A comparison of theoretical and solar-flare intensity ratios for the Fe XIX X-ray lines-Reference-Cited by-同舟云学术

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A comparison of theoretical and solar-flare intensity ratios for the Fe XIX X-ray lines

Published:1989-09 Issue:2 Volume:240 Page:421-444
ISSN:0035-8711
Container-title:Monthly Notices of the Royal Astronomical Society
language:en
Short-container-title:

Author:

Bhatia A. K.,Fawcett B. C.,Lemen J. R.,Mason H. E.,Phillips K. J. H.

Publisher

Oxford University Press (OUP)

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://academic.oup.com/mnras/article-pdf/240/2/421/18223782/mnras240-0421.pdf

Cited by 33 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. The XSTAR Atomic Database;Atoms;2021-02-05

2. RADIATIVE L-SHELL TRANSITIONS IN Fe XIX AND Fe XX IONS;The Astrophysical Journal Supplement Series;2009-12-22

3. Effective collision strengths for electron-impact excitation of transitions within the ground 1s 2 2s 2 2p 4 manifold of O-like Fe18+;International Journal of Quantum Chemistry;2009

4. 4.1.2.7 Flares;Solar System;2009

5. Atomic data from the IRON project;Astronomy & Astrophysics;2008-07-17

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