Retrieval of HCN Concentrations from Cassini/VIMS Limb Observations of the Titan's Upper Atmosphere

Details Retrieval of HCN Concentrations from Cassini/VIMS Limb Observations of the Titan's Upper Atmosphere Retrieval of HCN Concentrations from Cassini/VIMS Limb Observations of the Titan's Upper Atmosphere

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1189a&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1189

Computer Science

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Scientific paper

Vertical profiles of hydrogen cyanide (HCN) have been retrieved from Cassini/VIMS limb observations in the region from 600 to 1100 km of the Titan's atmosphere by analyzing the 3 μm emission. HCN concentrations show a very good correlation with solar zenith angles, for different latitudes and local times. This would indicate that HCN is in (or close to) photochemical equilibrium in the sounded region.

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