Effect of motions in prominences on the helium resonance lines in the extreme ultraviolet
Author:
Publisher
EDP Sciences
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://www.aanda.org/10.1051/0004-6361:20065775/pdf
Reference32 articles.
1. Electron collision strengths for all transitions among the n=1, 2, 3, 4 and 5 levels of He+
2. Excitation rate coefficients for transitions among the N = 1, 2, and 3 levels of He(+)
3. Allen, C. W. 1973, Astrophysical quantities (London: University of London, Athlone Press, 3rd Ed.)
4. On the Nature of Dark Extreme Ultraviolet Structures Seen bySOHO/EIT andTRACE
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