LINE RESPONSE FUNCTION OF STELLAR ATMOSPHERES AND EFFECTIVE DEPTH OF LINE FORMATION

被引:94
作者
BECKERS, JM
MILKEY, RW
机构
[1] SACRAMENTO PEAK OBSERV,CAMBRIDGE RES LABS,SUNSPOT,NM 88349
[2] KITT PEAK NATL OBSERV,TUCSON,AZ 85726
关键词
D O I
10.1007/BF00152353
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:289 / 292
页数:4
相关论文
共 3 条
[1]   HARVARD-SMITHSONIAN REFERENCE ATMOSPHERE [J].
GINGERICH, O ;
NOYES, RW ;
KALKOFEN, W ;
CUNY, Y .
SOLAR PHYSICS, 1971, 18 (03) :347-+
[2]   AVERAGE OPTICAL DEPTH OF FORMATION OF WEAK FRAUNHOFER LINES [J].
GURTOVENKO, E ;
RATNIKOVA, V ;
DEJAGER, C .
SOLAR PHYSICS, 1974, 37 (01) :43-52
[3]   INTERPRETATION OF VELOCITY FILTERGRAMS .I. EFFECTIVE DEPTH OF LINE FORMATION [J].
PARNELL, RL ;
BECKERS, JM .
SOLAR PHYSICS, 1969, 9 (01) :35-&