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Transport modeling of energetic electrons in the inner magnetosphere with synchrotron energy losses |
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| Authors: | G.I. Pugacheva D.M. Boscher A.A. Gusev I.M. Martin W.N. Spjeldvik |
| Affiliation: | 1University of Campinas, Instituto de Fisica, Depto. de Raios Cosmicos, 13083, Campinas, SP, Brazil 2Centre d'Etudes et de Recherches de Toulouse-Office National d'Etudes et de Recherches Aerospatiales, Dep. de Technologie Spatiale, Toulouse, France 3Weber State University, Department of Physics, Ogden, Utah 84408, USA |
| Abstract: | The resulting L-distributions and energy spectra of energetic magnetospheric electrons obtained from numerical solution of the radiation belt transport equation with and without accounting for electron synchrotron energy losses are compared. It is demonstrated that synchrotron losses play an important role in formation of the space and energetic distributions of electrons in the inner magnetosphere. |
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