电邮这篇文章 Growth of relativistic electron fluxes in the outer radiation belt according to data of the Arktika-M satellite (No. 1) during magnetic storms in October-November 2021
- 作者: Belakhovsky V.B1,2, Pilipenko V.A3, Kozyreva O.V3
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隶属关系:
- Polar Geophysical Institute
- Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences
- Institute of Physics of the Earth of the Russian Academy of Sciences
- 期: 卷 89, 编号 5 (2025)
- 页面: 708-717
- 栏目: Physics of Auroral Phenomena
- URL: https://bakhtiniada.ru/0367-6765/article/view/315190
- DOI: https://doi.org/10.31857/S0367676525050054
- ID: 315190
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详细
The paper analyzes variations in electron fluxes of various energies from 0.1 MeV to 2 MeV for CIR and CME magnetic storms in October-November 2021 according to data from the Russian satellites “Arktika-M” (No. 1) and “Elektro-L” (No. 2), as well as the satellite GOES-17. The analysis shows that during the stronger CME storm the level of relativistic electron fluxes was noticeably higher than during the weaker CIR storm both in geostationary orbit and in lower L-shells.
作者简介
V. Belakhovsky
Polar Geophysical Institute; Institute of Solar-Terrestrial Physics of the Siberian Branch of the Russian Academy of Sciences
Email: belakhov@mail.ru
Apatity, Russia; Irkutsk, Russia
V. Pilipenko
Institute of Physics of the Earth of the Russian Academy of SciencesMoscow, Russia
O. Kozyreva
Institute of Physics of the Earth of the Russian Academy of SciencesMoscow, Russia
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