MAVEN (Multiple Instrument Ensemble) In-situ Observations, Data Product Bundle, Key Parameter (KP), 4 s Data

Added DOI and PublicationInfo minted by LFB, metadata versioned up to SPASE 2.6.0, reviewed by LFB 20230727

The MAVEN In-situ Calibrated Level 2, L2, Science Data Bundle contains selected fully calibrated Data from the Neutral Gas and Ion Mass Spectrometer, NGIMS, Instrument and the Particles and Fields Package together with Ephemeris Information. The Particle and Fields In-situ Instrument Data are from the Extreme Ultraviolet, EUV, Langmuir Probe and Waves, LPW, Antenna, Magnetometer, MAG, Solar Energetic Particles, SEP, SupraThermal And Thermal Ion Composition, STATIC, Solar Wind Electron Analyzer, SWEA, and Solar Wind Ion Analyzer, SWIA, Instruments. All of these Data are in Physical Units and are averaged and/or sampled at a uniform 4 s Cadence. These In-situ Data are derived directly from the Level 2 Data. The Ephemeris Data are derived by using SPICE Libraries and Kernels provided by MAVEN Navigation, NAV, Team and Lockheed-Martin.

Please acknowledge the following: B.M. Jakosky, MAVEN Principal Investigator, J.G. Luhmann, MAVEN Principal Investigator, J.M. Grebowsky, MAVEN Project Scientist, R.E. Ergun, LPW, LPW/EUV Principal Investigator, J.E.P. Connerney, MAG Principal Investigator, P.R. Mahaffy, NGIMS Principal Investigator, D. Larson, SEP Principal Investigator, J.P. McFadden, STATIC Principal Investigator, D.G. Mitchell, SWEA Principal Investigator, and N.M. Schneider, SWIA Principal Investigator

Jakosky, Bruce, M.; Luhmann, Janet, G.; Grebowsky, Joseph, M.; Ergun, Robert, E.; Connerney, John, E. P.; Mahaffy, Paul, R.; Larson, Davin; McFadden, James, P.; Mitchell, Donald, G.; Schneider, Nicholas, M.

The Mars Atmosphere and Volatile Evolution, MAVEN, Mission Home Page, LASP, UC Boulder

General Information about the Mars Atmosphere and Volatile Evolution, MAVEN, Mission, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder, UCB

The Mars Atmosphere and Volatile Evolution, MAVEN, Langmuir Probe and Waves Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Langmuir Probe and Waves Instrument Home Page, Laboratory for Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Langmuir Probe and Waves, LPW, Instrument Space Science Reviews Publication

Andersson, L., Ergun, R.E., Delory, G.T., Eriksson, A., Westfall, J., Reed, H., McCauly, J., Summers, D., and D. Meyers, The Langmuir Probe and Waves (LPW) Instrument for MAVEN, Space Sci. Rev., 195, 173-198, 2015

NSSDC Master Catalog Listing, MAVEN Langmuir Probe and Waves, LPW, Instrument

NSSDC Master Catalog Listing for the MAVEN Langmuir Probe and Waves, LPW, Instrument, NSSDCA/COSPAR ID: 2013-063A-04

The Mars Atmosphere and Volatile Evolution, MAVEN, Langmuir Probe and Waves, LPW, Extreme Ultraviolet Monitor Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Langmuir Probe and Waves, LPW, Extreme Ultraviolet Monitor Instrument Home Page, Laboratory for Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Langmuir Probe and Waves, LPW, Extreme Ultraviolet Monitor, EUV, Instrument Space Science Reviews Publication

Eparvier, F.G., Chamberlin, P.C., Woods, T.N., and E.M.B. Thiemann, The Solar Extreme Ultraviolet Monitor for MAVEN, Space Sci. Rev., 195, 293-301, 2015

NSSDC Master Catalog Listing, MAVEN Langmuir Probe and Waves, LPW, Extreme Ultraviolet Monitor, EUV, Instrument

