STA_LB_IMPACT",
"spase://NASA/NumericalData/STEREO-A/IMPACT/LB/PT1M",
"spase://SMWG/Instrument/STEREO-A/IMPACT",
[
"EnergeticParticles",
"MagneticField"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/w8k5-zt97",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Beacon",
"",
"J. Luhmann",
"PT1M",
"2007-03-20T00:00:00.000",
"",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/IMPACT/MAG/RTN/LevelBeacon/PT0.125S",
"spase://SMWG/Instrument/STEREO-A/IMPACT/MAG",
"MagneticField",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/trbb-ff59",
"STEREO-A In-Situ Measurements of Particles and CME Transients (IMPACT) Fluxgate Magnetometer (MAG) Magnetic Field Vectors, in Radial-Tangential-Normal (RTN) Coordinates, Level Beacon (LB), PT0.125S Data",
"",
"Please acknowledge the Principal Investigator J.G. Luhmann for use of the Data",
"PT0.125S",
"2014-08-01T00:00:00.000",
"2015-11-30T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-A/PLASTIC/LB/Browse/PT1M",
"spase://SMWG/Instrument/STEREO-A/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"PLASTIC Beacon data has not been validated and should not be used for publication purposes",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/xbf2-ga61",
"STEREO-A Plasma and Supra-Thermal Ion Composition (PLASTIC) Beacon Browse Data",
"",
"A.B. Galvin, Please acknowledge the Principal Investigator, Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132 See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"PT1M",
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"2.6.0"
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[
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"spase://SMWG/Instrument/STEREO-B/Ephemeris",
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"https://doi.org/10.48322/ebxv-sx24",
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"",
"Please acknowledge J.G. Luhmann, A.B. Galvin, and C.T. Russell for providing the IMPACT and PLASTIC data used to generate the STEREO-A and STEREO-B COHOWeb data products and the Principal Investigator N.E. Papitashvili for use of the COHOWeb Data",
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"2014-09-27T16:00:00.000",
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"Level 1",
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"",
"2024-07-02T00:00:00",
"https://doi.org/10.48322/ar6g-kf51",
"STEREO-B IMPACT HET Level 1 Data",
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"Please acknowledge the STEREO IMPACT PI, Janet Luhmann of UCB, and NASA Space Physics Data Facility (SPDF)",
"PT1M",
"2006-12-01T00:00:08",
"2014-09-27T16:28:26",
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[
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"spase://SMWG/Instrument/STEREO-B/IMPACT/STE",
"spase://SMWG/Instrument/STEREO-B/IMPACT/SWEA",
"spase://SMWG/Instrument/STEREO-B/IMPACT",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"spase://SMWG/Instrument/STEREO-B/SWAVES"
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"MagneticField",
"ThermalPlasma"
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"https://doi.org/10.48322/5yvh-ye26",
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[
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"https://doi.org/10.48322/b6qg-8460",
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"2006-10-28T00:00:00.000",
"2014-09-27T23:59:59.999",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/d7cp-tn07",
"STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Low Energy Telescope (LET) 1-min Level 1 Ion Fluxes",
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"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT1M",
"2006-11-14T00:00:00",
"",
"",
"2.6.0"
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[
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"",
"Please acknowledge the STEREO IMPACT Principal Investigator J.G. Luhmann for use of the Data and the key IMPACT Magnetometer personnel: C.W. Smith and the late M.H. Acuna.",
"PT0.031S",
"2006-11-07T00:58:50.000",
"2013-01-08T16:20:28.000",
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"",
"Please acknowledge the STEREO IMPACT Principal Investigator J.G. Luhmann for use of the Data and the key IMPACT Magnetometer personnel: C.W. Smith and the late M.H. Acuna.",
"PT0.031S",
"2006-11-07T00:58:50.000",
"2013-01-08T16:20:28.000",
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"2023-07-30T12:34:56.789",
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"STEREO-B IMPACT/MAG Level 1 Data",
"The STEREO IMPACT/MAG Team",
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"",
"",
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"J. Luhmann",
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"2014-09-27T23:59:59.999",
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"spase://SMWG/Instrument/STEREO-B/IMPACT/SEPT",
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"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/y2fy-vb66",
"STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Solar Electron Proton Telescope (SEPT) 1-min Level 1 Electron and Proton Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT1M",
"2006-11-13T00:00:00",
"",
"",
"2.6.0"
],
[
"STB_L1_SIT",
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"spase://SMWG/Instrument/STEREO-B/IMPACT/SIT",
"EnergeticParticles",
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/5xz1-cj09",
"STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Suprathermal Ion Telescope (SIT)1-min Level 1 Multi-Z Ion Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT1M",
"2007-03-15T00:00:00",
"",
"",
"2.6.0"
],
[
"STB_L1_STE",
"spase://NASA/NumericalData/STEREO-B/IMPACT/STE/L1/PT10S",
"spase://SMWG/Instrument/STEREO-B/IMPACT/STE",
"EnergeticParticles",
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"",
"",
"The four sensors labelled \"U\" and numbered 1-4 are saturated and should not be used. Sensors providing usable data are labelled \"D\" and are numbered 5-8.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/zpas-wt14",
"STEREO-B IMPACT (In-Situ Measurements of Particles and CME Transients) Suprathermal Electron Telescope (STE) 10-s Level 1 Electron Spectra",
"",
"Please acknowledge the IMPACT P.I., Janet Luhmann of UCB",
"PT10S",
"2006-11-01T00:00:00",
"2009-05-14T00:00:00",
"This may be extended",
"2.6.0"
],
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"spase://SMWG/Instrument/STEREO-B/IMPACT/SWEA",
[
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"EnergeticParticles",
"InstrumentStatus"
],
"Heliosphere.Remote1AU",
"",
"",
"Since commissioning, the SWEA instruments on both STEREO spacecraft have registered difficult to characterize degradations in the solar wind core electron energies, probably due to charging effects. The nature of the degradations are such that the data are not reliable for electron measurements below 45 eV. However, halo and higher energy electrons are unaffected. Versions 4 and higher of the SWEA 3D distribution data products have these lower energies removed. Similarly, Versions 4 and higher of the SWEA pitch angle distribution products also remove these energies. Use of the SWEA pitch angle distributions for most purposes, for example, higher energy heat flux pitch angle distribbutions, PADs, should be largely unaffected. For more information regarding these issues, please contact Peter Schroeder, peters@ssl.berkeley.edu. If you have downloaded Version 3 or earlier Files, those files contain unreliable data below 45 eV and should be replaced with Version 4 files. Note that if the interpretation of these data become a significant focus in your work, you should obtain explicit prior permission from the PI of the experiment before publication.",
"",
"2023-07-31T12:34:56.789",
"https://doi.org/10.48322/9n2r-ch29",
"STEREO-B In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) 3-Dimensional Electron Distributions, Burst Mode, Level 1 (L1), 2 s Data",
"",
"Please acknowledge the Principal Investigator J.G. Luhmann for use of the Data",
"PT2S",
"2006-10-28T20:05:11.000",
"2014-02-26T22:51:47.000",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/L1/PT30S",
"spase://SMWG/Instrument/STEREO-B/IMPACT/SWEA",
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus"
],
"Heliosphere.Remote1AU",
"",
"",
"Since commissioning, the SWEA instruments on both STEREO spacecraft have registered difficult to characterize degradations in the solar wind core electron energies, probably due to charging effects. The nature of the degradations are such that the data are not reliable for electron measurements below 45 eV. However, halo and higher energy electrons are unaffected. Versions 4 and higher of the SWEA 3D distribution data products have these lower energies removed. Similarly, Versions 4 and higher of the SWEA pitch angle distribution products also remove these energies. Use of the SWEA pitch angle distributions for most purposes, for example, higher energy heat flux pitch angle distribbutions, PADs, should be largely unaffected. For more information regarding these issues, please contact Peter Schroeder, peters@ssl.berkeley.edu. If you have downloaded Version 3 or earlier Files, those files contain unreliable data below 45 eV and should be replaced with Version 4 files. Note that if the interpretation of these data become a significant focus in your work, you should obtain explicit prior permission from the PI of the experiment before publication.",
"",
"2023-07-31T12:34:56.789",
"https://doi.org/10.48322/qxwm-ja11",
"STEREO-B In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) 3-Dimensional Electron Distributions, Level 1 (L1), 30 s Data",
"",
"Please acknowledge the Principal Investigator J.G. Luhmann for use of the Data",
"PT30S",
"2006-10-28T20:05:49.000",
"2014-09-27T16:30:41.000",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/Spectra/L1/PT10S",
"spase://SMWG/Instrument/STEREO-B/IMPACT/SWEA",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/6pf0-rj33",
"STEREO-B In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) Spectra",
"",
"J. Luhmann",
"PT10S",
"2012-12-01T00:00:00.000",
"2013-12-31T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO-B/MAGPLASMA/L2/PT1M",
[
"spase://SMWG/Instrument/STEREO-B/Ephemeris",
"spase://SMWG/Instrument/STEREO-B/IMPACT",
"spase://SMWG/Instrument/STEREO-B/PLASTIC"
],
[
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"ThermalPlasma"
],
"Heliosphere.Remote1AU",
"",
"Level 2",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/qhr7-rz23",
"STEREO-B In-Situ Measurements of Particles and CME Transients from the Magnetometer and the Plasma and Suprathermal Ion and Composition Instruments (IMPACT/MAG, PLASTIC) Solar Wind Plasma Data",
"",
"J. Luhmann",
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"2006-01-01T00:00:00.000",
"2014-01-01T23:59:59.999",
"",
"2.6.0"
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[
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"spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT10M",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/fz6m-r327",
"STEREO-B Plasma and Suprathermal Ion Composition (PLASTIC) 10-min Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1H",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
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[
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"spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT1H",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/68d1-dm95",
"STEREO-B Plasma and Suprathermal Ion Composition (PLASTIC) 1-hour Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1H",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
],
[
"STB_L2_PLA_1DMAX_1MIN",
"spase://NASA/NumericalData/STEREO-B/PLASTIC/Protons/PT1M",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/jvzd-xj39",
"STEREO-B Plasma and Suprathermal Ion Composition (PLASTIC) 1-min Proton Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT1M",
"2007-02-14T00:00:00",
"",
"",
"2.6.0"
],
[
"STB_L2_PLA_IRON_Q_2HR",
"spase://NASA/NumericalData/STEREO-B/PLASTIC/Fe-abundance/PT2H",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/zvvy-0f37",
"STEREO-B Plasma and Suprathermal Ion Composition (PLASTIC) 2-hour Iron Plasma Parameters",
"",
"Please acknowledge STEREO PLASTIC Investigation (A.B. Galvin, PI) and NASA Contract NAS5-00132.",
"PT2H",
"2007-01-01T00:00:00",
"",
"",
"2.6.0"
],
[
"STB_L2_SWEA_PAD",
"spase://NASA/NumericalData/STEREO-B/IMPACT/SWEA/PAD/L2/PT30S",
"spase://SMWG/Instrument/STEREO-B/IMPACT/SWEA",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"Level 2",
"",
"",
"2025-09-18T12:12:34Z",
"https://doi.org/10.48322/spcw-2b07",
"STEREO-B In-Situ Measurements of Particles and CME Transients (IMPACT) Solar Wind Electron Analyzer (SWEA) Pitch Angle Distribution, Level 2 (L2), 30 s Data in CDF format",
"",
"Please acknowledge the Principal Investigator J. Luhmann for use of the Data",
"PT30S",
"2006-11-06T00:00:14",
"2014-09-27T16:30:41",
"",
"2.7.0"
],
[
"STB_L3_WAV_LFR",
"spase://NASA/NumericalData/STEREO-B/SWAVES/stb_l3_wav_lfr/PT15S",
"spase://SMWG/Instrument/STEREO-B/SWAVES",
[
"ElectricField",
"Waves"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2025-09-18T12:12:35Z",
"https://doi.org/10.48322/fpgg-t127",
"STEREO-B/WAVES Low Frequency Receiver, Data",
"",
"Please acknowledge the STEREO/Waves team. Data provided are Publicly available. If used in presentations or publications, please acknowledge STEREO/Waves Investigation (M. Maksimovic and S. D. Bale, PIs). Please read carefully the caveats attached to the data. For reporting purposes, we request bibliography information for any publication, etc., using these data. Please send information on the use of this data to M. Maksimovic and S. D. Bale (PIs).",
"PT15S",
"2006-10-28T00:00:00.000",
"",
"",
"2.7.0"
],
[
"STB_LB_IMPACT",
"spase://NASA/NumericalData/STEREO-B/IMPACT/LB/PT1M",
"spase://SMWG/Instrument/STEREO-B/IMPACT",
[
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"MagneticField"
],
"Heliosphere.Remote1AU",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/14sd-tb45",
"STEREO-B In-Situ Measurements of Particles and CME Transients (IMPACT) Beacon",
"",
"J. Luhmann",
"PT1M",
"2007-03-20T16:50:35",
"2014-09-27T23:59:59.999",
"",
"2.6.0"
],
[
"STB_LB_PLA_BROWSE",
"spase://NASA/NumericalData/STEREO-B/PLASTIC/LB/Browse/PT1M",
"spase://SMWG/Instrument/STEREO-B/PLASTIC",
"ThermalPlasma",
"Heliosphere.Remote1AU",
"",
"",
"PLASTIC Beacon data has not been validated and should not be used for publication purposes",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/8tpm-vt97",
"STEREO-B Plasma and Supra-Thermal Ion Composition (PLASTIC) Beacon Browse Data",
"",
"A.B. Galvin, Please acknowledge the Principal Investigator, Antoinette Galvin of the University of New Hampshire, and NASA contract NAS5-00132 See the rules of use available at http://stereo.sr.unh.edu/data/PLASTIC_Resources/index.htm.",
"PT1M",
"2011-07-07T00:00:00.000",
"2014-09-26T23:59:59.999",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/STEREO/SWAVES/DS/Combined/PT1M",
[
"spase://SMWG/Instrument/STEREO-A/SWAVES",
"spase://SMWG/Instrument/STEREO-B/SWAVES"
],
[
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"Spectrum"
],
[
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"Heliosphere.Inner",
"Jupiter"
],
"",
"",
"",
[
"Dynamic Spectrogram",
"Spectrogram",
"Solar radio burst",
"Type II Solar radio burst",
"Type III Solar radio burst",
"Jupiter DAM",
"Jovian Decametric Radiation"
],
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/6ra3-pg21",
"STEREO WAVES (SWAVES) Radio Intensity Spectra, both Ahead and Behind s/c",
[
"STEREO_LEVEL2_SWAVES",
"Solar TErrestrial RElations Observatory (STEREO) Waves (SWAVES) STEREO-A and STEREO-B Level 2 CDFs at NASA's CDAWeb"
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"THEMIS-B (P1/ARTEMIS-P1) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature",
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"V. Angelopoulos, C.W. Carlson, J. McFadden, NASA Contract NAS5-02099. Open Data for Scientific Use.",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/kyn5-0772",
"ARTEMIS P1 field-plasma merged data, near moon",
"THEMIS-B field-plasma merged data, near moon",
"Please acknowledge Vassilis Angelopoulos, THEMIS mission Principal Investigator, Charles.W.Carlson and Karl-Heinz.Glassmeier, Co-Investigators for ESA and FGM respectively, and Natalia Papitashvili at GSFC/SPDF",
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"Due to bit errors and data misdirection, ESA data (including moments) before April 27, 2007 should be considered dubious. Other data loss and formatting errors in the moments calculations and the ETC were not corrected until Aug. 6, 2007. Potential data from the EFI was not properly included in calculations between Nov. 18-22, 2007. EFI booms on THEMIS-B were not deployed until Nov 17, 2008, 06:00:00 UT. Moments data before this date is suspect to error from photoelectrons and spacecraft charging.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/2z69-n961",
"THEMIS-B: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature.",
"THEMIS-B MOM",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, C.W. Carlson, and J. McFadden.",
"PT3S",
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"Earth.Magnetosphere.Magnetotail",
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"Level 2",
"See THEMIS website for caveats",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/rwch-kk19",
"THEMIS-B: Search Coil Magnetometer 1/8s, 1/128s and 1/8192s Data",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission; also A. Roux and CETP for their work on the SCM.",
"PT0.125S",
"2007-02-24T00:00:00Z",
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"spase://SMWG/Instrument/THEMIS/B/SST",
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"EnergeticParticles",
"Spectrum"
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"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
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"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
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"",
"Level 2",
"Calibration for the SST is not complete. Currently there are no corrections for the dead layer. Other data products will be added later as calibration continues. Total list of expected data types can be found on the THEMIS website.",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/gmq5-6h27",
"THEMIS-B: Solid State Telescope (SST): Energy flux spectrogram, electron/ion ground-calculated fluxes (30 keV - 300 keV).",
"THEMIS-B SST",
"NASA Contract NAS5-02099",
"PT3S",
"2007-03-14T01:00:00",
"",
"",
"2.7.0"
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"spase://SMWG/Instrument/THEMIS/B/Ephemeris",
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"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
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"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-08-05T13:12:33Z",
"https://doi.org/10.48322/hycc-em64",
"THEMIS-B (P1/ARTEMIS-P1) Orbit (Ephemeris)",
"",
"V. Angelopoulos",
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"2007-02-18T00:14:00",
"2017-05-01T23:59:59.999",
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],
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"spase://SMWG/Instrument/THEMIS/C/Ephemeris",
