Electric field generation at the magnetospheric boundary for northward IMF

Details Electric field generation at the magnetospheric boundary for northward IMF Electric field generation at the magnetospheric boundary for northward IMF

Feb 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994jatp...56..153e&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 56, no. 2, p. 153-166

Physics

1

Atmospheric Boundary Layer, Atmospheric Diffusion, Electric Fields, Interplanetary Magnetic Fields, Kelvin-Helmholtz Instability, Magnetic Field Reconnection, Magnetohydrodynamic Flow, Magnetopause, Earth Ionosphere, Field Aligned Currents, Lorentz Force, Magnetosphere-Ionosphere Coupling, Polar Regions, Reynolds Number, Solar Terrestrial Interactions, Solar Wind

Scientific paper

We discuss three different processes which generate electric fields at the magnetopause during northward interplanetary magnetic field (IMF) conditions. These are (1) Petschek-type magnetic field reconnection, (2) magnetic field diffusion, and (3) viscous-like interaction resulting from the Kelvin-Helmholtz instability. For northward IMF all three processes lead to the formation of a boundary layer on closed magnetic field lines adjacent to the magnetospheric boundary. The thickness of the boundary layer depend on Petschek's parameter in the first case, the magnetic Reynolds number in the second case, and an effective Reynolds number in the third case. In each case coupling between the boundary layer and the ionosphere occurs via field-aligned currents. These field-aligned currents result from the penetration into the polar ionosphere of the electric field generated at the magnetospheric boundary. These currents are closed by a transverse current in the boundary layer and the associated Lorentz force causes a decrease of the kinetic energy of the solar wind plasma inside the boundary layer. As a result of this velocity decrease the thickness of the boundary layer increases on both flanks of the magnetosphere near the equatorial plane. The convergence of the boundary layer on the dawn and dusk sides leads to antisunward plasma flow in the magnetospheric tail.

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