On the current and maximum phases of solar cycle 24 in the galactic cosmic ray intensity

被引：0

作者：

Krainev, M. B. ^{[1
]}

Kalinin, M. S. ^{[1
]}

机构：

[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 119991, Russia

来源：

23RD EUROPEAN COSMIC RAY SYMPOSIUM (AND 32ND RUSSIAN COSMIC RAY CONFERENCE) | 2013年 / 409卷

关键词：

HELIOSPHERE; MODULATION; 11-YEAR;

D O I：

10.1088/1742-6596/409/1/012176

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We compare the current characteristics of the sunspot activity and cosmic ray intensity with those expected in the future maximum of the current solar cycle. The values for maximum phase are estimated from the correlation between characteristics in the maximum and in the inflection points (few years before maximum) for the previous solar cycles. The expected galactic cosmic ray phenomena typical for the maximum phase of solar cycle (Gnevyshev Gap effect, quasi-biannual oscillations and energetic hysteresis) are discussed.

引用

页数：4

共 50 条

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