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- W2041635917 abstract "The rotation of a toroidally confined plasma about its magnetic axis due to resistive diffusion is studied by means of a single fluid model in which the only dissipation occurs through a small scalar resistivity. The time evolution of the rotation is examined by considering the resistivity as inducing first-order time variation on a dissipationless steady state. The known instability of flows with small rotational velocity to rapidly speed up toward a critical speed is confirmed; more importantly, it is found that a shock which develops at the critical speed stabilizes the flow, so that the ultimate state of the system is characterized by steady rotation with a very weak shock front directed radially inward from the magnetic axis. The outward flux of plasma in this state is found to be essentially the Pfirsch-Schlüter flux enhanced by a factor of the square root of the aspect ratio." @default.
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- W2041635917 date "1971-02-01" @default.
- W2041635917 modified "2023-09-24" @default.
- W2041635917 title "Resistive Plasma Rotation and Shock Formation in Toroidal Geometry" @default.
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- W2041635917 doi "https://doi.org/10.1063/1.1693436" @default.
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