Prediction of the fine-scale irregular structure in Saturn’s A, B, and C rings

Details Prediction of the fine-scale irregular structure in Saturn’s A, B, and C rings Prediction of the fine-scale irregular structure in Saturn’s A, B, and C rings

Jan 2006

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006adspr..38..770g&link_type=abstract

Advances in Space Research, Volume 38, Issue 4, p. 770-776.

Physics

5

Scientific paper

In view of the possibility of employing CASSINI’s experiments for the diagnosis of Saturn’s rings, local N-body simulations of low and moderately high optical depth regions of Saturn’s rings are presented. A special emphasis is made on fine-scale spiral structures (irregular cylindric wave-type structures of the order of 100 m or so) of Saturn’s main A, B, and C rings. We predict that CASSINI spacecraft high-resolution images of Saturn’s main rings will reveal this kind of irregular microstructure.

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