Studying the properties of reconnection-driven turbulence

Abstract

Magnetic reconnection, often accompanied by turbulence interaction, is a ubiquitous phenomenon in astrophysical environments. However, the current understanding of the nature of turbulent magnetic reconnection remains insufficient. We investigate the statistical properties of reconnection turbulence in the framework of the self-driven reconnection. Using the open-source software package AMUN, we first perform numerical simulations of turbulent magnetic reconnection. We then obtain the statistical results of reconnection turbulence by traditional statistical methods such as the power spectrum and structure function. Our numerical results demonstrate: (1) the velocity spectrum of reconnection turbulence follows the classical Kolmogorov type of $E\propto k^{-5/3}$, while the magnetic field spectrum is steeper than the Kolmogorov spectrum, which are independent of limited resistivity, guide field, and isothermal or adiabatic fluid states; (2) most of the simulations show the anisotropy cascade, except that the presence of a guide field leads to an isotropic cascade; (3) reconnection turbulence is incompressible in the adiabatic state, with energy distribution dominated by the velocity solenoidal component; (4) different from pure magnetohydrodynamic (MHD) turbulence, the intermittency of the velocity field is stronger than that of the magnetic field in reconnection turbulence. The steep magnetic field spectrum, together with the velocity spectrum of Kolmogorov type, can characterize the feature of the reconnection turbulence. In the case of the presence of the guide field, the isotropy of the reconnection turbulence cascade is also different from the cascade mode of pure MHD turbulence. Our experimental results provide new insights into the properties of reconnection turbulence, which will contribute to advancing the self-driven reconnection theory.

9 pages, 6 figures and 1 table. Accepted for publication in A&A

References in corpus (35)

• Reconnection in a Weakly Stochastic Field
• Gamma-Ray Bursts in the Swift Era
• Compressible Magnetohydrodynamic Turbulence: mode coupling, scaling relations, anisotropy, new regime and astrophysical implications
• Fast magnetic reconnection in the plasmoid-dominated regime
• Numerical Tests of Fast Reconnection in Weakly Stochastic Magnetic Fields
• Discovery of Powerful Gamma-Ray Flares from the Crab Nebula
• Simulations of nonhelical hydromagnetic turbulence
• Scaling properties of three-dimensional magnetohydrodynamic turbulence
• Imaging coronal magnetic-field reconnection in a solar flare
• Scaling laws of resistive magnetohydrodynamic reconnection in the high-Lundquist-number, plasmoid-unstable regime
• Formation of Plasmoid Chains in Magnetic Reconnection
• Spectral energy dynamics in magnetohydrodynamic turbulence
• Magnetic reconnection and stochastic plasmoid chains in high-Lundquist-number plasmas
• 3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications
• Fast Magnetic Reconnection and Spontaneous Stochasticity
• The Crab Nebula as a standard candle in very high-energy astrophysics
• Kinetic turbulence in relativistic plasma: from thermal bath to non-thermal continuum
• Turbulent Magnetohydrodynamic Reconnection Mediated by the Plasmoid Instability
• Particle Acceleration in Turbulence and Weakly Stochastic Reconnection
• Turbulent kinetic energy in the energy balance of a solar flare
• Turbulent Magnetic Reconnection in Two Dimensions
• A statistical model of three-dimensional anisotropy and intermittency in strong Alfvénic turbulence
• Statistics of Reconnection-Driven Turbulence
• Reconnection-Driven Energy Cascade in Magnetohydrodynamic Turbulence
• A Particle Module for the PLUTO Code: I - an implementation of the MHD-PIC equations
• MHD Turbulence
• Ordinary and Viscosity-Damped MHD Turbulence
• Self-generated turbulence in magnetic reconnection
• Three-dimensional Spontaneous Magnetic Reconnection
• Kelvin-Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?
• Onset of turbulent fast magnetic reconnection observed in the solar atmosphere
• Three-dimensional Turbulent Reconnection within Solar Flare Current Sheet
• Turbulent reconnection acceleration
• Reconnection in weakly stochastic B-fields in 2D
• Magnetic reconnection-driven turbulence and turbulent reconnection acceleration