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.BP11.51
Abstract: BP11.00051 : STRAHL modeling of impurity transport on Wendelstein 7-X during the first divertor campaign*
Presenter:
P. J. Traverso
(Auburn University)
Authors:
P. J. Traverso
(Auburn University)
N. A. Pablant
(Princeton Plasma Phys Lab)
A. Langenberg
(Max Planck Inst)
R. Burhenn
(Max Planck Inst)
T. Wegner
(Max Planck Inst)
B. Geiger
(Max Planck Inst)
D. Zhang
(Max Planck Inst)
B. Buttenschön
(Max Planck Inst)
J. D. Kring
(Auburn University)
J. C. Schmitt
(Auburn University)
D. A. Maurer
(Auburn University)
W7-X Team
(Max Planck Inst)
In the first divertor operational phase (OP 1.2a) of Wendelstein 7-X, impurity transport experiments were performed with iron via laser blow-off injection. The x-ray imaging spectrometer systems, HR-XIS and XICS, were used to measure the He-like spectra at various input ECRH heating powers and plasma densities. These measured He-like iron spatial and temporal emissivities can then be used to estimate the He-like iron’s diffusion and convective velocity parameters. Utilizing the 1D transport code STRAHL, the spatial and temporal evolution of the He-like iron charge state is modeled for assumed stationary anomalous diffusion and convective velocity profiles. To match both the observed total He-like iron emissivity and a corresponding spatially inverted emissivity profile, a chi-squared minimization is done on the experimental data by varying the input spatial values of the anomalous diffusion and convective velocity parameters in STRAHL.
*This work is supported by U.S. Department of Energy Grant No. DE-SC00014529
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.BP11.51
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