X-ray emission-line ratios in MG XI as electron temperature diagnostics for solar flares and active regions-Reference-Cited by-同舟云学术

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X-ray emission-line ratios in MG XI as electron temperature diagnostics for solar flares and active regions

Published:1992-07 Issue: Volume:393 Page:815
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Keenan F. P.,Phillips K. J. H.,Harra L. K.,Conlon E. S.,Kingston A. E.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 5 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. Solar UV and X-ray spectral diagnostics;Living Reviews in Solar Physics;2018-08-31

2. Ultraviolet and X-Ray Spectroscopy of the Solar Atmosphere;CAM ASTROPH;2008

3. Chandra,Extreme Ultraviolet Explorer, and Very Large Array Observations of the Active Binary System σ2Coronae Borealis;The Astrophysical Journal;2003-01-10

4. Diagnosing selenium plasmas using SetXXVI and SetXXV line cluster ratios;Physical Review E;1997-03-01

5. SI XIII emission lines in solar flare x-ray spectra obtained with the P78-1 satellite;The Astrophysical Journal;1994-05

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