Inferences on the Emplacement Dynamics of Martian Impact Crater Ejecta: Constraints from MOLA Topography

Details Inferences on the Emplacement Dynamics of Martian Impact Crater Ejecta: Constraints from MOLA Topography Inferences on the Emplacement Dynamics of Martian Impact Crater Ejecta: Constraints from MOLA Topography

Mar 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999lpi....30.1735g&link_type=abstract

30th Annual Lunar and Planetary Science Conference, March 15-29, 1999, Houston, TX, abstract no. 1735

Physics

1

Scientific paper

A continuum flow model using cylindrical geometry is developed for
analyzing ejecta emplacement for martian rampart craters. New
constraints on the behavior of ejecta are suggested.

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