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"Earth.Magnetosphere.Magnetotail",
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"",
"Level 1",
"Typical cadence is 1 min, occasionally 3s.",
"",
"2021-04-27T15:38:11Z",
"",
"THEMIS-C Level 1 Probe State Data",
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"NASA Contract NAS5-02099",
"PT01M",
"2007-02-17T23:35:58",
"",
"",
"2.3.2"
],
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"spase://NASA/NumericalData/THEMIS/C/EFI/PT3S",
"spase://SMWG/Instrument/THEMIS/C/EFI",
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"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
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"Level 2",
"Measurements on the Axial booms, 5 and 6, may have large Errors due to their Proximity to the Spacecraft as the Axial Booms are much shorter than other Booms. The Spin Plane Booms for THEMIS were not deployed until January 14, 2008 at 1700 UT. Any EFI Measurements obtained prior to this Date and Time should not be used. See the THEMIS Website for more Information.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/gmr7-8198",
"THEMIS-C (P2/ARTEMIS-P2), Electric Field Instrument (EFI) Spacecraft measured Electric Field",
"",
"V. Angelopoulos, J. Bonnell, F. Mozer, NASA Contract NAS5-02099. Open Data for Scientific Use.",
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"2017-06-01T23:59:59.999",
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"Level 2",
"EFI booms for THEMIS C(P2) were deployed on 2007-05-16/21:00:00 UT. Before this time the spacecraft potential was not calculated accurately. Electron moments will not be distributed prior to this date and ion moments will less accurate. See THEMIS website for caveats(http://themis.ssl.berkeley.edu)",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/scc7-mj94",
"THEMIS-C: ESA electron/ion energy fluxes and moments",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: C. W. Carlson and J. P. McFadden for use of ESA data.",
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"2007-02-16T00:00:00",
"",
"",
"2.6.0"
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[
"spase://SMWG/Instrument/THEMIS/C/EFI",
"spase://SMWG/Instrument/THEMIS/C/SCM"
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[
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"MagneticField",
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"Heliosphere.NearEarth",
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"Earth.Magnetosphere.Magnetotail",
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],
"",
"",
"",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/ken1-sn21",
"THEMIS-C: Probe Electric Field Instrument and Search Coil Magnetometer Instrument, Digital Fields Board - digitally computed Filter Bank spectra and E12 peak and average in HF band (FBK).",
"",
"NASA Contract NAS5-02099",
"PT4S",
"2007-02-24T00:00:01",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/C/FFT/PT0.0556S",
[
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"spase://SMWG/Instrument/THEMIS/C/SCM"
],
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"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
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"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
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"Heliosphere.NearEarth"
],
"",
"",
"Data product cadence varies between 1/16 and 1/18 seconds.",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/mb5w-e618",
"THEMIS-C: On Board Fast Fourier Transform (FFT) power spectra of Electric (EFI) and Magnetic (SCM) field measurements, for particle and wave burst survey modes.",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, also John Bonnell, Michael Cully, Bob Ergun, and Alain Roux for their work on the FFT and related systems.",
"PT0.0556S",
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"Level 2",
"The THEMIS mission uses the coordinate name \" DSL\" for the coordinate system that is called \"SR2\" is the SPASE data model. See THEMIS website for caveats.",
"",
"2021-04-30T20:06:51Z",
"",
"THEMIS-C: Fluxgate Magnetometer Measurements 1/128s",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission, K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302",
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"2007-02-16T00:00:00Z",
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"",
"2.3.2"
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[
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"spase://SMWG/Instrument/THEMIS/C/FGM"
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"The electric field spin plane booms for THEMIS C were not deployed until May 16, 2007 at 2100 UT, any EFI measurements before this date should not be used.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/jg03-4q46",
"THEMIS-C: On Board spin fits (FIT) of Electric (EFI) and Magnetic (FGM) field. On-Board Spin-fit electric and magnetic field data",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: J. W. Bonnell and F. S. Mozer for use of EFI data.",
"PT3S",
"2008-01-14T17:00:00",
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"",
"2.6.0"
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[
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"spase://SMWG/Instrument/THEMIS/C/SST"
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"ThermalPlasma"
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"Level 2",
"See THEMIS Website for Caveats",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/svt8-nb52",
"THEMIS-C (P2/ARTEMIS-P2) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature",
"",
"V. Angelopoulos, C.W. Carlson, J. McFadden, NASA Contract NAS5-02099. Open Data for Scientific Use.",
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"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/szem-vt65",
"ARTEMIS P2 field-plasma merged data, near moon",
"THEMIS-C field-plasma merged data, near moon",
"Please acknowledge Vassilis Angelopoulos, THEMIS mission Principal Investigator, Charles.W.Carlson and Karl-Heinz.Glassmeier, Co-Investigators for ESA and FGM respectively, and Natalia Papitashvili at GSFC/SPDF",
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"EnergeticParticles",
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"Level 2",
"Due to bit errors and data misdirection, ESA data (including moments) before April 27, 2007 should be considered dubious. Other data loss and formatting errors in the moments calculations and the ETC were not corrected until Aug. 6, 2007. Potential data from the EFI was not properly included in calculations between Nov. 18-22, 2007. EFI booms on THEMIS-C were not deployed until May 16, 2007, 21:00:00 UT. Moments data before this date is suspect to error from photoelectrons and spacecraft charging.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/y91r-j665",
"THEMIS-C: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature.",
"THEMIS-C MOM",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, C.W. Carlson, and J. McFadden.",
"PT3S",
"2007-08-10T00:00:32",
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"",
"2.6.0"
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"Earth.Magnetosphere.Magnetotail",
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"Level 2",
"See THEMIS website for caveats",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/dw9h-k139",
"THEMIS-C: Search Coil Magnetometer 1/8s, 1/128s and 1/8192s Data",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission; also A. Roux and CETP for their work on the SCM.",
"PT0.125S",
"2007-02-24T00:00:00Z",
"",
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"Heliosphere.NearEarth"
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"Level 2",
"Calibration for the SST is not complete. Currently there are no corrections for the dead layer. Other data products will be added later as calibration continues. Total list of expected data types can be found on the THEMIS website.",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/hj63-0x15",
"THEMIS-C: Solid State Telescope (SST): Energy flux spectrogram, electron/ion ground-calculated fluxes (30 keV - 300 keV).",
"THEMIS-C SST",
"NASA Contract NAS5-02099",
"PT3S",
"2007-03-14T01:00:00",
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"",
"2.7.0"
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"Heliosphere.NearEarth",
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"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
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"",
"",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/tyjx-5g19",
"THEMIS-C (P2/ARTEMIS-P2) Orbit (Ephemeris)",
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"V. Angelopoulos",
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"2007-02-18T00:14:00",
"2017-05-01T23:59:59.999",
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"spase://SMWG/Instrument/THEMIS/D/Ephemeris",
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"",
"2021-04-27T15:38:11Z",
"",
"THEMIS-D Level 1 Probe State Data",
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"NASA Contract NAS5-02099",
"PT01M",
"2007-02-17T23:35:58",
"",
"",
"2.3.2"
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[
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"Earth.Magnetosphere.Main",
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],
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"Level 2",
"Measurements on the Axial booms, 5 and 6, may have large Errors due to their Proximity to the Spacecraft as the Axial Booms are much shorter than other Booms. The Spin Plane Booms for THEMIS were not deployed until January 14, 2008 at 1700 UT. Any EFI Measurements obtained prior to this Date and Time should not be used. See the THEMIS Website for more Information.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/5bb0-by57",
"THEMIS-D (P3), Electric Field Instrument (EFI) Spacecraft measured Electric Field",
"",
"V. Angelopoulos, J. Bonnell, F. Mozer, NASA Contract NAS5-02099. Open Data for Scientific Use.",
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"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 2",
"See THEMIS website for caveats(http://themis.ssl.berkeley.edu) EFI booms for THEMIS D(P3) were deployed on 2007-06-07/17:00:00 UT. Before this time the spacecraft potential was not calculated accurately. Electron moments will not be distributed prior to this date and ion moments will less accurate.",
"",
"2025-09-15T12:34:56.789",
"https://doi.org/10.48322/05m2-0k28",
"THEMIS-D: ESA electron/ion energy fluxes and moments",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: C. W. Carlson and J. P. McFadden for use of ESA data.",
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"2007-02-16T00:00:00",
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[
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[
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"spase://SMWG/Instrument/THEMIS/D/SCM"
],
[
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"MagneticField",
"Spectrum"
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[
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"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
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"",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/dj1x-mv94",
"THEMIS-D: Probe Electric Field Instrument and Search Coil Magnetometer Instrument, Digital Fields Board - digitally computed Filter Bank spectra and E12 peak and average in HF band (FBK).",
"",
"NASA Contract NAS5-02099",
"PT4S",
"2007-02-24T00:00:01",
"",
"",
"2.7.0"
],
[
"THD_L2_FFT",
"spase://NASA/NumericalData/THEMIS/D/FFT/PT0.0556S",
[
"spase://SMWG/Instrument/THEMIS/D/EFI",
"spase://SMWG/Instrument/THEMIS/D/SCM"
],
"Spectrum",
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"Data product cadence varies between 1/16 and 1/18 seconds.",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/jj19-0q58",
"THEMIS-D: On Board Fast Fourier Transform (FFT) power spectra of Electric (EFI) and Magnetic (SCM) field measurements, for particle and wave burst survey modes.",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, also John Bonnell, Michael Cully, Bob Ergun, and Alain Roux for their work on the FFT and related systems.",
"PT0.0556S",
"2007-02-24T00:00:00Z",
"",
"",
"2.7.0"
],
[
"THD_L2_FGM",
"spase://DLR/NumericalData/THEMIS/D/FGM/PT0.0078125S",
"spase://SMWG/Instrument/THEMIS/D/FGM",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"The THEMIS mission uses the coordinate name \" DSL\" for the coordinate system that is called \"SR2\" is the SPASE data model. See THEMIS website for caveats.",
"",
"2021-04-27T17:51:13Z",
"",
"THEMIS-D: Fluxgate Magnetometer Measurements 1/128s",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission, K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302",
"",
"2007-02-16T00:00:00Z",
"",
"",
"2.3.2"
],
[
"THD_L2_FIT",
"spase://NASA/NumericalData/THEMIS/D/Fits/PT3S",
[
"spase://SMWG/Instrument/THEMIS/D/EFI",
"spase://SMWG/Instrument/THEMIS/D/FGM"
],
[
"ElectricField",
"MagneticField"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 2",
"The electric field spin plane booms for THEMIS D were not deployed until June 07, 2007 at 1700 UT, any EFI measurements before this date should not be used.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/2acz-ef84",
"THEMIS-D: On Board spin fits (FIT) of Electric (EFI) and Magnetic (FGM) field. On-Board Spin-fit electric and magnetic field data",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: J. W. Bonnell and F. S. Mozer for use of EFI data.",
"PT3S",
"2008-01-14T17:00:00",
"",
"",
"2.6.0"
],
[
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"spase://NASA/NumericalData/THEMIS/D/GMOM/PT3S",
[
"spase://SMWG/Instrument/THEMIS/D/ESA",
"spase://SMWG/Instrument/THEMIS/D/SST"
],
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus",
"MagneticField",
"ThermalPlasma"
],
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"See THEMIS Website for Caveats",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/2j4s-8p65",
"THEMIS-D (P3) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature",
"",
"V. Angelopoulos, C.W. Carlson, J. McFadden, NASA Contract NAS5-02099. Open Data for Scientific Use.",
"PT3S",
"2007-03-09T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THD_L2_MOM",
"spase://NASA/NumericalData/THEMIS/D/MOM/PT3S",
"spase://SMWG/Instrument/THEMIS/D/MOM",
[
"ThermalPlasma",
"EnergeticParticles",
"IonComposition"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"Due to bit errors and data misdirection, ESA data (including moments) before April 27, 2007 should be considered dubious. Other data loss and formatting errors in the moments calculations and the ETC were not corrected until Aug. 6, 2007. Potential data from the EFI was not properly included in calculations between Nov. 18-22, 2007. EFI booms on THEMIS-D were not deployed until June 7, 2007, 17:00:00 UT. Moments data before this date is suspect to error from photoelectrons and spacecraft charging.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/ryqr-m277",
"THEMIS-D: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature.",
"THEMIS-D MOM",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, C.W. Carlson, and J. McFadden.",
"PT3S",
"2007-08-09T23:59:56",
"",
"",
"2.6.0"
],
[
"THD_L2_SCM",
"spase://NASA/NumericalData/THEMIS/D/SCM/PT0.125S",
"spase://SMWG/Instrument/THEMIS/D/SCM",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"See THEMIS website for caveats",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/m5dr-nh16",
"THEMIS-D: Search Coil Magnetometer 1/8s, 1/128s and 1/8192s Data",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission; also A. Roux and CETP for their work on the SCM.",
"PT0.125S",
"2007-02-24T00:00:00Z",
"",
"",
"2.6.0"
],
[
"THD_L2_SST",
"spase://NASA/NumericalData/THEMIS/D/SST/PT3S",
"spase://SMWG/Instrument/THEMIS/D/SST",
[
"IonComposition",
"EnergeticParticles",
"Spectrum"
],
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"Calibration for the SST is not complete. Currently there are no corrections for the dead layer. Other data products will be added later as calibration continues. Total list of expected data types can be found on the THEMIS website.",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/7fcg-ej20",
"THEMIS-D: Solid State Telescope (SST): Energy flux spectrogram, electron/ion ground-calculated fluxes (30 keV - 300 keV).",
"THEMIS-D SST",
"NASA Contract NAS5-02099",
"PT3S",
"2007-03-14T01:00:00",
"",
"",
"2.7.0"
],
[
"THD_OR_SSC",
"spase://NASA/NumericalData/THEMIS/D/Ephemeris/SSCWeb/PT1M",
"spase://SMWG/Instrument/THEMIS/D/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-08-05T13:12:34Z",
"https://doi.org/10.48322/nf5n-ew50",
"THEMIS-D (P3) Orbit (Ephemeris)",
"",
"V. Angelopoulos",
"PT1M",
"2007-02-18T00:14:00",
"2017-05-01T23:59:59.999",
"",
"2.7.0"
],
[
"THE_L1_STATE",
"spase://NASA/NumericalData/THEMIS/E/Ephemeris/PT01M",
"spase://SMWG/Instrument/THEMIS/E/Ephemeris",
"Ephemeris",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 1",
"Typical cadence is 1 min, occasionally 3s.",
"",
"2021-04-27T15:38:11Z",
"",
"THEMIS-E Level 1 Probe State Data",
"",
"NASA Contract NAS5-02099",
"PT01M",
"2007-02-17T23:35:58",
"",
"",
"2.3.2"
],
[
"THE_L2_EFI",
"spase://NASA/NumericalData/THEMIS/E/EFI/PT3S",
"spase://SMWG/Instrument/THEMIS/E/EFI",
"ElectricField",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"Measurements on the Axial booms, 5 and 6, may have large Errors due to their Proximity to the Spacecraft as the Axial Booms are much shorter than other Booms. The Spin Plane Booms for THEMIS were not deployed until January 14, 2008 at 1700 UT. Any EFI Measurements obtained prior to this Date and Time should not be used. See the THEMIS Website for more Information.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/vd0m-3766",
"THEMIS-E (P4), Electric Field Instrument (EFI) Spacecraft measured Electric Field",
"",
"V. Angelopoulos, J. Bonnell, F. Mozer, NASA Contract NAS5-02099. Open Data for Scientific Use.",
"PT3S",
"2007-02-24T00:00:00.000",
"",
"",
"2.6.0"
],
[
"THE_L2_ESA",
"spase://NASA/NumericalData/THEMIS/E/ESA/PT3S",
"spase://SMWG/Instrument/THEMIS/E/ESA",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 2",
"See THEMIS website for caveats(http://themis.ssl.berkeley.edu). EFI booms for THEMIS E(P4) were deployed on 2007-06-07/19:00:00 UT. Before this time the spacecraft potential was not calculated accurately. Electron moments will not be distributed prior to this date and ion moments will less accurate.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/ma73-rz55",
"THEMIS-E: ESA electron/ion energy fluxes and moments",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: C. W. Carlson and J. P. McFadden for use of ESA data.",
"",
"2007-02-16T00:00:00",
"",
"",
"2.6.0"
],
[
"THE_L2_FBK",
"spase://NASA/NumericalData/THEMIS/E/FBK/PT4S",
[
"spase://SMWG/Instrument/THEMIS/E/EFI",
"spase://SMWG/Instrument/THEMIS/E/SCM"
],
[
"ElectricField",
"MagneticField",
"Spectrum"
],
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/x1a6-8d82",
"THEMIS-E: Probe Electric Field Instrument and Search Coil Magnetometer Instrument, Digital Fields Board - digitally computed Filter Bank spectra and E12 peak and average in HF band (FBK).",
