Enviar artigo por via de e-mail Forbush decrease of cosmic rays in a toroidal model of a magnetic cloud
- Autores: Petukhova A.S.1, Petukhov I.S.1, Petukhov S.I.1, Grigoryev V.G.1
-
Afiliações:
- Institute of Cosmophysical Research and Aeronomy, Siberian Branch
- Edição: Volume 81, Nº 4 (2017)
- Páginas: 532-534
- Seção: 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
Citar
Acesso aberto
Acesso está concedido
Somente assinantes
Resumo
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.
Sobre autores
A. Petukhova
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Rússia, Yakutsk, 677980
I. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Autor responsável pela correspondência
Email: i_van@ikfia.sbras.ru
Rússia, Yakutsk, 677980
S. Petukhov
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Rússia, Yakutsk, 677980
V. Grigoryev
Institute of Cosmophysical Research and Aeronomy, Siberian Branch
Email: i_van@ikfia.sbras.ru
Rússia, Yakutsk, 677980
Arquivos suplementares
