Observations of variability in cosmic rays

被引：43

作者：

Bazilevskaya, GA ^{[1
]}

机构：

[1] Russian Acad Sci, PN Lebedev Phys Inst, Moscow 117924, Russia

来源：

SPACE SCIENCE REVIEWS | 2000年 / 94卷 / 1-2期

基金：

俄罗斯基础研究基金会;

关键词：

Atmosphere; Solar Activity; Time History; Activity Time; Flux Variation;

D O I：

10.1023/A:1026721912992

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Cosmic rays are the main source of ionization in the atmosphere at altitudes below 55-60 km. This circumstance, together with the fact that cosmic ray flux modulation closely mirrors the solar activity time history, makes cosmic rays a good candidate as a possible mediator in the solar variability - climate relationship. The observed cosmic ray flux variations are described with the aim of emphasizing the features which may be useful in the search of correlation between cosmic rays and atmospheric phenomena.

引用

页码：25 / 38

页数：14

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