Extreme‐Ultraviolet Emission Lines of Sxiiin Solar Active Region and Flare Spectra-Reference-Cited by-同舟云学术

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Extreme‐Ultraviolet Emission Lines of Sxiiin Solar Active Region and Flare Spectra

Published:2002-02-10 Issue:1 Volume:566 Page:521-527
ISSN:0004-637X
Container-title:The Astrophysical Journal
language:en
Short-container-title:ApJ

Author:

Keenan F. P.,Katsiyannis A. C.,Ryans R. S. I.,Reid R. H. G.,Zhang H. L.,Pradhan A. K.,Widing K. G.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://stacks.iop.org/0004-637X/566/i=1/a=521/pdf

Reference40 articles.

1. Atomic data for opacity calculations. II. Computational methods

2. A Discussion on the physics of the solar atmosphere - A.t.m. observations on the X u.v. emission from solar flares

3. The R-Matrix Theory of Atomic Processes

4. Spectral lines observed in solar flares between 171 and 630 angstroms

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1. Energy Levels, Transition Rates and Electron Impact Excitation Rates for the B-like Isoelectronic Sequence with Z = 24–30;The Astrophysical Journal Supplement Series;2018-11-06

2. Relativistic MR-MP Energy Levels for L-shell Ions of Sulfur and Argon;The Astrophysical Journal Supplement Series;2018-10-23

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

4. R-matrix electron-impact excitation data for the B-like iso-electronic sequence;Astronomy & Astrophysics;2012-11

5. R-matrix electron-impact excitation data for astrophysically abundant sulphur ions;Astronomy & Astrophysics;2011-09

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