Computer Science
Scientific paper
Oct 1976
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976icar...29..299t&link_type=abstract
(IAU, NASA, and NSF, Jupiter Colloquium, 30th, Tucson, Ariz., May 18-23, 1975.) Icarus, vol. 29, Oct. 1976, p. 299-306.
Computer Science
5
Atmospheric Composition, Gas Mixtures, Infrared Spectra, Jupiter Atmosphere, Ammonia, Frequency Response, Helium, Hydrogen, Methane, Molecular Spectra
Scientific paper
The paper presents some results of a theoretical and laboratory program to determine the thermal infrared spectral properties of the principal gaseous constituents of the atmosphere of Jupiter. Birnbaum (1975) has measured laboratory spectra in the 16- to 1000-micron wavelength range for hydrogen and hydrogen-helium mixtures at Jovian temperatures. These are compared with theoretically computed spectra in order to determine the temperature dependence of the line strengths in the pressure-induced rotational band and the overlap parameters from the translational band. Existing spectral data for methane do not agree well with measurements of the nu 4 band at room temperature. A revised allocation of line intensities is proposed. Existing data for the nu 2 (10-micron) band of ammonia agree reasonably well with measurements at room temperature and at -77 C, but there are some important discrepancies which remain to be explained.
Jones D. III A.
Taylor Fred W.
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