Analysis of Muon Flux Variations Caused by High-Speed Solar Wind During Periods of Low Solar Activity


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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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