Trapped proton fluxes measured on board LEO satellites in comparison with models

Details Trapped proton fluxes measured on board LEO satellites in comparison with models Trapped proton fluxes measured on board LEO satellites in comparison with models

Jun 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010adspr..45.1315k&link_type=abstract

Advances in Space Research, Volume 45, Issue 11, p. 1315-1321.

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The proton fluxes from the low-Earth orbital satellites databases (NPOES-17 and CORONAS-F) were analyzed for the quiet geomagnetic period in April 2005. The satisfactory consent was found between the experimental and the AP8 model fluxes of the trapped protons with energy more than ˜10 MeV. At the same time, trapped proton fluxes with energy less than 10 MeV measured by LEO satellites were higher than the ones predicted by the AP8 model in the region of the SAA (drift shell L < 1.5).

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