Galactic cosmic ray intensity in the inner and outer heliosphere in the epoch of the solar cycle 24 minimum

被引：0

作者：

Krainev M.B. ^{[1
]}

Kalinin M.S. ^{[1
]}

机构：

[1] Lebedev Physical Institute, Russian Academy of Sciences, Moscow 119991, Leninskii pr.

来源：

Bulletin of the Russian Academy of Sciences: Physics | 2009年 / 73卷 / 3期

基金：

俄罗斯基础研究基金会;

关键词：

Solar Cycle; Heliospheric Current Sheet; Solar Activity Minimum; Outer Heliosphere; Heliospheric Magnetic Field;

D O I：

10.3103/S1062873809030186

中图分类号：

学科分类号：

摘要：

The behavior of the observed and expected Galactic cosmic ray (GRC) intensity both near the Earth and in the outer heliosphere is considered. The hypothesis is discussed of the strong dependence of the GCR intensity in the interaction region of the solar and interstellar winds on the heliospheric magnetic field polarity in the epoch of a solar activity minimum. © Allerton Press, Inc. 2009.

引用

页码：340 / 342

页数：2

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