THEORETICAL-MODEL OF THE SOLAR CORONA DURING SUNSPOT MINIMUM .2. DYNAMIC APPROXIMATION

被引：8

作者：

OSHEROVICH, VA

GLINER, EB

TZUR, I

机构：

[1] COOPERAT INST RES ENVIRONM SCI,BOULDER,CO

[2] WASHINGTON UNIV,MCDONNELL CTR SPACE SCI,ST LOUIS,MO 63130

[3] NATL CTR ATMOSPHER RES,BOULDER,CO 80307

来源：

ASTROPHYSICAL JOURNAL | 1985年 / 288卷 / 01期

关键词：

D O I：

10.1086/162803

中图分类号：

P1 [天文学];

学科分类号：

0704 [天文学];

摘要：

引用

页码：396 / 400

页数：5

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[3]

NORTH-SOUTH ASYMMETRIES IN THE 530.3 NM CORONAL LINE FROM 1958 TO 1980 [J].

MOUSSAS, X ;

PAPASTAMATIOU, N ;

RUSIN, V ;

RYBANSKY, M .

SOLAR PHYSICS, 1983, 84 (1-2) :71-75

[4]

THEORETICAL-MODEL OF THE SOLAR CORONA DURING SUNSPOT MINIMUM .1. QUASI-STATIC APPROXIMATION [J].

OSHEROVICH, VA ;

TZUR, I ;

GLINER, EB .

ASTROPHYSICAL JOURNAL, 1984, 284 (01) :412-421

[5]

OSHEROVICH VA, 1985, UNPUB SOLAR PHYS

[6]

OSHEROVICH VA, 1982, 24 COSPAR M OTT

[7]

Saito K., 1970, Annals of the Tokyo Astronomical Observatory, V12, P53

[8]

UCHIDA Y, 1981, J ASTR AP, V15, P83

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