Abstract

This paper presents a review of multi-scale interactions between small-scale turbulence and large scale magnetic islands. In finite beta plasmas, zonal flows are relatively weak, and thus another electromagnetic coherent structure formation such as magnetic islands becomes important for regulating turbulence. In multi-scale interactions, large-scale modes dominate turbulent fluctuations even when the growth rate of the large-scale mode is much smaller than small-scale modes. On the other hand, small-scale modes influence large-scale modes when the large-scale modes are stable/marginally stable. Thus, the multi-scale interactions are categorized according to the stability of tearing mode (TM), which drives large-scale magnetic islands. When the TM is unstable, wide magnetic islands are produced, and as a result of the multi-scale interactions, the turbulent transport is significantly enhanced inside the separatrix of the island, because large-scale stable modes are excited by mutual interactions between turbulence and the island. On the other hand, a steep temperature gradient is formed around the separatrix of the island, which is consistent with zonal flow shear appearing at the separatrix. When the TM is stable/marginally stable, turbulence drives and sustains magnetic islands of width equal to multiples of the Larmor radius. This excitation of islands by turbulence can be related to the seed island formation of neo-classical TMs. The parity of fluctuations plays crucial role in the multi-scale nonlinear interactions, because pure twisting parity mode does not satisfy the nonlinear fluid/gyrokinetic equations. Magnetic islands belongs to the tearing parity mode and drift-wave instabilities normally belong to the twisting parity mode, and each parity is conserved in the linear growth of the instability. However, when the amplitude of the twisting parity mode becomes finite, the nonlinear energy transfer takes place from the twisting parity to tearing parity modes. Through this nonlinear parity mixture, the magnetic islands are produced by the turbulence. The influence of anomalous current drive and polarization current on the multi-scale interactions is discussed as well.

Highlights

  • Turbulence is considered to cause anomalous transport in magnetically confined plasmas [1,2,3], and is mainly driven by magnetic field on the cross-section vanishes

  • The turbulence modifies the threshold of magnetic island appearance predicted by the conventional resistive MHD analysis in terms of D¢

  • We have reviewed multi-scale nonlinear interactions of smallscale turbulence and large-scale magnetic islands

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Summary

Introduction

Turbulence is considered to cause anomalous transport in magnetically confined plasmas [1,2,3], and is mainly driven by. When coherent magnetic island chains appearing at different radii become wide and overlap each other, the degradation of confinement is significant and a disruption terminates the discharge of tokamak plasma [10] This is because the overlap of coherent magnetic islands results in stochastic magnetic field in wide range of radius, and flattening of temperature and density profiles is significantly enhanced. Neoclassical tearing mode (NTM) produces magnetic islands at a low-order rational surface and is one of primary instabilities limiting the achievable plasma pressure of high-β tokamak plasmas. Electromagnetic fluctuations give rise to a long wavelength MHD instability such as tearing modes (TMs) which reconnect the closed magnetic surfaces and degrade the confinement. Coherent magnetic islands that have a long wavenumber play an important role as well as the zonal magnetic field and zonal pressure field

Model equations
Fluid model used in simulations of toroidal plasma
Fluid model used in two-dimensional simulations
Parity symmetry in radial direction
Parity
Parity symmetry along a magnetic field line
Unstable against TM
Flux driven electromagnetic turbulence with TM
Coherent vortex flows
Magnetic field stochasticity
Anomalous current drive
Zonal flows
Non-flux-driven simulations
Magnetic island production by turbulence
Stable to TM
Summary
Influence of island on turbulence
Full Text
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