Bulletin of the American Physical Society
63rd Annual Meeting of the APS Division of Plasma Physics
Volume 66, Number 13
Monday–Friday, November 8–12, 2021; Pittsburgh, PA
Session UP11: Poster Session VIII:
Fundamental Plasma Physics - Analytical and Computational Techniques; Magnetic Reconnection; Antimatter Heliospheric, Magnetospheric, and Ionospheric Plasma Phenomena and Their Scaled Laboratory Experiments
MFE - DIII-D Tokamak II, ITER, HBT-EP, and Other Tokamaks
2:00 PM - 5:00 PM
Thursday, November 11, 2021
Room: Hall A
Abstract: UP11.00097 : Non-parametric inference of impurity transport coefficients in the ASDEX Upgrade tokamak*
Presenter:
Takashi Nishizawa
(Max Planck Institute for Plasma Physics)
Authors:
Takashi Nishizawa
(Max Planck Institute for Plasma Physics)
Ralph Dux
(Max Planck Institute for Plasma Physics)
Christian Schuster
(Max Planck Institute for Plasma Physics)
Marco Cavedon
(Max Planck Institute for Plasma Physics)
Elisabeth Wolfrum
(Max Planck Institute for Plasma Physics)
Udo von Toussaint
(Max Planck Institute for Plasma Physics)
Anton Jansen Van Vuuren
(University of Seville)
Diego J Cruz-Zabala
(University of Seville)
Pilar Cano-Megias
(University of Seville)
Collaboration:
the ASDEX Upgrade team
The transport properties of impurity ions are often experimentally characterized by using a diffusion coefficient D and a convection velocity v. Since the realistic experimental setups usually necessitate the determination of D and v under ill-posed conditions, rigorous comparisons between simulations and experiments cannot be made without addressing the model selection and uncertainty estimation problems. To this end, the Bayesian formalism has been applied to the impurity transport studies in recent years.
In this work, transport coefficients of light impurities (Ne, O, and C) in a Type-III ELMy H-mode plasma are inferred by using a non-parametric approach. Unlike spline functions, the non-parametric inference does not reduce the degrees of freedom for representing spatial profiles. Thus, all solutions that are consistent with the measurements and the prescribed smoothing conditions can be calculated. We report the D and v profile measurements from rho_pol=0.6-1.0.
*This work has been carried out within the framework of the EUROfusion Consor- tium and has received funding from the Euratom research and training programme 2014-2018 and 2019-2020 un- der grant agreement No 633053. The views and opinions expressed herein do not necessarily reflect those of the European Commission.
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