Physics
Scientific paper
Dec 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989jqsrt..42..437w&link_type=abstract
Journal of Quantitative Spectroscopy and Radiative Transfer (ISSN 0022-4073), vol. 42, Dec. 1989, p. 437-443.
Physics
9
Acetylene, Infrared Lasers, Laser Spectroscopy, Molecular Spectra, Semiconductor Lasers, Tunable Lasers, Doppler Effect, Gas Giant Planets, Planetary Atmospheres, Quantitative Analysis, Spectral Line Width, Vibrational Spectra
Scientific paper
Understanding of acetylene spectral features observed in the laboratory with high-resolution is a prerequisite for quantitative analyses of acetylene spectra in the planetary atmospheres of Titan, Saturn, and Jupiter. Line-intensity measurements on (C-12)2H2 near 13.7 microns were made using a tunable diode-laser spectrometer with a resolution of at least 0.0005 cm exp -5. Vibrational band intensities at 296 K were determined from the line-intensity measurements for the nu5-fundamental band of (C-12)2H2 and for a specified hotband of (C-12)2H2.
Blass William E.
Salanave Jean-Luc
Weber Matthias
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