NSSDC Master Catalog Listing for the MAVEN Langmuir Probe and Waves, LPW, Extreme Ultraviolet Monitor, EUV, Instrument, NSSDCA/COSPAR ID: 2013-063A-04

The Mars Atmosphere and Volatile Evolution, MAVEN, Magnetometer Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Magnetometer Instrument Home Page, Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder

MAVEN Magnetometer, MAG, Instrument Space Science Reviews Publication

Connerney, J.E.P., J. Espley, P. Lawton, S. Murphy, J. Odom, R. Oliversen, and D. Sheppard, The MAVEN Magnetic Field Investigation, Space Sci. Rev., 195, 257-291, 2015

NSSDC Master Catalog Listing, MAVEN Magnetometer, MAG, Instrument

NSSDC Master Catalog Listing for the MAVEN Magnetometer, MAG, Instrument, NSSDCA/COSPAR ID: 2013-063A-08

The Mars Atmosphere and Volatile Evolution, MAVEN, Neutral Gas and Ion Mass Spectrometer Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Neutral Gas and Ion Mass Spectrometer Instrument Home Page, Laboratory for Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Neutral Gas and Ion Mass Spectrometer, NGIMS, Instrument Space Science Reviews Publication

Mahaffy, P.R., Benna, M., King, T., Harpold, D.N., Arvey, R., Barciniak, M., Bendt, M., Carrigan, D., Errigo, T., Holmes, V., Johnson, C.S., Kellogg, J., Kimvilakani, P., Lefavor, M., Hengemihle, J., Jaeger, F., Lyness, E., Maurer, J., Melak, A., Noreiga, F., Noriega, M., Patel, K., Prats, B., Raaen, E., Tan, F., Weidner, E., Gundersen, C., Battel, S., Block, B.P., Arnett, K., Miller, R., Cooper, C., Edmonson, C., and J.T. Nolan,, The Neutral Gas and Ion Mass Spectrometer on the Mars Atmosphere and Volatile Evolution Mission, Space Sci. Rev., 195, 49-73, 2015

NSSDC Master Catalog Listing, MAVEN Neutral Gas and Ion Mass Spectrometer, NGIMS, Instrument

NSSDC Master Catalog Listing for the MAVEN Neutral Gas and Ion Mass Spectrometer, NGIMS, Instrument, NSSDCA/COSPAR ID: 2013-063A-02

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Energetic Particle Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Energetic Particle Instrument Home Page, Laboratory of Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Solar Energetic Particle, SEP, Instrument Space Science Reviews Publication

Larson, D.E., Lillis, R.J., Lee, C.O., Dunn, P.A., Hatch, K., Robinson, M., Glaser, D., Chen, J., Curtis, D., Tiu, C., Lin, R.P., Luhmann, J.G., and B.M. Jakosky, The MAVEN Solar Energetic Particle Investigation, Space Sci. Rev., 195, 153-172, 2015

NSSDC Master Catalog Listing, MAVEN Solar Energetic Particle, SEP, Instrument

NSSDC Master Catalog Listing for the MAVEN Solar Energetic Particle, SEP, Instrument, NSSDCA/COSPAR ID: 2013-063A-05

The Mars Atmosphere and Volatile Evolution, MAVEN, SupraThermal And Thermal Ion Composition Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, SupraThermal And Thermal Ion Composition Instrument Home Page, Laboratory of Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN SupraThermal And Thermal Ion Composition, STATIC, Instrument Space Science Reviews Publication

McFadden, J.P., Kortmann, O., Curtis, D., Dalton, G., Johnson, G., Abiad, R., Sterling, R., Hatch, K., Berg, P., Tiu, C., Gordon, D., Heavner, S., Robinson, M., Marckwordt, M., Lin, R., and B.M. Jakosky, MAVEN SupraThermal and Thermal Ion Compostion (STATIC) Instrument, Space Sci. Rev., 195, 199-256, 2015

