Inner Magnetosphere Results from Coupled MHD-RDM Modeling

Details Inner Magnetosphere Results from Coupled MHD-RDM Modeling Inner Magnetosphere Results from Coupled MHD-RDM Modeling

Dec 2003

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003agufmsm22a0226d&link_type=abstract

American Geophysical Union, Fall Meeting 2003, abstract #SM22A-0226

Physics

2708 Current Systems (2409), 2730 Magnetosphere: Inner, 2731 Magnetosphere: Outer, 2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling

Scientific paper

The Michigan MHD model (BATSRUS) and the Rice Convection Model (RCM) have been successfully coupled to more accurately simulate the physics in the inner and outer magnetosphere. This self-consistent combined model has been applied to several idealized solar wind input conditions. Results will be presented for a number of magnetic field reversals and magnitude changes. Analysis will include inner magnetospheric shielding, partial and symmetric ring currents, pressure distribution, and particularly 3D global current configurations.

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