Three-dimensional reconnection at the sun: Space observations and collisionless models

被引：1
|
作者：
Somov, BV
Kosugi, T
Litvinenko, YE
Sakao, T
Masuda, S
Oreshina, AV
Merenkova, EY
机构：
[1] Moscow MV Lomonosov State Univ, Inst Astron, Moscow 119899, Russia
[2] Inst Space & Astronaut Sci, Kanagawa 229, Japan
[3] Univ New Hampshire, Inst Study Earth Ocean & Space, Durham, NH 03824 USA
[4] Natl Astron Observ, Tokyo 181, Japan
[5] Nagoya Univ, STE Lab, Aichi, Japan
来源：
COMPARATIVE RECONNECTION STUDIES AT THE SUN AND IN PLANETARY MAGNETOSPHERES | 2002年 / 29卷 / 07期
关键词：
D O I：
10.1016/S0273-1177(02)00027-3
中图分类号：
V [航空、航天];
学科分类号：
08 ; 0825 ;
摘要：
The Yohkoh data on the site and mechanism of magnetic energy transformation into kinetic and thermal energies of a superhot plasma at the Sun require new models of reconnection under conditions of highly-anomalous resistivity, which are similar to that one observed in toroidal devices performed to study turbulent heating of a collisionless plasma, and its anomalous heat-conductive cooling. The models make intelligible the observed properties of the three-dimensional reconnection in solar flares. (C) 2002 COSPAR. Published by Elsevier Science Ltd. All rights reserved.
引用
收藏
页码：1035 / 1044
页数：10
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