Formation of Interdigitate Patterns on Martian Alluvial Fans

Details Formation of Interdigitate Patterns on Martian Alluvial Fans Formation of Interdigitate Patterns on Martian Alluvial Fans

Mar 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007lpi....38.1011h&link_type=abstract

38th Lunar and Planetary Science Conference, (Lunar and Planetary Science XXXVIII), held March 12-16, 2007 in League City, Texas

Physics

Scientific paper

The occurrence of interdigitate patterns on martian alluvial fans
suggests that the latter may have formed under high-density
sediment-gravity driven flows involving upslope aggradation and
backfilling from shifting feeder channels.

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