RECONNECTION IN THE SOLAR ATMOSPHERE

被引：4

作者：

ALY, JJ

机构：

[1] Service d'Astrophys., CE S., Gif sur Yvette

来源：

PLASMA PHYSICS AND CONTROLLED FUSION | 1992年 / 34卷 / 13期

关键词：

MAGNETOHYDRODYNAMICS; TRANSPORT THEORY; RECONNECTION THEORY; SOLAR ATMOSPHERE;

D O I：

10.1088/0741-3335/34/13/006

中图分类号：

O35 [流体力学]; O53 [等离子体物理学];

学科分类号：

070204 ; 080103 ; 080704 ;

摘要：

Some recent progress in the theory of magnetic reconnection in the solar corona are reviewed. In particular, the following topics are discussed in detail: (i) The eruptive behavior of a highly sheared magnetic arcade configuration, with formation and ejection of plasmoids - a possible model for solar flares. (ii) The heating of the coronal plasma by dissipation of spontaneously formed current sheets, and by turbulent reconnection leading to Taylor's relaxation.

引用

页码：1785 / 1794

页数：10