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

Mathematics

Scientific paper

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Radiation Belts, Magnetic Storms, Energetic Particles, Proton Flux Density, Crres (Satellite), Satellite Observation, Particle Flux Density, Mathematical Models, Time Dependence

Scientific paper

The objective of the study was to reproduce the radiation belt response to a geomagnetic storm on the 10 min-10 hr scale. For this purpose, the new Salammbo 4D code was applied to the January 24, 1991 event. The model is capable of reproducing flux variations on a time scale on the order of ten minutes. The proton dynamics is examined, and simulation results are compared against CRRES measurements.

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