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Detailed Reference Information |
Barlow, N.G., Koroshetz, J. and Dohm, J.M. (2001). Variations in the onset diameter for Martian layered ejecta morphologies and their implications for subsurface volatile reservoirs. Geophysical Research Letters 28: doi: 10.1029/2000GL012804. issn: 0094-8276. |
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We investigated regional variations in the onset diameter of craters displaying a single layer ejecta morphology within ¿30¿ latitude using Viking imagery. Our results generally agree with those of previous studies which show onset diameters of 5 to 6 km in the equatorial region, but we have identified localized regions with unusually small onset diameters. The largest region is located in Solis and Thaumasia Planae. The 3--5 km onset diameter range in this area indicates a near-surface ice-rich reservoir (depth ~110 m). This unusual concentration of near-surface ice may have resulted from magmatic-driven uplifts associated with the Tharsis rise, which modified parts of a regional aquifer/drainage basin system and resulted in the transfer and concentration of subsurface volatiles in this region. ¿ 2001 American Geophysical Union |
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Abstract |
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Keywords
Planetology, Solid Surface Planets, Impact phenomena (includes cratering), Planetology, Solid Surface Planets, Remote sensing, Planetology, Solid Surface Planets, Tectonics, Planetology, Solar System Objects, Mars |
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Publisher
American Geophysical Union 2000 Florida Avenue N.W. Washington, D.C. 20009-1277 USA 1-202-462-6900 1-202-328-0566 service@agu.org |
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