INTERPRETATION OF TI-I LINES OF EXCITATION-ENERGY 0.0-0.05 EV IN THE SOLAR SPECTRUM - USE OF NEW OSCILLATOR-STRENGTHS OF ACCURACY 0.5 PER CENT

被引：15

作者：

BLACKWELL, DE

SHALLIS, MJ

SIMMONS, GJ

机构：

[1] Department of Astrophysics, South Parks Road, Oxford, United Kingdom

来源：

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY | 1982年 / 199卷 / 01期

关键词：

All Open Access; Bronze;

D O I：

10.1093/mnras/199.1.37

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：37 / 42

页数：6

共 40 条

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[8] PRECISION-MEASUREMENT OF RELATIVE OSCILLATOR-STRENGTHS .6. MEASURES OF FE-I TRANSITIONS FROM LEVELS A5F1-5(0.86-1.01EV) WITH AN ACCURACY OF 0.5-PERCENT [J].

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[10] INTERPRETATION OF THE SOLAR SPECTRUM 300-900 NM .2. FE-I LINES OF EXCITATION POTENTIAL 0.00-1.01EV - USE OF NEW OSCILLATOR-STRENGTHS OF 0.5-PERCENT ACCURACY [J].

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SHALLIS, MJ .

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 1979, 186 (03) :673-684

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