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Helicity, a measure of the breakage of reflectional symmetry representing the topology of turbulent flows, contributes in a crucial way to their dynamics and to their fundamental statistical properties. We review several of their main…

等离子体物理 · 物理学 2022-02-16 Annick Pouquet , Nobumitsu Yokoi

This article reviews recent studies of scale interactions in magnetohydrodynamic turbulence. The present day increase of computing power, which allows for the exploration of different configurations of turbulence in conducting flows, and…

流体动力学 · 物理学 2015-05-19 P. D. Mininni

Turbulence in an incompressible fluid with and without a magnetic field as well as moderately compressible MHD turbulence are compared. For the magnetohydrodynamic (MHD) models the probability distribution functions of the velocity…

天体物理学 · 物理学 2007-05-23 Nicholas Hall , G. Kowal , A. Lazarian , Jungyeon Cho

A decomposition of the energy and helicity fluxes in a turbulent hydrodynamic flow is proposed. The decomposition is based on the projection of the flow to a helical basis that allows to investigate separately the role of interactions among…

流体动力学 · 物理学 2017-03-08 Alexandros Alexakis

Investigations of the inverse cascade of magnetic helicity are conducted with pseudospectral, three-dimensional direct numerical simulations of forced and decaying incompressible magnetohydrodynamic turbulence. The high-resolution…

太阳与恒星天体物理 · 物理学 2013-09-23 Wolf-Christian Müller , Shiva Kumar. Malapaka

Two-dimensional magnetohydrodynamics (2D MHD), forced at (a) large length scales or (b) small length scales, displays turbulent, but statistically steady, states with widely different statistical properties. We present a systematic,…

流体动力学 · 物理学 2019-06-27 Debarghya Banerjee , Rahul Pandit

The elliptical instability can take place in planetary cores and stars elliptically deformed by gravitational effects, where it generates large-scale three-dimensional flows assumed to be dynamo capable. In this work, we present the first…

经典物理 · 物理学 2013-09-10 David Cébron , Michael Le Bars , Pierre Maubert , Patrice Le Gal

Recent progress regarding the noncanonical Hamiltonian formulation of extended magnetohydrodynamics (XMHD), a model with Hall drift and electron inertia, is summarized. The advantages of the Hamiltonian approach are invoked to study some…

等离子体物理 · 物理学 2017-01-05 George Miloshevich , Manasvi Lingam , Philip J. Morrison

Two non-local asymptotic invariants of magnetic fields for the ideal magnetohydrodynamics are introduced. The velocity of variation of the invariants for a non-ideal magnetohydrodynamics with a small magnetic dissipation is estimated. By…

数学物理 · 物理学 2011-10-06 Petr M. Akhmet'ev

Roles of turbulence in the context of magnetic reconnection are investigated with special emphasis on the mutual interaction between flow (large-scale inhomogeneous structure) and turbulence. In order to evaluate the effective transport due…

太阳与恒星天体物理 · 物理学 2015-05-28 Nobumitsu Yokoi , Masahiro Hoshino

Dynamical studies of MHD turbulence on the one hand, and arguments based upon magnetic helicity on the other, have yielded seemingly contradictory estimates for the $\alpha$ parameter in turbulent dynamo theory. Here we show, with direct…

天体物理学 · 物理学 2007-05-23 Hongsong Chou , George B. Field

A scale-by-scale analysis of energy flux in the turbulent cascade can be performed using the spatially filtered magnetohydrodynamic (MHD) equations, while the gradient tensor invariants are widely used to characterise the structure of…

等离子体物理 · 物理学 2026-04-20 Conan M. Liptrott , Sandra C. Chapman , Bogdan Hnat , Nicholas W. Watkins

Two low-dimensional magnetohydrodynamic models containing three velocity and three magnetic modes are described. One of them (nonhelical model) has zero kinetic and current helicity, while the other model (helical) has nonzero kinetic and…

Magnetized turbulence is ubiquitous in many astrophysical and terrestrial plasmas but no universal theory exists. Even the detailed energy dynamics in magnetohydrodynamic (MHD) turbulence are still not well understood. We present a suite of…

星系天体物理 · 物理学 2023-02-06 Philipp Grete , Brian W. O'Shea , Kris Beckwith

We investigate the scaling behavior of longitudinal and transverse structure functions in homogeneous and isotropic magneto-hydrodynamic (MHD) turbulence by means of an exact hierarchy of structure function equations as well as by direct…

流体动力学 · 物理学 2017-05-03 J. Friedrich , H. Homann , T. Schäfer , R. Grauer

The role of the different helical components of the magnetic and velocity fields in the inverse spectral transfer of magnetic helicity is investigated through Fourier shell-to-shell transfer analysis. Both magnetic helicity and energetic…

等离子体物理 · 物理学 2021-07-07 Jean-Mathieu Teissier , Wolf-Christian Müller

Based on a decomposition of the magnetic field into potential and nonpotential components, magnetic energy and relative helicity can both also be decomposed into two quantities: potential and free energies, and volume-threading and…

太阳与恒星天体物理 · 物理学 2020-04-15 Luis Linan , Étienne Pariat , Guillaume Aulanier , Kostas Moraitis , Gherardo Valori

We perform direct numerical simulations of magnetohydrodynamic (MHD) turbulence with kinetic energy and cross helicity injections at large scales. We observe that the cross helicity changes sign as we go from large and intermediate scales…

等离子体物理 · 物理学 2020-01-10 V. Titov , R. Stepanov , N. Yokoi , M. Verma , R. Samtaney

An effect of the differential rotation on the nonlinear electromotive force in MHD turbulence is found. It includes a nonhelical $\alpha$ effect which is caused by a differential rotation, and it is independent of a hydrodynamic helicity.…

天体物理学 · 物理学 2007-05-23 I. Rogachevskii , N. Kleeorin

We present the results of simulations of forced turbulence in a slab where the mean kinetic helicity has a maximum near the mid-plane, generating gradients of magnetic helicity of both large and small-scale fields. We also study systems…

太阳与恒星天体物理 · 物理学 2010-11-30 A. Hubbard , A. Brandenburg