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Titlebook: Solar-Terrestrial Physics; Principles and Theor R. L. Carovillano,J. M. Forbes Conference proceedings 1983 D. Reidel Publishing Company, Do

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Solar-Wind Magnetosphere Coupling model. The basic element of solar-wind magnetosphere coupling is the magnetospheric convection flow driven by the solar-wind flow at their common boundary. The voltage across this flow is the fundamental measure of the coupling rate. The magnitude of this voltage, and its dependence on interplaneta
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Origins and Consequences of Parallel Electric Fieldsh electric fields exist has been observationally established only in the last five years (.., 1980). Early proponents of the pro-E. case pointed to the nearly monoenergetic beams of keV electrons observed above auroral arcs. Opponents argued against E. on both theoretical and observational grounds.
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Comparative Magnetospherespossible effects, related to finite ionospheric conductivity, flow of the external medium, or breakdown of radial stress balance, each of which becomes important beyond a particular characteristic distance.
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0067-0057 ollowed by the first theory conference in the field. This book is based upon the lectures presented at the School. Several years ago there was a convergence of efforts to promote the role of theory in space plasma physics. Reports from the National Academy of Sciences and NASA advisory committees do
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Solar System Magnetohydrodynamicstional and viscous forces of fluid dynamics. Magnetofluid mechanics applies to fluids that can carry electrical currents, such as liquid metals and plasmas. Our interest in Solar System MHD is confined to the latter.
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