Landscape formation through dissolution proceses on Titan: a 3D landscape evolution model approach - Archive ouverte HAL Accéder directement au contenu
Communication Dans Un Congrès Année : 2017

Landscape formation through dissolution proceses on Titan: a 3D landscape evolution model approach

Résumé

In this work, we are able to produce digital eleva-tion models developed by dissolution under Titan’s surface conditions. These DEMs are used to produce artificial SAR images of the surface in order to com-pare the landscapes with the actual Cassini/RADAR SAR images of Titan. Striking similarities are seen between both kind of SAR images, which suggest that the landscape generated could explain the patterns ob-served in Cassini data. Further work will include the statistical analysis of the produced landscapes in order to infer possible quantitative information about Titan’s polar reliefs.

Domaines

Planétologie
Fichier non déposé

Dates et versions

hal-01449807 , version 1 (30-01-2017)

Identifiants

  • HAL Id : hal-01449807 , version 1
  • OKINA : ua15505

Citer

Thomas Cornet, Cyril Fleurant, Benoit Seignovert, Daniel Cordier, Olivier Bourgeois, et al.. Landscape formation through dissolution proceses on Titan: a 3D landscape evolution model approach. 48th Lunar and Planetary Science Conference, 2017, The Woodlands, United States. ⟨hal-01449807⟩
237 Consultations
0 Téléchargements

Partager

Gmail Facebook X LinkedIn More