"",
"NASA Contract NAS5-02099",
"PT4S",
"2007-02-24T00:00:01",
"",
"",
"2.7.0"
],
[
"THE_L2_FFT",
"spase://NASA/NumericalData/THEMIS/E/FFT/PT0.0556S",
[
"spase://SMWG/Instrument/THEMIS/E/EFI",
"spase://SMWG/Instrument/THEMIS/E/SCM"
],
"Spectrum",
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"Data product cadence varies between 1/16 and 1/18 seconds.",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/424d-q741",
"THEMIS-E: On Board Fast Fourier Transform (FFT) power spectra of Electric (EFI) and Magnetic (SCM) field measurements, for particle and wave burst survey modes.",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, also John Bonnell, Michael Cully, Bob Ergun, and Alain Roux for their work on the FFT and related systems.",
"PT0.0556S",
"2007-02-24T00:00:00Z",
"",
"",
"2.7.0"
],
[
"THE_L2_FGM",
"spase://DLR/NumericalData/THEMIS/E/FGM/PT0.0078125S",
"spase://SMWG/Instrument/THEMIS/E/FGM",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"The THEMIS mission uses the coordinate name \" DSL\" for the coordinate system that is called \"SR2\" is the SPASE data model. See THEMIS website for caveats.",
"",
"2021-04-27T17:51:13Z",
"",
"THEMIS-E: Fluxgate Magnetometer Measurements 1/128s",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission, K. H. Glassmeier, U. Auster and W. Baumjohann for the use of FGM data provided under the lead of the Technical University of Braunschweig and with financial support through the German Ministry for Economy and Technology and the German Center for Aviation and Space (DLR) under contract 50 OC 0302",
"",
"2007-02-16T00:00:00Z",
"",
"",
"2.3.2"
],
[
"THE_L2_FIT",
"spase://NASA/NumericalData/THEMIS/E/Fits/PT3S",
[
"spase://SMWG/Instrument/THEMIS/E/EFI",
"spase://SMWG/Instrument/THEMIS/E/FGM"
],
[
"ElectricField",
"MagneticField"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.RadiationBelt"
],
"",
"Level 2",
"The electric field spin plane booms for THEMIS E were not deployed until June 07, 2007 at 1900 UT, any EFI measurements before this date should not be used.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/5g5k-ry70",
"THEMIS-E: On Board spin fits (FIT) of Electric (EFI) and Magnetic (FGM) field. On-Board Spin-fit electric and magnetic field data",
"",
"NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically: J. W. Bonnell and F. S. Mozer for use of EFI data.",
"PT3S",
"2008-01-14T17:00:00",
"",
"",
"2.6.0"
],
[
"THE_L2_GMOM",
"spase://NASA/NumericalData/THEMIS/E/GMOM/PT3S",
[
"spase://SMWG/Instrument/THEMIS/E/ESA",
"spase://SMWG/Instrument/THEMIS/E/SST"
],
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus",
"MagneticField",
"ThermalPlasma"
],
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"See THEMIS Website for Caveats",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/h36y-ta68",
"THEMIS-E (P4) Electron and Ion Moments (GMOM) Ground-Calculated Particle Energy Fluxes and Moments: Density, Velocity, Pressure and Temperature",
"",
"V. Angelopoulos, C.W. Carlson, J. McFadden, NASA Contract NAS5-02099. Open Data for Scientific Use.",
"PT3S",
"2007-03-09T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THE_L2_MOM",
"spase://NASA/NumericalData/THEMIS/E/MOM/PT3S",
"spase://SMWG/Instrument/THEMIS/E/MOM",
[
"ThermalPlasma",
"EnergeticParticles",
"IonComposition"
],
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"Due to bit errors and data misdirection, ESA data (including moments) before April 27, 2007 should be considered dubious. Other data loss and formatting errors in the moments calculations and the ETC were not corrected until Aug. 6, 2007. Potential data from the EFI was not properly included in calculations between Nov. 18-22, 2007. EFI booms on THEMIS-E were not deployed until June 7, 2007, 19:00:00 UT. Moments data before this date is suspect to error from photoelectrons and spacecraft charging.",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/x7y9-hx44",
"THEMIS-E: On Board moments: ESA and SST Electron/Ion moments, density, flux, velocity, pressure and temperature.",
"THEMIS-E MOM",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission, C.W. Carlson, and J. McFadden.",
"PT3S",
"2007-08-10T00:00:16",
"",
"",
"2.6.0"
],
[
"THE_L2_SCM",
"spase://NASA/NumericalData/THEMIS/E/SCM/PT0.125S",
"spase://SMWG/Instrument/THEMIS/E/SCM",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosheath"
],
"",
"Level 2",
"See THEMIS website for caveats",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/bbh4-cv70",
"THEMIS-E: Search Coil Magnetometer 1/8s, 1/128s and 1/8192s Data",
"",
"NASA Contract NAS5-02099, V. Angelopoulos for use of data from the THEMIS Mission; also A. Roux and CETP for their work on the SCM.",
"PT0.125S",
"2007-02-24T00:00:00Z",
"",
"",
"2.6.0"
],
[
"THE_L2_SST",
"spase://NASA/NumericalData/THEMIS/E/SST/PT3S",
"spase://SMWG/Instrument/THEMIS/E/SST",
[
"IonComposition",
"EnergeticParticles",
"Spectrum"
],
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"Calibration for the SST is not complete. Currently there are no corrections for the dead layer. Other data products will be added later as calibration continues. Total list of expected data types can be found on the THEMIS website.",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/5xv8-hc40",
"THEMIS-E: Solid State Telescope (SST): Energy flux spectrogram, electron/ion ground-calculated fluxes (30 keV - 300 keV).",
"THEMIS-E SST",
"NASA Contract NAS5-02099",
"PT3S",
"2007-03-14T01:00:00",
"",
"",
"2.7.0"
],
[
"THE_OR_SSC",
"spase://NASA/NumericalData/THEMIS/E/Ephemeris/SSCWeb/PT1M",
"spase://SMWG/Instrument/THEMIS/E/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere.Plasmasphere",
"Earth.Magnetosphere.RadiationBelt",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.Magnetotail",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/srak-qw30",
"THEMIS-E (P4) Orbit (Ephemeris)",
"",
"V. Angelopoulos",
"PT1M",
"2007-02-18T00:14:00",
"2017-05-01T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L1_ASK",
"spase://NASA/NumericalData/THEMIS/Ground/ASK/PT3S",
[
"spase://SMWG/Instrument/THEMIS/Ground/UCLA-GBO/CHBG/ASI",
"spase://SMWG/Instrument/THEMIS/Ground/CANMAG/ATHA/ASI"
],
"ImageIntensity",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:35Z",
"https://doi.org/10.48322/a2pk-b377",
"THEMIS Ground-based All Sky Imager Keogram, Level-1",
"THEMIS-Ground ASK",
"We acknowledge NASA contract NAS5-02099 and V. Angelopoulos for use of data from the THEMIS Mission. Specifically S. Mende and E. Donovan for use of the ASI data, and the CSA for logistical support in fielding and data retrieval from the GBO stations.",
"PT3S",
"2005-01-01T01:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_AKUL",
"spase://NASA/NumericalData/THEMIS/Ground/Akulivik/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Akulivik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/3y2q-2228",
"Akulivik (AKUL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-21T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Amderma/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Amderma/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/9pjw-pc58",
"Amderma (AMD) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2011-07-25T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Americus/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Americus/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/qpwn-6769",
"Americus (AMER) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2006-03-08T00:00:00.000",
"2012-10-22T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Tasiilaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Tasiilaq/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/2h21-ep86",
"Tasiilaq (AMK) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Andenes/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Andenes/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/5wqx-w755",
"Andenes (AND) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Arctic.Village/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Arctic.Village/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/qwjs-gm05",
"Arctic Village (ARCT) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"2009-02-03T22:59:59",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Athabasca/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Athabasca/Magnetometer",
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[
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],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/z960-2d21",
"Athabasca (ATHA) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2008-02-05T00:00:00",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Attu/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Attu/Magnetometer",
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[
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],
"",
"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/fnna-f309",
"Attu (ATU) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Barentsburg/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Barentsburg/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/025w-tb57",
"Barentsburg (BBG) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2017-02-10T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Bennington/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Bennington/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/sph7-yk94",
"Bennington (BENN) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"2015-04-27T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Bettles/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Bettles/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/4c18-7q57",
"Bettles (BETT) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"2011-04-01T22:59:59",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Brorfelde/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Brorfelde/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/acyc-yg85",
"Brorfelde (BFE) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2008-09-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Bjorn/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Bjorn/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/ydyw-hg07",
"Bjornoya (BJN) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Baker.Lake/Magnetometer/PT1S",
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[
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"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/k1db-pw22",
"Baker Lake (BLC) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Bay.Mills/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Bay.Mills/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/0h9h-5536",
"Bay Mills (BMLS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-09-27T20:49:42",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Boulder/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Boulder/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/ad0r-pm72",
"Boulder (BOU) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Baranov/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Baranov/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:36Z",
"https://doi.org/10.48322/9s0q-4927",
"Baranov (BRN) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2017-02-10T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://SMWG/Instrument/Ground/Barrow/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/fa7r-g588",
"Barrow (BRW) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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[
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"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/2gwx-z353",
"NASA Stennis Space Center (BSL) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-12T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Cambridge.Bay/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Cambridge.Bay/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/7t4e-r942",
"Cambridge Bay (CBB) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Carson.City/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Carson.City/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/s8rk-7s97",
"Carson City (CCNV) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2004-07-23T21:38:41",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Cape.Dorset/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Cape.Dorset/Magnetometer",
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[
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],
"",
"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/wzt9-6n82",
"Cape Dorset (CDRT/CDR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2007-01-14T00:00:00",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Chibougamau/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Chibougamau/Magnetometer",
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[
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"Earth.Surface"
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/4h6z-9h23",
"Chibougamau (CHBG) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-09-15T03:10:46",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Coral.Harbour/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Coral.Harbour/Magnetometer",
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[
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"Earth.Surface"
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"Level 2",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/4v7c-qc94",
"Coral Harbour (CHBR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge the Principal Investigator E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2012-07-16T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/College.International.Geophysical.Observatory/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/College/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/wz4n-kj76",
"College (CIGO) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Fairbanks/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/College/Magnetometer",
"MagneticField",
[
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"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/9zr0-g518",
"College (CMO) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Clyde.River/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Clyde.River/Magnetometer",
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[
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/wrwz-fs47",
"Clyde River (CRVR/CRV) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2008-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Dead.Horse/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Dead.Horse/Magnetometer",
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[
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/7hxr-ey55",
"Dead Horse (DED) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2010-03-22T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Dikson/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Dikson/Magnetometer",
"MagneticField",
[
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/7bjs-dn15",
"Dikson (DIK) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2011-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Danmarkshavn/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Danmarkshavn/Magnetometer",
"MagneticField",
[
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/8amt-aa15",
"Danmarkshavn (DMH) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Daneborg/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Daneborg/Magnetometer",
"MagneticField",
[
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"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/1ahm-hm81",
"Daneborg (DNB) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2007-01-01T00:00:00.000",
"2007-01-04T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Dombas/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Dombas/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/x2vb-kq56",
"Dombas (DOB) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
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[
"THG_L2_MAG_DON",
"spase://NASA/NumericalData/THEMIS/Ground/Donna/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Donna/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/5k4p-k337",
"Donna (DON) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2007-11-14T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_DRBY",
"spase://NASA/NumericalData/THEMIS/Ground/Derby/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Derby/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/b47e-ta41",
"Derby (DRBY) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-10-25T13:51:30",
"2014-05-19T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_EAGL",
"spase://NASA/NumericalData/THEMIS/Ground/Eagle/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Eagle/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/vfeb-r152",
"Eagle (EAGL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"2015-09-14T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_EKAT",
"spase://NASA/NumericalData/THEMIS/Ground/Ekati/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Ekati/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/fa8n-0e03",
"Ekati (EKAT) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-01-01T00:00:01",
"2007-09-12T20:58:57",
"",
"2.7.0"
],
[
"THG_L2_MAG_FCC",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.Churchill/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Fort.Churchill/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/48we-mh64",
"Fort Churchill (FCC) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_FHB",
"spase://NASA/NumericalData/THEMIS/Ground/Paamiut/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Paamiut/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/j9m8-3k65",
"Paamiut (FHB) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"Frederikshap Vector Magnetic Field 1.0 min Data",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2009-05-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Corbin/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Fredericksburg/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/1xpx-v270",
"Fredericksburg (FRD) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_FRN",
"spase://NASA/NumericalData/THEMIS/Ground/Fresno/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Fresno/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/ptx0-aw90",
"Fresno (FRN) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Fort.Simpson/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Fort.Simpson/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/x5x8-yz98",
"Fort Simpson (FSIM) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2006-11-01T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_FSJ",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.St.John/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Fort.St.John/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/sawq-yr43",
"Fort St. John (FSJ) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-05-23T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_FSMI",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.Smith/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Fort.Smith/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/hh0a-6414",
