SWS Observations and detection of water vapour on Titan

Details SWS Observations and detection of water vapour on Titan SWS Observations and detection of water vapour on Titan

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999esasp.427..157c&link_type=abstract

The Universe as Seen by ISO. Eds. P. Cox & M. F. Kessler. ESA-SP 427., p. 157

Computer Science

Iso/Sws, Infrared Planetology, Titan, Atmosphere, Water Vapor

Scientific paper

The Titan ISO/SWS data were acquired in January and December 1997 in the grating mode with resolving powers between 1000-3000. Their analysis yielded information on the thermal and compositional structure of the satellite's atmosphere on a disk average basis with higher precision than the Voyager data. From a particular observational sequence around 40 μm, the SWS data allowed the first detection of water vapor in Titan's upper atmosphere.

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