Numerical Simulations of the Interaction of Enceladus' Interaction With Saturn's Magnetosphere Using a 3D Multi-Species, Hall MHD Model

Details Numerical Simulations of the Interaction of Enceladus' Interaction With Saturn's Magnetosphere Using a 3D Multi-Species, Hall MHD Model Numerical Simulations of the Interaction of Enceladus' Interaction With Saturn's Magnetosphere Using a 3D Multi-Species, Hall MHD Model

Dec 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007agufm.p43a1009n&link_type=abstract

American Geophysical Union, Fall Meeting 2007, abstract #P43A-1009

Physics

2736 Magnetosphere/Ionosphere Interactions (2431)

Scientific paper

We have used our new multi-species, Hall MHD model to study the interaction of Saturn's magnetosphere with Enceladus. We used neutral densities, consistent with the values observed during the Cassini's July 14, 2005 flyby of Enceladus. We used a simple ion chemistry scheme and approximated the upstream conditions from CAPS and MAG observations. We compare our calculated plasma and magnetic field values with the observed ones.

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