Long-period variations of cosmic rays and the global magnetic field of the sun

被引：0
|
作者：
Okhlopkov, VP [1 ]
机构：
[1] Moscow State Univ, Skobeltsyn Res Inst Nucl Phys, Moscow 119899, Russia
来源：
SOLAR SYSTEM RESEARCH | 2000年 / 34卷 / 02期
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D O I：
暂无
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
Long-period (1-5-year) variations of Galactic Cosmic Rays (GCRs) are studied using the data of stratosphere sounding and neutron monitor measurements, as well as different manifestations of solar activity, in particular, the global magnetic field of the Sun as a star. It is shown that quasi-periodic variations of GCRs with three-year or shorter periods arise as a result of variations of the solar global magnetic field with the same periods, appear simultaneously with them, have an inverse phase, and respond to the sign of the field.
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页码：139 / 142
页数：4
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