Control of Magnetospheric Convection by the Spatial Distribution of Ionospheric Conductivities.

摘要

A self-consistent semianalytical model of magnetospheric convection including the effect of conductivities is presented. The motions of the inner edge of the magnetospheric ring current, and the associated field-aligned currents, produced by the externally imposed dawn-to-dusk potential drop across the magnetospheric cavity are computed by using a linear approximation. The coupling between the different diurnal harmonics in the local time variations of fields and currents produced by the local time dependence of ionospheric conductivities is described by an appropriate matrix formalism. The calculations show that the enhancement of auroral conductivities by electron precipitation in the auroral zone signficantly enhances both the typical duration and the absolute amplitude of the penetration of convection electric fields to midlatitudes. Furthermore, the local time variations of the convection electric field generated at midlatitudes by a sudden increase of the dawn-to-dusk potential drop are in good agreement, both at the initial time and after the steady state is reached, with the available statistical models of the disturbance midlatitude electric field. Keywords: Incoherent scatter; ionosphere; magnetosphere; electric fields; substorms; auroral zone; shielding of electric fields; Reprints.