电邮这篇文章 Forbush decrease of cosmic rays in a toroidal model of a magnetic cloud
- 作者: Petukhova A.S.1, Petukhov I.S.1, Petukhov S.I.1, Grigoryev V.G.1
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隶属关系:
- Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- 期: 卷 81, 编号 4 (2017)
- 页面: 532-534
- 栏目: Proceedings of the 34th National Conference on Cosmic Rays
- URL: https://journals.rcsi.science/1062-8738/article/view/185064
- DOI: https://doi.org/10.3103/S1062873817020320
- ID: 185064
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详细
The intensity of cosmic rays in a magnetic cloud is calculated. It is found that the duration of the Forbush decrease recovery is determined by the magnetic cloud orientation and the reduction in the magnetic field inside the magnetic cloud as it expands. The formation of the Forbush decrease is described in terms of the contributions from different sources of particles.
作者简介
A. Petukhova
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
I. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
编辑信件的主要联系方式.
Email: i_van@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
S. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
V. Grigoryev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
俄罗斯联邦, Yakutsk, 677980
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