NSSDC Master Catalog Listing, MAVEN SupraThermal And Thermal Ion Composition, STATIC, Instrument

NSSDC Master Catalog Listing for the MAVEN SupraThermal And Thermal Ion Composition, STATIC, Instrument, NSSDCA/COSPAR ID: 2013-063A-03

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Wind Electron Analyzer Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Wind Electron Analyzer Instrument Home Page, Laboratory of Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Solar Wind Electron Analyzer, SWEA, Instrument Space Science Reviews Publication

Mitchell, D.L., Mazelle, C., Sauvaud, J.-A., Thocaven, J.-J., Rouzaud, J., Fedorov, A., Rouger, P., Toublanc, D., Taylor, E., Gordon, D., Robinson, M., Heavner, S., Turin, P., Diaz-Aguado, M., Curtis, D.W., Lin, R.P., and B.M. Jakosky, The MAVEN Solar Wind Electron Analyzer, Space Sci. Rev., 200, 495-528, 2016

NSSDC Master Catalog Listing, MAVEN Solar Wind Electron Analyzer, SWEA, Instrument

NSSDC Master Catalog Listing for the MAVEN Solar Wind Electron Analyzer, SWEA, Instrument, NSSDCA/COSPAR ID: 2013-063A-07

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Wind Ion Analyzer Instrument Home Page, LASP, UC Boulder

The Mars Atmosphere and Volatile Evolution, MAVEN, Solar Wind Ion Analyzer Instrument Home Page, Laboratory for Atmospheric and Space Physics, LASP, University of Colorado, Boulder

MAVEN Solar Wind Ion Analyzer, SWIA, Instrument Space Science Reviews Publication

Halekas, J.S., Taylor, E.R., Dalton, G., Johnson, G., Curtis, D.W., McFadden, J.P., Mitchell, D.L., Lin, R.P., and B.M. Jakosky, The Solar Wind Ion Analyzer for MAVEN, Space Sci. Rev., 195, 125-151, 2015

NSSDC Master Catalog Listing, MAVEN Solar Wind Ion Analyzer, SWIA, Instrument

NSSDC Master Catalog Listing for the MAVEN Solar Wind Ion Analyzer, SWIA, Instrument, NSSDCA/COSPAR ID: 2013-063A-06

Please acknowledge the following: B.M. Jakosky, MAVEN Principal Investigator, J.G. Luhmann, MAVEN Principal Investigator, J.M. Grebowsky, MAVEN Project Scientist, R.E. Ergun, LPW, LPW/EUV Principal Investigator, J.E.P. Connerney, MAG Principal Investigator, P.R. Mahaffy, NGIMS Principal Investigator, D. Larson, SEP Principal Investigator, J.P. McFadden, STATIC Principal Investigator, D.G. Mitchell, SWEA Principal Investigator, and N.M. Schneider, SWIA Principal Investigator. Please acknowledge the Data Providers and CDAWeb when using these Data.

Epoch Time, Coordinated Universal Time, UTC, the Spacecraft Event Time, SCET, for each Data Record

The Epoch Time, UTC, is expressed the Time elapsed since 01-Jan-0000 00:00:00.000 without Leap Seconds with one Element per Ion Distribution (NUM_DISTS Elements) This Parameter exhibits an increasing Monotonic Progression

Derived from the LPW Sweep and when available from the Plasma Line

Electron Density, Minimum, Langmuir Probe and Waves, LPW, Antenna

Electron Density, Maximum, Langmuir Probe and Waves, LPW, Antenna

Electron Temperature, Minimum, Langmuir Probe and Waves, LPW, Antenna

Electron Temperature, Maximum, Langmuir Probe and Waves, LPW, Antenna

Spacecraft Potential, Minimum, Langmuir Probe and Waves, LPW, Antenna

Spacecraft Potential, Maximum, Langmuir Probe and Waves, LPW, Antenna

Electric Field Wave Power, 2 Hz to 100 Hz, Langmuir Probe and Waves, LPW, Antenna

