CLASSIFICATION OF MAGNETIC RECONNECTION DURING 2 CURRENT-LOOP COALESCENCE

被引：22

作者：

SAKAI, J

KOIDE, S

机构：

[1] Laboratory for Plasma Astrophysics and Fusion Science Department of Electronics, and Information Faculty of Engineering, Toyama University, Toyama

来源：

SOLAR PHYSICS | 1992年 / 142卷 / 02期

关键词：

D O I：

10.1007/BF00151463

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a classification of magnetic reconnection during two current loop coalescence, which may be quite important for the physical process of both solar flares and coronal loop heating in the solar active region. It is suggested that different kinds of the current loop coalescence processes could be identified from the soft X-ray telescope(SXT) of the " Yohkoh " satellite and the magnetic field data in the active region.

引用

页码：399 / 402

页数：4

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