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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Published inBulletin of the Russian Academy of Sciences. Physics Vol. 83; no. 5; pp. 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 Journal Article
LanguageEnglish
Published Moscow Pleiades Publishing 01.05.2019
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