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

Artem A. Abunin, Maria A. Abunina, Anatoly V. Belov, S. P. Gaidash, O. N. Kryakunova, Nikolay Nikolayevskiy, I. I. Pryamushkina, Л. А. Трефилова

2019

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DOI 10.3103/s1062873819050034
Data confidence 85 high
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Abstract

Abstract 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.