Fe XVIII emission-line intensities in the sun-Reference-Cited by-同舟云学术

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Fe XVIII emission-line intensities in the sun

Published:1992-01 Issue: Volume:385 Page:378
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

McKenzie D. L.,Keenan F. P.,McCann S. M.,Berrington K. A.,Hibbert A.,Mohan M.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 6 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. Fe XVIII emission lines in solar X-ray spectra;Solar Physics;1997

2. , and abundances derived from spectroscopic and sep analysis;Advances in Space Research;1997-01

3. Anomalous Coronal Neon Abundances in Quiescent Solar Active Regions;The Astrophysical Journal;1996-12-10

4. Collisonal excitation of Fe X due to electron impact using the R-matrix method;The Astrophysical Journal;1994-10

5. Effective collision strengths among the fifteen lowest states of FeXVII;Pramana;1993-06

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