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- W2292067534 abstract "Valles Marineris includes a series of troughs south of the Martian equator trending West to East for a distance of 4000 km. The aim of this paper is to derive the geomorphometric signature of this extraterrestrial feature on the basis of the digital elevation model derived from Mars Orbiter Laser Altimeter. More specifically, the canyon system was outlined and various geomorphometric parameters (elevation, massiveness, gradient, aspect, profile and planar curvature etc.) are computed in an attempt to characterize and segment the landscape. The geomorphometric data indicate that the Valles Marineris look more to an active tectonic zone of earth. In order to further verify it, the terrain within the canyon should be segmented to mountain and non-mountain terrain class and to compare the derived statistics to Great Basin (USA), Minor Asia and Zagros Ranges. Additionally isolated mountains, piedmonts and peneplains should be extracted and parametrically represented and compared to earth. Higher resolution elevation data is required too in order to examine the geomorphometry of valley mouths deposits and compare them to piedmont zones, alluvial fans and gravity cones of earth." @default.
- W2292067534 created "2016-06-24" @default.
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- W2292067534 date "2003-01-01" @default.
- W2292067534 modified "2023-09-23" @default.
- W2292067534 title "THE GEOMORPHOMETRIC SIGNATURE OF VALLES MARINERIS FROM M.O.L.A. D.E.M." @default.
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- W2292067534 doi "https://doi.org/10.6084/m9.figshare.1004636.v1" @default.
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