The resistive wall instability and critical flow velocity

被引:24
作者
Lashmore-Davies, CN [1 ]
机构
[1] UKAEA Fus, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
关键词
D O I
10.1063/1.1324657
中图分类号
O35 [流体力学]; O53 [等离子体物理学];
学科分类号
070204 ; 080103 ; 080704 ;
摘要
A cylindrical model with an equilibrium surface current and a uniform equilibrium plasma flow velocity parallel to the axis of the cylinder is used to investigate resistive wall instability. This system can be unstable to the ideal, external kink mode, which-can be stabilized by the presence of a perfectly conducting,wall. This-is the classic condition for the resistive wall instability and the effect of a plasma flow velocity on this mode is explored. II is noted that a stable kink mode, Doppler shifted by the flow velocity; can pass through zero frequency for a velocity which depends on the marginal condition for the external kink instability. The passage through zero frequency is the condition for the kink mode to carry negative energy. It is shown how this mode implies a critical flow speed at which the resistive wall mode is further destabilized, with a growth rate inversely proportional to the square root of the wall time. Under these circumstances, the resistive wall mode behaves more like an ideal instability. All flow velocities are shown to be potentially destabilizing and the flow velocity can produce a resistive wall instability even when the plasma is stable to the external kink mode in the absence of a wall. At velocities well above the critical flow speed, the, resistive wall growth rate is much reduced (inversely proportional to the wall time and to the flow speed). [DOI: 10.1063/1.1324657].
引用
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页码:151 / 157
页数:7
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