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Resistive instability in a uniformly rotating magnetoplasma

Published online by Cambridge University Press:  13 March 2009

A. D. Lunn
Affiliation:
Iviathematical Institute, Oxford

Extract

A closed set of guiding centre equations, derived for a rotating plasma in a static magnetic field, is applied to the problem of the stability of a plasma in a sheared field. The rotation is found to have a stabilizing effect in the absence of resistivity.

A pair of coupled, linear differential equations is derived for the rotating plasma in a weakly sheared field. Dispersion relations are obtained by phase integral methods and, in the absence of finite Larmor radius effects and rotation, instability growth rates proportional to η½13 are found which become proportional to when either is included. The inclusion of both finite Larmor radius and rotation gives growing instabilities proportional to η which are stabilized by the rotation when the finite Larmor radius terms predominate.

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Articles
Copyright
Copyright © Cambridge University Press 1971

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