Water vapor in Titan's atmosphere observed with Cassini/CIRS data

Details Water vapor in Titan's atmosphere observed with Cassini/CIRS data Water vapor in Titan's atmosphere observed with Cassini/CIRS data

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1487c&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1487

Physics

Scientific paper

In this paper we show the detection of the water lines present in the spectral range (60 - 560 cm-1) observed by the CIRS FP1 detector. The first estimate of water atmospheric abundance gives a value of about 0.14 ppb for a constant water vapour vertical profile, which corresponds to a water column abundance of 4.3x1014 molecules/cm2. Using a water profile increasesing with altitude up to 10 ppb at 400 km altitude the retrieved column abundance is 5.8x10+14 molecules/cm2.

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