Initial Correction for Atmospheric Scattering on Titan

Details Initial Correction for Atmospheric Scattering on Titan Initial Correction for Atmospheric Scattering on Titan

Oct 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011epsc.conf.1534v&link_type=abstract

EPSC-DPS Joint Meeting 2011, held 2-7 October 2011 in Nantes, France. http://meetings.copernicus.org/epsc-dps2011, p.1534

Computer Science

Scientific paper

We are using Cassini's Visual and Infrared Mapping Spectrometer (VIMS) and RADAR to correct atmospheric scattering on Titan to first order using the single scattering approximation with a reflective bottom boundary. Titan can scatter signal in many ways, however we have only implemented the most important. More scattering modes exist, but are beyond the scope of this model. The goal here is to empirically fit a full atmospheric transfer function for Titan using as much of the current data as possible. This function will then be used to find absolute surface reflectivities (albedos) that can be used to constrain composition.

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