Thermospheric production of O(1S) by dissociative recombination of vibrationally excited O2+-Reference-Cited by-同舟云学术

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Thermospheric production of O(1S) by dissociative recombination of vibrationally excited O2+

Published:1986-11 Issue:11 Volume:34 Page:1101-1107
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Yee Jeng-Hwa,Killeen T.L.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference18 articles.

1. The dissociative recombination of O2+: the quantum yield of O(1S) and O(1D);Abreu;J. geophys. Res.,1983

2. The O(1S) quantum yield from O2+ dissociative recombination;Bates;Planet. Space Sci.,1981

3. The neutral mass spectrometer on Dynamics Explorer B;Carrignan;Space Sci. Instrum.,1981

4. The OII (5577 Å) airglow: observations and excitation mechanisms;Federick;J. geo-phys. Res.,1976

5. Potential curves for the dissociative recombination;Guberman,1983

Cited by 17 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Airglow and Aurora in the Atmospheres of Venus and Mars;Venus and Mars: Atmospheres, Ionospheres, and Solar Wind Interactions;2013-03-18

2. Effect of solar activity on the latitudinal variation of peak emission rate of 557.7nm dayglow emission under equinox conditions;Journal of Atmospheric and Solar-Terrestrial Physics;2012-03

3. Dissociative Recombination of Molecular Ions;2008

4. The morphology of oxygen greenline dayglow emission;ANN GEOPHYS-ATM HYDR;1998

5. The O(;Annales Geophysicae;1996

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