Growth of Relativistic Electron Fluxes in the Outer Radiation Belt, According to Data from the Arktika-M (No. 1) Satellite during Magnetic Storms in October–November 2021
The authors analyze variations in electron fluxes of different energies of 0.1 to 2 MeV for CIR and CME magnetic storms in October–November 2021 according to data from the GOES-17 satellite and the Russian satellites Arktika-M (no. 1) and Elektro-L (no. 2). The analysis shows that the level of relativistic electron fluxes was noticeably higher during the stronger CME storm than during the weaker CIR storm in both geostationary orbit and lower L-shells.
Authors
- В. А. Пилипенко
- О. В. Козырева (ORCID: https://orcid.org/0000-0003-0825-151X)
- V. B. Belakhovsky (ORCID: https://orcid.org/0000-0001-8994-4363)
Institutions
- Polar Geophysical Institute (RU)
- Institute of Solar-Terrestrial Physics (RU)
- Schmidt Institute of Physics of the Earth (RU)
Publication Details
- Journal
- Bulletin of the Russian Academy of Sciences Physics
- Published
- 2025-05-01
- DOI
- https://doi.org/10.1134/s1062873825710992
- Primary Topic
- Ionosphere and magnetosphere dynamics
- Type
- article
- Field-Weighted Citation Impact
- 0.00