Global fluid turbulence simulations in the scrape-off layer of a stellarator island divertor

IF 2.1 3区 物理与天体物理 Q2 PHYSICS, FLUIDS & PLASMAS Journal of Plasma Physics Pub Date : 2024-04-22 DOI:10.1017/s002237782400045x
B. Shanahan, D. Bold, B. Dudson
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Abstract

Isothermal fluid turbulence simulations have been performed in the edge and scrape-off layer (SOL) of an analytic stellarator configuration with an island divertor, thereby providing numerical insight into edge turbulence in regions around islands in a stellarator. The steady-state transport follows the a curvature drive that is inverse to the major radius ( $1/R$ ) toward the outboard side, but large fluctuations are present throughout the island divertor region, with the average wavelength of similar size to the island width. The system exhibits a prominent $m=2$ , $n=5$ mode, where m is the poloidal mode number and n is the toroidal mode number, although other modes are present. The amplitude and radial extent of the density fluctuations are similar throughout the edge and SOL, but can decrease near island O-points. The fluctuations exhibit a predominantly positive skewness on the outboard midplane, indicating blob-like perturbations for the transport into the outer SOL. It is determined that a point on the separatrix is generally more correlated with regions outside of the SOL than a nearby reference point which does not lie on the separatrix.
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恒星器岛分流器刮流层中的全局流体湍流模拟
对带有岛屿分流器的分析恒星器配置的边缘和刮除层(SOL)进行了等温流体湍流模拟,从而为恒星器岛屿周围区域的边缘湍流提供了数值见解。稳态传输遵循与主半径(1/R$)成反比的曲率驱动向外侧移动,但在整个岛屿分流区域存在较大波动,平均波长与岛屿宽度大小相似。该系统表现出一个突出的 $m=2$ , $n=5$ 模式,其中 m 为极环模数,n 为环模数,但也存在其他模式。整个边缘和 SOL 的密度波动幅度和径向范围相似,但在岛屿 O 点附近会减小。在外侧中面上,波动主要呈现正偏度,这表明向 SOL 外部的传输存在类似于圆球的扰动。据测定,与不在分离矩阵上的附近参考点相比,分离矩阵上的某一点通常与 SOL 外部区域的相关性更大。
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来源期刊
Journal of Plasma Physics
Journal of Plasma Physics 物理-物理:流体与等离子体
CiteScore
3.50
自引率
16.00%
发文量
106
审稿时长
6-12 weeks
期刊介绍: JPP aspires to be the intellectual home of those who think of plasma physics as a fundamental discipline. The journal focuses on publishing research on laboratory plasmas (including magnetically confined and inertial fusion plasmas), space physics and plasma astrophysics that takes advantage of the rapid ongoing progress in instrumentation and computing to advance fundamental understanding of multiscale plasma physics. The Journal welcomes submissions of analytical, numerical, observational and experimental work: both original research and tutorial- or review-style papers, as well as proposals for its Lecture Notes series.
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