NUMERICAL MODELING OF QUASI-STATIC CORONAL LOOPS .1. UNIFORM ENERGY INPUT

被引：238

作者：

VESECKY, JF

ANTIOCHOS, SK

UNDERWOOD, JH

机构：

[1] STANFORD UNIV, DEPT APPL PHYS, STANFORD, CA 94305 USA

[2] STANFORD UNIV, INST PLASMA RES, STANFORD, CA 94305 USA

来源：

ASTROPHYSICAL JOURNAL | 1979年 / 233卷 / 03期

关键词：

D O I：

10.1086/157462

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：987 / 997

页数：11

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[4] EVAPORATIVE COOLING OF FLARE PLASMA [J].

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STURROCK, PA .

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[5] EVOLUTION OF SOFT X-RAY-EMITTING FLARE LOOPS [J].

ANTIOCHOS, SK ;

KRALL, KR .

ASTROPHYSICAL JOURNAL, 1979, 229 (02) :788-798

[6]

ANTIOCHOS SK, 1976, 679 STANF U I PLASM

[7]

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[9]

CRAIG IJD, 1976, ASTRON ASTROPHYS, V49, P239

[10] OBSERVATIONAL EVIDENCE OF CONTINUAL HEATING IN X-RAY EMITTING CORONAL LOOPS [J].

GERASSIMENKO, M ;

SOLODYNA, CV ;

NOLTE, JT .

SOLAR PHYSICS, 1978, 57 (01) :103-110

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