A HIGH-ENERGY INCREASE IN COSMIC-RAY INTENSITY

被引：0
|
作者：
VENKATESAN, D [1 ]
ANANTH, AG [1 ]
机构：
[1] INDIAN SPACE RES ORG,BANGALORE 560094,INDIA
来源：
CANADIAN JOURNAL OF PHYSICS | 1991年 / 69卷 / 8-9期
关键词：
D O I：
10.1139/p91-155
中图分类号：
O4 [物理学];
学科分类号：
0702 ;
摘要：
The increase in cosmic rays observed by neutron monitors with high-energy cutoff, on April 29, 1973, is interpreted to be a definite high-energy phenomenon. This is not associated with any solar flare or interplanetary disturbance. The association of the increase in intensity with geomagnetic index Dst variation indicates a possibility that the high-energy event was caused by a magnetospheric phenomenon.
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收藏
页码：984 / 987
页数：4
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