The galactic cosmic ray intensity fluctuations during perturbations of the solar wind in early November 2021
- 作者: Zverev A.S.1, Grigoryev V.G.1, Gololobov P.Y.1, Starodubtsev S.A.1
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隶属关系:
- Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
- 期: 卷 88, 编号 2 (2024)
- 页面: 323-326
- 栏目: Physics of Cosmic Rays
- URL: https://ter-arkhiv.ru/0367-6765/article/view/654772
- DOI: https://doi.org/10.31857/S0367676524020289
- EDN: https://elibrary.ru/RPTLHW
- ID: 654772
如何引用文章
详细
In order to develop methods for predicting negative manifestations of space weather, the dynamics of fluctuations in the intensity of galactic cosmic rays during geophysical disturbances in early November 2021 is studied. The obtained results point to the possibility of real-time short-term space weather forecasting based on the measurement data of the Russian national ground-based network of cosmic ray stations.
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作者简介
A. Zverev
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
编辑信件的主要联系方式.
Email: ZverevAS@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
V. Grigoryev
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
P. Gololobov
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
S. Starodubtsev
Shafer Institute of Cosmophysical Research and Aeronomy of the Siberian Branch of the Russian Academy of Sciences
Email: ZverevAS@ikfia.ysn.ru
俄罗斯联邦, Yakutsk
参考
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