Current sheets in the solar atmosphere

被引：1
|
作者：
Podgorny, AI
Podgorny, IM
机构：
[1] PN Lebedev Phys Inst, Moscow 117924, Russia
[2] Russian Acad Sci, Inst Astron, Moscow 109017, Russia
来源：
SUN AND ITS ATMOSPHERE | 1997年 / 20卷 / 12期
关键词：
D O I：
10.1016/S0273-1177(97)00911-3
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The 2D and 3D numerical simulation is used for the investigation of current sheet (CS) creation above the active region. The current sheet in the solar corona can be created either in vicinity of a magnetic field singular line by focusing disturbances or at the interaction of the super-Alfvenic plasma flow with the perpendicular magnetic field. (C) 1997 COSPAR. Published by Elsevier Science Ltd.
引用
收藏
页码：2309 / 2312
页数：4
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