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Modeling of pressure-induced far-infrared absorption spectra: Molecular hydrogen pairs

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/163482· OSTI ID:6174772
The collision-induced translational-rotational absorption coefficient for molecular hydrogen pairs has been computed from the fundamental theory by Meyer, Frommhold, and Birnbaum for temperatures from 40 to 300 K. Over the frequency range from approx.30 to 1500 cm , theoretical and measured profiles are in close agreement (+-5%). The theory is capable of generating reliable spectra of hydrogen pairs at temperatures for which no laboratory measurements exist. Since quantum line shape computations cannot be readily repeated elsewhere on account of their complexity, we identify simple, suitable functions which approximate the exact profiles closely (approx.1%), even in the far wings. The absorption spectra are well reproduced by simple three-parameters are determined by least-squares fits of the theoretical profiles. They vary smoothly with temperature T. The collision-induced translational-rotational absorption coefficient, ( ), of H2-H2 can thus be reliably and very rapidly reproduced on computers of small capacity, using codes with simple programming. This facilitates accurate computations of radiative transfer in modeling the atmospheres of the outer planets.
Research Organization:
University of Texas at Austin
OSTI ID:
6174772
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 296:2; ISSN ASJOA
Country of Publication:
United States
Language:
English