Time-dependent flows in the renovated model of the magnetosphere

Physics

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Atmospheric Models, Birkeland Currents, Magnetospheric Instability, Plasma Dynamics, Space Plasmas, Ion Motion, Magnetohydrodynamic Flow, Plasma Layers, Polar Caps, Time Dependence

Scientific paper

A revised empirical model of the magnetosphere, based on observations of Birkeland currents, is presented with earthward flow in the plasma sheet confined to the duskside. Convection (E x B drift) carries tail-associated features in the sunward direction. This competes with Birkeland-current-associated plasma depletion (divergence of ion drifts), which allows flux tubes to collapse to a more dipolar form, thereby moving tail-associated features in the antisunward direction. In substorm intensifications, depletion dominates, and the taillike region recedes from the earth. The recession appears to be unstable. A quantitative relationship between Birkeland currents and convection is developed and is used on published results. It indicates that 4 x 10 to the 20th ions drift off a plasma sheet flux tube as it collapses from taillike to dipolar.

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