A laboratory study of the 8.65 micron fundamental of (C-12)H3D at temperatures relevant to Titan's atmosphere

Details A laboratory study of the 8.65 micron fundamental of (C-12)H3D at temperatures relevant to Titan's atmosphere A laboratory study of the 8.65 micron fundamental of (C-12)H3D at temperatures relevant to Titan's atmosphere

Dec 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983jqsrt..30..517v&link_type=abstract

Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 30, Dec. 1983, p. 517-522.

Physics

12

Infrared Spectra, Methane, Satellite Atmospheres, Titan, Abundance, Deuterium, Low Temperature, Nitrogen, Pressure Broadening, Spectral Bands, Spectral Line Width, Transmittance, Vibrational Spectra

Scientific paper

Spectral transmittance measurements have been performed in the nu6-fundamental of (C-12)H3D at 153 K. Relevant to the studies of the emission spectra of Titan recorded by the IRIS instruments on board Voyagers 1 and 2, N2 has been used as the broadening gas. Excellent agreement between experimental and theoretical spectral transmittance has been the result of using N2-broadened line widths and their dependence upon temperature measured in the nu2-fundamental and S = 63.6 per(sq cm atm) for the absolute intensity of the nu6-fundamental.

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