POES-SEM2 2-second Particle Precipitation Data, MetOp-A (MetOp-2 before Oct2006 launch) [Important: these data have known contamination problems: please consult Rob Redmon (sem.poes@noaa.gov) for usage recommendations.] 

archive and instrument documentation at NOAA National Geophysical Data Center (NGDC)

MEPED Telescope Data Processing Algorithm Theoretical Basis Document (section 2.2.1)

POES N19 data: POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.) 

POES/MetOp: Particle Precipitation Data (These data have known contamination problems. Please consult provider rob.redmon@noaa.gov for usage recommendations.) 

The POES/MetOp SEM-2 data provide information about the particle radiation surrounding Earth and its effects on the atmosphere

Earth Science > Sun-earth Interactions > Ionosphere/Magnetosphere Particles > Electron Flux,Earth Science > Sun-earth Interactions > Ionosphere/Magnetosphere Particles 

Every effort has been made to provide the highest quality data but the instruments have known inherent limitations. Please contact the data provider for information on how to properly use the data.

Electron differential flux, TED, 0 degree telescope, 189-7980 eV

Electron differential flux, TED, 0 and 30 degree telescopes, 189 eV

Proton differential flux, TED, 0 and 30 degree telescopes, 189 eV

Electron integral energy flux, TED, 0 degree telescope, low energy (50-1000 eV)

Electron integral energy flux, TED, 0 degree telescope, high energy (1-20 keV)

Proton integral energy flux, TED, 0 degree telescope, low energy (50-1000 eV)

Proton integral energy flux, TED, 0 degree telescope, high energy (1-20 keV)

Electron atmospheric integral energy flux, TED, low energy (50-1000 eV), at 120 km

Proton atmospheric integral energy flux, TED, low energy (50-1000 eV), at 120 km

Electron and Proton total atmospheric integral energy flux, TED, at 120 km

Electron background integral energy flux, TED, 0 degree telescope, low energy

Proton background integral energy flux, TED, 0 degree telescope, low energy

Electron integral flux, MEPED, 0 degree telescope, >40 to >612 keV

Electron integral flux, MEPED, 90 degree telescope, >40 to >612 keV

Electron integral flux, MEPED, as spectrograms in energy for each telescope

% Error, Electron integral flux, MEPED, as spectrogram in energy for each telescope

Electron integral flux, MEPED, 0 and 90 degree telescopes, >40 keV

Proton differential flux, MEPED, 0 degree telescope, 39-2723 keV

Proton differential flux, MEPED, 90 degree telescope, 39-2723 keV

Proton Differential flux, MEPED, as spectrograms in energy for each telescope

Proton differential flux, MEPED, 0 and 90 degree telescopes, 39 keV

Proton integral flux, MEPED, 0 and 90 degree telescopes, >6174 keV 

Proton differential flux, MEPED Omni telescope, at center energies 25, 50, and 100 MeV,

proton differential flux. MEPED Omni telescope, as spectrograms in energy

---> By IGRF satellite coordinates (opposite velocity direction)


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