| Article ID | Journal | Published Year | Pages | File Type |
|---|---|---|---|---|
| 10701733 | Icarus | 2012 | 16 Pages |
Abstract
⺠A reflectivity map of Mars is obtained from the radar sounder SHARAD. ⺠We apply statistical models to retrieve surface roughness and dielectric constant. ⺠Scattering is the most important process dominating reflectivity over Mars. ⺠The non-stationary nature of most martian terrains is confirmed. ⺠RMS roughness can be obtained for slightly rough surfaces without any calibration.
Keywords
Related Topics
Physical Sciences and Engineering
Earth and Planetary Sciences
Space and Planetary Science
Authors
Cyril Grima, Wlodek Kofman, Alain Herique, Roberto Orosei, Roberto Seu,