Sheared flow amplification by vacuum magnetic islands in stellarator plasmas
Phys. Plasmas 8, 4111 (2001); doi:10.1063/1.1392996
Issue Date: September 2001
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There is some experimental evidence that the E×B flows have radial structure that may be linked to rational surfaces. This flow structure may result from a self-organization process involving nonlinear flow amplification through Reynolds stress and fluctuation reduction by sheared flows. In stellarators, a large contribution to the Reynolds stress comes from the coupling of the magnetic field component of a vacuum field island with a plasma instability. In this process, the self-organization principle seems to be marginal stability for the fluctuations driving the flow. ©2001 American Institute of Physics.
| History: | Received 8 May 2001; accepted 20 June 2001 |
| Permalink: |
http://link.aip.org/link/?PHPAEN/8/4111/1 |
KEYWORDS and PACS
- 52.55.Hc
Physics of plasmas and electric discharges Magnetic confinement and equilibrium Stellarators, torsatrons, heliacs, bumpy tori, and other toroidal confinement devices - 52.65.Kj
Physics of plasmas and electric discharges Plasma simulation Magnetohydrodynamic and fluid equation - 52.35.Ra
Physics of plasmas and electric discharges Waves, oscillations, and instabilities in plasmas and intense beams Plasma turbulence - YEAR: 2001
RELATED DATABASES
PUBLICATION DATA
1070-664X (print)
1089-7674 (online)
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