ANALYSIS OF MN-I LINES IN THE SOLAR SPECTRUM USING ACCURATE OSCILLATOR-STRENGTHS

被引：19

作者：

BOOTH, AJ ^{[1
]}

BLACKWELL, DE ^{[1
]}

SHALLIS, MJ ^{[1
]}

机构：

[1] OXFORD UNIV,DEPT EXTERNAL STUDIES,OXFORD OX1 2AJ,ENGLAND

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1984年 / 209卷 / 01期

关键词：

D O I：

10.1093/mnras/209.1.77

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：77 / 81

页数：5

共 28 条

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[13]

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CORLISS, C ;

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[15]

DELBOUILLE L, 1973, PHOTOSPHERIC ATLAS S

[16] MN(I) TRANSITION-PROBABILITIES AND THE MANGANESE SOLAR ABUNDANCE [J].

GREENLEE, TR ;

WHALING, W .

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[17] THE EMPIRICAL DETERMINATION OF DAMPING CONSTANTS IN THE SOLAR PHOTOSPHERE .1. PRELIMINARY-RESULTS FOR FE-I LINES [J].

GURTOVENKO, EA ;

KONDRASHOVA, NN .

SOLAR PHYSICS, 1980, 68 (01) :17-29

[18] PHOTOSPHERIC BARIUM SPECTRUM - SOLAR ABUNDANCE AND COLLISION BROADENING OF BA II LINES BY HYDROGEN [J].

HOLWEGER, H ;

MULLER, EA .

SOLAR PHYSICS, 1974, 39 (01) :19-30

[19]

HOLWEGER H, 1967, Z ASTROPHYS, V65, P365

[20]

KURUCZ RL, 1975, 362 SMITHS ASTR OBS

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