Spectra of van der Waals complexes (dimers) with applications to planetary atmospheres

Details Spectra of van der Waals complexes (dimers) with applications to planetary atmospheres Spectra of van der Waals complexes (dimers) with applications to planetary atmospheres

Sep 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jqsrt..40..177f&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 40, Sept. 1988, p. 177-184.

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Astronomical Spectroscopy, Atmospheric Composition, Dimers, Molecular Spectra, Planetary Atmospheres, Abundance, Argon, Hydrogen, Nitrogen, Titan

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The authors have attributed spectral features observed in the atmosphere of Titan by the Voyager i.r. experiment to weakly bound complexes of N2 and H2, dominant and minor constituents, respectively. They have also computed the abundance of H2-N2 dimers there. The current calculations include quantitative spectral line positions and intensities for N2-Ar and CO2-CO2 relating to Titan and Earth, and to Mars and Venus, respectively. This work suggests applications to spectra of planetary atmospheres obtained in spacecraft missions.

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