Wrinkle Ridges
Wrinkle Ridge is a tectonic landform characterized by low, asymmetric, sinuous topographic highs formed by compressional stresses in volcanic plains, typically on planetary surfaces, distinguishing it from other contractional features through its association with mare basalts and shallow thrust faulting.
134
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7.4K
Citations
326
Authors
173
Institutions
Publications per year
2017–2026
23
Variants
Wrinkle Ridge
134
Compressional tectonism on Mars
T. R. Watters · Journal of Geophysical Research Atmospheres · 1993 · 231 citations
1–5 of 134
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V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry, Russia
7 publications · 271 citations
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1–5 of 326
173
National Air and Space Museum
Washington, United States
11 h-index
27 publications
2.3K citations
Brown University
Providence, United States
10 h-index
29 publications
3.1K citations
Smithsonian Institution
Washington, United States
8 h-index
11 publications
304 citations
United States Geological Survey
Reston, United States
6 h-index
7 publications
737 citations
V.I. Vernadsky Institute of Geochemistry and Analytical Chemistry
Moscow, Russia
6 h-index
7 publications
248 citations
Planetary Science Institute
Tucson, United States
5 h-index
10 publications
1.7K citations
Arizona State University
Tempe, United States
5 h-index
22 publications
2K citations
University of Arizona
Tucson, United States
4 h-index
14 publications
1.7K citations
1–8 of 173
JGR · 29 publications · 2.9K citations
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11 publications · 398 citations
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9 publications · 367 citations
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5 publications · 110 citations
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5 publications · 543 citations
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