Model for the Emplacement of the Outer Ejecta Layer of Low Aspect-Ratio Layer Ejecta Craters by Turbulent Flow

Details Model for the Emplacement of the Outer Ejecta Layer of Low Aspect-Ratio Layer Ejecta Craters by Turbulent Flow Model for the Emplacement of the Outer Ejecta Layer of Low Aspect-Ratio Layer Ejecta Craters by Turbulent Flow

Mar 2012

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2012lpi....43.1081b&link_type=abstract

43rd Lunar and Planetary Science Conference, held March 19–23, 2012 at The Woodlands, Texas. LPI Contribution No. 1659, id.1081

Physics

1

Scientific paper

Our modeling and geomorphic analysis suggest that the outer ejecta layer
of low aspect-ratio layer ejecta (LARLE) craters may be fine-grain
ejecta deposited from a dilute, suspension-driven, gravity current
produced by collapse of the ejecta column.

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