Analysis of Venusian Wrinkle Ridge Morphometry Using Stereo‐Derived Topography: A Case Study From Southern Eistla Regio

Author:

Bethell E. M.1ORCID,Ernst R. E.12ORCID,Samson C.1

Affiliation:

1. Department of Earth Sciences Carleton University Ottawa ON Canada

2. Faculty of Geology and Geography Tomsk State University Tomsk Russia

Funder

Natural Sciences and Engineering Research Council of Canada

Ministry of Education and Science of the Russian Federation

Publisher

American Geophysical Union (AGU)

Subject

Space and Planetary Science,Earth and Planetary Sciences (miscellaneous),Geochemistry and Petrology,Geophysics

Reference84 articles.

1. A brittle model for Martian ridges constrained by surface geometry;Allemand P.;Academie des Sciences (Paris), Comptes Rendus, Serie II – Mecanique, Physique, Chimie, Sciences de la Terre et de l’Univers,1992

2. Tectonic effects of climate change on Venus

3. The tectonic architecture of wrinkle ridges on Mars

4. Regional and global stratigraphy of Venus: a preliminary assessment and implications for the geological history of Venus

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