Abstract:A minimal self-consistent model of the multiscale interaction of a tearing mode with drift wave turbulence is presented. A tearing instability in a cylindrical plasma interacting with electrostatic drift waves is considered, for reasons of simplicity. Wave kinetics and adiabatic theory are used to treat the feedback of tearing mode flows on the drift waves via shearing and radial advection. The stresses exerted by the self-consistently evolved drift wave population density on the tearing mode are calculated by… Show more
“…The case where the first term in the RHS of Eq. (42) is important has been discussed in, e.g., [18]. These findings illustrate the important roles of microscopic turbulence on the evolution of global perturbations, the integrated analyses of which require future intensive studies.…”
The dynamics of the tearing mode and microscopic resistive drift wave turbulence are studied by performing a nonlinear simulation based on a 4-field Reduced MHD model, placing an emphasis on the interaction between microscopic and transport processes. The simulation results show the importance of turbulent fluctuations for the onset of the tearing mode. The faster growth of microscopic fluctuations induces accelerated growth of the tearing mode, which is much faster than the linear growth rate. A turbulence-driven magnetic island is formed. This is based on the incoherent emission of the long wavelength mode by microscopic turbulence.
“…The case where the first term in the RHS of Eq. (42) is important has been discussed in, e.g., [18]. These findings illustrate the important roles of microscopic turbulence on the evolution of global perturbations, the integrated analyses of which require future intensive studies.…”
The dynamics of the tearing mode and microscopic resistive drift wave turbulence are studied by performing a nonlinear simulation based on a 4-field Reduced MHD model, placing an emphasis on the interaction between microscopic and transport processes. The simulation results show the importance of turbulent fluctuations for the onset of the tearing mode. The faster growth of microscopic fluctuations induces accelerated growth of the tearing mode, which is much faster than the linear growth rate. A turbulence-driven magnetic island is formed. This is based on the incoherent emission of the long wavelength mode by microscopic turbulence.
“…Gyro-kinetic and fluid simulations [16,17,18,13,19] of the influence of large magnetic islands on driftwave instabilities and micro-scale turbulence have uncovered new physics. Furthermore recent analytic work has provided fresh insights into the multi-scale interaction of microinstabilities and large scale magnetic islands [20,8,21].…”
Section: Effect Of Magnetic Islands On Drift-wave Turbulencementioning
Abstract.A finite radial temperature gradient has been observed to be maintained within magnetic islands in gyro-kinetic turbulence simulations despite the fast motion along the field, and is related to the trapped particles which do not move along the field around the island. Recent calculations of the interaction of drift wave turbulence with magnetic islands have shown that turbulence can exist within the separatrix, which in turn allows only the partial flattening of electron temperature profiles. Here we calculate, using a minimal drift-kinetic model, the effect on the bootstrap current in a tokamak. Consequences for the stability of the neo-classical tearing mode are discussed.
“…5 Effects of microturbulence on macro-MHD mode through nonlinear mode coupling are studied theoretically and numerically, and they are described by a negative eddy viscosity or by an anomalous resistivity. [8][9][10][11][12] On the other hand, the zonal flow caused by the turbulence can also affect the macro-MHD instability through the shearing of its radial structure. These effects of turbulence on macro-MHD should be simultaneously taken into account in numerical simulations.…”
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confidence: 99%
“…[8][9][10][11][12] On the other hand, the zonal flow caused by the turbulence can also affect the macro-MHD instability through the shearing of its radial structure. These effects of turbulence on macro-MHD should be simultaneously taken into account in numerical simulations.…”
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