Computer Science
Scientific paper
Jun 1989
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989rspta.328..235m&link_type=abstract
Royal Society (London), Philosophical Transactions, Series A (ISSN 0080-4614), vol. 328, 1989, p. 235-254.
Computer Science
5
Earth Ionosphere, Earth Magnetosphere, Plasma Dynamics, Plasmasphere, Space Plasmas, Auroral Zones, Cold Plasmas, Geomagnetism, Plasma Density, Solar Wind, Spatial Distribution
Scientific paper
Research concerning the transport and distribution of ionospheric plasma in the magnetosphere are reviewed, stressing the dichotomy in explanations given for the low plasma densities outside the plasmasphere. The convection/hot solar plasma model and the convection/loss model are considered. Observations of global ionospheric outflows are compared with theoretical studies. It is suggested that there is a need for a hybrid model of magnetospheric plasma in which terrestrial plasma is both lost into the solar wind and energized and trapped within the magnetosphere, inflating the geomagnetic field and excluding cold plasma from conjugate regions.
Chandler Michael O.
Chappell Charles R.
Moore Thomas Earle
Pollock C. J.
Waite H. Jr. J..
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