"Fort Smith (FSMI) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2006-11-01T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_FTN",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.Nelson/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Fort.Nelson/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/1ph3-gt78",
"Fort Nelson (FTN) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-04-09T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_FYKN",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.Yukon/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Fort.Yukon/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/f2zw-5d69",
"Fort Yukon (FYKN) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT0.5S",
"2006-01-01T01:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_FYTS",
"spase://NASA/NumericalData/THEMIS/Ground/Fort.Yates/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Fort.Yates/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/px5c-kg42",
"Fort Yates (FYTS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-09-02T19:51:45",
"2010-01-10T13:16:19",
"",
"2.7.0"
],
[
"THG_L2_MAG_GAKO",
"spase://NASA/NumericalData/THEMIS/Ground/Gakona/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Gakona/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:40Z",
"https://doi.org/10.48322/1ewb-6655",
"Gakona (GAKO) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2006-01-01T01:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GBAY",
"spase://NASA/NumericalData/THEMIS/Ground/Goose.Bay/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Goose.Bay/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/q12f-vd18",
"Goose Bay (GBAY) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-02-23T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GDH",
"spase://NASA/NumericalData/THEMIS/Ground/Qeqertarsuaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Qeqertarsuaq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/jnvs-4q81",
"Qeqertarsuaq (GDH) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GHB",
"spase://NASA/NumericalData/THEMIS/Ground/Nuuk/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Nuuk/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/jz41-9972",
"Nuuk (GHB) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"Godthap Vector Magnetic Field 1.0 min Data",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2009-05-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GILL",
"spase://NASA/NumericalData/THEMIS/Ground/Gillam/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Gillam/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/9xm5-8c66",
"Gillam (GILL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2006-11-29T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GJOA",
"spase://NASA/NumericalData/THEMIS/Ground/Gjoa.Haven/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Gjoa.Haven/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/zx06-jp03",
"Gjoa Haven (GJOA/GJO) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2008-08-22T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GLYN",
"spase://NASA/NumericalData/THEMIS/Ground/Glyndon/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Glyndon/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/qhv4-p471",
"Glyndon (GLYN) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_GUA",
"spase://NASA/NumericalData/THEMIS/Ground/Dededo/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Dededo/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/xjz5-vd24",
"Dededo (GUA) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HAN",
"spase://NASA/NumericalData/THEMIS/Ground/Hankasalmi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Hankasalmi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/k9tp-k722",
"Hankasalmi (HAN) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HLMS",
"spase://NASA/NumericalData/THEMIS/Ground/High.Latitude.Monitoring.Station/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Anchorage/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/4ye5-h612",
"Anchorage (HLMS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"2009-06-02T00:59:59",
"",
"2.7.0"
],
[
"THG_L2_MAG_HOMR",
"spase://NASA/NumericalData/THEMIS/Ground/Homer/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Homer/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/hxbv-p964",
"Homer (HOMR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"2009-06-24T13:59:59",
"",
"2.7.0"
],
[
"THG_L2_MAG_HON",
"spase://NASA/NumericalData/THEMIS/Ground/Ewa.Beach/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Honolulu/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:39Z",
"https://doi.org/10.48322/bd4v-8y55",
"Honolulu (HON) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HOP",
"spase://NASA/NumericalData/THEMIS/Ground/Hopen/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Hopen/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/c4y8-yv80",
"Hopen (HOP) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2008-09-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HOTS",
"spase://NASA/NumericalData/THEMIS/Ground/Hot.Springs/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Hot.Springs/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/432t-4h88",
"Hot Springs (HOTS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2004-09-09T00:00:00",
"2015-08-21T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_HOV",
"spase://NASA/NumericalData/THEMIS/Ground/Hov.Faroe.Islands/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Hov.Faroe.Islands/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/5y78-g044",
"Hov Faroe Islands (HOV) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2016-06-21T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HRIS",
"spase://NASA/NumericalData/THEMIS/Ground/Harris/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Harris/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/2ha6-a158",
"Harris (HRIS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2009-11-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_HRP",
"spase://NASA/NumericalData/THEMIS/Ground/Hornepayne/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Hornepayne/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:41Z",
"https://doi.org/10.48322/qcq3-yk70",
"Hornepayne (HRP) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-02-03T00:00:00.000",
"2013-04-08T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_IGLO",
"spase://NASA/NumericalData/THEMIS/Ground/Igloolik/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Igloolik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/7rwj-3d14",
"Igloolik (IGLO/IGL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2008-10-09T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_INUK",
"spase://NASA/NumericalData/THEMIS/Ground/Inukjuak/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Inukjuak/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"",
"Inukjuak (INUK) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-11T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_INUV",
"spase://NASA/NumericalData/THEMIS/Ground/Inuvik/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Inuvik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/3mqm-k396",
"Inuvik (INUV) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-08-13T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_IQA",
"spase://NASA/NumericalData/THEMIS/Ground/Iqaluit/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Iqaluit/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/3q61-db38",
"Iqaluit (IQA) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Ivalo/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Ivalo/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/8bm9-d262",
"Ivalo (IVA) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_JAN",
"spase://NASA/NumericalData/THEMIS/Ground/Jan.Mayen/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Jan.Mayen/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/vy43-w448",
"Jan Mayen (JAN) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2014-09-26T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_JCK",
"spase://NASA/NumericalData/THEMIS/Ground/Jackvik/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Jackvik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:42Z",
"https://doi.org/10.48322/28c1-fc43",
"Jackvik (JCK) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2010-09-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KAKO",
"spase://NASA/NumericalData/THEMIS/Ground/Kaktovik/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Kaktovik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"Level 2",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/93qm-w650",
"Kaktovik (KAKO) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Hampton, V. Angelopoulos, C.T. Russell, (University of Alaska, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT1S",
"2007-01-01T01:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KAPU",
"spase://NASA/NumericalData/THEMIS/Ground/Kapuskasing/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Kapuskasing/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/gwgx-qh96",
"Kapuskasing (KAPU) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-05-17T16:31:38",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KAR",
"spase://NASA/NumericalData/THEMIS/Ground/Karmoy/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Karmoy/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/ta3s-w676",
"Karmoy (KAR) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KENA",
"spase://NASA/NumericalData/THEMIS/Ground/Kenai/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Kenai/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"Level 2",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/kq36-wm23",
"Kenai (KENA) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Hampton, V. Angelopoulos, C.T. Russell, (University of Alaska, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT1S",
"2016-08-15T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KEV",
"spase://NASA/NumericalData/THEMIS/Ground/Kevo/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Kevo/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/1kx2-m636",
"Kevo (KEV) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KIAN",
"spase://NASA/NumericalData/THEMIS/Ground/Kiana/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Kiana/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/btns-pp34",
"Kiana (KIAN) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-09-07T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KIL",
"spase://NASA/NumericalData/THEMIS/Ground/Kilpisjarvi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Kilpisjarvi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/5h8z-np37",
"Kilpisjarvi (KIL) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KJPK",
"spase://NASA/NumericalData/THEMIS/Ground/Kuujjuarapik/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Kuujjuarapik/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/xryx-zv10",
"Kuujjuarapik (KJPK) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-17T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KODK",
"spase://NASA/NumericalData/THEMIS/Ground/Kodiak/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Kodiak/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/41ah-a907",
"Kodiak (KODK) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2010-01-01T00:00:00.000",
"2012-02-14T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_KUUJ",
"spase://NASA/NumericalData/THEMIS/Ground/Kuujjuaq/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Kuujjuaq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/y6f6-tk74",
"Kuujjuaq (KUUJ) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2007-11-27T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_KUV",
"spase://NASA/NumericalData/THEMIS/Ground/Kullorsuaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Kullorsuaq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/25vt-f385",
"Kullorsuaq (KUV) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LARG",
"spase://NASA/NumericalData/THEMIS/Ground/La.Ronge/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/La.Ronge/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/cwz0-sc68",
"La Ronge (LARG) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell and M. Connors, (University of California, Berkeley, University of California, Los Angeles and Athabasca University, respectively, NASA NAS5-02099)",
"PT0.5S",
"2008-10-17T20:44:41",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LCL",
"spase://NASA/NumericalData/THEMIS/Ground/Lucky.Lake/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Lucky.Lake/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/6d38-jb12",
"Lucky Lake (LCL) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-05-23T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_LETH",
"spase://NASA/NumericalData/THEMIS/Ground/Lethbridge/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Lethbridge/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/jkfh-p173",
"Lethbridge (LETH) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell and M. Connors, (University of California, Berkeley, University of California, Los Angeles and Athabasca University, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-09-23T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LOYS",
"spase://NASA/NumericalData/THEMIS/Ground/Loysburg/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Loysburg/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/e18e-kc57",
"Loysburg (LOYS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-10-28T14:25:45",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LOZ",
"spase://NASA/NumericalData/THEMIS/Ground/Lovozero/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Lovozero/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/d220-xb50",
"Lovozero (LOZ) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2017-02-10T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LREL",
"spase://NASA/NumericalData/THEMIS/Ground/Laurel/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Laurel/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/6zy4-as95",
"Laurel (LREL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2012-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_LRES",
"spase://NASA/NumericalData/THEMIS/Ground/Linares/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Linares/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/zfgn-je71",
"Linares (LRES) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"2011-04-15T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_LRG",
"spase://NASA/NumericalData/THEMIS/Ground/La.Ronge/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/La.Ronge/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/61y4-ae86",
"La Ronge (LRG) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-05-23T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_LRV",
"spase://NASA/NumericalData/THEMIS/Ground/Leirvogur/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Leirvogur/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:44Z",
"https://doi.org/10.48322/9gpd-8a88",
"Leirvogur (LRV) Ground-based Vector Magnetic Field (L2) 1,0 min Data",
"",
"Please acknowledge G. Bjornsson, (Science Institute, University of Iceland)",
"PT10S",
"2012-04-01T00:00:00.000",
"2012-04-03T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_LYFD",
"spase://NASA/NumericalData/THEMIS/Ground/Lyford/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Lyford/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/tc23-d740",
"Lyford (LYFD) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"2011-10-06T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_LYR",
"spase://NASA/NumericalData/THEMIS/Ground/Longyearbyen/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Longyearbyen/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/7gkb-9t94",
"Longyearbyen (LYR) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_MAS",
"spase://NASA/NumericalData/THEMIS/Ground/Masi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Masi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/4dsx-6f90",
"Masi (MAS) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_MCGR",
"spase://NASA/NumericalData/THEMIS/Ground/McGrath/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/McGrath/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/h90e-yw44",
"McGrath (MCGR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-08-31T22:22:02",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_MEA",
"spase://NASA/NumericalData/THEMIS/Ground/Meanook/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Meanook/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/7cw7-xg89",
"Meanook (MEA) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_MEK",
"spase://NASA/NumericalData/THEMIS/Ground/Mekrijarvi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Mekrijarvi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/0x54-sg48",
"Mekrijarvi (MEK) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_MUO",
"spase://NASA/NumericalData/THEMIS/Ground/Muono/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Muono/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/drgc-5b91",
"Muono (MUO) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_NAIN",
"spase://NASA/NumericalData/THEMIS/Ground/Nain/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Nain/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/gkna-v460",
"Nain (NAIN/NAN) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2007-06-08T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_NAL",
"spase://NASA/NumericalData/THEMIS/Ground/Nyalesund/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Nyalesund/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/6v7a-8645",
"Ny Alesund (NAL) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_NAQ",
"spase://NASA/NumericalData/THEMIS/Ground/Narsarsuaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Narsarsuaq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/w3qe-k466",
"Narsarsuaq (NRSQ/NAQ) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Colville.National.Forest/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Colville.National.Forest/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:38Z",
"https://doi.org/10.48322/vmkr-9r79",
"Colville National Forest (NEW) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Nordkapp/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Nordkapp/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/pnt6-1m31",
"Nordkapp (NOR) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2007-09-28T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_NRD",
"spase://NASA/NumericalData/THEMIS/Ground/Nord/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Nord/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/6ywk-ja53",
"Nord (NRD) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2007-01-01T00:00:00.000",
"2009-02-28T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Narsarsuaq/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Narsarsuaq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/6b02-9009",
"Narsarsuaq (NRSQ/NAQ) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2008-10-01T00:00:00.000",
