CORONAL HEATING BY STOCHASTIC MAGNETIC PUMPING

被引：162

作者：

STURROCK, PA

UCHIDA, Y

机构：

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

[2] UNIV TOKYO, TOKYO ASTRON OBSERV, MITAKA, TOKYO 181, JAPAN

来源：

ASTROPHYSICAL JOURNAL | 1981年 / 246卷 / 01期

关键词：

D O I：

10.1086/158926

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：331 / 336

页数：6

共 17 条

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[4]

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[8] DETERMINATION OF PLASMA PARAMETERS FROM SOFT-X-RAY IMAGES FOR CORONAL HOLES (OPEN MAGNETIC-FIELD CONFIGURATIONS) AND CORONAL LARGE-SCALE STRUCTURES (EXTENDED CLOSED-FIELD CONFIGURATIONS) [J].

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[9] THE HEATING OF THE SOLAR CHROMOSPHERE, PLAGES, AND CORONA BY MAGNETOHYDRODYNAMIC WAVES [J].

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[10] DYNAMICS OF QUIESCENT SOLAR CORONA [J].

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