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

被引：0
作者：
I. S. Petukhov
S. I. Petukhov
机构：
[1] Russian Academy of Sciences,Shafer Institute for Cosmophysical Research and Aeronomy
[2] Siberian Branch,undefined
来源：
Astronomy Letters | 2009年 / 35卷
关键词：
cosmic rays; shock wave; precursors of disturbances; 96.50.S-; 96.50.Vg; 96.50.sh; 96.50.Fm;
D O I：
暂无
中图分类号：
学科分类号：
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.
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页码：701 / 711
页数：10
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