Observations of the turbulence in the scrape-off-layer of Alcator C-Mod and comparisons with simulation

被引:207
作者
Terry, JL
Zweben, SJ
Hallatschek, K
LaBombard, B
Maqueda, RJ
Bai, B
Boswell, CJ
Greenwald, M
Kopon, D
Nevins, WM
Pitcher, CS
Rogers, BN
Stotler, DP
Xu, XQ
机构
[1] MIT, Plasma Sci & Fus Ctr, Cambridge, MA 02139 USA
[2] Princeton Plasma Phys Lab, Princeton, NJ 08543 USA
[3] Max Planck Inst Plasma Phys, D-85748 Garching, Germany
[4] Los Alamos Natl Lab, Los Alamos, NM 87545 USA
[5] Lawrence Livermore Natl Lab, Livermore, CA 94550 USA
[6] Dartmouth Coll, Hanover, NH 03755 USA
关键词
D O I
10.1063/1.1564090
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
The intermittent turbulent transport in the scrape-off-layer (SOL) of Alcator C-Mod [I.H. Hutchinson, R. Boivin, P.T. Bonoli , Nucl. Fusion 41, 1391 (2001)] is studied experimentally by imaging with a very high density of spatial measurements. The two-dimensional structure and dynamics of emission from a localized gas puff are observed, and intermittent features (also sometimes called "filaments" or "blobs") are typically seen. The characteristics of the spatial structure of the turbulence and their relationship to the time-averaged SOL profiles are discussed and compared with those measured on the National Spherical Torus Experiment [M. Ono, S. M. Kaye, Y.-K. M. Pong , Nucl. Fusion 40, 557 (2000)]. The experimental observations are compared also with three-dimensional nonlinear numerical simulations of edge turbulence. Radial profiles of the poloidal wave number spectra and the poloidal scale length from the simulations are in reasonable agreement with those obtained from the experimental images, once the response of the optical system is accounted for. The resistive ballooning mode is the dominant linear instability in the simulations. The ballooning character of the turbulence is also consistent with fluctuation measurements made at the inboard and outboard midplane, where normalized fluctuation levels are found to be about 10 times smaller on the inboard side. For discharges near the density limit, turbulent structures are seen on closed flux surfaces. (C) 2003 American Institute of Physics.
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页码:1739 / 1747
页数:9
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