High-Energy Magnetospheric Electrons and Different Types of Disturbances of the Interplanetary Medium

The effects interplanetary disturbances induced by coronal plasma ejections and the high-velocity solar wind from coronal holes have on high-energy ( E > 2 MeV) magnetospheric electrons are investigated. Experimental data collected over 30 years of observations (1986–2017) are analyzed. Coronal p...

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Bibliographic Details
Published in:Bulletin of the Russian Academy of Sciences. Physics 2019-05, Vol.83 (5), p.579-581
Main Authors: Abunin, A. A., Abunina, M. A., Belov, A. V., Gaidash, S. P., Kryakunova, O. N., Nikolaevskiy, N. F., Pryamushkina, I. I., Trefilova, L. A.
Format: Article
Language:English
Subjects:
Hadrons
Heavy Ions
Nuclear Physics
Physics
Physics and Astronomy
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Summary:The effects interplanetary disturbances induced by coronal plasma ejections and the high-velocity solar wind from coronal holes have on high-energy ( E > 2 MeV) magnetospheric electrons are investigated. Experimental data collected over 30 years of observations (1986–2017) are analyzed. Coronal plasma ejections and high-velocity outflows from coronal holes are shown to have different effects on the behavior of high-energy electrons: the latter create stronger electron fluxes at geostationary orbits than the former.
ISSN:1062-8738
1934-9432
DOI:10.3103/S1062873819050034