Characteristics of the Inner and Middle Magnetosphere: Results From the Coupled Michigan MHD Model and the Rice Convection Model

Computer Science – Performance

Scientific paper

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2708 Current Systems (2409), 2730 Magnetosphere: Inner, 2736 Magnetosphere/Ionosphere Interactions, 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 with steady 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. The coupled-code simulation will be compared with results from RCM runs and algorithms.

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