Evidence for Radiative Recombination of O+ Ions as a Significant Source of O 844.6 nm Emission Excitation
Author:
Affiliation:
1. Department of Electrical and Computer Engineering; University of Illinois at Urbana-Champaign; Urbana IL USA
2. Computational Physics, Inc.; Chelmsford MA USA
Funder
National Science Foundation
Publisher
Wiley
Subject
Space and Planetary Science,Geophysics
Reference29 articles.
1. The OI844.6 nm emission in evening twilight;Bahsoun-Hamade;Geophysical Research Letters,1989
2. Thermospheric OI 844.6-nm emission in twilight;Bahsoun-Hamade;Journal of Geophysical Research,1994
3. International reference ionosphere-status 1995/96;Bilitza;Advances in Space Research,1997
4. Excitation by line coincidence;Bowen;Publications of the Astronomical Society of the Pacific,1947
5. Solar Lyman-β fluorescence mechanisms in the upper atmosphere;Brandt;Astrophysical Journal,1959
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