在低温等离子体中利用建模和机器学习的氦线发射光谱测量等离子体参数

S. Kajita, D. Nishijima
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摘要

众所周知,氦(He)原子的线强度比(LIR)取决于电子密度($n_{\rm e}$)和温度($T_{\rm e}$),因此被广泛用于评估这些参数,这就是所谓的 He I LIR 方法。在这种传统方法中,测量的 LIR 与使用碰撞辐射(CR)模型计算的理论值进行比较,以找到最佳的 $n_{\rm e}$ 和 $T_{\rm e}$。基本的碰撞辐射模型已经过改进,以考虑多种效应。例如,在弱电离等离子体中,辐射捕获会在很大程度上发生,从而导致 LIRs 发生重大变化。这种效应已与光学逸散因子一起被纳入 CR 模型。最近,人们利用机器学习(ML)探索了一种新方法来评估He I LIRs中的$n_{\rm e}$和$T_{\rm e}$。在 ML 辅助 LIR 方法中,利用训练数据开发了一个预测模型,训练数据包括输入(测量的 LIRs)和期望/已知输出(测量的 $n_{\rm e}$ 或来自其他诊断的 $T_{\rm e}$)。结果表明,这种新方法不仅对氦气,而且对其他物种的 n_{\rm e}$ 和 T_{\rm e}$ 预测结果都优于使用传统方法和 CR 模型的预测结果。
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Helium line emission spectroscopy to measure plasma parameters using modeling and machine learning in low temperature plasmas
Line intensity ratios (LIRs) of helium (He) atoms are known to depend on electron density, $n_{\rm e}$, and temperature, $T_{\rm e}$, and thus are widely utilized to evaluate these parameters, which is the so-called He I LIR method. In this conventional method, measured LIRs are compared with theoretical values calculated using a collisional-radiative (CR) model to find the best possible $n_{\rm e}$ and $T_{\rm e}$. Basic CR models have been improved to take into account several effects. For instance, radiation trapping can occur to a significant degree in weakly ionized plasmas, leading to major alterations of LIRs. This effect has been included with optical escape factors in CR models. A new approach to the evaluation of $n_{\rm e}$ and $T_{\rm e}$ from He I LIRs has recently been explored using machine learning (ML). In the ML-aided LIR method, a predictive model is developed with training data, which consist of input (measured LIRs) and desired/known output (measured $n_{\rm e}$ or $T_{\rm e}$ from other diagnostics). It has been demonstrated that this new method predicts $n_{\rm e}$ and $T_{\rm e}$ better than using the conventional method coupled with a CR model, not only for He but also for other species.
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