Theoretical emission line strengths for Ne VII compared to EUV solar observations-Reference-Cited by-同舟云学术

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Theoretical emission line strengths for Ne VII compared to EUV solar observations

Published:1991-02 Issue:2 Volume:131 Page:291-296
ISSN:0038-0938
Container-title:Solar Physics
language:en
Short-container-title:Sol Phys

Author:

Keenan F. P.

Publisher

Springer Science and Business Media LLC

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/BF00151639.pdf

Reference19 articles.

1. Arnaud, M. and Rothenflug, R.: 1985, Astron. Astrophys. Suppl. 60, 425.

2. Berrington, K. A.: 1985, J. Phys. B18, L395.

3. Berrington, K. A., Burke, P. G., Dufton, P. L., and Kingston, A. E.: 1977, J. Phys. B10, 1465.

4. Berrington, K. A., Burke, P. G., Dufton, P. L., and Kingston, A. E.: 1985, Atomic Data Nucl. Data Tables 33, 195.

5. Doyle, J. G.: 1983, Solar Phys. 89, 115.

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

2. Electron impact collision strengths in Ne VII;Atomic Data and Nuclear Data Tables;2012-07

3. X-ray spectrum of Be-like ions in recombining plasmas;Advances in Space Research;2000-01

4. NeVII emission lines in the solar EUV spectrum;Solar Physics;1999

5. Spectroscopic diagnostics applicable to the UV and EUV spectra of astrophysical sources;Space Science Reviews;1996-02

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