INFLUENCE OF MAGNETIC-FIELD STRUCTURE ON CONDUCTION COOLING OF FLARE LOOPS

被引：86

作者：

ANTIOCHOS, SK

STURROCK, PA

机构：

[1] STANFORD UNIV,INST PLASMA RES,STANFORD,CA 94305

[2] STANFORD UNIV,DEPT APPL PHYS,STANFORD,CA 94305

来源：

关键词：

D O I：

10.1007/BF00162458

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：359 / 367

页数：9

共 8 条

[1]

[Anonymous], IAU S

COX, DP ;

TUCKER, WH .

[3]

Culhane J. L., 1970, Solar Physics, V15, P394, DOI 10.1007/BF00151847

FISHER, RR .

[5] HEATING AND COOLING OF THERMAL X-RAY PLASMA IN SOLAR-FLARES [J].

MOORE, RL ;

DATLOWE, DW .

[6]

RUST DM, 1973, SOL PHYS, V33, P445

[7]

SPITZER L, 1962, PHYSICS FULLY IONIZS

[8] MODEL FOR SOURCE OF SOLAR-FLARE X-RAYS [J].

STRAUSS, FM ;

PAPAGIANNIS, MD .