Infrared line widths at planetary atmospheric temperatures

Details Infrared line widths at planetary atmospheric temperatures Infrared line widths at planetary atmospheric temperatures

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jqsrt..39...13v&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 39, Jan. 1988, p. 13-25.

Computer Science

24

Atmospheric Temperature, Infrared Spectra, Line Spectra, Planetary Temperature, Temperature Dependence, Atmospheric Composition, Carbon Dioxide, Helium, Hydrogen, Nitrogen, Oxygen

Scientific paper

Recent theoretical models and measurements of the variation of collision-broadened line width with temperature in the infrared are discussed for temperatures relevant to planetary atmospheres. The present review is restricted to lines broadened by H2, N2, O2, CO2, and He, the lines formed in the atmospheres of Jupiter, Saturn, Uranus, and Neptune. The design for a low-temperature absorption cell consisting of a nickel-coated copper tube is described. The lack of an adequate theoretical model for variation of the collision-broadened line width with temperature in terms of the molecular constants of the colliding partners is pointed out.

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