Numerical simulation of the gravitational collapse of meteorite craters

Details Numerical simulation of the gravitational collapse of meteorite craters Numerical simulation of the gravitational collapse of meteorite craters

Feb 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992avest..26...77p&link_type=abstract

Astronomicheskii Vestnik (ISSN 0320-930X), vol. 26, Jan.-Feb. 1992, p. 77-82. In Russian.

Mathematics

Logic

Gravitational Collapse, Incompressible Flow, Liquid Flow, Mathematical Models, Meteorite Craters, Computerized Simulation, Hypervelocity Impact, Lunar Craters

Scientific paper

A numerical model of impact-crater gravitational collapse is presented. The model consists of a numerical method for solving viscous incompressible fluid flows - the markers-and-cells method - and a numerical analog of the Bingham rheological model - the biviscous model. The model is used to estimate deformations of the rock underlying complex impact craters and some other characteristic values. Ways of improving the model are indicated.

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