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Role of resistivity and viscosity in the excitation of stable m = 0 modes during the RFP sawtooth crash
Visco-resistive magnetohydrodynamic simulations are used to investigate the role of resistivity and viscosity in the reversed field pinch sawtooth crash. Specifically, we examine the temporal behavior of the linearly stable (m, n) = (0, 1) mode. Both volume-averaged dissipation and dissipation level...
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Published in: | Physics of plasmas 2018-11, Vol.25 (11) |
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Main Authors: | , , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | Visco-resistive magnetohydrodynamic simulations are used to investigate the role of resistivity and viscosity in the reversed field pinch sawtooth crash. Specifically, we examine the temporal behavior of the linearly stable (m, n) = (0, 1) mode. Both volume-averaged dissipation and dissipation levels in the region near the m = 0 resonance are found to influence characteristic time scales. Increasing resistivity causes the mode rise time, fall time, and total crash duration to decrease, while increasing viscosity has the opposite effect. Examination of energy flow during the sawtooth crash reveals that despite the linear stability of the (0, 1) mode, it receives most of its energy from the mean current profile during the crash rather than from nonlinear interactions with other modes. Resistivity and viscosity do not impact mode behavior directly through dissipative energy loss but rather through modification of the large scale current profile evolution and radial structure of the mode. Computational results are compared to experimental data from the Madison Symmetric Torus and found to largely agree when resistivity and viscosity are similar. |
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ISSN: | 1070-664X 1089-7674 |
DOI: | 10.1063/1.5054578 |