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Fast recovery of vacuum magnetic configuration of the W7-X stellarator using function parametrization and artificial neural networks

机译:使用功能参数化和人工神经网络快速恢复W7-X恒星发生器的真空磁配置

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摘要

W7-X, a five-period, fully optimized stellarator, currently under construction at IPP-Greifswald, Germany, is built with superconducting coils to show the steady state capability of stellarators. However, the steady state needs continuous equilibrium information for monitoring and controlling the discharge. Although the timescales are long compared with tokamaks, the computational effort for calculating three-dimensional magnetohydrodynamic equilibria is also orders of magnitude higher. This has led us to start the development of a fast equilibrium recovery for W7-X. As a starting point and also for investigating the richness of magnetic configurations, of which only nine physically interesting examples have been examined till now, a fast recovery of vacuum magnetic configurations, described by the flux surface geometry and profile parameters, is carried out using the function parametrization (FP) and artificial neural networks (ANN) methods. Additionally, we parametrize the detectable major magnetic island chains (5/6, 5/5, 5/4) in the form of their locations, (r{sub}(eff)){sup}(is), and their width, w{sup}(is). The quality of FP recovery is compared with ANN, where the vacuum parameters are non-linearly regressed in terms of linear combinations of the coil currents. The results show that a quadratic FP model is generally sufficient for a good recovery of the parameters which are related to the magnetic axis. However, a cubic model is necessary for modelling accurately the magnetic island-related parameters. ANN models offer no improvement over the cubic FP model.
机译:W7-X是一种五周期,经过全面优化的恒星器,目前正在德国IPP-Greifswald建造,它采用超导线圈制造,以显示恒星器的稳态能力。但是,稳态需要连续的平衡信息来监视和控制放电。尽管与托卡马克相比时标很长,但是用于计算三维磁流体动力平衡的计算量也要高几个数量级。这导致我们开始开发W7-X的快速平衡回收率。作为出发点,也是为了研究磁结构的丰富性,到目前为止,仅检查了九个物理有趣的示例,使用磁通表面几何形状和轮廓参数描述的真空磁结构的快速恢复已通过磁通表面几何形状和轮廓参数进行描述。函数参数化(FP)和人工神经网络(ANN)方法。此外,我们以其位置(r {sub}(eff)){sup}(is)及其宽度的形式对可检测的主要磁岛链(5 / 6、5 / 5、5 / 4)进行参数化。 w {sup}(是)。 FP恢复的质量与ANN进行了比较,在ANN中,真空参数根据线圈电流的线性组合非线性回归。结果表明,二次FP模型通常足以良好恢复与磁轴相关的参数。但是,立方模型对于准确地建模与磁岛相关的参数是必需的。与三次FP模型相比,ANN模型没有任何改进。

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