Inner Magnetosphere Simulations - Coupling the Michigan MHD Model with the Rice Convection Model.

Details Inner Magnetosphere Simulations - Coupling the Michigan MHD Model with the Rice Convection Model. Inner Magnetosphere Simulations - Coupling the Michigan MHD Model with the Rice Convection Model.

Dec 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001agufmsm42a0830d&link_type=abstract

American Geophysical Union, Fall Meeting 2001, abstract #SM42A-0830

Computer Science

Performance

2730 Magnetosphere: Inner, 2736 Magnetosphere/Ionosphere Interactions, 2753 Numerical Modeling

Scientific paper

The adaptive-grid Michigan MHD model (BATSRUS) has been coupled to a new high performance Rice Convection Model (RCM). This fully coupled code allows us to self-consistently simulate the physics in the inner magnetosphere, including Region 1 and Region 2 currents. We will describe the two models and how they are coupled, report on the results of a synthetic event with the coupled code and show a comparison with and without coupling.

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