"2009-12-13T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_NUR",
"spase://NASA/NumericalData/THEMIS/Ground/Nurmijarvi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Nurmijarvi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:46Z",
"https://doi.org/10.48322/jbx1-za55",
"Nurmijarvi (NUR) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_OTT",
"spase://NASA/NumericalData/THEMIS/Ground/Ottawa/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Ottawa/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/d1rf-a974",
"Ottawa (OTT) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_OUJ",
"spase://NASA/NumericalData/THEMIS/Ground/Oulujarvi/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Oulujarvi/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/2cmv-e979",
"Oulujarvi (OUJ) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PANG",
"spase://NASA/NumericalData/THEMIS/Ground/Pangnirtung/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Pangnirtung/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/h2j7-1x13",
"Pangnirtung (PANG/PGG) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2008-10-04T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PBK",
"spase://NASA/NumericalData/THEMIS/Ground/Pevek/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Pevek/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/th5e-5477",
"Pevek (PBK) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2011-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PBLO",
"spase://NASA/NumericalData/THEMIS/Ground/Pueblo/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Pueblo/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/03g1-jx95",
"Pueblo (PBLO) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2009-05-13T00:00:00.000",
"2012-05-02T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_PCEL",
"spase://NASA/NumericalData/THEMIS/Ground/Purcell/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Purcell/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/35k3-m683",
"Purcell (PCEL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PEL",
"spase://NASA/NumericalData/THEMIS/Ground/Pello/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Pello/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/qehh-fe61",
"Pello (PEL) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG0",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.0/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.0/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/870b-pj49",
"PENGUIn-0 (PG0) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2014-12-28T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG1",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.1/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.1/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/zk2w-6f34",
"PENGUIn-1 (PG1) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2008-01-09T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG2",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.2/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.2/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/q06y-h567",
"PENGUIn-2 (PG2) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2009-01-08T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG3",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.3/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.3/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/684a-c538",
"PENGUIn-3 (PG3) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2013-01-05T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG4",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.4/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.4/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/qwtb-3133",
"PENGUIn-4 (PG4) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2014-01-05T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PG5",
"spase://NASA/NumericalData/THEMIS/Ground/PENGUIn.5/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/PENGUIn.5/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/xt02-9750",
"PENGUIn-5 (PG5) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge C.R. Clauer, (Virginia Tech)",
"PT1S",
"2016-01-06T00:00:00.000",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PGEO",
"spase://NASA/NumericalData/THEMIS/Ground/Prince.George/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Prince.George/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/mfda-0y07",
"Prince George (PGEO) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-01-01T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PINA",
"spase://NASA/NumericalData/THEMIS/Ground/Pinawa/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Pinawa/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/zhgb-tm93",
"Pinawa (PINA) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2006-11-01T00:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PINE",
"spase://NASA/NumericalData/THEMIS/Ground/Pine.Ridge/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Pine.Ridge/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/yxac-ha85",
"Pine Ridge (PINE) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2004-09-09T00:00:00",
"2014-01-29T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_PKS",
"spase://NASA/NumericalData/THEMIS/Ground/Park.Site/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Park.Site/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:47Z",
"https://doi.org/10.48322/ftjm-0g23",
"Park Site (PKS) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-04-14T23:59:59.999",
"",
"2.7.0"
],
[
"THG_L2_MAG_POKR",
"spase://NASA/NumericalData/THEMIS/Ground/Poker.Flat/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Poker.Flat/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/2mwd-0b93",
"Poker Flat (POKR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2007-01-01T01:00:00",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PTRS",
"spase://NASA/NumericalData/THEMIS/Ground/Petersburg/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Petersburg/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/b066-pr48",
"Petersburg (PTRS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2004-09-19T01:42:03",
"",
"",
"2.7.0"
],
[
"THG_L2_MAG_PUVR",
"spase://NASA/NumericalData/THEMIS/Ground/Puvirnituq/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Puvirnituq/Magnetometer",
"MagneticField",
[
"Earth.NearSurface.Ionosphere",
"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/hqg9-fh29",
"Puvirnituq (PUVR) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-07T00:00:00.000",
"",
"",
"2.7.0"
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"spase://SMWG/Instrument/Ground/Radisson/Magnetometer",
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[
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],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/mnpt-6993",
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"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-21T00:00:00.000",
"",
"",
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[
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"spase://SMWG/Instrument/Ground/Ranua/Magnetometer",
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],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/0qbt-p065",
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"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
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"",
"",
"2.7.0"
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"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/rv8j-xt36",
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"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2006-11-01T00:00:00",
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"",
"2.7.0"
],
[
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],
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"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/gc1q-9m38",
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"",
"Please acknowledge E.S. Steinmetz, (Augsburg College)",
"PT0.5S",
"2008-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://SMWG/Instrument/Ground/Red.Deer/Magnetometer",
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],
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"",
"",
"",
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"https://doi.org/10.48322/swe9-bz27",
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"Please acknowledge V. Angelopoulos, C.T. Russell and M. Connors, (University of California, Berkeley, University of California, Los Angeles and Athabasca University, respectively, NASA NAS5-02099)",
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"",
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],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Richardson/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Richardson/Magnetometer",
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],
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"",
"",
"",
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"https://doi.org/10.48322/wkpr-mj03",
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"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-04T00:00:00.000",
"2010-12-31T23:59:59.999",
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"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Remus/Magnetometer/PT0.5S",
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],
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"",
"",
"",
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"https://doi.org/10.48322/qp3z-ar59",
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"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-08-24T19:21:53",
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"",
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],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Roemoe/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Roemoe/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/jvfw-p866",
"Romo (ROE) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2008-09-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Priddis/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Priddis/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:48Z",
"https://doi.org/10.48322/4w47-kg29",
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"",
"Please acknowledge V. Angelopoulos, C.T. Russell and M. Connors, (University of California, Berkeley, University of California, Los Angeles and Athabasca University, respectively, NASA NAS5-02099)",
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"2005-10-02T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Rorvik/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Rorvik/Magnetometer",
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[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/w5gb-h148",
"Rorvik (RVK) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Salluit/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Salluit/Magnetometer",
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[
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"",
"",
"",
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"https://doi.org/10.48322/hj03-gx95",
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"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-21T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://SMWG/Instrument/Ground/San.Antonio/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/dm5c-am32",
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"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"2015-12-31T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Schefferville/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Schefferville/Magnetometer",
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],
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"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/tkkb-8h83",
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"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2015-04-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Ittoqqortoormiit/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Ittoqqortoormiit/Magnetometer",
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[
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"",
"",
"",
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"https://doi.org/10.48322/zqjd-ej54",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"2015-01-05T23:59:59.999",
"",
"2.7.0"
],
[
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"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-26T00:00:00.000",
"",
"",
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],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Sand.Point/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Shumagin/Magnetometer",
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"",
"",
"",
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"https://doi.org/10.48322/w2t2-v658",
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"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Sitka/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Sitka/Magnetometer",
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[
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],
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"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/1mn4-kn89",
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"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-05-12T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Cayey/Magnetometer/PT1S",
"spase://SMWG/Instrument/WDC/San.Juan/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:37Z",
"https://doi.org/10.48322/p94k-8f79",
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"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
"PT1S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Maniitsoq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Maniitsoq/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:45Z",
"https://doi.org/10.48322/y7gj-2430",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-02-05T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Snap.Lake/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Snap.Lake/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/hgae-es63",
"Snap Lake (SNAP) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2008-10-22T19:43:07",
"2013-10-16T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Sanikiluaq/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Sanikiluaq/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/vgh0-dc91",
"Sanikiluaq (SNKQ) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge I. Mann, (University of Alberta)",
"PT0.5S",
"2007-07-09T00:00:00",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Solund/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Solund/Magnetometer",
"MagneticField",
[
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],
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"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/9g5v-sb20",
"Solund (SOL) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Soroya/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Soroya/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
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"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/t7wr-t979",
"Soroya (SOR) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2007-01-08T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Kangerlussuaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Kangerlussuaq/Magnetometer",
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[
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"",
"",
"",
"",
"2025-08-05T13:12:43Z",
"https://doi.org/10.48322/frwd-xa34",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Stanford/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Stanford/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/9dmy-2p51",
"Stanford (STFD) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2009-01-01T00:00:00.000",
"2013-07-08T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Saint.Felicien/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Saint.Felicien/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/5qq5-sz78",
"Saint-Felicien (STFL) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge M. Connors, I. Schofield, (Athabasca University)",
"PT0.5S",
"2014-10-25T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/St.Johns/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/St.Johns/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/0d48-8w66",
"St. John (STJ) Ground-based Vector Magnetic Field (L2) 1.0 s Data",
"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Summit/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Summit/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/0q9m-6f92",
"Summit (SUM) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2016-05-23T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Savissivik/Magnetometer/PT20S",
"spase://SMWG/Instrument/Ground/Savissivik/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:50Z",
"https://doi.org/10.48322/bq1b-jj23",
"Savissivik (SVS) Ground-based Vector Magnetic Field (L2) 20.0 s Data",
"",
"Please acknowledge H. Gleisner, (Danish Meteorological Institute, Denmark)",
"PT20S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Shawano/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Shawano/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:51Z",
"https://doi.org/10.48322/9rbb-9287",
"Shawano (SWNO) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-10-17T18:31:02",
"2014-03-10T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Thule.Air.Base/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Thule.Air.Base/Magnetometer",
"MagneticField",
[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/1kex-bg51",
"Thule Air Base (TAB) Ground-based Vector Magnetic Field (L2) 1.0 min Data",
"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
"PT1M",
"2013-07-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Tartu/Magnetometer/PT10S",
"spase://SMWG/Instrument/Ground/Tartu/Magnetometer",
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[
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],
"",
"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/8cmp-0162",
"Tartu (TAR) Ground-based Vector Magnetic Field (L2) 10.0 s Data",
"",
"Please acknowledge L. Juusola, (Finnish Meteorological Institute)",
"PT10S",
"2017-01-01T00:00:00.000",
"",
"",
"2.7.0"
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"spase://NASA/NumericalData/THEMIS/Ground/Tristan.da.Cunha/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Tristan.da.Cunha/Magnetometer",
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[
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/m7cj-rz83",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2009-09-01T00:00:00.000",
"",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Qaanaaq/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Qaanaaq/Magnetometer",
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"Earth.Surface"
],
"",
"",
"",
"",
"2025-08-05T13:12:49Z",
"https://doi.org/10.48322/r9kd-4071",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
],