Integrated Wave Power from the onboard calculated FFT for Frequencies that are important for Wave Heating

Electric Field Wave Power, 2 Hz to 100 Hz, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Antenna

This Data Quality Flag ranges in Value from 0 to 100, where 100 represents the highest Confidence Level, use Data with a Data Quality Flag greater than or equal to 50

Electric Field Wave Power, 100 Hz to 800 Hz, Langmuir Probe and Waves, LPW, Antenna

Electric Field Wave Power, 100 Hz to 800 Hz, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Antenna

Electric Field Wave Power, 800 Hz to 1000 Hz, Langmuir Probe and Waves, LPW, Antenna

Electric Field Wave Power, 800 Hz to 1000 Hz, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Antenna

EUV Irradiance Wave Power, 0.1 nm to 7.0 nm Bandpass, Langmuir Probe and Waves, LPW, Antenna Instrument, Extreme Ultraviolet, EUV, Detector

EUV Irradiance Wave Power, 0.1 nm to 7.0 nm, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Instrument, Extreme Ultraviolet, EUV, Detector

Data Quality Flag Value Definitions: 0=Good Solar, 1=Occultation, 2=No Pointing Info, 3=Sun not fully in Field of View, FOV, 4=Sun not in Field of View, FOV, 5=Windowed, 6=Eclipse, 7=Spare

EUV Irradiance Wave Power, 17 nm to 22 nm Bandpass, Langmuir Probe and Waves, LPW, Instrument, Extreme Ultraviolet, EUV, Detector

EUV Irradiance Wave Power, 17 nm to 22 nm, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Instrument, Extreme Ultraviolet, EUV, Detector

EUV Irradiance Wave Power Lyman-alpha Bandpass, Langmuir Probe and Waves, LPW, Instrument, Extreme Ultraviolet, EUV, Detector

EUV Irradiance Wave Power, Lyman-alpha, Data Quality Flag, DQ, Langmuir Probe and Waves, LPW, Instrument, Extreme Ultraviolet, EUV, Detector

Density of Solar Wind or Magnetosheath Electrons based on Moments of the Electron Distribution after correcting for the Spacecraft Potential

Solar Wind Electron Density, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Statistical Uncertainty, one Sigma, not including Systematic Error

Solar Wind Electron Temperature, Solar Wind Electron Analyzer, SWEA

Temperature of Solar Wind or Magnetosheath Electrons based on Moments of the Electron Distribution after correcting for the Spacecraft Potential

Solar Wind Electron Temperature, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Temperature Statistical Uncertainty, one Sigma, not including Systematic Error

Solar Wind Electron Energy Flux, Parallel, 5 eV to 100 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux parallel to the Magnetic Field Vector, 0° to 90° Pitch Angle

Solar Wind Electron Energy Flux, Parallel, 5 eV to 100 eV, DQ, SWEA

Solar Wind Electron Energy Flux, Parallel, 5 eV to 100 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Parallel, 100 eV to 500 eV, SWEA

Solar Wind Electron Energy Flux, Parallel, 100 eV to 500 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Parallel, 100 eV to 500 eV, SWEA, DQ

Solar Wind Electron Energy Flux, Parallel, 100 eV to 500 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Parallel, 500 eV to 1000 eV, SWEA

Solar Wind Electron Energy Flux, Parallel, 500 eV to 1000 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Parallel, 500 eV to 1000 eV, DQ, SWEA

Solar Wind Electron Energy Flux, Parallel, 500 eV to 1000 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 5 eV to 100 eV, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 5 eV to 100 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux antiparallel to the Magnetic Field Vector, 90° to 180° Pitch Angl)

Solar Wind Electron Energy Flux, Antiparallel, 5 eV to 100 eV, DQ, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 5 eV to 100 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 100 eV to 500 eV, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 100 eV to 500 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux antiparallel to the Magnetic Field Vector, 90° to 180° Pitch Angle

