Galactic cosmic ray intensity dynamics in the presence of large-scale solar wind disturbances

被引：8
|
作者：
Petukhov, I. S. [1 ]
Petukhov, S. I. [1 ]
机构：
[1] Russian Acad Sci, Shafer Inst Cosmophys Res & Aeron, Siberian Branch, Yakutsk 677980, Russia
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 2009年 / 35卷 / 10期
关键词：
cosmic rays; shock wave; precursors of disturbances; IMF-COLLIMATED OUTWARD; MEAN FREE PATHS; SHOCK DECREASE; FORBUSH; ACCELERATION; PRECURSORS; INCREASE;
D O I：
10.1134/S1063773709100077
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
We have developed a method of relativistic particle trajectories to model the cosmic ray intensity dynamics in the presence of solar wind disturbances. The probability of detecting the precursors of disturbances has been found to depend on various conditions. In general, the dynamics of the distribution of precursors at the magnetospheric surface is in agreement with measurements.
引用
收藏
页码：701 / 711
页数：11
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