MULTI-COMPONENT MODELS FOR FORMATION OF CHROMOSPHERIC CA-II K LINE .2. EFFECT OF VELOCITY FIELDS

被引：35

作者：

CRAM, LE

机构：

来源：

关键词：

D O I：

10.1007/BF00148703

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：375 / &

共 20 条

[1]

Athay R. G., 1968, SOL PHYS, V4, P176

ATHAY, RG .

[3] FORMATION OF CAII K-LINE CORE WITH ARBITRARY TEMPERATURE MINIMA [J].

BEEBE, HA .

[4] CA-II RESONANCE LINES IN NON-HOMOGENEOUS CHROMOSPHERES [J].

BEEBE, HA ;

JOHNSON, HR .

[5]

CANNON CJ, 1970, SOLAR PHYS, V161, P255

[6]

GOLDBERG L, 1959, SOLAR PHYS, V129, P119

[7]

JEFFRIES JT, 1960, SOLAR PHYS, V131, P695

[8]

JEFFRIES JT, 1958, SOLAR PHYS, V127, P667

[9] LINE FORMATION IN A DIFFERENTIALLY MOVING NON-LTE ATMOSPHERE [J].

KULANDER, JL .

OSTERBROCK, DE .