Magnetic reconnection events in the interplanetary space

被引：8
|
作者：
Wei, FS [1 ]
Schwenn, R [1 ]
Hu, Q [1 ]
机构：
[1] CHINESE ACAD SCI,CTR SPACE SCI & APPL RES,BEIJING 100080,PEOPLES R CHINA
来源：
SCIENCE IN CHINA SERIES E-TECHNOLOGICAL SCIENCES | 1997年 / 40卷 / 05期
关键词：
interplanetary space; magnetic reconnection; heliospheric physics;
D O I：
10.1007/BF02917160
中图分类号：
T [工业技术];
学科分类号：
08 ;
摘要：
Magnetic field and plasma measurements in the period of 1975-1981 with 0.18-h averages from Hellos spacecrafts are analyzed. Ir is discovered that magnetic reconnection phenomena exist in the interplanetary space. By means of the reconstruction of magnetic field configuration in the azimuth angle plane, it is found that the magnetic reconnection event with time scale of the order of day is a significant form of magnetic reconnection phenomena in the interplanetary space, which consists of a mediate body (or a plasma bulk) and two magnetic separator lines. It could originate from coronal mass ejection event or magnetic cloud in the interplanetary space. Numerical simulation has reproduced the basic characteristics of the magnetic reconnection events.
引用
收藏
页码：463 / 471
页数：9
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