Turbulent General Magnetic Reconnection
arXiv:1412.2254 · doi:10.1088/0004-637X/807/2/137
Abstract
Plasma flows with an MHD-like turbulent inertial range, such as the solar wind, require a generalization of General Magnetic Reconnection (GMR) theory. We introduce the slip-velocity source vector, which gives the rate of development of slip velocity per unit arc length of field line. The slip source vector is the ratio of the curl of the non ideal electric field in the Generalized Ohm's Law and the magnetic field strength. It diverges at magnetic nulls, unifying GMR with magnetic null-point reconnection. Only under restrictive assumptions is the slip velocity related to the gradient of the quasi potential (integral of parallel electric field along field lines). In a turbulent inertial range the curl becomes extremely large while the parallel component is tiny, so that line slippage occurs even while ideal MHD becomes accurate. The resolution of this paradox is that ideal MHD is valid for a turbulent inertial-range only in a weak sense which does not imply magnetic line freezing. The notion of weak solution is explained in terms of spatial coarse-graining and renormalization group (RG) theory. We give an argument for the weak validity of the ideal Ohm's law in the inertial range, via rigorous estimates of the terms in the Generalized Ohm's Law for an electron-ion plasma. All of the nonideal terms (from collisional resistivity, Hall field, electron pressure anisotropy, and electron inertia) are shown to be irrelevant in the RG sense and large-scale reconnection is thus governed solely by ideal dynamics. We briefly discuss some implications for heliospheric reconnection, in particular for deviations from the Parker spiral model of interplanetary magnetic field. Solar wind observations show that reconnection in a turbulence broadened heliospheric current sheet, consistent with the Lazarian-Vishniac theory, leads to slip velocities that cause field lines to lag relative to the spiral model.
arXiv comment35 pages, 9 figures
References in corpus (26)
- Reconnection in a Weakly Stochastic Field
- Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas
- Spectrum of magnetohydrodynamic turbulence
- MHD Turbulence Revisited
- On the Spectrum of Magnetohydrodynamic Turbulence
- Fast Magnetic Reconnection and Spontaneous Stochasticity
- The slow-mode nature of compressible wave power in solar wind turbulence
- Scaling of the electron dissipation range of solar wind turbulence
- Scale decomposition in compressible turbulence
- Finite dissipation and intermittency in magnetohydrodynamics
- Scale-Locality of Magnetohydrodynamic Turbulence
- A model of acceleration of Anomalous Cosmic Rays by Reconnection in the Heliosheath
- A Numerical Simulation of the Reconnection Layer in 2D Resistive MHD
- Diffusion of magnetic field and removal of magnetic flux from clouds via turbulent reconnection
- Stochastic Flux-Freezing and Magnetic Dynamo
- Multi-Scale Gradient Expansion of the Turbulent Stress Tensor
- Frame Dependence of the Electric Field Spectrum of Solar Wind Turbulence
- Parallel electric field generation by Alfven wave turbulence
- Correlations at large scales and the onset of turbulence in the fast solar wind
- The Breakdown of Alfven's Theorem in Ideal Plasma Flows
- Alignment and scaling of large-scale fluctuations in the solar wind
- Puzzles of the interplanetary magnetic field in the inner heliosphere
- An iterative semi-implicit scheme with robust damping
- Gyrofluid description of Alfvenic turbulence and its parallel electric field
- Turbulent Diffusion of Lines and Circulations
- The scale-free texture of the fast solar wind
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- Spectrum and Anisotropy of Turbulence from Multi-Frequency Measurement of Synchrotron Polarization
- Heliosheath Processes and the Structure of the Heliopause: Modeling Energetic Particles, Cosmic Rays, and Magnetic Fields
- Damping of Alfven waves by Turbulence and its Consequences: from Cosmic-Rays Streaming to Launching Winds
- Coarse-Grained Incompressible Magnetohydrodynamics: analyzing the turbulent cascades
- Cascades and Dissipative Anomalies in Compressible Fluid Turbulence
- Fluidization of collisionless plasma turbulence
- An Onsager Singularity Theorem for Turbulent Solutions of Compressible Euler Equations
- Constraints on ion vs. electron heating by plasma turbulence at low beta
- Cascades and Dissipative Anomalies in Nearly Collisionless Plasma Turbulence
- Turbulence in the outer heliosphere
- Kelvin-Helmholtz versus Tearing Instability: What Drives Turbulence in Stochastic Reconnection?
- Fast magnetic reconnection structures in Poynting-flux dominated jets
- Gamma-ray Bursts Induced by Turbulent Reconnection
- Cascades and Dissipative Anomalies in Relativistic Fluid Turbulence
- Nonlinear turbulent dynamo during gravitational collapse
- Turbulent reconnection acceleration
- Magnetic stochasticity and diffusion
- Nanoflare Theory Revisited
- Magnetic reconnection and thermal equilibration
- Statistical Analysis of Stochastic Magnetic Fields
- On the large-scale sweeping of small-scale eddies in turbulence -- A filtering approach
- Magnetic reconnection with null and X-points
- Example of exponentially enhanced magnetic reconnection driven by a spatially-bounded and laminar ideal flow
- The rapid destruction of toroidal magnetic surfaces
- Two-dimensional modeling of the tearing-mode-governed magnetic reconnection in the large-scale current sheet above the two-ribbon flare
- Power and spatial complexity in stochastic reconnection
- Mean fields and fluctuations in compressible magnetohydrodynamic flows
- Local analysis of fast magnetic reconnection
- Generation and Effects of Electromotive Force in Turbulent Stochastic Reconnection