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Published in 2019 at "Journal of Glaciology"
DOI: 10.1017/jog.2019.54
Abstract: Abstract The Martian mid-latitudes contain numerous small water-ice deposits, collectively termed viscous flow features (VFFs). The shape and topography of the deposits contain information on their past flow history and formation process. In order to…
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Keywords:
topography;
non linear;
lobate debris;
debris apron ... See more keywords