Pressure-induced absorption in the infrared - A data base for the modelling of planetary atmospheres

Details Pressure-induced absorption in the infrared - A data base for the modelling of planetary atmospheres Pressure-induced absorption in the infrared - A data base for the modelling of planetary atmospheres

Sep 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991jgr....9617501b&link_type=abstract

(International Conference on Laboratory Research for Planetary Atmospheres, 2nd, Charlottesville, VA, Oct. 21, 1990, Proceedings

Statistics

Computation

11

Absorption Spectra, Gas Giant Planets, Infrared Absorption, Planetary Atmospheres, Pressure Effects, Data Bases, Infrared Spectra, Molecular Spectra, Rotational Spectra

Scientific paper

The present study reports recent progress related to the modeling of various pressure-induced absorption bands of binary molecular systems involving dissimilar and like pairs of molecules such as H2, He, N2, and CH4. References are made to the existing efforts based on quantum line shape computations that reproduce the laboratory measurements of pressure-induced absorption closely. The findings are presented as a data base permitting an evaluation of pressure-induced absorption as a function of frequency, temperature, and gas density for various binary molecular systems and spectral bands in the infrared region of the spectrum. Line shape computations based on isotropic interaction potentials are found to be very successful for modeling pressure-induced spectra for most systems of interest for planetary atmospheres, including the summed contributions of bound dimers.

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