Solar Wind Electron Energy Flux, Antiparallel, 100 eV to 500 eV, DQ, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 100 eV to 500 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 500 eV to 1000 eV, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 500 eV to 1000 eV, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 500 eV to 1000 eV, DQ, SWEA

Solar Wind Electron Energy Flux, Antiparallel, 500 eV to 1000 eV, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Spectrum Shape Parameter, Solar Wind Electron Analyzer, SWEA

Solar Wind Electron Energy Spectrum Shape Parameter used to distingush between Ionospheric Photoelectrons and Solar Wind Electrons

Solar Wind Electron Energy Spectrum Shape Parameter, Data Quality Flag, DQ, Solar Wind Electron Analyzer, SWEA

Solar Wind Total Ion Number Density from Onboard Moment Calculation, assuming 100% Protons, Solar Wind Ion Analyzer, SWIA

Solar Wind Total Ion Number Density, Data Quality Flag, DQ, Solar Wind Ion Analyzer, SWIA

Data Quality Flag: 0=Bad, 1=Good, the Flag indicates whether the Distribution is well-measured and the Decommutation Parameters are Definite

Solar Wind Bulk Ion Flow Velocity, Cartesian Coordinates, from Onboard Moment Calculation, assuming 100% Protons, Solar Wind Ion Analyzer, SWIA

Solar Wind Bulk Ion Flow Velocity, Cartesian Coordinates, Data Quality Flag, DQ, Solar Wind Ion Analyzer, SWIA

Solar Wind Scalar Ion Temperature from Onboard Moment Calculation, assuming 100% Protons, Solar Wind Ion Analyzer, SWIA

Solar Wind Scalar Ion Temperature, Data Quality Flag, DQ, Solar Wind Ion Analyzer, SWIA

Solar Wind Ion Dynamic Pressure computed on the Ground from Density and Velocity Moments, assuming 100% Protons, Solar Wind Ion Analyzer, SWIA

Solar Wind Ion Dynamic Pressure, Data Quality Flag, DQ, Solar Wind Ion Analyzer, SWIA

Data Quality Flag Definitions: 0=Bad, 1=Good, the Flag indicates whether the Distribution is well-measured and the Decommutation Parameters are Definite

Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Integer Flag Bits: Valid=0, Flag=1. See the SIS Key Parameter Data Product Description for Bit Descriptions. This Parameter is formatted as a Floating Point Number in order to include NaN Values for Data Gaps.

Proton, H⁺, Number Density, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Number Density below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Proton, H⁺, Number Density, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Number Density, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Number Density below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Singly charged Oxygen Ion, O⁺, Number Density, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Number Density, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Number Density below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Doubly charged Oxygen Ion, O⁺², Number Density, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Ram Temperature, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Ram Temperature below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Proton, H⁺, Ram Temperature, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Ram Temperature, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Ram Temperature below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Singly charged Oxygen Ion, O⁺, Ram Temperature, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺⁺, Ram Temperature, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺⁺, Ram Temperature below a to be determined, TBD, Altitude determined from Application ID, APID, c6, 32 Energies ⨯ 64 Masses, while in Ram Mode or Conic Mode

Doubly charged Oxygen Ion, O⁺², Ram Temperature, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², MAVEN Articulated Payload Platform, MAVEN_APP, Flow Velocity, Cartesian Coordinates, below a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Ram Mode or Conic Mode, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², MAVEN_APP Flow Velocity, DQ, STATIC

Doubly charged Oxygen Ion, O⁺², MAVEN Articulated Payload Platform, MAVEN_APP, Flow Velocity, Cartesian Coordinates, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Flow Velocity, Mars Solar Orbital, MSO, Cartesian Coordinates, below a to be determined, TBD, Altitude while in Ram Mode or Conic Mode, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Flow Velocity, Mars Solar Orbital, MSO, Cartesian Coordinates, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Omnidirectional Flux, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Omnidirectional Flux above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Proton, H⁺, Characteristic Energy, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Omnidirectional Characteristic Energy above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Proton, H⁺, Characteristic Energy, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Helium Ion, He⁺, Omnidirectional Flux, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Helium Ion, He⁺, Omnidirectional Flux above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Singly charged Helium Ion, He⁺, Omnidirectional Characteristic Energy, STATIC

