Methane spectral line widths and shifts, and dependences on physical parameters-Reference-Cited by-同舟云学术

Methane spectral line widths and shifts, and dependences on physical parameters

Published:1991 Issue:E2 Volume:96 Page:17483
ISSN:0148-0227
Container-title:Journal of Geophysical Research
language:en
Short-container-title:J. Geophys. Res.

Author:

Fox K.,Quillen D. T.,Jennings D. E.,Wagner J.,Plymate C.

Publisher

American Geophysical Union (AGU)

Subject

Paleontology,Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Atmospheric Science,Earth-Surface Processes,Geochemistry and Petrology,Soil Science,Water Science and Technology,Ecology,Aquatic Science,Forestry,Oceanography,Geophysics

Link

http://www.agu.org/journals/je/v096/iE02/91JE01678/91JE01678.pdf

Reference11 articles.

1. Methane absorption in the atmosphere of Saturn: Rotational temperature and abundance from the 3v3 band;Bergstralh;Icarus,1973

2. Methane absorption in the Jovian atmosphere, II, Absorption line formation;Bergstralh;Icarus,1973

3. Spectral shifts of methane in collisions with hydrogen, helium, nitrogen, and argon;Fox;J. Quant. Spectrosc. Radiat. Transfer,1989

4. Spectroscopic studies of methane in collisions with rare gas atoms and diatomic molecules;Fox;J. Mol. Struct.,1990

5. Measurements of argon-, helium-, hydrogen-, and nitrogen-broadened widths of methane lines near 9000 cm-1;Fox;J. Quant. Spectrosc. Radiat. Transfer,1988

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