THE C-I OPACITY AND PHYSICAL STRUCTURE OF COOL, VERY DENSE-PLASMA IN THE SOLAR CORONA

被引：12

作者：

FOUKAL, P

机构：

来源：

ASTROPHYSICAL JOURNAL | 1981年 / 245卷 / 01期

关键词：

D O I：

10.1086/158810

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：304 / 314

页数：11

共 33 条

[1]

ALDROVANDI SM, 1973, ASTRON ASTROPHYS, V25, P137

[2] SOLAR SPICULES [J].

BECKERS, JM .

ANNUAL REVIEW OF ASTRONOMY AND ASTROPHYSICS, 1972, 10 :73-&

[3]

BONNET RM, 1980, APJ, V237, P47

[4] FINE-STRUCTURE OF SOLAR ATMOSPHERE IN FAR ULTRAVIOLET [J].

BRUECKNER, GE ;

BARTOE, JDF .

SOLAR PHYSICS, 1974, 38 (01) :133-156

[5]

DUPREE AK, 1976, ASTROPHYS J, V209, P621, DOI 10.1086/154759

[6] EXTREME-ULTRAVIOLET SPECTRUM OF A SOLAR ACTIVE REGION [J].

DUPREE, AK ;

HUBER, MCE ;

NOYES, RW ;

PARKINSON, WH ;

REEVES, EM ;

WITHBROE, GL .

ASTROPHYSICAL JOURNAL, 1973, 182 (01) :321-333

[7] H-ALPHA FINE-STRUCTURE AND CHROMOSPHERIC FIELD [J].

FOUKAL, P .

SOLAR PHYSICS, 1971, 20 (02) :298-&

[8] MAGNETIC LOOPS, DOWNFLOWS, AND CONVECTION IN SOLAR CORONA [J].

FOUKAL, P .

ASTROPHYSICAL JOURNAL, 1978, 223 (03) :1046-&

[9]

FOUKAL P, 1975, FLARE RELATED MAGNET, P125

[10]

Foukal P. V., 1974, ASTROPHYS J LETT, V193, P143

← 1 2 3 4 →