Singly charged Helium Ion, He⁺, Omnidirectional Characteristic Energy, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Helium Ion, He⁺, Omnidirectional Characteristic Energy above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Singly charged Helium Ion, He⁺, Omnidirectional Characteristic Energy, DQ, STATIC

Singly charged Helium Ion, He⁺, Omnidirectional Characteristic Energy, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Omnidirectional Flux, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Omnidirectional Flux above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Singly charged Oxygen Ion, O⁺, Omnidirectional Characteristic Energy, STATIC

Singly charged Oxygen Ion, O⁺, Omnidirectional Characteristic Energy, SupraThermal And Thermal Ion Composition, STATIC

Singly charged Oxygen Ion, O⁺, Omnidirectional Characteristic Energy above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Singly charged Oxygen Ion, O⁺, Omnidirectional Characteristic Energy, DQ, STATIC

Singly charged Oxygen Ion, O⁺, Omnidirectional Characteristic Energy, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Omnidirectional Flux, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Omnidirectional Flux above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Doubly charged Oxygen Ion, O⁺², Omnidirectional Characteristic Energy, STATIC

Doubly charged Oxygen Ion, O⁺², Omnidirectional Characteristic Energy, SupraThermal And Thermal Ion Composition, STATIC

Doubly charged Oxygen Ion, O⁺², Omnidirectional Characteristic Energy above a to be determined, TBD, Altitude determined from Application ID, APID, c6 while in Pickup, Eclipse and Protect Mode

Doubly charged Oxygen Ion, O⁺², Omnidirectional Characteristic Energy, DQ, STATIC

Doubly charged Oxygen Ion, O⁺², Omnidirectional Characteristic Energy, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Characteristic Direction Vector in Mars Solar Orbital, MSO, Coordinates for the Flux measured above a to be determined, TBD, Altitude determined from a to be determined, TBD, Application ID, APID, while in Pickup and Scan Mode, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Characteristic Angular Width, SupraThermal And Thermal Ion Composition, STATIC

Proton, H⁺, Flux Angular Width above a to be determined, TBD, Altitude determined from a to be determined, TBD, Application ID, APID, while in Pickup and Scan Mode

Proton, H⁺, Characteristic Angular Width, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Dominant Pickup Ion, Characteristic Direction Vector, MSO, STATIC

Dominant Pickup Ion, Characteristic Direction Vector in Mars Solar Orbital, MSO, Coordinates for the Flux measured above a to be determined, TBD, Altitude determined from a to be determined, TBD, Application ID, APID, while in Pickup and Scan Mode, SupraThermal And Thermal Ion Composition, STATIC

Dominant Pickup Ion, XYZ-direction of Flux in Mars Solar Orbital, MSO, Coordinates for the Flux measured above a to be determined, TBD, Altitude determined from the Application ID, APID, D0 and CE while in Pickup Mode, Eclipse Mode, or Protect Mode

Dominant Pickup Ion Characteristic Angular Width, SupraThermal And Thermal Ion Composition, STATIC

Dominant Pickup Ion Flux Angular Width above a to be determined, TBD, Altitude determined from the Application ID, APID, D0 and CE while in Pickup Mode, Eclipse Mode, or Protect Mode

Dominant Pickup Ion Characteristic Angular Width, Data Quality Flag, DQ, SupraThermal And Thermal Ion Composition, STATIC

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 1-Forward, Solar Energetic Particles, SEP

Number Flux of Ions, integrated over the Energy Range from 0.03 MeV to 1.0 MeV

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 1-Forward, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Standard Uncertainty in Total Ion Flux, based on Poisson Statistics

