Does geomagnetic storm magnitude depend on solar flare importance?

被引:6
|
作者
Yermolaev, Yu. I. [1 ]
Yermolaev, M. Yu. [1 ]
机构
[1] Russian Acad Sci, Space Res Inst, Moscow 117997, Russia
基金
俄罗斯基础研究基金会;
关键词
CORONAL MASS EJECTIONS; EVENTS; CMES;
D O I
10.1134/S0010952509060021
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
In order to predict space weather effects, solar flares are often used as precursors of magnetic storms on the Earth. In particular, possible relation between the solar flare importance and magnetic storm intensity is discussed in some papers. However, published results contradict each other. We compare the published results on the flare-storm dependence and discuss possible causes of this disagreement: (1) different intervals of observation, (2) differing statistics, and (3) different methods of identification of events and their comparison. Our analysis has shown that the fact of occurrence and the magnitude of a geomagnetic storm cannot be determined, generally, using only the solar flare importance. However, analyzing additional information on the coronal mass ejection (CME), associated with the geomagnetic storm, one can offer an algorithm for the storm magnitude prediction on the basis of flare importance.
引用
收藏
页码:460 / 465
页数:6
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