Email this article Impact of Different Types of Interplanetary Medium Disturbances of High-Energy Electrons on the Geostationary Orbit
- Authors: Abunin A.A.1,2, Abunina M.A.1, Belov A.V.1, Gaidash S.P.1, Eroshenko E.A.1, Kryakunova O.N.3,4, Nikolaevskii N.F.3, Pryamushkina I.I.1, Trefilova L.A.1
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Affiliations:
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
- V.V. Gorodovikov Kalmyk State University
- Institute of the Ionosphere Subsidiary Limited Liability Partnership
- Lebedev Physical Institute, Russian Academy of Sciences
- Issue: Vol 59, No 7 (2019)
- Pages: 878-884
- Section: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/157843
- DOI: https://doi.org/10.1134/S0016793219070041
- ID: 157843
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Abstract
Specific features of the behavior of streams of relativistic magnetospheric electrons at energies higher than 2 MeV on geostationary orbits during different types of interplanetary disturbances are studied. More than 30 years (1986–2019) of observations of these particles onboard the GOES satellites is analyzed. It is shown that plasma coronal ejections and high-speed streams from coronal holes differently influence the behavior of high-energy electrons. High-speed streams from coronal holes are more effective In formation of electron flux rises than solar plasma ejections.
About the authors
A. A. Abunin
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences; V.V. Gorodovikov Kalmyk State University
Author for correspondence.
Email: abunin@izmiran.ru
Russian Federation, TroitskMoscow, 108840; Elista, 358000
M. A. Abunina
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Author for correspondence.
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
A. V. Belov
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
S. P. Gaidash
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
E. A. Eroshenko
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
O. N. Kryakunova
Institute of the Ionosphere Subsidiary Limited Liability Partnership; Lebedev Physical Institute, Russian Academy of Sciences
Email: abunina@izmiran.ru
Kazakhstan, Almaty, 050020; Moscow, 119991
N. F. Nikolaevskii
Institute of the Ionosphere Subsidiary Limited Liability Partnership
Email: abunina@izmiran.ru
Kazakhstan, Almaty, 050020
I. I. Pryamushkina
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
L. A. Trefilova
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radio Wave Propagation (IZMIRAN), Russian Academy of Sciences
Email: abunina@izmiran.ru
Russian Federation, TroitskMoscow, 108840
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