模拟和分析 MAST-U 的高 K 电子尺度湍流诊断结果

David C. Speirs, Juan Ruiz-Ruiz, Maurizio Giacomin, Valerian H. Hall-Chen, Alan D. R. Phelps, Roddy Vann, Peter G. Huggard, Hui Wang, Anthony Field, Kevin Ronald
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引用次数: 0

摘要

不同空间和时间尺度上的等离子体湍流在确定托卡马克中可达到的约束水平方面起着关键作用,而根据实验测量结果开发跨尺度湍流效应的简化数字模型则是必不可少的一步。MAST-U 是一个装备精良的设施,拥有测量等离子体边缘离子和电子尺度湍流的仪器。然而,核心电子湍流的测量具有挑战性,尤其是在H模式下。利用一种新的合成诊断方法,我们提出了基于毫米波的集体散射仪器的模拟测量规格,该仪器针对测量MAST-U核心和边缘的正态和双态电子尺度湍流进行了优化。我们开发了一个强大的建模框架,将波束跟踪技术与陀螺动力学模拟相结合,以预测测量的灵敏度、定位和光谱范围。对于所构建的 MAST 022769 射束,可测量的最大归一化双正态波数为 $k_{\perp} \rho_{e} \rho_{e} \rho_{e} \rho_{e} \rho_{e} 。\sim 0.6$,而$k_{perp} \rho_{e} \sim 0.6$。在基座附近的定位长度$L_{FWHM}$为${sim$ 0.4 m,在核心处为$k_{perp} \rho_{e} \sim 0.79$,在基座附近为$k_{perp} \rho_{e} \sim 0.79$。\rho_{e} \sim0.1$ 到 $k_{perp} 时的 ~0.08m\rho_{e} \sim 0.45$。利用CGYRO陀螺动能模拟光谱对022769号卫星进行的合成诊断分析表明,ETG扰动峰值光谱强度的波数正好在仪器从核心到基座的可测量范围内。所提出的诊断方法为研究即将在 MAST-U 上进行的非电感、基于微波的电流驱动实验相关的湍流和凝聚新机制提供了机会,并可深入了解跨尺度湍流效应,同时适合在 STEP 等未来反应堆的燃烧等离子体情况下运行。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Simulation and analysis of a high-k electron scale turbulence diagnostic for MAST-U
Plasma turbulence on disparate spatial and temporal scales plays a key role in defining the level of confinement achievable in tokamaks, with the development of reduced numerical models for cross-scale turbulence effects informed by experimental measurements an essential step. MAST-U is a well-equipped facility having instruments to measure ion and electron scale turbulence at the plasma edge. However, measurement of core electron scale turbulence is challenging, especially in H mode. Using a novel synthetic diagnostic approach, we present simulated measurement specifications of a proposed mm-wave based collective scattering instrument optimised for measuring both normal and binormal electron scale turbulence in the core and edge of MAST-U. A powerful modelling framework has been developed that combines beam-tracing techniques with gyrokinetic simulations to predict the sensitivity, localisation and spectral range of measurement. For the reconstructed MAST 022769 shot, a maximum measurable normalised bi-normal wavenumber of $k_{\perp} \rho_{e} \sim 0.6$ was predicted in the core and $k_{\perp} \rho_{e} \sim 0.79$ near the pedestal, with localisation lengths $L_{FWHM}$ ranging from $\sim$ 0.4 m in the core at $k_{\perp} \rho_{e} \sim 0.1$ to ~0.08m at $k_{\perp} \rho_{e} \sim 0.45$. Synthetic diagnostic analysis for the 022769 shot using CGYRO gyrokinetic simulation spectra reveal that ETG turbulence wavenumbers of peak spectral intensity comfortably fall within the measurable range of the instrument from the core to the pedestal. The proposed diagnostic opens up opportunities to study new regimes of turbulence and confinement in association with upcoming non-inductive, microwave based current drive experiments on MAST-U and can provide insight into cross-scale turbulence effects, while having suitability to operate during burning plasma scenarios on future reactors such as STEP.
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