Enhancement of the helium resonance lines in the solar atmosphere by suprathermal electron excitation - II. Non-Maxwellian electron distributions
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/341/1/143/18645568/341-1-143.pdf
Reference79 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. Abundances of the elements: Meteoritic and solar
4. Coulomb collisions and coronal heating by velocity filtration
5. Ultraviolet Emission-Line Intensities and Coronal Heating by Velocity Filtration: Collisionless Results
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