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 NM9: Mini-Conference on Plasma–Material Interactions in Fusion Devices: ITER and Beyond. III. Helium and Impurity Effects on PMI
9:30 AM–12:30 PM,
Wednesday, November 7, 2018
OCC
Room: C123
Chair: Ane Lasa Esquisabel, University of Tennessee
Abstract ID: BAPS.2018.DPP.NM9.6
Abstract: NM9.00006 : Quantification on the Effect of Uncertainty On Impurity Migration In PISCES-A Simulated With GITR
11:25 AM–11:45 AM
Presenter:
Tim Younkin
(Oak Ridge National Lab, University of Tennessee)
Authors:
Tim Younkin
(Oak Ridge National Lab, University of Tennessee)
Khachick Sargsyan
(Sandia National Laboratories)
Tiernan Casey
(Univ of California - Berkeley)
Habib Nasri Najm
(Sandia Natl Labs)
Russ Doerner
(Univ of California, San Diego)
Daisuke Nishijima
(Univ of California - San Diego)
David L Green
(Oak Ridge National Lab)
John Canik
(Oak Ridge National Lab)
Ane Lasa
(Oak Ridge National Lab)
Philip C Roth
(Oak Ridge National Lab)
Davide Curreli
(Univ of Illinois - Urbana)
Jon T Drobny
(Univ of Illinois - Urbana)
Parker Forehand
(University of Tennessee)
Brian Wirth
(University of Tennessee)
The extreme heat, charged particle, and neutron flux / fluence to plasma facing materials in magnetically confined fusion devices has motivated research to understand, predict, and mitigate the associated detrimental effects. Of relevance to the ITER divertor is the helium interaction with the tungsten divertor, the resulting erosion and migration of impurities.
The linear plasma device PISCES A [1] has performed dedicated experiments for ~10^22 m-2s-1 flux, 250 eV He exposed tungsten targets to assess the net and gross erosion of tungsten and volumetric transport.
We present results of the erosion / migration / re-deposition of W during the experiment from the GITR (Global Impurity Transport) code coupled to materials response models. Specifically, the modeled and experimental W I emission spectroscopy data for the 429.4 nm wavelength and net erosion through target and collector mass difference measurements are compared. Bayesian inference is applied to the background plasma profile measurements (Te,ne) and data fitting in order to produce an uncertain input model for GITR. This allows for a bounding in the predictions of the experimental observables based on the uncertainty in the input data and models.
[1] R.P. Doerner Nucl. Fusion 52 (2012)
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.NM9.6
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