Description of Solar Cosmic Ray Propagation in the Interplanetary Medium on the Basis of the Kinetic Equation
- Authors: Fedorov Y.I.1, Shakhov B.A.1
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Affiliations:
- Main Astronomical Observatory
- Issue: Vol 34, No 3 (2018)
- Pages: 107-122
- Section: Space Physics
- URL: https://ogarev-online.ru/0884-5913/article/view/178047
- DOI: https://doi.org/10.3103/S0884591318030042
- ID: 178047
Cite item
Abstract
The propagation of solar cosmic rays in interplanetary space is considered based on the kinetic equation. The expression for cosmic ray density under instantaneous particle injection by a point-like source is obtained. The set of a differential equation system for harmonics of cosmic ray distribution function is obtained starting from the kinetic equation. The cosmic ray transport equation, taking into account the presence of the second harmonic of particle angular distribution, is derived and the solution of this equation is obtained.
Keywords
About the authors
Yu. I. Fedorov
Main Astronomical Observatory
Author for correspondence.
Email: fedorov@mao.kiev.ua
Ukraine, Kyiv, 03680
B. A. Shakhov
Main Astronomical Observatory
Email: fedorov@mao.kiev.ua
Ukraine, Kyiv, 03680
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