FORMATION OF MG I 4571 A IN SOLAR ATMOSPHERE .4. EMPIRICAL VS SYNTHETIC ANALYSES

被引:4
作者
ALTROCK, RC [1 ]
机构
[1] SACRAMENTO PEAK OBSERV,SUNSPOT,NM 88349
关键词
D O I
10.1007/BF00149598
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
引用
收藏
页码:37 / 56
页数:20
相关论文
共 8 条
[1]   FORMATION OF MGI 4571 A IN SOLAR ATMOSPHERE .1. MODEL ANALYSIS OF A ONE-DIMENSIONAL STATIC ATMOSPHERE [J].
ALTROCK, RC ;
CANNON, CJ .
SOLAR PHYSICS, 1972, 26 (01) :21-&
[2]  
ATHAY RG, 1972, RADIATION TRANSPORT
[3]   ANALYSIS OF SPECTRAL-LINE PROFILES .2. AN APPLICATION TO SOLAR SODIUM D-LINES [J].
CURTIS, GW ;
JEFFERIES, JT .
ASTROPHYSICAL JOURNAL, 1967, 150 (3P1) :1061-+
[4]  
HEARN AG, 1973, ASTRON ASTROPHYS, V23, P347
[5]  
KUNASZ CV, 1973, ASTRON ASTROPHYS, V28, P15
[6]   INVERSION OF LIMB-DARKENING EQUATION USING PRONY ALGORITHM [J].
WHITE, OR .
ASTROPHYSICAL JOURNAL, 1968, 152 (1P1) :217-&
[7]   ANALYSIS OF CENTER-TO-LIMB VARIATIONS IN HALPHA, HBETA, AND HGAMMA [J].
WHITE, OR .
ASTROPHYSICAL JOURNAL, 1963, 137 (04) :1217-&
[8]   MEASUREMENTS OF LIMB DARKENING IN FORBIDDEN MGI LINE AT 4571.1 A [J].
WHITE, OR ;
SLAUGHTER, CD ;
ALTROCK, RC ;
BRAULT, JW .
SOLAR PHYSICS, 1972, 23 (01) :18-+