Behavior of High-Energy Magnetospheric Electrons in Solar Cycles 22–24

Kryakunova O.N. Belov A.V. Abunin A.A. Nikolayevskiy N.F. Abunina M.A. Baideldinov U.S. Sultangazinov S.K. Seifullina B.B. Tsepakina I.L.
August 2021 Pleiades journals

Bulletin of the Russian Academy of Sciences: Physics
2021 #85 Issue 8 904 - 906 pp.

Abstract: The behavior of high-energy magnetospheric electrons with energies of >2 MeV in geostationary orbit during solar cycles 22–24 is considered. It is shown that the most increases in electrons occurs during the declining phase of solar activity, when a greater number of geoeffective coronal holes are observed. The 2003–2015 data show there is generally a correspondence between the behavior of the number of increases in electrons and the area of geoeffective coronal holes.

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Institute of Ionosphere, Almaty, 050020, Kazakhstan
Institute of Physics, Russian Academy of Sciences, Moscow, 119991, Russian Federation
Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation, Russian Academy of Sciences, Moscow, 108840, Russian Federation

Institute of Ionosphere
Institute of Physics
Institute of Terrestrial Magnetism

10 лет помогаем публиковать статьи Международный издатель

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