Отправить статью по E-mail Forbush decrease of cosmic rays in a toroidal model of a magnetic cloud
- Авторы: Petukhova A.S.1, Petukhov I.S.1, Petukhov S.I.1, Grigoryev V.G.1
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Учреждения:
- Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- Выпуск: Том 81, № 4 (2017)
- Страницы: 532-534
- Раздел: 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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Аннотация
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.
Об авторах
A. Petukhova
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Россия, Yakutsk, 677980
I. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Автор, ответственный за переписку.
Email: i_van@ikfia.sbras.ru
Россия, Yakutsk, 677980
S. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Россия, Yakutsk, 677980
V. Grigoryev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Россия, Yakutsk, 677980
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