Multi-Spacecraft Observations of Magnetic Reconnection in the Solar Wind

被引：2

作者：

Enzl, J. ^{[1
]}

Prech, L. ^{[1
]}

Safrankova, J. ^{[1
]}

Nemecek, Z. ^{[1
]}

机构：

[1] Charles Univ Prague, Fac Math & Phys, CR-18000 Prague 8, Czech Republic

来源：

PROCEEDINGS OF THE THIRTEENTH INTERNATIONAL SOLAR WIND CONFERENCE (SOLAR WIND 13) | 2013年 / 1539卷

关键词：

Solar Wind; Magnetic Reconnection;

D O I：

10.1063/1.4811012

中图分类号：

TE [石油、天然气工业]; TK [能源与动力工程];

学科分类号：

0807 ; 0820 ;

摘要：

We discuss magnetic reconnection occurring at the boundary between the interplanetary coronal mass ejection sheath and magnetic cloud-like structure (MCL). Multi-spacecraft observations of this event allow us to conclude that such type of reconnection persists more than 50 minutes and the reconnection exhaust can be detected over a distance larger than 130 R-E. The analysis of the event suggests that the observed velocity of the accelerated flow inside the exhaust decreases with the distance from the reconnection X-line.

引用

页码：159 / 162

页数：4

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