Propagation of Galactic Cosmic Rays in the Outer Heliosphere

被引：1
作者：
Fedorov, Yu. I. [1 ]
机构：
[1] Natl Acad Sci Ukraine, Main Astron Observ, UA-03143 Kiev, Ukraine
来源：
KINEMATICS AND PHYSICS OF CELESTIAL BODIES | 2017年 / 33卷 / 02期
关键词：
LOCAL INTERSTELLAR SPECTRA; VOYAGER; SOLAR MODULATION; MAGNETIC-FIELD; ANISOTROPIES; HELIOSHEATH; HELIOPAUSE; INTENSITY; PARTICLES; TRANSPORT;
D O I：
10.3103/S0884591317020039
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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.
引用
收藏
页码：63 / 78
页数：16
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