Initial Correction for Atmospheric Scattering on Titan

Computer Science

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

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.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Initial Correction for Atmospheric Scattering on Titan does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Initial Correction for Atmospheric Scattering on Titan, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Initial Correction for Atmospheric Scattering on Titan will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1486205

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.