Boundary Conditions on the Formation of Ramparts on Fluidized Ejecta Deposits Around Martian Impact Craters

Details Boundary Conditions on the Formation of Ramparts on Fluidized Ejecta Deposits Around Martian Impact Craters Boundary Conditions on the Formation of Ramparts on Fluidized Ejecta Deposits Around Martian Impact Craters

Mar 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005lpi....36.2127f&link_type=abstract

36th Annual Lunar and Planetary Science Conference, March 14-18, 2005, in League City, Texas, abstract no.2127

Physics

1

Scientific paper

We present a model for the formation of rampart deposits and explore
various source boundary conditions. We find that only modest initial
velocities (<40 m/s) and source flow depths (<30 m) are required
to reproduce observed morphologies.

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