Helicon full-wave modeling with scrape-off-layer turbulence on the DIII-D tokamak

被引:8
|
作者
Lau, Cornwall [1 ]
Brookman, Michael [2 ]
Dimits, Andris [3 ]
Dudson, Ben [4 ]
Martin, Elijah [1 ]
Pinsker, Robert I. [2 ]
Thomas, Matt [4 ]
Van Compernolle, Bart [2 ]
机构
[1] Oak Ridge Natl Lab, Oak Ridge, TN 37830 USA
[2] Gen Atom, San Diego, CA USA
[3] Lawrence Livermore Natl Lab, Livermore, CA USA
[4] Univ York, York Plasma Inst, York, N Yorkshire, England
关键词
helicon; current drive; DIII-D tokamak; turbulence; full-wave modeling; scrape-off-layer; POWER-PLANT; HIGH-FIELD; PLASMA; SCATTERING;
D O I
10.1088/1741-4326/ac36f3
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
Helicon waves have been recently proposed as an off-axis current drive actuator due to their expected high current drive efficiency in the mid-radius region in high beta tokamaks. This paper focuses on a numerical study to better understand effects of scrape-off-layer (SOL) turbulence on helicon wave propagation and absorption on the DIII-D tokamak using a recently developed helicon full-wave model with turbulent density inputs from synthetic single wavelength SOL turbulence and first-principles HERMES multi-wavelength turbulence models. With both input turbulence models, three key effects are observed: the helicon wave can scatter to undesirable locations in the plasma, large helicon wave electric fields can form in localized regions near the SOL turbulence, and the helicon wave can mode convert to slow waves in the SOL. This is shown to cause helicon wave refraction to undesirable locations and strong helicon wave absorption in the SOL resulting in significantly less helicon wave power in the core plasma. Using synthetic SOL turbulence, the simulations additionally show that high amplitudes and long wavelengths greater than a few cm on average have the largest effect on modifying the helicon wave propagation and absorption; the modeling predicts, for example, that approximately 60% of helicon power can be absorbed in the SOL for n/n similar to 0.8 and lambda_perp similar to 0.05 m. Several potential physical mechanisms that may explain the interaction of helicon waves with SOL turbulence in these simulations are discussed.
引用
收藏
页数:16
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