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"spase://NASA/NumericalData/THEMIS/Ground/Tiksi/Magnetometer/PT1M",
"spase://SMWG/Instrument/Ground/Tiksi/Magnetometer",
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],
"",
"",
"",
"",
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"https://doi.org/10.48322/km0g-cq16",
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"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2011-01-01T00:00:00.000",
"",
"",
"2.7.0"
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"Earth.Surface"
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"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/4mrh-va47",
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"",
"Please acknowledge D. Hampton, (University of Alaska)",
"PT1S",
"2015-04-23T00:00:00.000",
"2015-04-24T23:59:59.999",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/The.Pas/Magnetometer/PT0.5S",
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],
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"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/6k2w-zf06",
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"Flin Flon Vector Magnetic Field 0.5 s Data",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2006-01-01T00:00:01",
"",
"",
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"spase://NASA/NumericalData/THEMIS/Ground/Trapper.Creek/Magnetometer/PT1S",
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"https://doi.org/10.48322/x87k-fy69",
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"",
"Please acknowledge D. Hampton, (University of Alaska)",
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"2007-01-01T01:00:00",
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"",
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],
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"",
"",
"",
"2025-08-05T13:12:52Z",
"https://doi.org/10.48322/zb23-2583",
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"",
"Please acknowledge Tromso Geophysical Observatory, (UiT The Arctic University of Norway)",
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"2006-12-30T00:00:00.000",
"",
"",
"2.7.0"
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/rxcb-bs74",
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"",
"Please acknowledge C.A. Finn, (United States Geological Survey, Golden)",
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"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://SMWG/Instrument/Ground/Ukiah/Magnetometer",
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/hbr1-zv19",
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"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
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"2004-10-01T23:52:14",
"",
"",
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Uummannaq/Magnetometer/PT1M",
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],
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/gf9b-gb66",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://SMWG/Instrument/Ground/Upernavik/Magnetometer",
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/bbat-6g35",
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"",
"Please acknowledge C. Stolle, J. Matzka, (DTU Space, Denmark)",
"PT1M",
"2007-01-01T00:00:00.000",
"",
"",
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"spase://SMWG/Instrument/Ground/Victoria/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/1ep7-k022",
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"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2007-01-01T00:00:00.000",
"2007-01-03T23:59:59.999",
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/vwqt-mq35",
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"",
"Please acknowledge O. Troshichev, (Arctic and Antarctic Research Institute)",
"PT1M",
"2017-02-10T00:00:00.000",
"",
"",
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"spase://SMWG/Instrument/Ground/Val.d.Or/Magnetometer",
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"",
"",
"",
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"https://doi.org/10.48322/hx6b-2f20",
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"",
"Please acknowledge V. Angelopoulos, C.T. Russell and M. Connors, (University of California, Berkeley, University of California, Los Angeles and Athabasca University, respectively, NASA NAS5-02099)",
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"2005-11-06T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Whitehorse/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Whitehorse/Magnetometer",
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[
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"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/20k0-dp16",
"Whitehorse (WHIT) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
"PT0.5S",
"2005-07-11T22:45:47",
"",
"",
"2.7.0"
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[
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"spase://NASA/NumericalData/THEMIS/Ground/Whitehorse/Magnetometer/PT1S",
"spase://SMWG/Instrument/Ground/Whitehorse/Magnetometer",
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[
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"",
"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/ec95-7d95",
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"",
"Please acknowledge K. Hayashi, (University of Tokyo)",
"PT1S",
"2007-01-01T00:00:00.000",
"2013-05-23T23:59:59.999",
"",
"2.7.0"
],
[
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"spase://NASA/NumericalData/THEMIS/Ground/Wallops.Island/Magnetometer/PT0.5S",
"spase://SMWG/Instrument/Ground/Wallops.Island/Magnetometer",
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[
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"",
"",
"",
"",
"2025-08-05T13:12:53Z",
"https://doi.org/10.48322/bfjt-9v74",
"Wallops Island (WLPS) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (United States Air Force Academy, University of California, Los Angeles)",
"PT0.5S",
"2012-01-01T00:00:00.000",
"2013-08-25T23:59:59.999",
"",
"2.7.0"
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[
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"spase://SMWG/Instrument/Ground/Worthington/Magnetometer",
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"",
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"",
"2025-08-05T13:12:54Z",
"https://doi.org/10.48322/jt14-s139",
"Worthington (WRTH) Ground-based Vector Magnetic Field (L2) 0.5 s Data",
"",
"Please acknowledge P. Chi, (University of California, Los Angeles)",
"PT0.5S",
"2007-01-01T00:00:00.000",
"",
"",
"2.7.0"
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[
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"spase://SMWG/Instrument/Ground/Yellowknife/Magnetometer",
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"",
"",
"",
"",
"2025-08-05T13:12:54Z",
"https://doi.org/10.48322/8st3-qf10",
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"",
"Please acknowledge D. Calp, (Geological Survey of Canada)",
"PT1S",
"2008-10-24T00:00:00.000",
"",
"",
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[
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"spase://SMWG/Instrument/Ground/Yellowknife/Magnetometer",
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"",
"",
"",
"2025-08-05T13:12:54Z",
"https://doi.org/10.48322/dctt-r668",
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"",
"Please acknowledge V. Angelopoulos, C.T. Russell, (University of California, Berkeley, University of California, Los Angeles, respectively, NASA NAS5-02099)",
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"2008-10-22T17:27:54",
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[
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"2007-12-11T00:00:00.000Z",
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"2002-01-08T00:00:00.000",
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"https://doi.org/10.48322/3x4k-mx60",
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"2015-12-31T23:49:42.000",
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"https://doi.org/10.48322/ze5g-gm91",
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"Please acknowledge the Principal Investigator D.J. McComas for use of the Data",
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"2017-12-26T23:59:00.000",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/pcsr-8685",
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"Please acknowledge the CDAWeb team at GSFC/SPDF.",
"PT15M",
"2007-04-18T00:01:38Z",
"2018-12-12T23:59:59Z",
"",
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"",
"D.J. McComas, H.J. Fahr",
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"2018-12-12T23:59:59Z",
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[
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"spase://NASA/NumericalData/TWINS1/ENA/TISTORM/PT72S",
"spase://SMWG/Instrument/TWINS1/ENA",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/cre5-4g28",
"TWINS 1 Images of Plasma Sheet Ion Temperature during Storms calculated from Energetic Neutral Atom (ENA) Measurements",
"",
"D.J. McComas, A.M. Keesee",
"PT72S",
"2008-06-15T05:31:00.000",
"2013-12-09T03:10:59.999",
"",
"2.6.0"
],
[
"TWINS2_AT_DEF",
"spase://NASA/NumericalData/TWINS2/Ephemeris/Attitude/Definitive/PT0.512S",
"spase://SMWG/Instrument/TWINS1/Ephemeris",
"Ephemeris",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/btg2-gm95",
"TWINS-2 Ephemeris, Definitive Spacecraft Attitude, PT0.512S Data",
"",
"Please acknowledge the Principal Investigator D.J. McComas for use of the Data",
"PT0.512S",
"2008-04-14T00:53:59.000",
"2016-10-27T23:59:59.000",
"",
"2.6.0"
],
[
"TWINS2_L1_IMAGER",
"spase://NASA/NumericalData/TWINS2/ENA/L1/PT15M",
"spase://SMWG/Instrument/TWINS2/ENA",
"NeutralAtomImages",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/1tsg-7729",
"TWINS 2 Neutral-atom L1 Images and Movies",
"",
"Please acknowledge the CDAWeb team at GSFC/SPDF.",
"PT15M",
"2008-05-02T04:45:27Z",
"2016-10-26T03:45:47.000Z",
"",
"2.6.0"
],
[
"TWINS2_L1_LAD",
"spase://NASA/NumericalData/TWINS2/LAD/L1/PT1.333S",
"spase://SMWG/Instrument/TWINS2/LAD",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath"
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"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/yvt8-0a64",
"TWINS 2 Lyman Alpha Detector (LAD) Geocorona",
"",
"D.J. McComas, H.J. Fahr",
"PT1.333S",
"2008-05-02T04:45:26",
"2016-10-26T23:59:59.999",
"",
"2.6.0"
],
[
"TWINS2_OR_DEF",
"spase://NASA/NumericalData/TWINS2/Ephemeris/PT1M45S",
"spase://SMWG/Instrument/TWINS2/Ephemeris",
"Ephemeris",
"Earth.Magnetosphere",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"TWINS 2 - Spacecraft Ephemeris",
"",
"",
"PT1M45S",
"2001-04-11T00:03:22.394Z",
"2016-12-31T23:59:59.999Z",
"",
"2.3.2"
],
[
"TWINS2_TISTORM_IMAGER",
"spase://NASA/NumericalData/TWINS2/ENA/TISTORM/PT72S",
"spase://SMWG/Instrument/TWINS2/ENA",
"ImageIntensity",
[
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosheath"
],
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/6g4w-d971",
"TWINS 2 Images of Plasma Sheet Ion Temperature during Storms calculated from Energetic Neutral Atom (ENA) Measurements",
"",
"D.J. McComas, A.M. Keesee",
"PT72S",
"2008-06-14T18:00:00.000",
"2013-12-09T03:11:59.999",
"",
"2.6.0"
],
[
"TWINS_M2_ENA",
"spase://NASA/NumericalData/TWINS/ENA/MagnetosphericIonTemperatures/ModifiedData/PT10M",
[
"spase://SMWG/Instrument/TWINS1/ENA",
"spase://SMWG/Instrument/TWINS1/Ephemeris",
"spase://SMWG/Instrument/TWINS2/ENA",
"spase://SMWG/Instrument/TWINS2/Ephemeris"
],
[
"Ephemeris",
"ThermalPlasma"
],
[
"Earth.Magnetosphere.Main",
"Earth.Magnetosphere.RadiationBelt",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Plasmasphere"
],
"",
"",
"",
"",
"2025-08-05T13:12:54Z",
"https://doi.org/10.48322/grxp-5t19",
"TWINS 1, TWINS 2 Storm Time Equatorial Magnetospheric Ion Temperatures derived from Energetic Neutral Fluxes (ENA), Modified Data 2 (MD2), 10 min Data",
"",
"Please acknowledge the Principal Investigator D.J. McComas for use of the Data",
"PT10M",
"2009-07-21T00:00:00.000",
"2017-11-07T23:59:59.999",
"",
"2.7.0"
],
[
"UY_1MIN_VHM",
"spase://NASA/NumericalData/Ulysses/FGM/GSFC/SPDF/PT1M",
"spase://SMWG/Instrument/Ulysses/FGM",
"MagneticField",
[
"Heliosphere.Inner",
"Heliosphere.Outer",
"Heliosphere.NearEarth"
],
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses magnetic field 1-min data",
"",
"Please acknowledge CDAWeb and the Principal Investigator, A. Balogh of Imperial College, London, UK.",
"PT1M",
"1990-10-25T00:00:00Z",
"2009-06-30T00:00:00Z",
"",
"2.3.2"
],
[
"UY_1SEC_VHM",
"spase://NASA/NumericalData/Ulysses/FGM/PT01S",
"spase://SMWG/Instrument/Ulysses/FGM",
"MagneticField",
[
"Heliosphere.Inner",
"Heliosphere.Outer",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses High Resolution Magnetic Field Data",
"",
"Please acknowledge the Principal Investigator, A. Balogh of Imperial College, London, UK. and the repository from which you accessed the data.",
"PT01S",
"1990-10-25T16:50:46Z",
"2009-06-30T23:59:59Z",
"",
"2.3.2"
],
[
"UY_ALPHA-DISTRIBUTIONS_SWOOPS",
"spase://NASA/NumericalData/Ulysses/SWOOPS/AlphaParticle/FitParameters/PT4M",
[
"spase://SMWG/Instrument/Ulysses/Ephemeris",
"spase://SMWG/Instrument/Ulysses/FGM",
"spase://SMWG/Instrument/Ulysses/SWOOPS"
],
[
"EnergeticParticles",
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses Solar Wind Observations Over the Poles of the Sun (SWOOPS) Alpha Particle Distribution Functions, Level H2, 4 min Data",
"",
"D.J. McComas, B.E. Goldstein, M.M. Neugebauer, A. Tenerani",
"PT4M",
"1990-11-18T12:56:11.000",
"2009-06-30T15:38:12.000",
"",
"2.3.2"
],
[
"UY_ALPHA-FIT-PARAMETERS_SWOOPS",
"spase://NASA/NumericalData/Ulysses/SWOOPS/AlphaParticle/ParticleDistributions/PT4M",
[
"spase://SMWG/Instrument/Ulysses/Ephemeris",
"spase://SMWG/Instrument/Ulysses/FGM",
"spase://SMWG/Instrument/Ulysses/SWOOPS"
],
[
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2022-05-25T12:34:56.789",
"",
"Ulysses Solar Wind Observations Over the Poles of the Sun (SWOOPS) Alpha Particle Distribution Function Fitting Parameters, Key Parameter (K0), 4 min Data",
"",
"D.J. McComas, B.E. Goldstein, M.M. Neugebauer, A. Tenerani",
"PT4M",
"1990-11-18T12:56:11.000",
"2009-06-30T15:38:12.000",
"",
"2.4.0"
],
[
"UY_ALPHA-MOMENTS_SWOOPS",
"spase://NASA/NumericalData/Ulysses/SWOOPS/AlphaParticle/Moments/PT4M",
[
"spase://SMWG/Instrument/Ulysses/Ephemeris",
"spase://SMWG/Instrument/Ulysses/FGM",
"spase://SMWG/Instrument/Ulysses/SWOOPS"
],
[
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Heliosphere.Outer"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses Solar Wind Observations Over the Poles of the Sun (SWOOPS) Alpha Particle Distribution Function Hot Plasma Moments, Level H1, 4 min Data",
"",
"D.J. McComas, B.E. Goldstein, M.M. Neugebauer, A. Tenerani",
"PT4M",
"1990-11-18T12:56:11.000",
"2009-06-30T15:38:12.000",
"",
"2.3.2"
],
[
"UY_COHO1HR_MERGED_MAG_PLASMA",
"spase://NASA/NumericalData/Ulysses/MAGandPLS/PT1H",
[
"spase://SMWG/Instrument/Ulysses/FGM",
"spase://SMWG/Instrument/Ulysses/SWOOPS"
],
[
"MagneticField",
"ThermalPlasma"
],
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses hourly merged magnetic field and plasma data",
"",
"Please acknowledge the magnetic field and plasma Principal Investigators, Drs. A. Balogh and D. McComas, and NSSDC or GSFC-SPDF",
"PT1H",
"1990-10-25T00:00:00",
"2008-10-18T00:00:00",
"Plasma data do not start until Nov. 18, 1990. As of 12/31/2008, magnetic field data end on Feb. 29, 2008. Plasma data become quite sparse after ~May 19, 2008. Data may be extended.",
"2.3.2"
],
[
"UY_H0_GLG",
"spase://NASA/NumericalData/Ulysses/SWICS/GSFC/SPDF/PT13M",
"spase://SMWG/Instrument/Ulysses/SWICS",
"ThermalPlasma",
[
"Heliosphere.Outer",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses olar Wind Ion Composition Spectrometer (SWICS) Full Resolution Matrix Rate Data",
"",
"Please acknowledge G. Gloeckler (P.I.)",
"PT13M",
"1990-11-08T00:00:00",
"2000-12-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_AT1",
"spase://NASA/NumericalData/Ulysses/COSPIN/AT/Ion/Fluxes/SpinAveraged/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/AT",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Anisotropy Telescopes (AT) Proton and Helium Spin-Averaged and Sectored Coincidence Fluxes, 10 min Data",
"COSPIN-AT-Fluxes-PT10M",
"Please acknowledge the COSPIN AT Lead Investigators, AT Group Leader Andre Balogh and AT Co-PI Silvia Dalla",
"PT10M",
"1990-10-22T00:00:00.000",
"2008-12-31T23:59:59.999",
"",
"2.2.9"
],
[
"UY_M0_AT2",
"spase://NASA/NumericalData/Ulysses/COSPIN/AT/Ion/Fluxes/SpinAveraged/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/AT",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-03-29T17:14:50Z",
"",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Anisotropy Telescopes (AT) Proton and Helium Spin-Averaged and Sectored Coincidence Fluxes, 10 min Data",
"COSPIN-AT-Fluxes-PT10M",
"Please acknowledge the COSPIN AT Lead Investigators, AT Group Leader Andre Balogh and AT Co-PI Silvia Dalla",
"PT10M",
"1990-10-22T00:00:00.000",
"2008-12-31T23:59:59.999",
"",
"2.2.9"
],
[
"UY_M0_BAE",
"spase://NASA/NumericalData/Ulysses/SWOOPS/ElectronParams/PT335.00S",
"spase://SMWG/Instrument/Ulysses/SWOOPS",
"ThermalPlasma",
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses SWOOPS Electron N and T Parameters Data",
"",
"",
"PT335.00S",
"1990-11-18T00:00:00",
"2008-08-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_BAI",
"spase://NASA/NumericalData/Ulysses/SWOOPS/IonParams/CDF/PT335S",
"spase://SMWG/Instrument/Ulysses/SWOOPS",
"ThermalPlasma",
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses SWOOPS Ion Parameters high resolution Data.",
"",
"",
"PT335S",
"1990-11-18T00:00:00",
"2009-06-30T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_GRB",
"spase://NASA/NumericalData/Ulysses/SWICS/GSFC/SPDF/GRB/PT5M",
"spase://SMWG/Instrument/Ulysses/SWICS",
"Irradiance",
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses GRB data via CDAWeb",
"",
"",
"PT5M",
"1990-11-10T00:02:30",
"2006-12-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_HET",
"spase://NASA/NumericalData/Ulysses/COSPIN/HET/Rates/SpinAveraged/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/HET",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/s9mg-he04",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Energy Telescope (HET) Ion and Electron Spin-Averaged Coincidence Counting Rates, 10 min Data",
"COSPIN-HET-RATES-PT10M",
"Please acknowledge R. Bruce McKibben, Space Science Center, University of New Hampshire",
"PT10M",
"1990-10-22T00:00:00.000",
"2009-06-10T23:59:59.999",
"",
"2.6.0"
],
[
"UY_M0_HFT",
"spase://NASA/NumericalData/Ulysses/COSPIN/HFT/Ion/Fluxes/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/HFT",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Flux Telescope (HFT) Proton and Heavy Ion Spin-Averaged and Sectored Counting Rate based Nominal Fluxes, 10 min Average Data",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) High Flux Telescope (HFT) Energetic (MeV) Nuclei Nominal Fluxes, 10 min Average Data",
"Please acknowledge the COSPIN HFT Lead Investigator, J. David Anglin",
"PT10M",
"1990-10-22T00:00:00.000",
"2007-04-20T23:59:59.999",
"",
"2.3.2"
],
[
"UY_M0_KET",
