Physical modeling of radiation belt response to geomagnetic storm. II - On a 10 hour-10 day time scale

Details Physical modeling of radiation belt response to geomagnetic storm. II - On a 10 hour-10 day time scale Physical modeling of radiation belt response to geomagnetic storm. II - On a 10 hour-10 day time scale

Aug 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997adspr..20..381b&link_type=abstract

Advances in Space Research, vol. 20, p. 381

Mathematics

1

Radiation Belts, Magnetic Storms, Energetic Particles, Electron Distribution, Time Dependence, Crres (Satellite), Satellite Observation, Mathematical Models, Electron Flux Density, High Energy Electrons

Scientific paper

The Salammbo 3D code was applied to the January 25, 1991 event in an attempt to reproduce the radiation belt response to a geomagnetic storm on the 10 hr-10 day time scale. The model can successfully reproduce flux variations that occur over a time scale on the order of half a day. The electron dynamics is characterized, and results obtained from the model are presented. Finally, simulation results are compared with CRRES measurements of electron fluxes.

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