CISM: Center for Integrated Space Weather Modelling

Rice Convection Model

Bastille Day Storm

The Rice Convection Model incorporates energy- and charge-dependent gradient and curvature drifts in the inner magnetosphere, given an MHD-specification of both magnetic field and plasma boundary conditions. Coupling back to the MHD code will modify the pressure evolution in the inner magnetosphere.

Click on image at left to enlarge.

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