MHD Turbulence
arXiv:1910.03585 · doi:10.1007/s41115-019-0005-8
Abstract
We review the current status of research in MHD turbulence theory and numerical experiments and their applications to astrophysics and solar science. We introduce general tools for studying turbulence, basic turbulence models, MHD equations and their wave modes. Subsequently, we cover the theories and numerics of Alfvenic turbulence, imbalanced turbulence, small-scale dynamos and models and numerics for supersonic MHD turbulence.
58 pages, 37 figures
References in corpus (60)
- Theory of Star Formation
- Control of star formation by supersonic turbulence
- Astrophysical magnetic fields and nonlinear dynamo theory
- Astrophysical gyrokinetics: kinetic and fluid turbulent cascades in magnetized weakly collisional plasmas
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- Exact relation for correlation functions in compressible isothermal turbulence
- Dynamic Alignment in Driven Magnetohydrodynamic Turbulence
- Velocity Field of Compressible MHD Turbulence: Wavelet Decomposition and Mode Scalings
- Imbalanced Strong MHD Turbulence
- Nonhelical inverse transfer of a decaying turbulent magnetic field
- Density scaling and anisotropy in supersonic MHD turbulence
- Exact Relation with Two-point Correlation Functions and Phenomenological Approach for Compressible Magnetohydrodynamic Turbulence
- Role of cross helicity in magnetohydrodynamic turbulence
- The Spectral Slope and Kolmogorov Constant of MHD turbulence
- Turbulence-induced magnetic fields and the structure of Cosmic Ray modified shocks
- Strong Imbalanced Turbulence
- Growth of Magnetic Fields Induced by Turbulent Motions
- Residual Energy Spectrum of Solar Wind Turbulence
- Structures of the magnetoionic media around the FR I radio galaxies 3C 31 and Hydra A
- Polarization intermittency in MHD and its influence on turbulent cascade
- Universal Nonlinear Small-Scale Dynamo
- Anisotropy of Imbalanced Alfvenic Turbulence in Fast Solar Wind
- Scale-dependence of magnetic helicity in the solar wind
- Alpha effect and turbulent diffusion from convection
- A supersonic turbulence origin of Larson's laws
- Comparison of spectral slopes of magnetohydrodynamic and hydrodynamic turbulence and measurements of alignment effects
- Spectra of strong MHD Turbulence from high-resolution simulations
- Magnetic fields in the nearby spiral galaxy IC 342: A multi-frequency radio polarization study
- Self-similar energetics in large clusters of galaxies
- Structure of Stationary Strong Imbalanced Turbulence
- New relations for correlation functions in Navier-Stokes turbulence
- Turbulent Amplification and Structure of the Intracluster Magnetic Field
- On the Nature of Incompressible Magnetohydrodynamic Turbulence
- Three-dimensional Spontaneous Magnetic Reconnection
- Basic Properties of MHD Turbulence in the Inertial Range
- Alignment and scaling of large-scale fluctuations in the solar wind
- A Kolmogorov-Like Exact Relation for Compressible Polytropic Turbulence
- Evolving waves and turbulence in the outer corona and inner heliosphere: the accelerating expanding box
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Cited by in corpus (38)
- Physical Processes in Star Formation
- Dissipation measures in weakly-collisional plasmas
- Turbulent magnetic-field amplification in the first 10 milliseconds after a binary neutron star merger: comparing high-resolution and large eddy simulations
- Standard Self-Confinement and Extrinsic Turbulence Models for Cosmic Ray Transport are Fundamentally Incompatible with Observations
- The FIP and Inverse FIP Effects in Solar Flares
- Magnetic field fluctuations in anisotropic, supersonic turbulence
- The impact of magnetic fields on cosmological galaxy mergers. I: Reshaping gas and stellar discs
- 3D Simulations of Oxygen Shell Burning with and without Magnetic Fields
- Magnetic reconnection as an energy cascade process
- As a matter of dynamical range -- scale dependent energy dynamics in MHD turbulence
- As a matter of tension -- kinetic energy spectra in MHD turbulence
- Extension of the sub-grid-scale gradient model for compressible magnetohydrodynamics turbulent instabilities
- Artificial neural network subgrid models of 2-D compressible magnetohydrodynamic turbulence
- Magnetohydrodynamics with Physics Informed Neural Operators
- Long-term GRMHD simulation of magnetic field in isolated neutron stars
- Turbulence modelling in neutron star merger simulations
- Energetic Particle Acceleration in Compressible Magnetohydrodynamic Turbulence
- Gamma-ray halos around pulsars: impact on pulsar wind physics and galactic cosmic ray transport
- Nanoflare Theory Revisited
- An analytical model of turbulence in Parker spiral geometry and associated magnetic field line lengths
- Physics-Informed Machine Learning for Modeling Turbulence in Supernovae
- Lagrangian statistics of a shock-driven turbulent dynamo in decaying turbulence
- Parameter study of decaying magnetohydrodynamic turbulence
- Gradient measurement of synchrotron polarization diagnostic: Application to spatially separated emission and Faraday rotation regions
- Analytic characterization of sub-Alfvénic turbulence energetics
- Scale Statistics of Current Sheets in Relativistic Collisionless Plasma Turbulence
- Local magneto-shear instability in Newtonian gravity
- Studying the properties of compressible MHD turbulence by synchrotron fluctuation statistics
- Revisiting Kinematic Fast Dynamo in 3-dimensional magnetohydrodynamic plasmas: Dynamo transition from non-Helical to Helical flows
- Studying the properties of reconnection-driven turbulence
- Measurement of the scaling slope of compressible magnetohydrodynamic turbulence by synchrotron radiation statistics
- Pseudo-spectral solver versus grid-based solver: A quantitative accuracy test using GMHD3D and PLUTO4.4
- Statistical signatures of interstellar turbulence in dust polarization maps
- Turbulence in Magnetised Neutron Stars
- Towards convergence of turbulent dynamo amplification in cosmological simulations of galaxies
- High-energy Particle Transport in Three-dimensional Anisotropic Turbulent Magnetic Fields
- Magnetic field and kinetic helicity evolution in simulations of interacting disk galaxies
- Introduction to Strong Alfvénic MHD Turbulence