THERMALLY CONDUCTIVE FLOWS IN CORONAL HOLES

被引：25

作者：

STEINOLFSON, RS ^{[1
]}

TANDBERGHANSSEN, E ^{[1
]}

机构：

[1] NASA,GEORGE C MARSHALL SPACE FLIGHT CTR,HUNTSVILLE,AL 35812

来源：

SOLAR PHYSICS | 1977年 / 55卷 / 01期

关键词：

D O I：

10.1007/BF00150877

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：99 / 109

页数：11

共 17 条

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[4]

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[5]

CUPERMAN S, 1972, ASTROPHYS J, V177, P555, DOI 10.1086/151732

[6]

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[7] SOLAR-INTERPLANETARY MODELING - 3-D SOLAR-WIND SOLUTIONS IN PRESCRIBED NON-RADIAL MAGNETIC-FIELD GEOMETRIES [J].

DURNEY, BR ;

PNEUMAN, GW .

SOLAR PHYSICS, 1975, 40 (02) :461-486

[8]

KOPP RA, 1976, SOL PHYS, V49, P43, DOI 10.1007/BF00221484

[9] PROPERTIES OF A CORONAL HOLE DERIVED FROM EXTREME-ULTRAVIOLET OBSERVATIONS [J].

MUNRO, RH ;

WITHBROE, GL .

ASTROPHYSICAL JOURNAL, 1972, 176 (02) :511-&

[10]

MUNRO RH, SOLAR PHYS

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