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.BP11.66
Abstract: BP11.00066 : Impurity studies with Charge Exchange Spectroscopy on W7-X*
Presenter:
Lilla Vanó
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Authors:
Lilla Vanó
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Jürgen Baldzuhn
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Sergey Bozhenkov
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Oliver Ford
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany, Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Robert C Wolf
(Max-Planck-Institute for Plasma Physics, Greifswald, Germany)
Charge Exchange Recombination Spectroscopy (CXRS) is a diagnostic suitable for impurity studies as it measures the emission of low-Z ions. This presentation will give an overview of the passive and active CXRS systems on the Wendelstein 7-X (W7-X) stellarator. The understanding of the behavior of impurities and the control of their concentrations is necessary to adjust the desired radiation level.
During the 2017 experiment campaign of W7-X, a passive CXRS system was employed to observe impurity line emission from the plasma edge. The analysis focuses on inverted spectral radiance, temperature and rotational velocity profiles of carbon-VI. In the analyzed plasmas, the carbon-VI emission seems to be localized inside the last closed flux surface. The experimental observations will be supported by the first comparison with transport modeling using the STRAHL-code.
The active CXRS system requires an external neutral source to give an electron to the fully stripped low-Z ions in the plasma. Neutral Beam Injection (NBI) will be in operation for the first time during the 2018 W7-X campaign. A dedicated spectroscopic observation system has been set-up and the first active measurements will be carried out.
*Work supported by EUROfusion.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.66
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