The State Transion Model of the Substorm

Physics

Scientific paper

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2740 Magnetospheric Configuration And Dynamics, 2753 Numerical Modeling, 2788 Storms And Substorms

Scientific paper

The substorm onset ought to be on the production of enhanced convection under the southward IMF condition. The onset must correspond to the criticality in this convection system rather than to the local instability. The week point of present substorm models is the lack of global self-consistency within the framework of convection system. Where, the primary substances that must be set to the frame of self-consistency are convection flows in the magnetosphere and the ionosphere, filed aligned current systems, ionospheric currents, and energy conversion processes. In this system, the MHD processes primarily determine the position of criticality, since the initial and destination states controlling the criticality and transition are slowly varying convection states. The kinetic effects control the pathway between the states. Global current systems and plasma population regimes associated with the substorm must be fed from the development of MHD force balance controlling the substorm convection. Consequently, substorm models in the next decade must develop from a modular model to a globally self-consistent model.

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