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- W2011609985 abstract "A laboratory experiment is described which simulates some aspects of the interaction of the solar wind and the geomagnetic field. In this experiment, a Mach 2 hydrogen plasma stream from a pulsed coaxial gun was directed against a dipole magnetic field. The shape of the windward side of the magnetic cavity and the circulation of the sheet currents in the boundary were found to be in general agreement with results based on the single-particle model. But the supersonic-fluid model is appropriate for the interpretation of further results. A nonluminous arc-shaped region resembling a bow shock wave appeared upstream from the nose of the cavity, and the plasma was observed to flow irreversibly through this region and around the cavity. Time-resolved photographs depict the dynamics of the interaction, revealing drifts of the plasma near the interface layer and penetration of the plasma into the magnetic cavity. At times following the impact of the plasma on the field, the field near the magnet was found to be asymmetric and generally lower than the normal dipole field. The recovery time of the field to the dipole value was long in comparison with the decay time of the plasma pulse from the gun." @default.
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- W2011609985 date "1964-06-01" @default.
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- W2011609985 title "Interaction of a supersonic plasma stream with a dipole magnetic field" @default.
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- W2011609985 doi "https://doi.org/10.1029/jz069i011p02257" @default.
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