用机器学习分析磁约束下离子温度梯度湍流,发现几何形状决定热输运强度。
How does ion temperature gradient turbulence depend on magnetic geometry? Insights from data and machine learning
- 基于20万+仿真数据,用深度学习和分类模型识别影响湍流的关键几何特征。
- 不同几何下热通量差异可达数个数量级,压缩区坏曲率是最重要的控制因素。
- 结果可推广至新构型评估,适合等离子体物理与人工智能交叉研究者。
磁几何对聚变等离子体湍流输运水平有显著影响。本文利用超过20万次非轴对称几何下的离子温度梯度湍流非线性模拟数据,结合多种机器学习方法进行建模与分析。数据集涵盖优化与随机生成的托卡马克与仿星器平衡态。在固定梯度条件下,不同几何构型间的湍流热通量相差可达数个数量级,且高/低通量构型呈现明显趋势。采用回归与分类技术从数据中提取模式。由于吉罗动力学方程的对称性,热通量及其回归结果应具有平行坐标系中特征的平移不变性,类似计算机视觉中的平移不变性。多种回归模型(包括卷积神经网络与决策树)在保留测试构型上均展现出合理预测能力,其中CNN表现最优。通过斯皮尔曼相关性、顺序特征选择与沙普利值分析特征重要性,一致发现对热通量影响最大的几何参数是坏曲率区域的通量面压缩程度,其次为地心曲率大小。这两项特征与已有理论提出的代理指标高度吻合,且本方法可自然扩展更多特征以提升精度。该数据集随论文公开,可用于验证其他代理模型,我们发现多个已有文献提出的近似指标与热通量及稳定性边界均有良好相关性。
原文摘要 · Abstract (English)
Magnetic geometry has a significant effect on the level of turbulent transport in fusion plasmas. Here, we model and analyze this dependence using multiple machine learning methods and a dataset of > 200,000 nonlinear simulations of ion-temperature-gradient turbulence in diverse non-axisymmetric geometries. The dataset is generated using a large collection of both optimized and randomly generated stellarator equilibria. At fixed gradients, the turbulent heat flux varies between geometries by several orders of magnitude. Trends are apparent among the configurations with particularly high or low heat flux. Regression and classification techniques from machine learning are then applied to extract patterns in the dataset. Due to a symmetry of the gyrokinetic equation, the heat flux and regressions thereof should be invariant to translations of the raw features in the parallel coordinate, similar to translation invariance in computer vision applications. Multiple regression models including convolutional neural networks (CNNs) and decision trees can achieve reasonable predictive power for the heat flux in held-out test configurations, with highest accuracy for the CNNs. Using Spearman correlation, sequential feature selection, and Shapley values to measure feature importance, it is consistently found that the most important geometric lever on the heat flux is the flux surface compression in regions of bad curvature. The second most important feature relates to the magnitude of geodesic curvature. These two features align remarkably with surrogates that have been proposed based on theory, while the methods here allow a natural extension to more features for increased accuracy. The dataset, released with this publication, may also be used to test other proposed surrogates, and we find many previously published proxies do correlate well with both the heat flux and stability boundary.
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