Recent Advances on The He/Ne beam diagnostic for line ratio spectroscopy in the Island Divertor of Wendelstein 7-X

POSTER

Abstract

            A line-ratio spectroscopy system based on thermal helium and neon collisional radiative models (CRM) has been implemented and successfully shown to enable measurement of ne and Te above two magnetically connected divertor targets in the standard divertor configuration of the Wendelstein 7-X optimized stellarator. Spectral line emission from gas injection is channeled to multiple Czerny-Turner spectrometers, allowing high spectral resolution measurements of diagnostic helium lines. Neon has also been implemented in select discharges to investigate the expansion of the measurement envelope of the diagnostic into the low Te and high ne regime found in detached discharges.

            In this work, in-situ measurements of gas cloud atomic density distribution from a gas injector identical to those installed at W7-X are presented. Also presented are forward modeling results of the diagnostic based on these gas puff measurements. These profiles facilitate the forward modeling of the diagnostic for future improvements to e.g. collection optics. Also shown are comparisons between helium beam data and multipurpose manipulator probe data using a novel flux coordinate system, an improvement over previous field-tracing methods for diagnostic comparison within the 5/5 island chain. This comparison provides evidence supporting the observation of hollow temperature profiles in the device’s 5/5 island chain. 

*Acknowledgement: This work has been funded by the Department of Energy under grant DE-SC0014210. This work has been carried out within the framework of the EUROfusion Consortium and has received funding from the Euratom research and training programme 2014-2018 and 2019-2020 under grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission.

Presenters

  • Erik R Flom

    • University of Wisconsin - Madison

Authors

  • Erik R Flom

    • University of Wisconsin - Madison
  • Oliver Schmitz

    • University of Wisconsin - Madison
  • Tullio Barbui

    • Princeton Plasma Physics Laboratory
    • PPPL
  • Marcin Jakubowski

    • Max Planck Institute for Plasma Physics
  • Frederik Henke

    • Max Planck Institute for Plasma Physics
  • Maciej Krychowiak

    • Max Planck Institute for Plasma Physics
  • Ralf König

    • Max Planck Institute for Plasma Physics
  • Stuart D Loch

    • Auburn University
  • Jorge M Munoz Burgos

    • Astro Fusion Spectre LLC
  • John C Schmitt

    • Auburn University