Coupled Michigan MHD - Rice Convection Model Results

Details Coupled Michigan MHD - Rice Convection Model Results Coupled Michigan MHD - Rice Convection Model Results

Dec 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002agufmsm22a0567d&link_type=abstract

American Geophysical Union, Fall Meeting 2002, abstract #SM22A-0567

Computer Science

Performance

2730 Magnetosphere: Inner, 2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling

Scientific paper

A new high performance Rice Convection Model (RCM) has been coupled to the adaptive-grid Michigan MHD model (BATSRUS). This fully coupled code allows us to self-consistently simulate the physics in the inner and middle magnetosphere. A study will be presented of the basic characteristics of the inner and middle magnetosphere in the context of a single coupled-code run for idealized storm inputs. The analysis will include region-2 currents, shielding of the inner magnetosphere, partial ring currents, pressure distribution, magnetic field inflation, and distribution of pV^gamma.

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