Development of a layered precipitation structure during the process of magnetospheric convection

Details Development of a layered precipitation structure during the process of magnetospheric convection Development of a layered precipitation structure during the process of magnetospheric convection

Dec 1976

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1976ge%26ae..16.1061l&link_type=abstract

Geomagnetizm i Aeronomiia, vol. 16, Nov.-Dec. 1976, p. 1061-1065. In Russian.

Physics

Auroral Arcs, Electron Precipitation, Geomagnetic Tail, Ionospheric Disturbances, Magnetospheric Instability, Proton Precipitation, Atmospheric Stratification, E Region, High Temperature Plasmas, Ionospheric Currents, Magnetospheric Ion Density, Magnetospheric Proton Density

Scientific paper

The instability of the precipitation into the ionosphere of energetic particle fluxes which convect together with the magnetospheric plasma out of the magnetospheric tail is analyzed. It is shown that, making allowance for the gradient drift of hot particles, the electron and proton structures must develop independently and must have a different orientation when observed simultaneously: the electron structures are extended in the NE-SW direction and the proton structures, in the NW-SE direction.

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