Analysis of Muon Flux Variations Caused by High-Speed Solar Wind During Periods of Low Solar Activity
- Autores: Konovalova A.Y.1, Astapov I.I.1, Barbashina N.S.1, Osetrova N.V.1, Mishutina Y.N.1, Shutenko V.V.1, Yashin I.I.1
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Afiliações:
- National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
- Edição: Volume 82, Nº 6 (2019)
- Páginas: 909-915
- Seção: Elementary Particles and Fields
- URL: https://journals.rcsi.science/1063-7788/article/view/195416
- DOI: https://doi.org/10.1134/S1063778819660311
- ID: 195416
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Resumo
The influence of a high-speed solar wind on the state of magnetosphere, as well as on the cosmic ray flux registered on the Earth’s surface by the muon hodoscope URAGAN (MEPhI) is discussed. The results of the analysis of the parameters of muon flux local anisotropy in the periods of low solar activity (2008–2009 and 2017–2018) during geomagnetic disturbances caused by the high-speed solar wind are presented.
Sobre autores
A. Konovalova
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Autor responsável pela correspondência
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
I. Astapov
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
N. Barbashina
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
N. Osetrova
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
Y. Mishutina
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
V. Shutenko
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
I. Yashin
National Research Nuclear University MEPhI (Moscow Engineering Physics Institute)
Email: YKonovalova@mephi.ru
Rússia, Moscow, 115409
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