Solar plasma diagnostic for O III spectral lines by using the collision excitation model-Reference-Cited by-同舟云学术

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Solar plasma diagnostic for O III spectral lines by using the collision excitation model

Published:2015-05 Issue:10 Volume:66 Page:1508-1510
ISSN:0374-4884
Container-title:Journal of the Korean Physical Society
language:en
Short-container-title:Journal of the Korean Physical Society

Author:

He Jian,Zhang Qingguo

Publisher

Korean Physical Society

Subject

General Physics and Astronomy

Link

http://link.springer.com/content/pdf/10.3938/jkps.66.1508.pdf

Cited by 9 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Calculation of averaged collision strength of magnesium for non-Maxwellian distributions in plasma;Modern Physics Letters B;2019-08-07

2. Calculation of Kappa-Averaged Collision Strengths of Silicon VIII Ion for a Non-Maxwellian Distribution;Journal of the Korean Physical Society;2018-11

3. Electron density of the magnesium XII doublet in the solar corona by use of a collision excitation model;Spectroscopy Letters;2018-01-02

4. Temperature diagnostics of plasma under optically-thin conditions;Modern Physics Letters B;2017-11-06

5. κ distribution of carbon II doublet in the solar transition region;Journal of Atmospheric and Solar-Terrestrial Physics;2017-11

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