2022
DOI: 10.5194/epsc2022-59
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Clues to the subsurface fault pattern of circum-Tharsis wrinkle ridges

Abstract: <p><strong>Introduction</strong></p> <p>Wrinkle ridges are significant landforms on planetary bodies, and most of them occur in flood basalt units of large igneous provinces, [1]-[2]. On Mars, the circum-Tharsis wrinkle ridge system developed under compressional stresses associated with the response of the lithosphere due to the Tharsis volcanic load [1]. The morphology of ridges shows large variations and may reflect subsurface fault patter… Show more

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