Energy transfer of O(1S) atoms in collision with O(3P) atoms-Reference-Cited by-同舟云学术

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Energy transfer of O(1S) atoms in collision with O(3P) atoms

Published:1985-07 Issue:7 Volume:33 Page:825-830
ISSN:0032-0633
Container-title:Planetary and Space Science
language:en
Short-container-title:Planetary and Space Science

Author:

Yee Jeng-Hwa,Dalgarno A.

Publisher

Elsevier BV

Subject

Space and Planetary Science,Astronomy and Astrophysics

Reference11 articles.

1. Twilight and nightglow spectral line shapes of oxygen γ6300 and γ5577 radiation;Biondi;Planet. Space Sci.,1968

2. Energy transfer in oxygen-hydrogen collisions;Cooper;Planet. Space Sci.,1984

3. Doppler profiles of the 5577 Å airglow;Hays;Planet. Space Sci.,1971

4. he signature profile of O(1S) in the airglow;Hernandez;Planet. Space Sci.,1971

5. Non-thermal line profiles from O(1S) in the thermospheric nightglow;Killeen;Appl. Opt.,1981

Cited by 21 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. Escape of O(3P), O(1D), and O(1S) from the Martian atmosphere;Icarus;2018-01

2. Escape and evolution of Mars's CO2 atmosphere: Influence of suprathermal atoms;Journal of Geophysical Research: Planets;2017-06

3. Hot oxygen and carbon escape from the martian atmosphere;Planetary and Space Science;2014-08

4. The escape of O from Mars: Sensitivity to the elastic cross sections;Icarus;2014-01

5. Venus' atomic hot oxygen environment;Journal of Geophysical Research;2010-12-30

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