Influence of tearing instability on magnetohydrodynamic turbulence
arXiv:1804.02754 · doi:10.1103/PhysRevE.98.033209
Abstract
It has been proposed recently by Loureiro & Boldyrev [Phys. Rev. Lett. 118, 245101 (2017)] and Mallet et al. [Mon. Not. R. Astron. Soc. 468, 4862 (2017)] that strongly anisotropic current sheets formed in the inertial range of magnetohydrodynamic turbulence become affected by the tearing instability at scales smaller than a critical scale , and larger than the dissipation scale of turbulence. If true, this process can modify the nature of energy cascade at smaller scales, leading to a new, tearing-mediated regime of magnetohydrodynamic (MHD) turbulence. In this work we present a numerical study of strongly anisotropic, two-dimensional turbulent eddies, and we demonstrate that the tearing instability can indeed compete with their nonlinear evolution. The results, therefore, provide direct numerical support for the picture that a new regime of MHD turbulence can exist below .
arXiv comment5 pages, 7 figures
References in corpus (30)
- Instability of current sheets and formation of plasmoid chains
- A weak turbulence theory for incompressible MHD
- Spectrum of magnetohydrodynamic turbulence
- Simulations of Incompressible MHD Turbulence
- MHD Turbulence Revisited
- Simulations of nonhelical hydromagnetic turbulence
- On the Spectrum of Magnetohydrodynamic Turbulence
- Impact of dimensionless numbers on the efficiency of MRI-induced turbulent transport
- Recent progress in astrophysical plasma turbulence from solar wind observations
- Spectral energy dynamics in magnetohydrodynamic turbulence
- Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence
- Dynamic Alignment in Driven Magnetohydrodynamic Turbulence
- Nature of Kinetic Scale Turbulence in the Earth's Magnetosheath
- Turbulent Magnetohydrodynamic Reconnection Mediated by the Plasmoid Instability
- Anisotropy of Alfvénic Turbulence in the Solar Wind and Numerical Simulations
- Three-Dimensional Structure of Solar Wind Turbulence
- Role of magnetic reconnection in MHD turbulence
- Disruption of sheetlike structures in Alfvénic turbulence by magnetic reconnection
- Collisionless Reconnection in Magnetohydrodynamic and Kinetic Turbulence
- Disruption of Alfvénic turbulence by magnetic reconnection in a collisionless plasma
- Magnetohydrodynamic turbulence mediated by reconnection
- Numerical Measurements of the Spectrum in Magnetohydrodynamic Turbulence
- Energy spectra stemming from interactions of Alfven waves and turbulent eddies
- Magnetic Reconnection May Control the Ion-Scale Spectral Break of Solar Wind Turbulence
- Magnetohydrodynamic Turbulence in the Plasmoid-Mediated Regime
- Measures of Three-Dimensional Anisotropy and Intermittency in Strong Alfvénic Turbulence
- Strong magnetohydrodynamic turbulence with cross helicity
- Energy Dissipation in Magnetohydrodynamic Turbulence: Coherent Structures or "Nanoflares"?
- Scaling properties of small-scale fluctuations in magnetohydrodynamic turbulence
- Influence of a large-scale field on energy dissipation in magnetohydrodynamic turbulence
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- 3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications
- The interplay of magnetically-dominated turbulence and magnetic reconnection in producing nonthermal particles
- Large-scale Compression Acceleration during Magnetic Reconnection in a Low- Plasma
- The Acceleration of Charged Particles and Formation of Power-law Energy Spectra in Nonrelativistic Magnetic Reconnection
- Kinetic turbulence in shining pair plasma: intermittent beaming and thermalization by radiative cooling
- Kelvin-Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?
- Role of reconnection in inertial kinetic-Alfven turbulence
- Fast Magnetic Reconnection with Turbulence in High Lundquist Number Limit
- Particle energization in relativistic plasma turbulence: solenoidal versus compressive driving
- Nonlinear Reconnection in Magnetized Turbulence
- Turbulence and particle acceleration in a relativistic plasma
- Scalings Pertaining to Current Sheet Disruption Mediated by the Plasmoid Instability
- Tearing instability in Alfvén and kinetic-Alfvén turbulence
- Electron-Scale Current Sheets and Energy Dissipation in 3D Kinetic-Scale Plasma Turbulence with Low Electron Beta
- Particle acceleration and pitch-angle evolution in relativistic turbulence
- Whistler-Alfvén turbulence in a non-neutral ultrarelativistic pair plasma