AbstractThe 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 ∼10MeV. At the same time, trapped proton fluxes with energy less than 10MeV 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).
Trapped proton fluxes measured on board LEO satellites in comparison with models
Advances in Space Research ; 45 , 11 ; 1315-1321
2010-01-26
7 pages
Aufsatz (Zeitschrift)
Elektronische Ressource
Englisch
Trapped proton fluxes measured on board LEO satellites in comparison with models
Online Contents | 2010
|Proton fluxes measured by low-orbit satellites
Online Contents | 2008
|Proton fluxes measured by low-orbit satellites
Springer Verlag | 2008
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