Numerical Study of Field-reversed Configurations: The Formation and Ion Spin-up | |
Belova, E. V. ; Davidson, R. C. ; Ji, H. ; Yamada, M. ; Cothran, C. D. ; Brown, M. R. ; Schaffer, M. J. | |
Princeton University. Plasma Physics Laboratory. | |
关键词: Numerical Simulation; Saturation; Decay; 75 Condensed Matter Physics, Superconductivity And Superfluidity; 70 Plasma Physics And Fusion Technology; | |
DOI : 10.2172/840784 RP-ID : PPPL-4075 RP-ID : AC02-76CH03073 RP-ID : 840784 |
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美国|英语 | |
来源: UNT Digital Library | |
【 摘 要 】
Results of three-dimensional numerical simulations of field-reversed configurations (FRCs) are presented. Emphasis of this work is on the nonlinear evolution of magnetohydrodynamic (MHD) instabilities in kinetic FRCs, and the new FRC formation method by counter-helicity spheromak merging. Kinetic simulations show nonlinear saturation of the n = 1 tilt mode, where n is the toroidal mode number. The n = 2 and n = 3 rotational modes are observed to grow during the nonlinear phase of the tilt instability due to the ion spin-up in the toroidal direction. The ion toroidal spin-up is shown to be related to the resistive decay of the internal flux, and the resulting loss of particle confinement. Three-dimensional MHD simulations of counter-helicity spheromak merging and FRC formation show good qualitative agreement with results from the SSX-FRC experiment. The simulations show formation of an FRC in about 20-30 Alfven times for typical experimental parameters. The growth rate of the n = 1 tilt mode is shown to be significantly reduced compared to the MHD growth rate due to the large plasma viscosity and field-line-tying effects.
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