Analysis of Nonlinear Density Waves in Saturn's Rings in the Light of Cassini Radio-science Data

Details Analysis of Nonlinear Density Waves in Saturn's Rings in the Light of Cassini Radio-science Data Analysis of Nonlinear Density Waves in Saturn's Rings in the Light of Cassini Radio-science Data

Sep 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006dps....38.3806r&link_type=abstract

American Astronomical Society, DPS meeting #38, #38.06; Bulletin of the American Astronomical Society, Vol. 38, p.553

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Scientific paper

By contrast with the Voyager mission, Cassini provides us with many different radio optical depths profiles of Saturn's main rings. This provides us with new constraints which open the possibility to quantify in a much better way the physics of the ring-satellite interaction on the one hand, and the ring rheology on the other.
To this purpose, we have developed a new method of analysis of density-waves, that makes simultaneous use of several radio-science profiles for a given wave. This method of analysis will be presented, along with first results for typical waves.

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