Physics
Scientific paper
Feb 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003phrvl..90f1102s&link_type=abstract
Physical Review Letters, vol. 90, Issue 6, id. 061102
Physics
6
Planetary Rings, Granular Flow: Mixing, Segregation And Stratification, Pattern Formation, Saturn
Scientific paper
Viscous overstability (oscillatory instability) may play an important role in the formation of small scale structure in dense planetary rings such as Saturn’s B ring. We investigate the growth and saturation of such modes in local particle simulations. Starting from a hydrodynamic model, we develop a set of ordinary differential equations to model the evolution of the amplitudes of the linearly overstable modes in the nonlinear regime. The NASA/ESA space probe Cassini can make direct observations of these modes in Saturn’s rings, including their sizes and temporal development.
Salo Heikki
Schmidt Jürgen
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