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 PO5: Boundary, Plasma Materials Interactions, Stellarators
2:00 PM–5:00 PM,
Wednesday, November 7, 2018
OCC
Room: B113-114
Chair: Oliver Schmitz, University of Wisconsin
Abstract ID: BAPS.2018.DPP.PO5.13
Abstract: PO5.00013 : Modeling of nano-meter scale dust grains in tokamak*
4:24 PM–4:36 PM
Presenter:
Zhuang Liu
(Dalian University of Technology, Lawrence Livermore Natl Lab)
Authors:
Zhuang Liu
(Dalian University of Technology, Lawrence Livermore Natl Lab)
Xiaotao Xiao
(Chinese Academy of Sciences, Lawrence Livermore Natl Lab)
Nami Li
(Lawrence Livermore Natl Lab, Dalian University of Technology)
Xueqiao Xu
(Lawrence Livermore Natl Lab)
Dezhen Wang
(Dalian University of Technology)
In this work, the NDS (Nano-meter Dust Simulation), which evaluates the charging and ablation processes of the dust grains, has been done under BOUT++ framework. The guiding-center orbits of dust particles are tracked in tokamak plasmas, whose parameters are obtained from BOUT++, a highly desirable C++ code package for performing parallel plasma fluid simulations with an arbitrary number of equations in 3D curvilinear coordinates. The Hamiltonian guiding center equation of motion is utilized to describe the velocity and acceleration of dust grains at arbitrary time step. Calculations with the coupled NDS-BOUT++ codes provide results such as trajectories and distributions of dust particles with different components, sizes, and velocities for different tokamak geometries. The distribution of tungsten impurity, resulted from ablated tungsten dust grains for several typical scenarios, is also assessed. Preliminary results show in some cases, tungsten dust grains can cross the seperatrix and survive for several ms before ablated completely, which will significantly contribute to core contamination.
*LLNL contract DE-AC52- 07NA27344 for USDOE SC-FES , National Key R&D Program of China No. 2017YFE030168 , National Natural Science Foundation of China under Grant Nos. 11675037
To cite this abstract, use the following reference: http://meetings.aps.org/link/BAPS.2018.DPP.PO5.13
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