Current loop coalescence in dusty plasmas

被引：0
|
作者：
Sakai, JI [1 ]
Cramer, NF [1 ]
机构：
[1] Toyama Univ, Fac Engn, Lab Plasma Astrophys, Toyama 9308555, Japan
来源：
FRONTIERS IN DUSTY PLASMAS | 2000年
关键词：
D O I：
10.1016/B978-044450398-5/50039-7
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：
The weakly ionized plasmas that occur in protostellar disks and in the cores of molecular clouds generally have a dust component. We consider the effects of the presence of charged dust on magnetic reconnection process. We investigate the dynamics of two current loops coalescence, for both cases; partial and complete magnetic reconnection. It is shown that the field-free gas produced during the two loops coalescence with complete magnetic reconnection would be able to initiate star formation.
引用
收藏
页码：289 / 294
页数：6
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