Neoclassical effects on solar plasma loops

被引：1

作者：

Tan, BL ^{[1
]}

Huang, GL ^{[1
]}

机构：

[1] Chinese Acad Sci, Purple Mt Observ, Nanjing 210008, Peoples R China

来源：

CORONAL AND STELLAR MASS EJECTIONS | 2005年 / 226期

关键词：

Sun : coronal mass ejections (CMEs); flares; magnetic fields; MHD;

D O I：

10.1017/S1743921305000712

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Tokamak physics shows that there will be a, neoclassical effect in current-carrying plasma loops. We apply the theory to solar coronal loops and hope to find a fast magnetic reconnection mechanism for understanding solar flares and CMEs.

引用

页码：279 / 280

页数：2

共 6 条

[1] DIFFUSION DRIVEN PLASMA CURRENTS AND BOOTSTRAP TOKAMAK [J].

BICKERTON, RJ ;

CONNOR, JW ;

TAYLOR, JB .

NATURE-PHYSICAL SCIENCE, 1971, 229 (04) :110-+

[2] The radio signature of twisted magnetic ropes and reconnection site in the low corona [J].

Huang, GL ;

Wu, HA ;

Grechnev, VV ;

Sych, RA ;

Altyntsev, AT .

SOLAR PHYSICS, 2003, 213 (02) :341-358

[3]

Qu W. X., 1985, Technical Report No. UWPR-85-5

[4]

WESSON J, 1997, TOKAMAK

[5]

Zaitsev VV, 1998, ASTRON ASTROPHYS, V337, P887

[6]

ZHANG ZD, 2000, CORONAL PHYS

← 1 →