Strong Imbalanced Turbulence
@article{Beresnyak2007StrongIT, title={Strong Imbalanced Turbulence}, author={Andrey Beresnyak and Alex Lazarian}, journal={The Astrophysical Journal}, year={2007}, volume={682}, pages={1070 - 1075} }
We consider stationary, forced, imbalanced, or cross helical MHD Alfvénic turbulence where the waves traveling in one direction have higher amplitudes than the opposite waves. This paper is dedicated to so-called strong turbulence, which cannot be treated perturbatively. Our main result is that the anisotropy of the weak waves is stronger than the anisotropy of strong waves. We propose that critical balance, which was originally conceived as a causality argument, has to be amended by what we…
91 Citations
STRUCTURE OF STATIONARY STRONG IMBALANCED TURBULENCE
- Physics
- 2009
In this paper, we systematically study the spectrum and structure of incompressible magnetohydrodynamic turbulence by means of high-resolution direct numerical simulations. We considered both…
MHD–KINETIC TRANSITION IN IMBALANCED ALFVÉNIC TURBULENCE
- Physics
- 2016
Alfvénic turbulence in space is usually imbalanced: amplitudes of waves propagating parallel and anti-parallel to the mean magnetic field are unequal. It is commonly accepted that the turbulence is…
Properties of balanced and imbalanced relativistic alfvénic magnetohydrodynamic turbulence
- Physics
- 2014
When the magnetic field is so strong that the magnetic energy density is much larger than that of matter, magnetic perturbations propagate along the magnetic field lines, and the speed of propagation…
Modeling Imbalanced Collisionless Alfvén Wave Turbulence with Nonlinear Diffusion Equations
- PhysicsThe Astrophysical Journal
- 2019
A pair of nonlinear diffusion equations in Fourier space is used to study the dynamics of strong Alfvén wave turbulence, from MHD to electron scales. Special attention is paid to the regime of…
Strong magnetohydrodynamic turbulence with cross helicity
- Physics
- 2009
Magnetohydrodynamics (MHD) provides the simplest description of magnetic plasma turbulence in a variety of astrophysical and laboratory systems. MHD turbulence with nonzero cross helicity is often…
Spectrum of weak magnetohydrodynamic turbulence.
- PhysicsPhysical review letters
- 2009
Based on high-resolution numerical simulations, it is proposed that turbulence spontaneously generates a condensate of the residual energy E(v) - E(b) at small field-parallel wave numbers.
IMBALANCED RELATIVISTIC FORCE-FREE MAGNETOHYDRODYNAMIC TURBULENCE
- Physics
- 2013
When magnetic energy density is much larger than that of matter, as in pulsar/black hole magnetospheres, the medium becomes force-free and we need relativity to describe it. As in non-relativistic…
Imbalanced kinetic Alfvén wave turbulence: from weak turbulence theory to nonlinear diffusion models for the strong regime
- PhysicsJournal of Plasma Physics
- 2019
A two-field Hamiltonian gyrofluid model for kinetic Alfvén waves retaining ion finite Larmor radius corrections, parallel magnetic field fluctuations and electron inertia, is used to study turbulent…
Strong Anisotropic MHD Turbulence with Cross Helicity
- Physics
- 2008
This paper proposes a new phenomenology for strong incompressible MHD turbulence with nonzero cross helicity. This phenomenology is then developed into a quantitative Fokker-Planck model that…
Three-dimensional Simulation of the Fast Solar Wind Driven by Compressible Magnetohydrodynamic Turbulence
- PhysicsThe Astrophysical Journal
- 2019
Using a three-dimensional compressible magnetohydrodynamic (MHD) simulation, we have reproduced the fast solar wind in a direct and self-consistent manner, based on the wave/turbulence-driven…
References
SHOWING 1-10 OF 35 REFERENCES
Imbalanced Weak Magnetohydrodynamic Turbulence
- Physics
- 2003
Weak MHD turbulence consists of waves that propagate along magnetic field lines, in both directions. When two oppositely directed waves collide, they distort each other, without changing their…
Simulations of Magnetohydrodynamic Turbulence in a Strongly Magnetized Medium
- Physics
- 2001
We analyze three-dimensional numerical simulations of driven incompressible magnetohydrodynamic (MHD) turbulence in a periodic box threaded by a moderately strong external magnetic field. We sum over…
Anisotropic Turbulence of Shear-Alfvén Waves
- Physics
- 2001
Weak turbulence of shear-Alfvén waves is considered in the limit of strongly anisotropic pulsations that are elongated along the external magnetic field. The kinetic equation thus derived agrees with…
On the Spectrum of Magnetohydrodynamic Turbulence
- PhysicsPhysical review letters
- 2006
We propose a phenomenological model for incompressible magnetohydrodynamic turbulence. We argue that nonlinear-wave interaction weakens as the energy cascade proceeds to small scales; however, the…
Strong MHD helical turbulence and the nonlinear dynamo effect
- PhysicsJournal of Fluid Mechanics
- 1976
To understand the turbulent generation of large-scale magnetic fields and to advance beyond purely kinematic approaches to the dynamo effect like that introduced by Steenbeck, Krause & Radler (1966)’…
Simulations of Incompressible Magnetohydrodynamic Turbulence
- Physics
- 2001
We simulate incompressible MHD turbulence using a pseudospectral code. Our major conclusions are: (1) MHD turbulence is most conveniently described in terms of counterpropagating shear Alfvén and…
Statistical anisotropy of magnetohydrodynamic turbulence.
- PhysicsPhysical review. E, Statistical, nonlinear, and soft matter physics
- 2003
Direct numerical simulations of decaying and forced magnetohydrodynamic (MHD) turbulence without and with mean magnetic field are analyzed by higher-order two-point statistics and an intermittency model based on the log-Poisson approach, zeta(p)=p/g(2)+1-(1/g)( p/g), is able to describe the observed structure function scalings.
Compressible sub-Alfvénic MHD turbulence in low-beta plasmas.
- PhysicsPhysical review letters
- 2002
It is found that production of slow and fast modes by Alfvénic turbulence is suppressed, and Alfvén modes in compressible regime exhibit scalings and anisotropy similar to those in incompressible regime.
Fully developed anisotropic hydromagnetic turbulence in interplanetary space
- Physics
- 1980
The solar-wind magnetohydrodynamic turbulence is observed to be made mainly of Alfvenic fluctuations propagating away from the sun. It is shown that such an asymmetric state is a general consequence…
Compressible magnetohydrodynamic turbulence: mode coupling, scaling relations, anisotropy, viscosity-damped regime and astrophysical implications
- Physics
- 2003
We present numerical simulations and explore scalings and anisotropy of compressible magnetohydrodynamic (MHD) turbulence. Our study covers both gas-pressure-dominated (high β) and…