Interesting features of convection within the plasmasphere

Details Interesting features of convection within the plasmasphere Interesting features of convection within the plasmasphere

Jan 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988jatp...50...41h&link_type=abstract

Journal of Atmospheric and Terrestrial Physics (ISSN 0021-9169), vol. 50, Jan. 1988, p. 41-43.

Physics

1

Atmospheric Conductivity, Convective Flow, Geomagnetism, Plasmasphere, Whistlers, Earth Magnetosphere, Ionospheric Drift, Ionospheric Propagation, Solar Terrestrial Interactions

Scientific paper

Convection within the plasmasphere arises from the rotation of the earth's magnetic field, electric fields in the ionosphere which map up to greater altitudes, and the dawn-dusk magnetospheric electric field produced by the interaction of the solar wind with the earth's magnetic field. It is believed that the contributions of ionospheric and magnetospheric electric fields may give rise to density inhomogeneities and turbulence in the plasmasphere.

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