Pablant N A, Langenberg A, Alonso J A, Bitter M, Bozhenkov S A, Ford O P, Hill K W, Kring J, Marchuck O, Svensson J, Traverso P, Windisch T, Yakusevitch Y
Princeton Plasma Physics Laboratory, Princeton, New Jersey 08540, USA.
Max-Planck-Institut für Plasmaphysik, Greifswald 17491, Germany.
Rev Sci Instrum. 2021 Apr 1;92(4):043530. doi: 10.1063/5.0043513.
X-ray ray tracing is used to develop ion-temperature corrections for the analysis of the X-ray Imaging Crystal Spectrometer (XICS) used at Wendelstein 7-X (W7-X) and perform verification on the analysis methods. The XICS is a powerful diagnostic able to measure ion-temperature, electron-temperature, plasma flow, and impurity charge state densities. While these systems are relatively simple in design, accurate characterization of the instrumental response and validation of analysis techniques are difficult to perform experimentally due to the requirement of extended x-ray sources. For this reason, a ray tracing model has been developed that allows characterization of the spectrometer and verification of the analysis methods while fully considering the real geometry of the XICS system and W7-X plasma. Through the use of ray tracing, several important corrections have been found that must be accounted for in order to accurately reconstruct the ion-temperature profiles. The sources of these corrections are described along with their effect on the analyzed profiles. The implemented corrections stem from three effects: (1) effect of sub-pixel intensity distribution during de-curving and spatial binning, (2) effect of sub-pixel intensity distribution during forward model evaluation and generation of residuals, and (3) effect of defocus and spherical aberrations on the instrumental response. Possible improvements to the forward model and analysis procedures are explored, along with a discussion of trade-offs in terms of computational complexity. Finally, the accuracy of the tomographic inversion technique in stellarator geometry is investigated, providing for the first time a verification exercise for inversion accuracy in stellarator geometry and a complete XICS analysis tool-chain.
X射线射线追踪用于为文德恩斯坦7-X(W7-X)上使用的X射线成像晶体光谱仪(XICS)的分析开发离子温度校正,并对分析方法进行验证。XICS是一种强大的诊断工具,能够测量离子温度、电子温度、等离子体流和杂质电荷态密度。虽然这些系统在设计上相对简单,但由于需要扩展X射线源,仪器响应的精确表征和分析技术的验证很难通过实验来进行。出于这个原因,已经开发了一种射线追踪模型,该模型在充分考虑XICS系统和W7-X等离子体的实际几何形状的同时,可以对光谱仪进行表征并验证分析方法。通过使用射线追踪,已经发现了几个重要的校正,为了准确重建离子温度分布,必须考虑这些校正。描述了这些校正的来源及其对分析分布的影响。所实施的校正源于三种效应:(1)去弯曲和空间分箱过程中亚像素强度分布的效应,(2)正向模型评估和残差生成过程中亚像素强度分布的效应,以及(3)散焦和球差对仪器响应的效应。探讨了正向模型和分析程序可能的改进,以及在计算复杂性方面的权衡讨论。最后,研究了托卡马克几何形状断层反演技术的准确性,首次提供了托卡马克几何形状反演准确性的验证练习和完整的XICS分析工具链。