Turbulent regimes in collisions of 3D Alfvén-wave packets
arXiv:2207.04301 · doi:10.3847/1538-4357/ac93fe
Abstract
Using 3D gyrofluid simulations, we revisit the problem of Alfven-wave (AW) collisions as building blocks of the Alfvenic cascade and their interplay with magnetic reconnection at magnetohydrodynamic (MHD) scales. Depending on the large-scale nonlinearity parameter (the ratio between AW linear propagation time and nonlinear turnover time), different regimes are observed. For strong nonlinearities (), turbulence is consistent with a dynamically aligned, critically balanced cascade--fluctuations exhibit a scale-dependent alignment , a spectrum and spectral anisotropy. At weaker nonlinearities (small ), a spectral break marking the transition between a large-scale weak regime and a small-scale tearing-mediated range emerges, implying that dynamic alignment occurs also for weak nonlinearities. At the alignment angle shows a stronger scale dependence than in the regime, i.e. at , and at . Dynamic alignment in the weak regime also modifies the large-scale spectrum, scaling roughly as for and as for . A phenomenological theory of dynamically aligned turbulence at weak nonlinearities that can explain these spectra and the transition to the tearing-mediated regime is provided; at small , the strong scale dependence of the alignment angle combines with the increased lifetime of turbulent eddies to allow tearing to onset and mediate the cascade at scales that can be larger than those predicted for a critically balanced cascade by several orders of magnitude. Such a transition to tearing-mediated turbulence may even supplant the usual weak-to-strong transition.
arXiv comment13 pages, 5 figures, 1 table; accepted for publication in The Astrophysical Journal
References in corpus (56)
- Spectrum of magnetohydrodynamic turbulence
- Universality of solar wind turbulent spectrum from MHD to electron scales
- Scattering of Cosmic Rays by Magnetohydrodynamic Interstellar Turbulence
- The Evolution and Role of Solar Wind Turbulence in the Inner Heliosphere
- Gyrokinetic Simulations of Solar Wind Turbulence from Ion to Electron Scales
- Recent progress in astrophysical plasma turbulence from solar wind observations
- Cosmic Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field
- Turbulence and Particle Heating in Advection-Dominated Accretion Flows
- Scattering of energetic particles by anisotropic magnetohydrodynamic turbulence with a Goldreich-Sridhar power spectrum
- Statistical Analysis of Current Sheets in Three-Dimensional Magnetohydrodynamic Turbulence
- Power and spectral index anisotropy of the entire inertial range of turbulence in the fast solar wind
- Dynamic Alignment in Driven Magnetohydrodynamic Turbulence
- Turbulence, magnetic fields and plasma physics in clusters of galaxies
- Turbulent Magnetohydrodynamic Reconnection Mediated by the Plasmoid Instability
- Magnetic reconnection as a driver for a sub-ion scale cascade in plasma turbulence
- Role of magnetic reconnection in MHD turbulence
- Rapid directional alignment of velocity and magnetic field in magnetohydrodynamic turbulence
- Multiscale nature of the dissipation range in gyrokinetic simulations of Alfvénic turbulence
- Disruption of sheetlike structures in Alfvénic turbulence by magnetic reconnection
- Polarization intermittency in MHD and its influence on turbulent cascade
- Alfven Wave Collisions, The Fundamental Building Block of Plasma Turbulence I: Asymptotic Solution
- Collisionless Reconnection in Magnetohydrodynamic and Kinetic Turbulence
- New Regime of MHD Turbulence: Cascade Below Viscous Cutoff
- Disruption of Alfvénic turbulence by magnetic reconnection in a collisionless plasma
- Hybrid-Kinetic Simulations of Ion Heating in Alfvénic Turbulence
- Magnetohydrodynamic turbulence mediated by reconnection
- Role of the Plasmoid Instability in Magnetohydrodynamic Turbulence
- A statistical model of three-dimensional anisotropy and intermittency in strong Alfvénic turbulence
- Kinetic cascade in solar-wind turbulence: 3D3V hybrid-kinetic simulations with electron inertia
- Dual phase-space cascades in 3D hybrid-Vlasov-Maxwell turbulence
- Fully kinetic versus reduced-kinetic modelling of collisionless plasma turbulence
- Critical Balance and the Physics of MHD Turbulence
- Magnetohydrodynamic Turbulence in the Plasmoid-Mediated Regime
- Basic Properties of MHD Turbulence in the Inertial Range
- Reconciling cosmic-ray transport theory with phenomenological models motivated by Milky-Way data
- Measures of Three-Dimensional Anisotropy and Intermittency in Strong Alfvénic Turbulence
- Alignment and scaling of large-scale fluctuations in the solar wind
- On stochastic heating and its phase-space signatures in low- kinetic turbulence
- Kinetic plasma turbulence: recent insights and open questions from 3D3V simulations
- The theory of cosmic-ray scattering on pre-existing MHD modes meets data
- Colliding Alfvénic wave packets in MHD, Hall and kinetic simulations
- Fluid and gyrofluid modeling of low- plasmas: phenomenology of kinetic Alfvén wave turbulence
- Turbulent electromagnetic fields at sub-proton scales: two-fluid and full-kinetic plasma simulations
- Three-dimensional magnetic reconnection in particle-in-cell simulations of anisotropic plasma turbulence
- Imbalanced kinetic Alfvén wave turbulence: from weak turbulence theory to nonlinear diffusion models for the strong regime
- Fluid simulations of plasma turbulence at ion scales: comparison with Vlasov-Maxwell simulations
- Weak Alfvénic turbulence in relativistic plasmas II: Current sheets and dissipation
- Nonlinear energy transfer and current sheet development in localized Alfven wavepacket collisions in the strong turbulence limit
- Spectrum of kinetic plasma turbulence at 0.3-0.9 astronomical units from the Sun
- Temporal Analysis of Dissipative Structures in Magnetohydrodynamic Turbulence
- Spectral signatures of recursive magnetic field reconnection
- Characterizing current structures in 3D hybrid-kinetic simulations of plasma turbulence
- The scale-free texture of the fast solar wind
- Inverse cascade and magnetic vortices in kinetic Alfvén-wave turbulence
- Extended Scaling Laws in Numerical Simulations of MHD Turbulence
- Direct kinetic Alfvén wave energy cascade in the presence of imbalance
Cited by in corpus (3)
- Internal gravity waves in stratified flows with and without vortical modes
- Revisiting the role of cosmic-ray driven Alfvén waves in pre-existing magnetohydrodynamic turbulence. I. Turbulent damping rates and feedback on background fluctuations
- Gyrofluid simulations of turbulence and reconnection in space plasmas