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Title: Magnetohydrodynamic Turbulence Mediated by Reconnection

Journal Article · · Astrophysical Journal
 [1];  [2]
  1. Department of Physics, University of Wisconsin-Madison, Madison, WI 53706 (United States)
  2. Plasma Science and Fusion Center, Massachusetts Institute of Technology, Cambridge MA 02139 (United States)

Magnetic field fluctuations in magnetohydrodynamic turbulence can be viewed as current sheets that are progressively more anisotropic at smaller scales. As suggested by Loureiro and Boldyrev and Mallet et al., below a certain critical thickness, λ{sub c}, such current sheets become tearing-unstable. We propose that the tearing instability changes the effective alignment of the magnetic field lines in such a way as to balance the eddy turnover rate at all scales smaller than λ{sub c}. As a result, turbulent fluctuations become progressively less anisotropic at smaller scales, with the alignment angle increasing as θ∼(λ/λ{sub ∗}){sup −4/5+β}, where λ{sub ∗}∼L{sub 0}S{sub 0}{sup −3/4} is the resistive dissipation scale. Here L {sub 0} is the outer scale of the turbulence, S {sub 0} is the corresponding Lundquist number, and 0⩽β<4/5 is a parameter. The resulting Fourier energy spectrum is E(k{sub ⊥})∝k{sub ⊥}{sup −11/5+2β/3}, where k{sub ⊥} is the wavenumber normal to the local mean magnetic field, and the critical scale is λ{sub c}∼S{sub L}{sup −(4−5β)/(7−20β/3)}. The simplest model corresponds to β = 0, in which case the predicted scaling formally agrees with one of the solutions obtained in Mallet et al. from a discrete hierarchical model of abruptly collapsing current sheets, an approach different from and complementary to ours. We also show that the reconnection-mediated interval is non-universal with respect to the dissipation mechanism. Hyper-resistivity of the form η-tilde k{sup 2+2s} leads (in the simplest case of β = 0) to the different transition scale λ{sub c}∼L{sub 0} S-tilde {sub 0}{sup −4/(7+9s)} and the energy spectrum E(k{sub ⊥})∝k{sub ⊥}{sup −(11+9s)/(5+3s)}, where S-tilde {sub 0} is the corresponding hyper-resistive Lundquist number.

OSTI ID:
22875967
Journal Information:
Astrophysical Journal, Vol. 844, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 0004-637X
Country of Publication:
United States
Language:
English

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Cited By (27)

The multi-scale nature of the solar wind journal December 2019
On the Fourier Contribution of Strong Current Sheets to the High‐Frequency Magnetic Power SpectralDensity of the Solar Wind journal February 2020
Transition from ion-coupled to electron-only reconnection: Basic physics and implications for plasma turbulence journal August 2019
Diffusion regions and 3D energy mode development in spontaneous reconnection journal July 2019
Scalings pertaining to current sheet disruption mediated by the plasmoid instability journal September 2019
3D turbulent reconnection: Theory, tests, and astrophysical implications journal January 2020
The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A* journal June 2018
Spectral signatures of recursive magnetic field reconnection journal November 2019
Two-temperature, Magnetically Arrested Disc simulations of the jet from the supermassive black hole in M87 journal April 2019
Magnetohydrodynamic Turbulence in the Plasmoid-mediated Regime journal February 2018
Stochastic Reconnection for Large Magnetic Prandtl Numbers journal June 2018
Large-scale Compression Acceleration during Magnetic Reconnection in a Low- β Plasma journal October 2018
Electron and Proton Heating in Transrelativistic Guide Field Reconnection journal February 2019
Dynamic Evolution of Current Sheets, Ideal Tearing, Plasmoid Formation and Generalized Fractal Reconnection Scaling Relations journal August 2019
The Interplay of Magnetically Dominated Turbulence and Magnetic Reconnection in Producing Nonthermal Particles journal November 2019
Magnetic Reconnection as a Driver for a Sub-ion-scale Cascade in Plasma Turbulence journal November 2017
Turbulence in Magnetized Pair Plasmas journal October 2018
Properties of the Turbulence Associated with Electron-only Magnetic Reconnection in Earth’s Magnetosheath journal June 2019
Magnetohydrodynamic Turbulence in the Plasmoid-Mediated Regime text January 2018
The role of electron heating physics in images and variability of the Galactic Centre black hole Sagittarius A* text January 2018
Role of the Plasmoid Instability in Magnetohydrodynamic Turbulence text January 2018
Electron and Proton Heating in Transrelativistic Guide Field Reconnection text January 2019
Dynamic evolution of current sheets, ideal tearing, plasmoid formation and generalized fractal reconnection scaling relations text January 2019
Diffusion regions and 3D energy mode development in spontaneous reconnection text January 2019
Spectral signatures of recursive magnetic field reconnection text January 2019
Scalings Pertaining to Current Sheet Disruption Mediated by the Plasmoid Instability text January 2019
3D Turbulent Reconnection: Theory, Tests and Astrophysical Implications text January 2020

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