On the structure of galactic cosmic ray intensity during its long-term variations

被引：2
|
作者：
M. B. Krainev
M. S. Kalinin
机构：
[1] Russian Academy of Sciences,Lebedev Physical Institute
来源：
Bulletin of the Russian Academy of Sciences: Physics | 2013年 / 77卷 / 5期
关键词：
Solar Wind; Solar Cycle; Transport Equation; Kalinin; Calculated Intensity;
D O I：
10.3103/S1062873813050316
中图分类号：
学科分类号：
摘要：
The structure of GCR intensity and its changes during the solar magnetic cycle are analyzed by numerically solving its transport equation. We propose a research method that allows us to use the intermediate results from numerical calculations, to resolve the intensity of galactic cosmic rays into components caused by sunspot and magnetic solar cycles, and to monitor the changes in energy in different parts of the heliosphere and different phases of the cycle. A method for dividing intensity into its components associated with the main physical processes determining the modulation of galactic cosmic rays is also proposed.
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页码：510 / 512
页数：2
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