Colin Swee, Benedikt Geiger, Oliver Ford, Mark Nornberg, Martin O’Mullane, Peter Poloskei, Felix Reimold, Thilo Romba, Thomas Wegner and the W7-X Team
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引用次数: 0
摘要
最近在 W7-X 恒星器上安装的高速电荷交换诊断仪被用来识别杂质注入后 500 nm 附近的几条高 n Rydberg 发射线。观测到的高 n Rydberg 转变的波长与杂质种类无关,并且来自电离状态从 14+ 到 45+ 的离子,这表明这种方法可用于各种重杂质。此外,由于高 n 能级不太可能被电子撞击激发填充,因此几乎观察不到被动信号。新开发的诊断方法与对高 n Rydberg 状态的观测相结合,提供了对多种电荷状态的空间分辨高速测量,并在贝叶斯推理框架下进行分析,以确定杂质扩散和对流剖面。2023 年实验活动的测量结果确凿地显示了核心的高扩散和向内挤压,远高于新古典理论的预测。
Impurity transport study based on measurement of visible wavelength high-n charge exchange transitions at W7-X
A recently installed high-speed charge exchange diagnostic at the W7-X stellarator has been used to identify several high-n Rydberg emission lines near 500 nm following impurity injections. The wavelengths of observed high-n Rydberg transitions are independent of the impurity species and originate from ions with ionization states ranging from 14+ to 45+ suggesting that this approach can be applied to a variety of heavy impurities. Moreover, little to no passive signal is observed since the high-n energy levels are unlikely to be populated by electron impact excitation. The combination of the newly developed diagnostic and the observation of high-n Rydberg states provides spatially resolved, high-speed measurements of multiple charge states which are analyzed in a Bayesian inference framework to determine both impurity diffusion and convection profiles. Measurements from the 2023 experimental campaign conclusively show high diffusion and an inward pinch in the core, well above predictions by neoclassical theory.