"spase://NASA/NumericalData/Ulysses/COSPIN/KET/Rates/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/KET",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Kiel Electron Telescope (KET) Proton, Helium, and Electron Spin-Integrated Counting Rates Data, 10 min Average Data",
"COSPIN-KET-RAT-10M",
"Please acknowledge the COSPIN PI, R. Bruce McKibben, the KET Co-PI, Bernd Heber, and the UDS and/or NSSDC",
"PT10M",
"1990-10-23T00:00:00.000",
"2008-12-31T23:59:59.999",
"",
"2.3.2"
],
[
"UY_M0_LET",
"spase://NASA/NumericalData/Ulysses/COSPIN/LET/Fluxes/PT10M",
"spase://SMWG/Instrument/Ulysses/COSPIN/LET",
"EnergeticParticles",
"Heliosphere.Outer",
"",
"",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses Cosmic Ray and Solar Particle Investigation (COSPIN) Low Energy Telescope (LET) Spin-Integrated Ion Fluxes and Electron Counting Rates, 10 min Average Data",
"COSPIN-LET-RAT-10M",
"Please acknowledge the COSPIN PI, R. Bruce McKibben, the lead LET Co-PI, Richard G. Marsden, and the UDS and/or NSSDC",
"PT10M",
"1990-10-23T00:00:00.000",
"2008-12-31T23:59:59.999",
"",
"2.3.2"
],
[
"UY_M0_PFRA",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/PFRA/PT10M",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"Waves.Passive"
],
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses URAP PFR average 10-min Electric Field Data",
"",
"",
"PT10M",
"1990-11-03T00:00:00",
"2008-08-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_PFRP",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/PFRP/PT10M",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"Waves.Passive"
],
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses URAP PFR Peak 10-min Electric Field Data",
"",
"",
"PT10M",
"1990-11-03T00:00:00",
"2008-08-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_R144",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/RAR/CDF/PT144S",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"ElectricField"
],
[
"Heliosphere.Inner",
"Heliosphere.Outer",
"Jupiter",
"Sun.Corona"
],
"",
"",
"Ulyssses URAP Interference and other issues affecting data interpretation - see Ulysses URAP - Interference and other issues affecting data interpretation http://vwo.nasa.gov/urap/URAP_InterpretationIssues/urap_interpretation.html and URAP - User Notes http://ulysses-ops.esa.int/ulysses/archive/urap_un.html",
[
"Dynamic Spectrogram",
"Spectrogram",
"Solar radio burst",
"Jovian Kilometric Radiation",
"KOM",
"bKOM",
"Jovian Hectometric Radiation",
"HOM",
"Type II Solar radio burst",
"Type III Solar radio burst",
"UHR",
"Upper hybrid resonance",
"VLF Emissions",
"ULF Emissions",
"Whistler"
],
"2021-04-27T15:38:11Z",
"",
"Ulysses Unified Radio and Plasma wave (URAP) Radio Astronomy Receiver (RAR) 144 Second Data",
[
"Ulysses Unified Radio and Plasma Wave Experiment - Radio Astronomy Receiver 144 Second Resolution Data",
"UY_M0_R144"
],
"Please acknowledge the Principal Investigator, R J MacDowall, of the NASA Goddard Space Flight Center, Greenbelt, MD, USA, and Mike Lancaster and Cecil Tranquille of the Ulysses Data System, ESA/ESTEC, Noordwijk, NL",
"PT144S",
"1990-11-03T19:30:00Z",
"2007-11-26T18:30:00Z",
"",
"2.3.2"
],
[
"UY_M0_RARA",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/RARA/PT10M",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"Waves.Passive"
],
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses URAP RAR 10 min. Electric Field Data",
"",
"",
"PT10M",
"1990-11-03T00:00:00",
"2008-08-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_RARP",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/RARP/PT10M",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"Waves.Passive"
],
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses URAP RAR Peak 10-min Electric Field Data",
"",
"",
"PT10M",
"1990-11-03T00:00:00",
"2008-08-31T00:00:00",
"",
"2.3.2"
],
[
"UY_M0_WFBA",
"spase://NASA/NumericalData/Ulysses/URAP/GSFC/SPDF/WFBA/PT10M",
"spase://SMWG/Instrument/Ulysses/URAP",
[
"Waves.Passive",
"Waves.Passive"
],
"Heliosphere.Outer",
"",
"CALIBRATED",
"",
"",
"2021-04-27T15:38:11Z",
"",
"Ulysses URAP WFA 10-min Magnetic Field Average Data",
"",
"",
"PT10M",
"1990-11-03T00:00:00",
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"2.6.0"
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"2006-12-31T00:00:00",
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"https://doi.org/10.48322/rjwx-xr84",
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"2023-07-30T12:34:56.789",
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"2023-07-30T12:34:56.789",
"https://doi.org/10.48322/mtan-4b60",
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"J.D. Richardson, F. Bagenal, Please acknowledge the Voyager 1 and Voyager 2 PLS PI, J.D. Richardson, MIT, and the Data Set Producer, F. Bagenal of the University of Colorado. For Public Distribution but Users are advised to contact F. Bagenal on Questions about how the Data were produced.",
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"2023-07-30T12:34:56.789",
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"",
"Please acknowledge the Voyager 2 PLS Principal Investigator, J.D. Richardson, from the Massacusetts Institute of Technology for providing the Data. For Public Distribution but Users are advised to contact J.D. Richardson on Questions about how the Data were produced.",
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"Please acknowledge the Voyager 2 PLS Principal Investigator, J.D. Richardson, from the Massacusetts Institute of Technology for providing the Data. For Public Distribution but Users are advised to contact J.D. Richardson on Questions about how the Data were produced.",
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"Please acknowledge the Voyager 2 PLS Principal Investigator, J.D. Richardson, from the Massacusetts Institute of Technology for providing the Data. For Public Distribution but Users are advised to contact J.D. Richardson on Questions about how the Data were produced.",
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"https://doi.org/10.48322/c201-q577",
"Wind 3DP 24-sec ESSA-HIGH Electron Omnidirectional Fluxes",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT24S",
"1994-12-20T15:10:03.000Z",
"",
"",
"2.3.2"
],
[
"WI_ELM2_3DP",
"spase://NASA/NumericalData/Wind/3DP/EESA_LOW/Moments",
"spase://SMWG/Instrument/Wind/3DP",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"",
"Note Feb2015 Correct spacecraft potential is important to scientifically useful results .No documentation found on how this potential has been calculated.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/4tk0-a011",
"Wind 3DP EESA-LOW Electron Moments",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"",
"1994-11-15T12:54:33.000Z",
"",
"",
"2.3.2"
],
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"spase://NASA/NumericalData/Wind/3DP/ELPD/PT96S",
"spase://SMWG/Instrument/Wind/3DP",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"1",
"There are several variables in the data files which are not populated in the publicly available data product. These variables include EDENS, TEMP, QP, QM, QT, REDF, and VSW.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/kesf-re26",
"Wind 3DP EESA-LOW Electron Pitch-Angle Distributions",
"",
"User will acknowledge the Wind 3DP Team in any publication resulting from use of this data.",
"PT96S",
"1994-11-15T12:53:43Z",
"",
"",
"2.3.2"
],
[
"WI_ELSP_3DP",
"spase://NASA/NumericalData/Wind/3DP/EESA/ElectronSpectra/PT100S",
"spase://SMWG/Instrument/Wind/3DP",
"EnergeticParticles",
[
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"Heliosphere.Inner",
"Heliosphere.NearEarth"
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"",
"Calculated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/cbvx-4034",
"Wind Hot Plasma and Charged Particles (3DP) Electron Electrostatic Analyzer (EESA) Low, Omnidirectional Flux Spectra, 5 eV to 1100 eV, 24 s Data",
"",
"Please acknowledge the Principal Investigator R.P. Lin and S.D. Bale for use of the Data",
"PT24S",
"1994-11-15T12:54:34.000",
"2018-11-12T23:58:24.000",
"",
"2.3.2"
],
[
"WI_EMFITS_E0_3DP",
"spase://NASA/NumericalData/Wind/3DP/EMFITS/PT100S",
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"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/ndp9-8t38",
"Wind 3DP Solar Wind Plasma Corrected Electron Moments (EMFITS), 100 s Data",
"",
"R.P. Lin, S.D. Bale, Contact 3DP PI, S.D. Bale, bale@ssl.berkeley.edu Contact 3DP PI, S.D. Bale, bale@ssl.berkeley.edu.",
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"1995-01-01T00:00:00.000",
"2004-12-31T23:59:59.999",
"",
"2.3.2"
],
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"spase://NASA/NumericalData/Wind/3DP/EM/PT3S",
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"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/bsy7-7789",
"Wind 3DP Electron Plasma Moments",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT3S",
"1994-11-15T12:53:43.000Z",
"",
"",
"2.3.2"
],
[
"WI_EPACT_STEP-DIFFERENTIAL-ION-FLUX-1HR",
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"spase://SMWG/Instrument/Wind/EPACT",
[
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"Ephemeris",
"MagneticField",
"ThermalPlasma"
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"Heliosphere.Inner",
"Heliosphere.NearEarth"
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"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/6654-mc20",
"Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential Ion Fluxes, 1 h Data",
"",
"Mihir Desai",
"PT1H",
"1994-11-21T00:00:00.000",
"2017-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"WI_EPACT_STEP-DIRECTIONAL-DIFF-CNO-FLUX-10MIN",
"spase://NASA/NumericalData/Wind/EPACT/STEP/Directional/DifferentialFlux/CNO/PT10M",
"spase://SMWG/Instrument/Wind/EPACT",
[
"EnergeticParticles",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
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"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/0y67-vc97",
"Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Carbon, Nitrogen, and Oxygen Fluxes, 10 min Data",
"",
"Mihir Desai",
"PT10M",
"1994-11-21T00:00:00.000",
"2017-12-31T23:58:32.000",
"",
"2.3.2"
],
[
"WI_EPACT_STEP-DIRECTIONAL-DIFF-FE-FLUX-10MIN",
"spase://NASA/NumericalData/Wind/EPACT/STEP/Directional/DifferentialFlux/Iron/PT10M",
"spase://SMWG/Instrument/Wind/EPACT",
[
"EnergeticParticles",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/t2mh-c690",
"Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Iron Fluxes, 10 min Data",
"",
"Mihir Desai",
"PT10M",
"1994-11-21T00:00:00.000",
"2017-12-31T23:58:32.000",
"",
"2.3.2"
],
[
"WI_EPACT_STEP-DIRECTIONAL-DIFF-H-FLUX-10MIN",
"spase://NASA/NumericalData/Wind/EPACT/STEP/Directional/DifferentialFlux/Hydrogen/PT10M",
"spase://SMWG/Instrument/Wind/EPACT",
[
"EnergeticParticles",
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"MagneticField",
"ThermalPlasma"
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[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/c7fp-nf79",
"Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Hydrogen Fluxes, 10 min Data",
"",
"Mihir Desai",
"PT10M",
"1994-11-21T00:00:00.000",
"2017-12-31T23:58:32.000",
"",
"2.3.2"
],
[
"WI_EPACT_STEP-DIRECTIONAL-DIFF-HE-FLUX-10MIN",
"spase://NASA/NumericalData/Wind/EPACT/STEP/Directional/DifferentialFlux/Helium/PT10M",
"spase://SMWG/Instrument/Wind/EPACT",
[
"EnergeticParticles",
"Ephemeris",
"MagneticField",
"ThermalPlasma"
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[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/z4p2-ky35",
"Wind Energetic Particle Acceleration Composition Transport (EPACT) SupraThermal Energetic Particle Telescope (STEP) Differential, Directional Helium Fluxes, 10 min Data",
"",
"Mihir Desai",
"PT10M",
"1994-11-21T00:00:00.000",
"2017-12-31T23:58:32.000",
"",
"2.3.2"
],
[
"WI_H0_MFI",
"spase://NASA/NumericalData/Wind/MFI/PT03S",
"spase://SMWG/Instrument/Wind/MFI",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main"
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"",
"Level 2",
"Note comments about versioning in the text description above",
"Magnetic field",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/av38-wn55",
"Wind Magnetic Field Investigation (MFI) Composite Data",
"",
"User will acknowledge the Wind MFI instrument team, and the site from which data are pulled, in any publication resulting from the use of these data.",
"PT3S",
"1994-11-12T16:00:00Z",
"",
"",
"2.3.2"
],
[
"WI_H0_SWE",
"spase://NASA/NumericalData/Wind/SWE/H0/PT06S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Heliosphere.Inner",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/2jxp-7x36",
"Wind Solar Wind Experiment (SWE) Electron Moments Parameters (6-12s rate) (1994-2001)",
[
"WI_H0_SWE_v01",
"WI_H0_SWE_v02"
],
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT06S",
"1994-12-29T00:00:02.409Z",
"2001-05-31T23:59:57.381Z",
"",
"2.3.2"
],
[
"WI_H0_WAV",
"spase://NASA/NumericalData/Wind/WAVES/PlasmaDensity/H0/PT18S",
"spase://SMWG/Instrument/Wind/WAVES",
[
"ElectricField",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/thkc-wf80",
"Wind Plasma and Radio Waves (WAVES) Electron Plasma Densities, Level H0 (H0), 17.664 s Data",
"",
"Please acknowledge the Principal Investigator M.L. Kaiser for use of the Data",
"PT17.664S",
"1994-11-12T00:00:25.000",
"2019-01-18T23:59:38.000",
"",
"2.3.2"
],
[
"WI_H1_SWE",
"spase://NASA/NumericalData/Wind/SWE/Definitive/PT92S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/nasd-j276",
"Wind Solar Wind Experiment (SWE) 92-sec Definitive Solar Wind Proton Data",
"",
"Please acknowledge the Wind/SWE ion instrument team (Lazarus, Kasper), the SWE PI (Ogilvie), and the site from which you pulled the data.",
"PT92S",
"1995-01-01T00:00:19.526Z",
"2004-11-15T23:58:49.756Z",
"As of August, 2011, it was expected that updates to near-current time would become available very soon.",
"2.3.2"
],
[
"WI_H1_WAV",
"spase://NASA/NumericalData/Wind/WAVES/DS/PT1M",
"spase://SMWG/Instrument/Wind/WAVES",
[
"Waves.Passive",
"Spectrum"
],
[
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"Earth.NearSurface.Plasmasphere",
"Earth.NearSurface.AuroralRegion",
"Earth.NearSurface.PolarCap",
"Heliosphere.Inner"
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"",
"",
"",
[
"Dynamic Spectrogram",
"Spectrogram",
"AKR",
"Auroral hiss",
"Auroral Kilometric Radiation",
"Chorus",
"Continuum radiation",
"Myriametric radiation",
"Plasmaspheric Hiss",
"Solar radio burst",
"Terrestrial Kilometric Radiation",
"TKR",
"Type II Solar radio burst",
"Type III Solar radio burst",
"UHR",
"Upper hybrid resonance",
"VLF Station",
"VLF Transmitter",
"Whistler"
],
"2021-06-22T18:48:59Z",
"https://doi.org/10.48322/ys2k-6162",
"Wind Radio/Plasma Wave, (WAVES) Hi-Res Parameters CDF",
[
"WIND WAVES RADIO CDF format at CDAWeb",
"WI_H1_WAV",
"Wind_WAVES_Electric-Field-Intensities_1min_cdf"
],
"Users please acknowledge Coordinated Data Analysis Web (CDAWeb) at the NASA Goddard Space Flight Center and Wind/Waves Principal Investigators Jean-Louis Henry Bougeret and Robert J MacDowall",
"PT1M",
"1994-11-11T16:00:00Z",
"",
"",
"2.3.2"
],
[
"WI_H2_MFI",
"spase://NASA/NumericalData/Wind/MFI/PT0.092S",
"spase://SMWG/Instrument/Wind/MFI",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main"
],
"",
"",
"Note comments about versioning in the text description above",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/0v0h-df27",
"Wind Magnetic Field Investigation (MFI) Data at full resolution",
"",
"User will acknowledge the Wind MFI instrument team, and the server from which the data were accessed, in any publication resulting from the use of these data.",
"PT0.092S",
"1994-11-12T16:00:00Z",
"",
"",
"2.3.2"
],
[
"WI_H3-RTN_MFI",
"spase://NASA/NumericalData/Wind/MFI/RTN/PT03S",
"spase://SMWG/Instrument/Wind/MFI",
"MagneticField",
[
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
"Earth.Magnetosphere.Main"
],
"",
"",
"Note comments about versioning in the text description above",
"Magnetic field",
"2023-09-18T00:00:00",
"https://doi.org/10.48322/s1d0-5q92",
"Wind Magnetic Field Investigation (MFI) Composite Data in RTN Coordinates",
"",
"User will acknowledge the Wind MFI instrument team, and the site from which data are pulled, in any publication resulting from the use of these data.",
"PT3S",
"1994-11-12T16:00:00Z",
"",
"",
"2.6.0"
],
[
"WI_H3_SWE",
"spase://NASA/NumericalData/Wind/SWE/H3/PT12S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Heliosphere.Inner",
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],
"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/xdpr-7352",
"Wind Solar Wind Experiment (SWE) Electron Pitch-Angle Distributions (12-15s rate) (New Mode)",
"WI_H3_SWE_v01",
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT12S",
"2002-08-16T00:00:00Z",
"",
"Ranges from instrument reconfiguration up to present.",
"2.3.2"
],
[
"WI_H4-RTN_MFI",
"spase://NASA/NumericalData/Wind/MFI/RTN/PT0.092S",
"spase://SMWG/Instrument/Wind/MFI",
"MagneticField",
[
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"Earth.Magnetosheath",
"Earth.Magnetosphere",
"Earth.Magnetosphere.Magnetotail",
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"",
"",
"Note comments about versioning in the text description above",
"",
"2023-09-18T00:00:00",
"https://doi.org/10.48322/s1kf-0b54",
"Wind Magnetic Field Investigation (MFI) Full Resolution Data in RTN Coordinates",
"",
"User will acknowledge the Wind MFI instrument team, and the server from which the data were accessed, in any publication resulting from the use of these data.",
"PT0.092S",
"1994-11-12T16:00:00Z",
"",
"",
"2.6.0"
],
[
"WI_H4_SWE",
"spase://NASA/NumericalData/Wind/SWE/H4/PT06S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
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"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/wx5n-w132",
"Wind Solar Wind Experiment (SWE) Electron Pitch-Angle Distributions (6-12s rate) (VEIS-era Mode)",
"WI_H4_SWE_v01",
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT06S",
"1994-11-30T00:00:00Z",
"2001-07-10T00:00:35Z",
"Ranges from instrument commissioning up to reconfiguration.",
"2.3.2"
],
[
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"spase://NASA/NumericalData/Wind/SWE/H5/PT12S",
"spase://SMWG/Instrument/Wind/SWE",
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"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/chaz-z942",
"Wind Solar Wind Experiment (SWE) Electron Quadrature Moments Parameters (12-15s rate) (New Mode)",
"WI_H5_SWE_v01",
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT12S",
"2002-08-16T00:00:00Z",
"",
"Ranges from instrument reconfiguration up to present.",
"2.3.2"
],
[
"WI_K0_3DP",
"spase://NASA/NumericalData/Wind/3DP/KP/PT92S",
"spase://SMWG/Instrument/Wind/3DP",
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"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/kwfz-zk29",
"Wind 3DP 92-sec Key Parameter Data",
"",
"User will acknowledge the Wind 3DP Team in any publication resulting from use of this data.",
"PT92S",
"1994-11-15T12:53:43Z",
"",
"",
"2.3.2"
],
[
"WI_K0_EPA",
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"spase://SMWG/Instrument/Wind/EPACT",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/x9am-dd03",
"Wind Energetic Particle Acceleration, Composition and Transport (EPACT) 92s KP Fluxes",
"",
