FE (12) IN CORONA EMISSION

被引：6

作者：

ROZELOT, JP

机构：

[1] Observatoire du Pic-du-Midi, Bagnères-de-Bigorre

来源：

SOLAR PHYSICS | 1969年 / 8卷 / 01期

关键词：

D O I：

10.1007/BF00150660

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Assuming that FeXII is reduced to 16 energy levels, we have computed the relative intensities of 21 spectral lines as a function of two parameters, temperature and electron density. Results are briefly discussed and summarized in Figures 1-21. © 1969 D. Reidel Publishing Company.

引用

页码：91 / &

共 13 条

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ASTROPHYSICAL JOURNAL, 1964, 140 (03) :1192-&

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