Information on resource 'Abundance Vertical Profile at Titan with Cassini/CIRS'

This database displays the temperature vertical profiles in Titan's atmosphere at nine different latitudes between 100 and 500 km. These profiles were retrieved from the infrared spectra acquired by the Composite Infrared Spectrometer (CIRS) aboard the Cassini spacecraft. The retrieval method and the description of the used dataset is detailed by Vinatier et al., 2009, Analysis of Cassini/CIRS limb spectra of Titan acquired during the nominal mission. I: Hydrocarbons, nitriles and CO2 vertical mixing ratio profiles, Icarus, in press. doi:10.1016/j.icarus.2009.08.013

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please put reference to http://adsabs.harvard.edu/abs/2010Icar..205..559V and facilities of VOParis using Europlanet environment

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