Other
Scientific paper
Apr 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993icar..102..240c&link_type=abstract
Icarus (ISSN 0019-1035), vol. 102, no. 2, p. 240-260.
Other
48
Atmospheric Composition, Infrared Spectra, Satellite Atmospheres, Titan, Vertical Distribution, Benzene, Carbon Monoxide, Cyanides, Infrared Space Observatory (Iso), Methane, Water Vapor, Saturn, Satellites, Titan, Models, Spectra, Wavelength, Infrared, Thermal Properties, Techniques, Remote Sensing, Temperature, Abundance, Laboratory Studies, Simulation, Methane, Distribution, Stratosphere, Parameters, Atmosphere, Composition, Molecules, Spectroscopy, Space, Calculations, Iso Satellite, Cassini Mission, Ir
Scientific paper
The observability of minor species in Titan's atmosphere in its infrared thermal range is systematically studied and modeled to generate synthetic spectra. The model results on methane, water vapor, benzene, allene, and other heavier trace molecules are used to illustrate the capabilities of instruments aboard the Infrared Space Observatory, in particular a high-resolution composite infrared spectrometer, to determine vertical distributions of the molecules in a few hours of integration time.
Arie E.
Bezard Bruno
Bjoraker Gordon
Coustenis Athena
Dang-Nhu M.
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