Bulletin of the American Physical Society
60th Annual Meeting of the APS Division of Plasma Physics
Volume 63, Number 11
Monday–Friday, November 5–9, 2018; Portland, Oregon
Session BP11: Poster Session I: HEDP; General Stellarator; Wendelstein 7-X; Heating, Current Drive, and Energetic Ions (9:30am-12:30pm)
Monday, November 5, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.BP11.65
Abstract: BP11.00065 : The He/Ne beam diagnostic for line ratio spectroscopy in the island divertor of Wendelstein 7-X*
Presenter:
Erik Flom
(University of Wisconsin)
Authors:
Tullio Barbui
(Univ of Wisconsin, Madison)
Erik Flom
(University of Wisconsin)
Florian Effenberg
(Univ of Wisconsin, Madison)
Oliver Schmitz
(Univ of Wisconsin, Madison)
Marcin Jakubowski
(Max Planck Inst Plasmaphysik)
Maciej Krychowiak
(Max Planck Inst Plasmaphysik)
Ralf Koenig
(Max Planck Inst Plasmaphysik)
Jorge M. Muñoz Burgos
(Astro Fusion Spectre)
Stuart Loch
(Auburn Univ)
The line-ratio spectroscopy system on thermal He and Ne enables measurement of ne and Te in front of the horizontal divertor target, across the 5/5 island in the standard magnetic configuration. For the second divertor campaign of Wendelstein 7-X the observation system has been upgraded adding 27 new vertical lines-of-sight to the existing 27 horizontal ones. These lines are channeled to a 20cm and a 32cm focal length Czerny-Turner spectrometer allowing observation of the He and Ne lines as well as impurities and H lines with high spectral resolution. Gas injection is enabled by two boxes with 5 fast piezo valves each, mounted directly behind the divertor plates in one upper and one lower divertor module, which are magnetically connected in the 5/5 island configuration. He was used as routine gas while Ne was tested in order to extend the applicability of the diagnostic to the detached divertor regime at very low Te (≪10eV). In this work Te/ne profiles across the divertor island are shown for different island widths. Results from Ne injection and the status of the development of a dedicated collisional-radiative model for Ne will be discussed.
*This work has been funded by the Department of Energy under grant DE-SC0014210 and by EUROfusion under grant No 633053.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.65
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