"Dr. Tycho T. Von Rosenvinge",
"PT92S",
"1994-11-16T00:00:00",
"",
"",
"2.3.2"
],
[
"WI_K0_MFI",
"spase://NASA/NumericalData/Wind/MFI/KeyParameter/PT92S",
"spase://SMWG/Instrument/Wind/MFI",
[
"Ephemeris",
"InstrumentStatus",
"MagneticField"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/pxak-n392",
"Wind Magnetic Fields Instrument (MFI) Magnetic Field Vector and Spacecraft Position, Key Parameter (K0), 92 s Data",
"",
"Please acknowledge the Principal Investigator R.P. Lepping for use of the Data",
"PT92S",
"2017-07-01T00:00:00.000",
"2019-01-18T23:59:20.000",
"",
"2.3.2"
],
[
"WI_K0_SMS",
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[
"spase://SMWG/Instrument/Wind/SMS/STICS",
"spase://SMWG/Instrument/Wind/SMS/SWICS"
],
[
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"IonComposition"
],
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"",
"Calibrated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/wms0-rv35",
"Wind SMS Key Parameter 4-hour Data",
"",
"Principle Investigator G. Gloeckler and the Wind team",
"PT4H",
"1994-12-12T00:00:00",
"2000-05-27T23:59:59",
"",
"2.3.2"
],
[
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"spase://SMWG/Instrument/Wind/Ephemeris",
[
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"InstrumentStatus"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/0qwn-gj84",
"Wind Ephemeris, Spacecraft Spin Phase, Key Parameter (K0), 92 s Data",
"",
"Please acknowledge the Principal Investigator R.A. Hoffman for use of the Data",
"PT92S",
"1994-11-01T09:06:02.000",
"2019-01-18T23:58:35.000",
"",
"2.3.2"
],
[
"WI_K0_SWE",
"spase://NASA/NumericalData/Wind/SWE/IonMoments/KeyParameter/PT99S",
"spase://SMWG/Instrument/Wind/SWE",
[
"Ephemeris",
"InstrumentStatus",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calculated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/3zky-gy15",
"Wind Solar Wind Experiment (SWE) Thermal Plamsa Moments, Key Parameter (K0), 99 s Data",
"",
"Please acknowledge the Principal Investigator K.W. Ogilvie for use of the Data",
"PT99S",
"1994-11-01T12:00:00.000",
"2019-01-18T23:58:49.000",
"",
"2.3.2"
],
[
"WI_K0_WAV",
"spase://NASA/NumericalData/Wind/WAVES/ElectricFieldIntensity/KeyParameter/PT3M",
"spase://SMWG/Instrument/Wind/WAVES",
[
"ElectricField",
"InstrumentStatus",
"ThermalPlasma"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Calibrated",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/mfc5-cc53",
"Wind Plasma and Radio Waves (WAVES) Electric Field Intensities and Electron Plasma Densities, Key Parameter (K0), 3 min Data",
"",
"Please acknowledge the Principal Investigator M.L. Kaiser for use of the Data",
"PT3M",
"1994-11-10T00:01:30.000",
"2019-01-18T23:58:30.000",
"",
"2.3.2"
],
[
"WI_L2-1HOUR-SEP_EPACT-APE_B",
"spase://NASA/NumericalData/Wind/EPACT/SEP/PT1H",
"spase://SMWG/Instrument/Wind/EPACT",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/k50r-er56",
"Wind Energetic Particle Acceleration, Composition and Transport (EPACT) APE-B Telescope Proton Fluxes 18.90 to 21.90 MeV, Level 2, 1 hr Data",
"",
"T.T. Von Rosenvinge, D.V. Reames",
"PT1H",
"1994-01-01T00:00:00.000",
"2016-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"WI_L2-1HOUR-SEP_EPACT-LEMT",
"spase://NASA/NumericalData/Wind/EPACT/LEMT/L2/PT1H",
"spase://SMWG/Instrument/Wind/EPACT",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2025-08-05T13:13:00Z",
"https://doi.org/10.48322/n0f2-3519",
"Wind EPACT/LEMT 1-Hr He,C,O,Ne,Si,Fe Solar Energetic Particle Intensities Level 2 Data",
"",
"Dr. Tycho T. Von Rosenvinge",
"PT1H",
"1994-11-03T00:00:00.000Z",
"",
"",
"2.7.0"
],
[
"WI_L2-30MIN_SMS-STICS-AFM-MAGNETOSPHERE",
"spase://NASA/NumericalData/Wind/SMS/STICS/AngularFluxMap/Level2/Magnetosphere/PT30M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
"Earth.Magnetosphere",
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/f2m8-ex57",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Angular Flux Maps (AFMs), Level 2 (L2), 30-minute Data in Magnetosphere",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT30M",
"1995-08-01T00:05:19.000",
"2004-04-28T23:37:06.000",
"",
"2.6.0"
],
[
"WI_L2-30MIN_SMS-STICS-AFM-SOLARWIND",
"spase://NASA/NumericalData/Wind/SMS/STICS/AngularFluxMap/Level2/SolarWind/PT30M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/57np-qg69",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Angular Flux Maps (AFMs), Level 2 (L2), 30-minute Data in Solar Wind",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT30M",
"1995-01-01T00:07:11.000",
"",
"",
"2.6.0"
],
[
"WI_L2-30MIN_SMS-STICS-ERPA-MAGNETOSPHERE",
"spase://NASA/NumericalData/Wind/SMS/STICS/EnergyResolvedPitchAngleDistribution/Level2/Magnetosphere/PT30M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
"Earth.Magnetosphere",
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/s1x2-0h63",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Energy-Resolved Pitch-Angle Distributions (ERPAs), Level 2 (L2), 30-minute Data in Magnetosphere",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT30M",
"1995-08-01T00:05:19.000",
"2004-04-28T23:37:06.000",
"",
"2.6.0"
],
[
"WI_L2-30MIN_SMS-STICS-ERPA-SOLARWIND",
"spase://NASA/NumericalData/Wind/SMS/STICS/EnergyResolvedPitchAngleDistribution/Level2/SolarWind/PT30M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/yd5h-ty18",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Energy-Resolved Pitch-Angle Distributions (ERPAs), Level 2 (L2), 30-minute Data in Solar Wind",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT30M",
"1995-01-01T00:07:11.000",
"",
"",
"2.6.0"
],
[
"WI_L2-3MIN_SMS-STICS-VDF-MAGNETOSPHERE",
"spase://NASA/NumericalData/Wind/SMS/STICS/DistributionFunction/Level2/Magnetosphere/PT3M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
"Earth.Magnetosphere",
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/bm5n-eg33",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Velocity Distribution Functions (VDFs), Level 2 (L2), 3-minute Data in Magnetosphere",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT3M",
"1995-08-01T00:05:19.000",
"2004-04-28T23:55:32.000",
"",
"2.6.0"
],
[
"WI_L2-3MIN_SMS-STICS-VDF-SOLARWIND",
"spase://NASA/NumericalData/Wind/SMS/STICS/DistributionFunction/Level2/SolarWind/PT3M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/h28x-0w82",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Velocity Distribution Functions (VDFs), Level 2 (L2), 3-minute Data in Solar Wind",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT3M",
"1995-01-01T00:07:11.000",
"",
"",
"2.6.0"
],
[
"WI_L2-5MIN-SEP_EPACT-LEMT",
"spase://NASA/NumericalData/Wind/EPACT/LEMT/L2/PT5M",
"spase://SMWG/Instrument/Wind/EPACT",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/5jq3-gs16",
"Wind EPACT/LEMT 5-min key parameter flux data",
"",
"Dr. Tycho T. Von Rosenvinge",
"PT5M",
"1994-11-16T00:00:00",
"",
"",
"2.3.2"
],
[
"WI_L2_3MIN_SMS-STICS-NVT-MAGNETOSPHERE",
"spase://NASA/NumericalData/Wind/SMS/STICS/Moments/Level2/Magnetosphere/PT3M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
"Earth.Magnetosphere",
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/wnzt-eh29",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Moments, Level 2 (L2), 3-minute Data in Magnetosphere",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT3M",
"1995-08-01T00:05:19.000",
"2004-04-28T23:55:32.000",
"",
"2.6.0"
],
[
"WI_L2_3MIN_SMS-STICS-NVT-SOLARWIND",
"spase://NASA/NumericalData/Wind/SMS/STICS/Moments/Level2/SolarWind/PT3M",
"spase://SMWG/Instrument/Wind/SMS/STICS",
"IonComposition",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"Level 2",
"",
"",
"2024-03-14T00:00:00",
"https://doi.org/10.48322/2mh5-qw88",
"Wind SMS Suite SupraThermal Ion Composition Spectrometer (SMS/STICS) Ion Moments, Level 2 (L2), 3-minute Data in Solar Wind",
"",
"Please acknowledge the Principal Investigator S. T. Lepri for use of the Data",
"PT3M",
"1995-01-01T00:07:11.000",
"",
"",
"2.6.0"
],
[
"WI_L3-DUSTIMPACT_WAVES",
"spase://NASA/NumericalData/Wind/WAVES/DustImpact/PT1S",
"spase://SMWG/Instrument/Wind/WAVES",
"ElectricField",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/635a-nc73",
"Wind Plasma and Radio Waves (WAVES) Time Domain Sampler (TDS) Dust Impact, Level 3, 1 s Data",
"",
"D.M. Malaspina, L.B. Wilson III, R.J. MacDowall, We would like to thank the Wind/WAVES team, especially Keith Goetz, Paul J. Kellogg, Kris Kersten, and Josh Lynch for their Support with Data Retrieval and Calibration. Please Cite or Reference the Wind WAVES Paper by J.-L. Bougeret et al., 1995 in Space Sci. Rev. and Work by D.M. Malaspina et al., 2014 in Geophys. Res. Lett., doi:10.1002/2013GL058786. We would also appreciate a Reference to the Wind Dust Impact Database Paper: D.M. Malaspina et al., 2016, in J. Geophys. Res., doi:10.1002/2016JA023209.",
"PT1S",
"1995-01-01T00:00:00.000",
"2016-01-01T23:59:59.999",
"",
"2.3.2"
],
[
"WI_M0_SWE",
"spase://NASA/NumericalData/Wind/SWE/M0/PT12S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Heliosphere.Inner",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/jsqc-vm88",
"Wind Solar Wind Experiment (SWE) Averaged Electron Pitch Angle Distribution (12-15s rate)",
"WI_M0_SWE_v01",
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT12S",
"2002-08-16T00:00:00Z",
"",
"Time span ranges from instrument reconfiguration up to present.",
"2.3.2"
],
[
"WI_M2_SWE",
"spase://NASA/NumericalData/Wind/SWE/M2/PT06S",
"spase://SMWG/Instrument/Wind/SWE",
"ThermalPlasma",
[
"Heliosphere.NearEarth",
"Heliosphere.Inner",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"Solar Wind Plasma",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/dq7x-fd74",
"Wind Solar Wind Experiment (SWE) Averaged Electron Pitch Angle Distribution (6-12s rate)",
"WI_M2_SWE_v01",
"Please acknowledge the Wind/SWE electron instrument team and NASA/GSFC.",
"PT06S",
"1994-12-29T00:00:00Z",
"2001-07-09T23:59:59Z",
"Ranges from instrument commissioning up to reconfiguration.",
"2.3.2"
],
[
"WI_OR_DEF",
"spase://NASA/NumericalData/Wind/Ephemeris/definitive/PT10M",
"spase://SMWG/Instrument/Wind/Ephemeris",
"Ephemeris",
[
"Heliosphere",
"Heliosphere.NearEarth",
"Heliosphere.Inner"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/t0jm-c908",
"Wind Definitive Orbit, 10 min Data, Spacecraft Position and Velocity in GCI, GSE, GSM, HEC, and HG Coordinates",
"",
"",
"PT10M",
"1994-11-01T10:47:18Z",
"1997-07-01T23:50:00Z",
"",
"2.3.2"
],
[
"WI_OR_PRE",
"spase://NASA/NumericalData/Wind/Ephemeris/predicted/PT10M",
"spase://SMWG/Instrument/Wind/Ephemeris",
"Ephemeris",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2025-08-05T13:13:00Z",
"https://doi.org/10.48322/73de-sf52",
"Wind predicted Spacecraft Positions, 10 min Data",
"",
"",
"PT10M",
"1997-04-06T00:00:00Z",
"",
"",
"2.7.0"
],
[
"WI_PLSP_3DP",
"spase://NASA/NumericalData/Wind/3DP/PLSP/PT24S",
"spase://SMWG/Instrument/Wind/3DP",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/c4mf-9n52",
"Wind 3DP 24-sec Ion OmniDirectional Fluxes and Moments",
"",
"User will acknowledge the Wind 3DP Team in any publication resulting from use of this data.",
"PT24S",
"1994-11-15T12:53:43Z",
"",
"",
"2.3.2"
],
[
"WI_PM_3DP",
"spase://NASA/NumericalData/Wind/3DP/PM/PT03S",
"spase://SMWG/Instrument/Wind/3DP",
"ThermalPlasma",
"Heliosphere.NearEarth",
"",
"1",
"Users of these data are advised that higher quality, but lower time resolution, proton moment data are available in the Wind/3DP PLSP data product.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/s8e6-aw08",
"Wind 3DP PESA Moments Data",
"",
"User will acknowledge the Wind 3DP Team in any publication resulting from use of this data.",
"PT03S",
"1994-11-15T12:53:43Z",
"",
"",
"2.3.2"
],
[
"WI_SFPD_3DP",
"spase://NASA/NumericalData/Wind/3DP/SST_Foil/PD/PT24S",
"spase://SMWG/Instrument/Wind/3DP",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"General Notes per Lynn Wilson Jan 2015: The solid-state telescope (SST) for Wind 3DP electrons returns a velocity distribution function containing 7 energy bins and 48 solid-angle bins. The automated CDF routine appears to remove all the following solid-angle bins: [7,8,9,15,31,32,33] = sun/anti-sun look directions, and [20,21,22,23,44,45,46,47] = low geometry factor bins (also correspond to the SST Thick anti-coincidence detector bins). The sun/anti-sun directions are removed to avoid X-ray and EUV contamination, which is often seen during solar flares. The onset looks exactly like the GOES X-ray observations, which is kind of fun but not what we want to look at. Unfortunately, these look directions can correspond to the magnetic field direction, which can limit the times when we would like to examine SEP events. General Notes per Lynn Wilson Jan 2015: Note that SST Open (e.g., wi_sopd_3dp_00000000_v01.cdf) software removes the following additional solid-angle bins: [0,1,24,25] = noisy. Additionally, SST Open has 9 energy channels from ~70 keV to ~6.7 or 7.1 MeV, depending on the mode the instrument is in. It does not appear that the routine mk_sosp_cdf.pro removes any of these ...bad... look directions, so that should be noted as well. General Notes per Lynn Wilson Jan 2015: Inside the radiation belts, both Foil and Open saturate and suffer from penetrating particles. The instruments are not shielded, so they can only provide relative changes when in these regions. General Notes per Lynn Wilson Jan 2015: The data all look like they are in units of number flux or # cm-2 s-1 sr-1 eV-1.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/aawb-c884",
"Wind 3DP SST Foil Electron Energy-Angle Distributions",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT24S",
"1994-11-15T12:56:18.000Z",
"",
"",
"2.3.2"
],
[
"WI_SFSP_3DP",
"spase://NASA/NumericalData/Wind/3DP/SST_Foil/SP/PT24S",
"spase://SMWG/Instrument/Wind/3DP",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"General Notes per Lynn Wilson Jan 2015: The solid-state telescope (SST) for Wind 3DP electrons returns a velocity distribution function containing 7 energy bins and 48 solid-angle bins. The automated CDF routine appears to remove all the following solid-angle bins: [7,8,9,15,31,32,33] = sun/anti-sun look directions, and [20,21,22,23,44,45,46,47] = low geometry factor bins (also correspond to the SST Thick anti-coincidence detector bins). The sun/anti-sun directions are removed to avoid X-ray and EUV contamination, which is often seen during solar flares. The onset looks exactly like the GOES X-ray observations, which is kind of fun but not what we want to look at. Unfortunately, these look directions can correspond to the magnetic field direction, which can limit the times when we would like to examine SEP events. General Notes per Lynn Wilson Jan 2015: Note that SST Open (e.g., wi_sopd_3dp_00000000_v01.cdf) software removes the following additional solid-angle bins: [0,1,24,25] = noisy. Additionally, SST Open has 9 energy channels from ~70 keV to ~6.7 or 7.1 MeV, depending on the mode the instrument is in. It does not appear that the routine mk_sosp_cdf.pro removes any of these ...bad... look directions, so that should be noted as well. General Notes per Lynn Wilson Jan 2015: Inside the radiation belts, both Foil and Open saturate and suffer from penetrating particles. The instruments are not shielded, so they can only provide relative changes when in these regions. General Notes per Lynn Wilson Jan 2015: The data below all look like they are in units of number flux or # cm-2 s-1 sr-1 eV-1. I believe the CDAWeb units are correct for most of these.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/wd3x-9a34",
"Wind 3DP SST Foil Electron Omnidirectional Fluxes",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT24S",
"1994-11-15T12:56:18.000Z",
"",
"",
"2.3.2"
],
[
"WI_SOPD_3DP",
"spase://NASA/NumericalData/Wind/3DP/SST_Open/PD/PT24S",
"spase://SMWG/Instrument/Wind/3DP",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/yw1c-yf03",
"Wind 3DP SST Open Proton Energy-Angle Distributions",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT24S",
"1994-11-15T12:56:18.000Z",
"",
"",
"2.3.2"
],
[
"WI_SOSP_3DP",
"spase://NASA/NumericalData/Wind/3DP/SST_Open/SP/PT24S",
"spase://SMWG/Instrument/Wind/3DP",
"EnergeticParticles",
"Heliosphere.NearEarth",
"",
"",
"General Notes per Lynn Wilson Jan 2015: The solid-state telescope (SST) for Wind 3DP electrons returns a velocity distribution function containing 7 energy bins and 48 solid-angle bins. The automated CDF routine appears to remove all the following solid-angle bins: [7,8,9,15,31,32,33] = sun/anti-sun look directions, and [20,21,22,23,44,45,46,47] = low geometry factor bins (also correspond to the SST Thick anti-coincidence detector bins). The sun/anti-sun directions are removed to avoid X-ray and EUV contamination, which is often seen during solar flares. The onset looks exactly like the GOES X-ray observations, which is kind of fun but not what we want to look at. Unfortunately, these look directions can correspond to the magnetic field direction, which can limit the times when we would like to examine SEP events. General Notes per Lynn Wilson Jan 2015: Note that SST Open (e.g., wi_sopd_3dp_00000000_v01.cdf) software removes the following additional solid-angle bins: [0,1,24,25] = noisy. Additionally, SST Open has 9 energy channels from ~70 keV to ~6.7 or 7.1 MeV, depending on the mode the instrument is in. It does not appear that the routine mk_sosp_cdf.pro removes any of these ...bad... look directions, so that should be noted as well. General Notes per Lynn Wilson Jan 2015: Inside the radiation belts, both Foil and Open saturate and suffer from penetrating particles. The instruments are not shielded, so they can only provide relative changes when in these regions. General Notes per Lynn Wilson Jan 2015: The data below all look like they are in units of number flux or # cm-2 s-1 sr-1 eV-1. I believe the CDAWeb units are correct for most of these.",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/wkk0-y398",
"Wind 3DP SST Open Proton Omniderectional Fluxes",
"",
"Principle Investigators Robert Lin and Stuart Bale, the Wind 3DP team, and the Space Physics Data Facility (SPDF)/NASA GSFC",
"PT24S",
"1994-11-15T12:56:18.000Z",
"",
"",
"2.3.2"
],
[
"WI_STRAHL0_SWE",
"spase://NASA/NumericalData/Wind/SWE/Strahl/PT12S",
"spase://SMWG/Instrument/Wind/SWE",
"EnergeticParticles",
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/4mxn-2e20",
"Wind Solar Wind Experiment (SWE) Strahl Detector Two Dimensional Electron Angular Distributions, (H4), 12 s Data",
"",
"K. Ogilvie",
"PT12S",
"1995-01-01T00:00:00.000",
"2001-05-30T23:59:59.999",
"",
"2.3.2"
],
[
"WI_SW-ION-DIST_SWE-FARADAY",
"spase://NASA/NumericalData/Wind/SWE/FaradayCup/IonDistribution/PT92S",
"spase://SMWG/Instrument/Wind/SWE",
[
"ElectricField",
"EnergeticParticles",
"InstrumentStatus"
],
[
"Heliosphere",
"Heliosphere.Inner",
"Heliosphere.NearEarth",
"Earth.Magnetosheath",
"Earth.Magnetosphere.Magnetotail"
],
"",
"",
"",
"",
"2021-05-31T12:34:56.789",
"https://doi.org/10.48322/6vrg-6n41",
"Wind Solar Wind Experiment (SWE) Faraday Cup, Solar Wind Plasma Reduced Ion Distribution Functions, 92 s Data",
"",
"Please acknowledge the PI K.W. Ogilvie, NASA GSFC, 301-286-5904, Keith.W.Ogilvie@nasa.gov, and A.J. Lazarus, MIT, 617-253-4284, ajl@space.mit.edu.",
"PT92S",
"1994-11-17T19:50:45.000",
"2018-12-24T23:58:47.000",
"",
"2.3.2"
]
]
}