Solar cycle in galactic cosmic ray intensity in inner and outer heliospheres

被引：0

作者：

Lebedev Physical Institute, Russian Academy of Sciences, Moscow 119991, Russia ^{[1
]}

不详 ^{[2
]}

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来源：

Bull. Russ. Acad. Sci. Phys. | 2006年 / 6卷 / 940-944期

关键词：

Orbits - Protons - Solar radiation - Upper atmosphere;

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摘要：

We consider the Solar Cycle, i.e., the 22-year variation in the galactic cosmic ray intensity, caused by the dynamo process in the Sun. This phenomenon is observed in the Earth's orbit (using neutron moniors, spacecraft, and stratospheric data) and in the outer heliosphere (PIONEER-10, VOYAGER-1, -2 spacecraft). © 2006 by Allerton Press, Inc.

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