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).


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    Title :

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


    Contributors:

    Published in:

    Advances in Space Research ; 45 , 11 ; 1315-1321


    Publication date :

    2010-01-26


    Size :

    7 pages




    Type of media :

    Article (Journal)


    Type of material :

    Electronic Resource


    Language :

    English





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