Extension of XGC kinetic simulation codes to magnetic mirror configurations
ORAL
Abstract
The XGC codes, developed to simulate the edge regions of tokamak plasmas, are modified to carry out kinetic simulations of axisymmetric magnetic mirror configurations. The XGC codes are particle in cell kinetic codes that include a virtual sheath condition where magnetic field lines run into end plates. The XGC1 code is a fully five dimensional kinetic code that is used to investigate turbulence, while the faster XGC0 code uses the axisymmetric average electrostatic potential in order to simulate charged particle drifts, losses and collisional effects. Kinetic electron computations, neutral beam injection, atomic physics and the effects of thermal neutrals are included in the XGC codes. Changes are being made to allow the XGC codes to accept mirror equilibria and to run without a toroidal magnetic field component. The XGC0 code will be used to compute particle dynamics, electrostatic potentials, and moments of the distribution functions including plasma flows in mirror configurations. \newline [1] C.S. Chang, S. Ku, H. Weitzner, Phys. Plasmas {\bf 11} (2004) 2649
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Authors
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G. Bateman
Lehigh U.
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A.Y. Pankin
Lehigh U.
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A.H. Kritz
Lehigh U.
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T. Rafiq
Lehigh U.
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G.Y. Park
NYU, NYU Courant Institute
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Seung-Hoe Ku
NYU Courant Institute, New York University, Courant Institute Mathematical Sciences
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C.S. Chang
New York University, and the CPES Team, NYU, NYU Courant Institute, KAIST, New York University
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W. Horton
Institute for Fusion Studies, Institute of Fusion Studies, University of Texas at Austin, UT Austin, IFS
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J. Pratt
UT Austin, IFS