Saturn's rotation and plasma convection

Details Saturn's rotation and plasma convection Saturn's rotation and plasma convection

Aug 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007epsc.conf..934f&link_type=abstract

European Planetary Science Congress 2007, Proceedings of a conference held 20-24 August, 2007 in Potsdam, Germany. Online at ht

Physics

Scientific paper

The "tongue" model of corotating rotationally driven convection proposed by Goldreich & Farmer (2007) appears to explain many of the features now known to be modulated at the SKR period, i.e. magnetospheric plasma enhancement, magnetic perturbations, and the SKR itself. We shall discuss how well this model holds up to the latest data from Cassini, and suggest the physical reasons for the existence of such a stable, broad convection pattern.

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