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 NP11: Poster Session V: Laser-plasma Particle Acceleration; HEDP; Turbulence and Transport; DIII-D Tokamak; Machine Learning, Data Science (9:30am-12:30pm)
Wednesday, November 7, 2018
OCC
Room: Exhibit Hall A1&A
Abstract ID: BAPS.2018.DPP.NP11.67
Abstract: NP11.00067 : Understanding the RMP and density pump-out physics from a coupled gyrokinetic-MHD simulation*
Presenter:
Robert Hager
(Princeton Plasma Phys Lab)
Authors:
Robert Hager
(Princeton Plasma Phys Lab)
Nathaniel Mandrachia Ferraro
(Princeton Plasma Phys Lab)
C-S Chang
(Princeton Plasma Phys Lab)
Raffi Nazikian
(Princeton Plasma Phys Lab)
Density pump-out caused by external resonant magnetic perturbations (RMP) is studied in a model DIII-D discharge with advanced coupled gyrokinetic-MHD simulation. RMP has been accepted into the ITER design as the primary control tool to suppress edge localized modes (ELMs). Strong RMPs, however, often reduce edge particle confinement (pump-out), which degrades fusion efficiency. In our advanced model, the perturbed plasma equilibrium is calculated with the M3D-C1 code. This equilibrium (including the RMP) is coupled into the edge gyrokinetic XGC suite of codes, which calculate neoclassical and turbulent transport, background plasma and ExB profile evolution including neutral particle physics and X-point orbit loss. In the zero-turbulence limit, we find a significant increase of (neoclassical) radial particle fluxes to levels similar to experimental observations. Edge turbulence intensity rises up to 50% due to the RMPs, mostly from the weakening of the ExB shearing rate, which is not enough to explain the density pump-out without the increase of neoclassical fluxes.
*Work supported by the U.S. DOE under contracts DE-AC02-09CH11466 (PPPL)and DE-FC02-04ER54698 (DIII-D), and by ALCF and NERSC for computing resources.
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.NP11.67
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