Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
10701505 | Icarus | 2011 | 8 Pages |
Abstract
⺠Passive and active data from the Cassini RADAR are examined for their implications on the radar-bright regions of Titan. ⺠Kirchhoff's law of thermal radiation and the assumption of a generic low-loss scattering subsurface is the basis for a combined emission-backscatter (CEB) model developed for this purpose. ⺠Some of the regions are too bright to be explained by this model. ⺠We conclude that organized structure on or in the surface is present that enhances the backscatter.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
M.A. Janssen, A. Le Gall, L.C. Wye,