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Identification of important error fields in stellarators using the Hessian matrix method

机译:使用Hessian矩阵方法识别恒星中的重要误差场

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Error fields are predominantly attributed to inevitable coil imperfections. Controlling error fields during coil fabrication and assembly is crucial for stellarators. Excessively tight coil tolerance increases time and cost, and, in part, led to the cancellation of the National Compact Stellarator Experiment and delay of W7-X. In this paper, we improve the recently proposed Hessian matrix method to rapidly identify important coil deviations. Two of the most common figures of merit, magnetic island size and quasi-symmetry, are analytically differentiated over coil parameters. By extracting the eigenvectors of the Hessian matrix, we can directly identify sensitive coil deviations in the order of the eigenvalues. The new method is applied to the upcoming Chinese First Quasi-axisymmetric Stellarator configuration. Important perturbations that enlarge n/m= 4/11 islands and deteriorate quasi-axisymmetry of the magnetic field are successfully determined. The results suggest each modular coil should have separate tolerance and some certain perturbation combinations will produce significant error fields. By relaxing unnecessary coil tolerance, this method will hopefully lead to a substantial reduction in time and cost.
机译:误差场主要归因于不可避免的线圈缺陷。线圈制造和组装过程中控制误差场对于恒星器至关重要。过度严格的线圈公差会增加时间和成本,并在一定程度上导致取消了国家紧凑型恒星器实验和W7-X的延迟。在本文中,我们改进了最近提出的Hessian矩阵方法,以快速识别重要的线圈偏差。两种最常见的品质因数,即磁岛尺寸和准对称性,在线圈参数上有分析区别。通过提取Hessian矩阵的特征向量,我们可以按照特征值的顺序直接识别敏感的线圈偏差。该新方法将应用于即将推出的中国“第一个准轴对称恒星器”配置。成功确定了扩大n / m = 4/11岛并恶化磁场的准轴对称性的重要扰动。结果表明,每个模块化线圈应具有单独的公差,并且某些特定的扰动组合会产生明显的误差场。通过放宽不必要的线圈公差,该方法有望大大减少时间和成本。

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