Cosmic rays in relation to space weather

被引：106
|
作者：
Kudela, K
Storini, M
Hofer, MY
Belov, A
机构：
[1] Slovak Acad Sci, Inst Expt Phys, Kosice 04353, Slovakia
[2] CNR, IFSI, I-00133 Rome, Italy
[3] Univ Bern, Inst Phys, CH-3012 Bern, Switzerland
[4] IZMIRAN, Troitsk 142092, Moscow, Russia
来源：
SPACE SCIENCE REVIEWS | 2000年 / 93卷 / 1-2期
关键词：
D O I：
10.1023/A:1026540327564
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A review of selected experimental results relevant for the use of cosmic ray records in Space Weather research is presented. Interplanetary perturbations, initiated in the solar atmosphere, affect galactic cosmic rays. In some cases their influence on the cosmic ray intensity results in data signatures that can possibly be used to predict geomagnetic storm onsets. Case studies illustrating the complexity of the cosmic ray effects and related geomagnetic activity precursors are discussed. It is shown that some indices for cosmic ray activity are good tools for testing the reliability of cosmic ray characteristics for Space Weather forecasts. A brief summary of the influence of cosmic rays on the ozone layer is also given. The use of cosmic ray data for Space Weather purposes is still in its infant stage, but suggestions for both case and statistical studies are made.
引用
收藏
页码：153 / 174
页数：22
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