Correlation of changes in the outer-zone relativistic-electron population with upstream solar wind and magnetic field measurements

被引：170

作者：

Blake, JB

Baker, DN

Turner, N

Ogilvie, KW

Lepping, RP

机构：

[1] UNIV COLORADO,ATMOSPHER & SPACE PHYS LAB,BOULDER,CO 80309

[2] NASA,GODDARD SPACE FLIGHT CTR,GREENBELT,MD 20771

来源：

GEOPHYSICAL RESEARCH LETTERS | 1997年 / 24卷 / 08期

关键词：

D O I：

10.1029/97GL00859

中图分类号：

P [天文学、地球科学];

学科分类号：

07 ;

摘要：

A study has been made of the correlation of the population of relativistic electrons in the outer-zone magnetosphere with the properties of the solar wind (speed, density, magnetic field) during a solar minimum period, The study is based upon observations made in the Spring of 1995 with sensors aboard 1994-026 and WIND. It is found that a large relativistic electron enhancement depends upon a substantial solar-wind speed increase associated with precursor solar-wind density enhancement, and, in particular, upon a southward turning of the interplanetary magnetic field.

引用

页码：927 / 929

页数：3

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