To monitor energy spectra and relative composition of solar electrons, protons and He nuclei
Spectrometer for the energy spectra and relative composition of protons (18-250 MeV), helium nuclei (18-350 MeV/n) and C, SI and Fe ions (34-270 MeV/n) of solar, interplanetary and galactic origins, the energy spectra of solar flare and precipitating electrons from about 0.4 to about 30 MeV
Coverage / Cycle
Flown on an R&D satellite
1992 to 2012-11-13
Satellites this instrument is flying on
Note: a red tag indicates satellites no longer operational, a
green tag indicates operational satellites, a blue tag indicates
Solar and space environment monitors Energetic particle spectrometer
No WIGOS subcomponents have been defined.
Primary mission objectives Alpha particles differential directional flux Electron differential directional flux Heavy ion flux energy and mass spectrum Proton differential directional flux Show all Show fewer
Tentative Evaluation of Measurements
The following list indicates which measurements can
retrieved from this category of instrument. To see a full Gap Analysis by Variable,
click on the respective variable.
Note: table can be sorted by clicking on the column headers