STIMULATED DISSIPATION OF MAGNETIC DISCONTINUITIES AND THE ORIGIN OF SOLAR-FLARES

被引：41

作者：

PARKER, EN ^{[1
]}

机构：

[1] UNIV CHICAGO, ENRICO FERMI INST, DEPT ASTRON, CHICAGO, IL 60637 USA

来源：

关键词：

D O I：

10.1007/BF00148522

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：297 / 308

页数：12

共 86 条

[81]

VANHOVEN G, 1981, SOLAR FLARE MAGNETOH, P217

[82] THEORETICAL MODELS OF MAGNETIC-FIELD LINE MERGING .1. [J].

VASYLIUNAS, VM .

[83] TRIGGERING AND SUBSEQUENT DEVELOPMENT OF A SOLAR-FLARE [J].

VORPAHL, JA .

[84]

WEBB DF, 1980, MONOGRAPH SKYLAB WOR, V2, P471

[85] MASS AND ENERGY-FLOW IN SOLAR CHROMOSPHERE AND CORONA [J].

WITHBROE, GL ;

NOYES, RW .

[86]

ZAIDMAN EG, 1987, UNPUB ASTROPHYS J