Structure of ELMs in MAST and the implications for energy deposition

被引:76
作者
Kirk, A [1 ]
Wilson, HR
Akers, R
Conway, NJ
Counsell, GF
Cowley, SC
Dowling, J
Dudson, B
Field, A
Lott, F
Lloyd, B
Martin, R
Meyer, H
Price, M
Taylor, D
Walsh, M
机构
[1] UKAEA Euratom Fus Assoc, Culham Sci Ctr, Abingdon OX14 3DB, Oxon, England
[2] Univ London Imperial Coll Sci Technol & Med, Dept Phys & Astron, London SW7 2BZ, England
[3] Univ Calif Los Angeles, Los Angeles, CA 90095 USA
[4] Univ Oxford, Clarendon Lab, Oxford OX1 3PU, England
[5] Walsh Sci Ltd, Culham Sci Ctr, Abingdon OX14 3EB, Oxon, England
关键词
D O I
10.1088/0741-3335/47/2/008
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
This paper presents a description of the spatial and temporal structure of edge-localized modes (ELMs) observed in the MAST tokamak. Filamentary enhancements of visible light are observed on photographic images of the plasma obtained during ELMs. Comparisons with simulations show that these filaments are consistent with following field lines at the outboard edge of the plasma. The toroidal mode number of these filaments has been extracted from a study of the discrete peaks observed in the ion saturation current recorded by a mid-plane reciprocating probe. A study of the time delay of these peaks with respect to the onset of the ELM has been used to calculate an effective radial velocity for the expansion of the filaments. A comparison of this derived radial velocity as a function of distance from the last closed flux surface with simulations indicates that the filament is accelerating away from the plasma. Evidence for the temporal evolution of the ELM comes from studies of outboard mid-plane Thomson scattering density profiles. In addition, a study of the toroidal velocity as a function of radius shows that during an ELM the strong velocity shear near the edge of the plasma; normally present in H-modes, is strongly reduced. The picture that emerges is that the ELM can be viewed as being composed of filamentary structures that are generated on a 100 mus timescale, accelerate away from the plasma edge, are extended along a field line and have a typical toroidal mode number similar to10. The implications of these filaments for the energy deposition on plasma facing components are discussed.
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页码:315 / 333
页数:19
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