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 1-Reverse, Solar Energetic Particles, SEP

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 1-Reverse, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 2-Forward, Solar Energetic Particles, SEP

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 2-Forward, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 2-Reverse, Solar Energetic Particles, SEP

Ion Energy Flux, 30 keV to 1000 keV, Field of View, FOV, 2-Reverse, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 1-Forward, Solar Energetic Particles, SEP

Number Flux of Electrons, integrated over the Energy Range from 30 keV to 300 keV

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 1-Forward, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Standard Uncertainty in Total Electron Flux, based on Poisson Statistics

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 1-Reverse, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 1-Reverse, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 2-Forward, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 2-Forward, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 2-Reverse, Solar Energetic Particles, SEP

Electron Energy Flux, 30 keV to 300 keV, Field of View, FOV, 2-Reverse, Data Quality Flag, DQ, Solar Energetic Particles, SEP

Look Direction, 1-Forward, Mars Solar Orbital, MSO, Cartesian Coordinates, Solar Energetic Particles, SEP

Look Direction, 1-Reverse, MSO, Cartesian Coordinates, Solar Energetic Particles, SEP

Look Direction, 2-Forward, MSO, Cartesian Coordinates, Solar Energetic Particles, SEP

Look Direction, 2-Reverse, MSO, Cartesian Coordinates, Solar Energetic Particles, SEP

Magnetic Field Vector, Mars Solar Orbital, MSO, Cartesian Coordinates, Magnetometer, MAG

Magnetic Field Vector, Mars Solar Orbital, MSO, Cartesian Coordinates, Data Quality Flag, DQ, Magnetometer, MAG

Magnetic Field Vector, Geographic, GEO, Cartesian Coordinates, Magnetometer, MAG

Magnetic Field Vector, Geographic, GEO, Cartesian Coordinates, Data Quality Flag, DQ, Magnetometer, MAG

Magnetic Field Deviation from the Mean Magnitude of the Magnetic Field, Magnetometer, MAG

Magnetic Field Deviation from the Mean Magnitude of the Magnetic Field, Data Quality Flag, Magnetometer, MAG

Neutral Helium, He, Number Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Helium, He, Number Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

He Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

NIV=Neutral Inbound Verified, NIU=Neutral Inbound Unverified, NOV=Neutral Outbound Verified, NOU=Neutral Outbound Unverified

Neutral Oxygen, O Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Oxygen, O Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Oxygen, O Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Carbon Monoxide, CO Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Carbon Monoxide, CO Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Carbon Monoxide, CO Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Molecular Nitrogen, N₂, Number Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Molecular Nitrogen, N₂, Number Density, Precision, NGIMS

Neutral Molecular Nitrogen, N₂, Number Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Molecular Nitrogen, N₂, Number Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Nitric Oxide, NO, Number Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Nitric Oxide, NO, Number Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Nitric Oxide, NO, Number Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Argon, Ar, Number Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Argon, Ar, Number Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Neutral Argon, Ar, Number Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Carbon Dioxide, CO₂, Number Density, Neutral Gas and Ion Mass Spectrometer, NGIMS

Carbon Dioxide, CO₂, Number Density, Precision, Neutral Gas and Ion Mass Spectrometer, NGIMS

Carbon Dioxide, CO₂, Number Density, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 32+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 32+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 32+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Data Quality Flag Values: SCP=Spacecraft Potential available and used as computed by STATIC, SC0=Spacecraft Potential not available

Ion Density, 44+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 44+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 44+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 30+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 30+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 30+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 16+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 16+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 16+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 28+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 28+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 28+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 12+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 12+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 12+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 17+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 17+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 17+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 14+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, Precision, 14+ Atomic Mass Units, Da, Neutral Gas and Ion Mass Spectrometer, NGIMS

Ion Density, 14+ Atomic Mass Units, Da, Data Quality Flag, DQ, Neutral Gas and Ion Mass Spectrometer, NGIMS

