Propagation of galactic cosmic rays in the outer heliosphere
- Authors: Fedorov Y.I.1
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Affiliations:
- Main Astronomical Observatory
- Issue: Vol 33, No 2 (2017)
- Pages: 63-78
- Section: Space Physics
- URL: https://journal-vniispk.ru/0884-5913/article/view/177950
- DOI: https://doi.org/10.3103/S0884591317020039
- ID: 177950
Cite item
Abstract
The propagation of galactic cosmic rays in heliospheric magnetic fields is studied. An approximate solution to the cosmic ray transport equation has been derived on the basis of a method that takes into account the small value of anisotropy of particle angular distribution. The spatial and energy distributions of the cosmic ray intensity and anisotropy have been investigated, and estimates of cosmic ray energy flux have been carried out.
About the authors
Yu. I. Fedorov
Main Astronomical Observatory
Author for correspondence.
Email: fedorov@mao.kiev.ua
Ukraine, Kyiv, 03143
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