THEORETICAL LINE INTENSITIES .4. SOURCE FUNCTIONS AND EQUIVALENT WIDTHS

被引：5
作者：
ATHAY, RG
机构：
来源：
ASTROPHYSICAL JOURNAL | 1966年 / 144卷 / 03期
关键词：
D O I：
10.1086/148710
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
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页码：1159 / &
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共 12 条
[1]   DEPARTURES FROM THERMODYNAMIC EQUILIBRIUM IN CHROMOSPHERIC MGI, CAI, AND 0I [J].
ATHAY, RG ;
HOUSE, LL .
ASTROPHYSICAL JOURNAL, 1962, 135 (02) :500-&
[2]   THEORETICAL LINE INTENSITIES .I. STRONG EMISSION LINES [J].
ATHAY, RG .
ASTROPHYSICAL JOURNAL, 1965, 142 (02) :724-&
[3]  
AVRETT EH, 1964, JILA16 REP BOULD
[4]  
HUMMER DG, 1965, FEB P HARV SMITHS C
[5]   SOURCE FUNCTION IN A NON-EQUILIBRIUM ATMOSPHERE .3. THE INFLUENCE OF A CHROMOSPHERE [J].
JEFFERIES, JT ;
THOMAS, RN .
ASTROPHYSICAL JOURNAL, 1959, 129 (02) :401-407
[6]   SOURCE FUNCTION IN A NON-EQUILIBRIUM ATMOSPHERE .6. THE FREQUENCY DEPENDENCE OF THE SOURCE FUNCTION FOR RESONANCE LINES [J].
JEFFERIES, JT ;
WHITE, OR .
ASTROPHYSICAL JOURNAL, 1960, 132 (03) :767-774
[7]   SOURCE FUNCTION IN A NON-EQUILIBRIUM ATMOSPHERE .2. DEPTH DEPENDENCE OF SOURCE FUNCTION FOR RESONANCE AND STRONG SUBORDINATE LINES [J].
JEFFERIES, JT ;
THOMAS, RN .
ASTROPHYSICAL JOURNAL, 1958, 127 (03) :667-675
[8]   THE SOURCE FUNCTION IN A NON-EQUILIBRIUM ATMOSPHERE .5. CHARACTER OF THE SELF-REVERSED EMISSION CORES OF CA+ H AND K [J].
JEFFERIES, JT ;
THOMAS, RN .
ASTROPHYSICAL JOURNAL, 1960, 131 (03) :695-704
[9]  
OXENIUS J, 1965, J QUANT SPECTROSC RA, V5, P771
[10]  
SKUMANICH A, IN PRESS
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