Мақаланы E-mail арқылы жіберу Forbush decrease of cosmic rays in a toroidal model of a magnetic cloud
- Авторлар: Petukhova A.S.1, Petukhov I.S.1, Petukhov S.I.1, Grigoryev V.G.1
-
Мекемелер:
- Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- Шығарылым: Том 81, № 4 (2017)
- Беттер: 532-534
- Бөлім: 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
Дәйексөз келтіру
Ашық рұқсат
Рұқсат берілді
Тек жазылушылар үшін
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.
Авторлар туралы
A. Petukhova
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Ресей, Yakutsk, 677980
I. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Хат алмасуға жауапты Автор.
Email: i_van@ikfia.sbras.ru
Ресей, Yakutsk, 677980
S. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Ресей, Yakutsk, 677980
V. Grigoryev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Ресей, Yakutsk, 677980
Қосымша файлдар