Spacecraft Position Vector, Geographic, GEO, Cartesian Coordinates

Spacecraft Position Vector, Mars Solar Orbital, MSO, Cartesian Coordinates

Spacecraft Position, Geographic, GEO, Longitude, calculated by using SPICE Toolkit Software and Kernels

Longitudinal Component of Location of the MAVEN Spacecraft with respect to Mars

Spacecraft Position, Geographic, GEO, Latitude, calculated by using SPICE Toolkit Software and Kernels

Latitudinal (areodetic) Component of Location of the MAVEN Spacecraft with respect to IAU Mars Ellipsoid, Equatorial Radius of 3396.2 km, Polar Radius of

Spacecraft Position, Solar Zenith Angle calculated by using SPICE Toolkit Software and Kernels

Angle measured from MAVEN to the Geometric Center of the Solar Disc, as described by using a horizontal Coordinate System

Spacecraft Position, Local Time calculated by using SPICE Toolkit Software and Kernels

Spacecraft Position, Altitude, Aeroid calculated by using SPICE Toolkit Software and Kernels

Spacecraft Areodetic Altitude with respect to the IAU Mars Ellipsoid, Equatorial Radius of 3396.2 km

Spacecraft Attitude, Unit Vector, Geographic, GEO, Cartesian Coordinates

Spacecraft Attitude, Unit Vector, Mars Solar Orbital, MSO, Cartesian Coordinates

MAVEN Articulated Payload Platform, MAVEN_APP, Attitude, Unit Vector, Geographic, GEO, Cartesian Coordinates

Pointing Direction of Articulated Payload Platform, Z-axis of MAVEN Articulated Payload Platform Base Plate, MAVEN_APP_BP, Frame, in GEO Coordinates

MAVEN Articulated Payload Platform, MAVEN_APP, Attitude, Unit Vector, Mars Solar Orbital, MSO, Cartesian Coordinates

Orbit Number calculated by using SPICE Toolkit Software and Kernels

The Orbit Number Increments each time MAVEN reaches Geometric Periapsis

Spacecraft Inbound/Outbound Flag calculated by using SPICE Toolkit Software and Kernels

Inbound, I, is from Geometric Apoapsis to next Geometric Periapsis in Time, Outbound, O, is the reverse from Geometric Periapsis to Geometric Apoapsis in Time

Mars Planetary Position, Solar Longitude, Ls, calculated by using SPICE Toolkit Software and Kernels

Mars Planetary Position, Solar Longitude: Ls equal to 0° represents Northern Spring Equinox, Ls equal to 90° represents Northern Summer Solstice, etc.

Mars-Sun Distance calculated by using SPICE Toolkit Software and Kernels

Mars Planetary Position, Subsolar Point Longitude Geographic, GEO, Cartesian Coordinates as calculated by using SPICE Toolkit Software and Kernels

Mars Planetary Position, Subsolar Point Latitude Geographic, GEO, Cartesian Coordinates as calculated by using SPICE Toolkit Software and Kernels

Sub-Mars Point on the Sun, Longitude calculated by using SPICE Toolkit Software and Kernels

Sub-Mars Point on the Sun, Latitude calculated by using SPICE Toolkit Software and Kernels

Rotation Matrix, International Astronomical Union, IAU, MARS Coordinates to MAVEN Mars Solar Orbital, MSO, Coordinates as calculated by using SPICE Toolkit Software and Kernels. Column 1 Labels from COMPNO_3: [ 1, 2, 3]. Column 2 Labels from COMPNO_3: [ 1, 2, 3].

Rotation Matrix, MAVEN Spacecraft Coordinates to MAVEN Mars Solar Orbital, MSO, Coordinates as calculated by using SPICE Toolkit Software and Kernels. Column 1 Labels from COMPNO_3: [ 1, 2, 3]. Column 2 Labels from COMPNO_3: [ 1, 2, 3].

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