DSMC simulation of the vertical structure of planetary rings

Details DSMC simulation of the vertical structure of planetary rings DSMC simulation of the vertical structure of planetary rings

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001a%26a...380..761f&link_type=abstract

Astronomy and Astrophysics, v.380, p.761-775 (2001)

Astronomy and Astrophysics

Astrophysics

1

Planets: Rings

Scientific paper

A statistical Monte Carlo method (DSMC) is developed to simulate
granular flows occurring in dense planetary rings. The accuracy of the
method is assessed through a comparison with existing molecular dynamics
simulations of the vertical structure of planetary rings with and
without self-gravity effects.

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