Please use this identifier to cite or link to this item: http://repositorio.unicamp.br/jspui/handle/REPOSIP/62229
Type: Artigo de periódico
Title: Numerical modeling of magnetospheric electron radial transport with accounting synchrotron radiation losses
Author: Pugacheva, GI
Gusev, AA
Martin, IM
Boscher, DM
Bourdarie, S
Spjeldvik, WN
Abstract: A spatial 3-Dimensional distribution of the electron component of the Earth's radiation belts obtained by numerical solution of the diffusive transport equation taking into account both Coulomb collisional interaction losses and synchrotronic radiation (SR) energy degradation is presented. For boundary conditions, high energy, 3-16 MeV, electron fluxes observed at geosynchronous orbit by the GOES-7 spacecraft were used. Comparisons of electron distributions with and without the inclusion of SR losses show that energy losses from relativistic electrons substantially influence energy and space distributions of not only relativistic electron fluxes, but also of hundred keV electron fluxes.
Country: EUA
Editor: Amer Geophysical Union
Rights: embargo
Identifier DOI: 10.1029/98GL00990
Date Issue: 1998
Appears in Collections:Unicamp - Artigos e Outros Documentos

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