Characterisation of haze, cloud and surface with VIMS onboard Cassini

Details Characterisation of haze, cloud and surface with VIMS onboard Cassini Characterisation of haze, cloud and surface with VIMS onboard Cassini

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf..460r&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.460

Physics

Scientific paper

We have used a model of atmosphere properties, coupled with radiative transfer solver to analyse observations of Titan made by VIMS about haze, clouds and surface. The model is validated with the DISR observations : we use the haze and cloud properties retrieved from observations made during Huygens descent [1] to model the intensity as observed by VIMS at locations close to Huygens landing site. We then use this model to characterise the haze and cloud layer near the pole. We also use this model to give quantitative information about the surface albedo.

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