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- W1648379890 abstract "For the case of aligned magnetic and rotational axes we solve a fluid version of the Lorentz-Dirac equation, in the Landau approximation, for a two-component plasma. We start from an approximately force-free initial condition and numerically integrate the full equations of motion for a time equal to 1.6% of one stellar rotation period. We find that the system tends to a charge-separated state in which a negative charge region above the poles is separated by a vacuum gap from a positive charge region near the equator. We see the formation of force-free regions and a tendency of the vacuum gap to spread as the integrations proceed. The negative charge above the polar region is electrostatically bound and there is a force-free region towards which negative charge tends to flow" @default.
- W1648379890 created "2016-06-24" @default.
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- W1648379890 date "1993-02-01" @default.
- W1648379890 modified "2023-09-28" @default.
- W1648379890 title "Numerical simulation of the aligned neutron-star magnetosphere" @default.
- W1648379890 hasPublicationYear "1993" @default.
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