| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 1766548 | Advances in Space Research | 2010 | 7 Pages |
Abstract
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 â¼10Â MeV. At the same time, trapped proton fluxes with energy less than 10Â MeV measured by LEO satellites were higher than the ones predicted by the AP8 model in the region of the SAA (drift shell LÂ <Â 1.5).
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Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
N.V. Kuznetsov, N.I. Nikolaeva,