Specific features of the rigidity spectrum of Forbush effects
- 作者: Klyueva A.I.1, Belov A.V.2, Eroshenko E.A.2
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隶属关系:
- Main Astronomical Observatory
- Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
- 期: 卷 57, 编号 2 (2017)
- 页面: 177-189
- 栏目: Article
- URL: https://journals.rcsi.science/0016-7932/article/view/156183
- DOI: https://doi.org/10.1134/S0016793217020050
- ID: 156183
如何引用文章
详细
We analyze variations in the rigidity spectrum of primary cosmic rays during Forbush effects recorded in cycles 20–24 of solar activity on the basis of data from the global network of neutron monitor stations processed by global survey. We investigate variations in the rigidity spectrum index of Forbush effects as a function of the solar activity level, phases of the effect, polarity the total magnetic field of the Sun, type and parameters of the source of cosmic ray modulation, etc. Comprehensive analysis of our results revealed regularities in the dynamics of the energy spectrum of galactic cosmic rays that reflect the dynamic processes occurring in the interplanetary space.
作者简介
A. Klyueva
Main Astronomical Observatory
编辑信件的主要联系方式.
Email: a.klyuyeva@gmail.co
乌克兰, Kiev
A. Belov
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
编辑信件的主要联系方式.
Email: abelov@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 142190
E. Eroshenko
Pushkov Institute of Terrestrial Magnetism, Ionosphere, and Radiowave Propagation
Email: abelov@izmiran.ru
俄罗斯联邦, Troitsk, Moscow, 142190
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