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Rotationally driven drift modes in the tandem mirror

Journal Article · · IFS Newsl.; (United States)
OSTI ID:5398898
Previous studies of the drift modes in axisymmetric model of the tandem mirror focused on the axial eigenvalue problem with density and temperature gradients driving instability and the angular rotation only accounting for the Doppler shift of the wave frequency to the laboratory frame. The angular rotation Omega of the plasma, however, introduces inertial forces not present in the static plasma. Both the coriolis force and the centrifugal force act preferentially on the ions producing charge separation that changes the low frequency dynamics of the plasma. This paper discussed the effects of these inertial forces on the stability and transport from drift modes in the tandem mirror.
OSTI ID:
5398898
Journal Information:
IFS Newsl.; (United States), Journal Name: IFS Newsl.; (United States) Vol. 3:1; ISSN IFSNE
Country of Publication:
United States
Language:
English

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