ON THE POTENTIAL OF INTERPLANETARY SCINTILLATION FOR PREDICTING GEOMAGNETIC-ACTIVITY

被引:7
|
作者
HAPGOOD, M
HARRISON, R
机构
[1] Space Science Department, Rutherford Appleton Laboratory, Chilton, Oxfordshire
关键词
D O I
10.1029/94GL00372
中图分类号
P [天文学、地球科学];
学科分类号
07 ;
摘要
A survey of IPS, geomagnetic and interplanetary medium data has been used to interpret the weak correlation between IPS data and geomagnetic activity. Our results indicate that: (i) we can use IPS data to predict the maximum possible level of geomagnetic activity, given the state of the solar wind; but (ii) to predict the actual level of activity we also require an estimate the coupling between the solar wind and the magnetosphere. This is the first time that the potential (and the limitations) of IPS for predicting geomagnetic activity have been demonstrated quantitatively in a comprehensive survey.
引用
收藏
页码:637 / 640
页数:4
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