Latitudinal structures of discrete arcs resulting from viscous interaction between sheared plasma flows

Physics

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Earth Magnetosphere, Magnetohydrodynamic Flow, Shear Flow, Viscous Flow, Auroral Zones, Current Density, Earth Ionosphere, Electron Acceleration, Field Aligned Currents, Ionospheric Currents, Magnetosphere-Ionosphere Coupling

Scientific paper

The role of viscous interactions between sunward and antisunward magnetospheric plasma flows in quasi-steady magnetosphere-ionosphere (MS-IS) coupling is investigated by means of numerical simulations, modeling the latitudinal structures of discrete arcs. Model assumptions include MS-IS current conservation, adiabatic electron motion along magnetic-field lines, and maintenance of upward and downward field-aligned currents by vorticity-induced space charges in the flow-reversal region. An effective conductance due to anomalous viscosity is introduced, and an expression relating the dc field-aligned current density to the magnetospheric electric field is obtained. A diagram of the model MS-IS system is provided, and the results are presented in graphs. The dominant role of a magnetospheric potential structure (of characteristic width about 10 km) in determining the arc latitudinal structure is demonstrated.

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