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Adv Space Res ; 21(12): 1665-8, 1998.
Article in English | MEDLINE | ID: mdl-11542883

ABSTRACT

New experimental data obtained on the orbital station 'MIR' in 1991 during solar maximum are discussed. Electron fluxes with Ee>75 keV were registered for three different directions as well as for electrons with Ee>300 and 600 keV. Spatial and time distributions of electron fluxes in the trapping region are presented. In the inner radiation belt an additional maximum is observed at L=1.25-1.35, and the fluxes in the 22-05h MLT interval are 2-3 orders of magnitude smaller, than during other local times. In this region a flattening of the electron spectrum is observed. The results obtained were compared with the AE-8 model.


Subject(s)
Electrons , Models, Theoretical , Solar Activity , Space Flight/instrumentation , Altitude , Atlantic Ocean , South America , Spacecraft/instrumentation
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