Article ID | Journal | Published Year | Pages | File Type |
---|---|---|---|---|
8866847 | Remote Sensing of Environment | 2018 | 12 Pages |
Abstract
Linear dunes discovered in the equatorial regions of Titan by the Cassini-Huygens mission are morphologically very similar to these linear dune fields in the Egyptian Sahara. Hence, assessing the variability of morphology and radar backscatter properties of Titan's dunes as a function of their heights can help constrain the ambiguities associated with their internal structure and formation history and provide insights into Titan's paleo-wind regimes.
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Computers in Earth Sciences
Authors
Priyanka Sharma, Essam Heggy, Tom G. Farr,