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相关论文: On the Spectrum of Magnetohydrodynamic Turbulence

200 篇论文

A novel model of incompressible magnetohydrodynamic turbulence in the presence of a strong external magnetic field is proposed for explanation of recent numerical results. According to the proposed model, in the presence of the strong…

天体物理学 · 物理学 2008-11-26 G. Gogoberidze

We propose a phenomenological theory of strong incompressible magnetohydrodynamic turbulence in the presence of a strong large-scale external magnetic field. We argue that in the inertial range of scales, magnetic-field and velocity-field…

天体物理学 · 物理学 2007-05-23 Stanislav Boldyrev

The solar wind and the interstellar medium are permeated by large-scale magnetic fields that render magnetohydrodynamic (MHD) turbulence anisotropic. In the weak-turbulence limit in which three-wave interactions dominate, analytical and…

太阳与恒星天体物理 · 物理学 2011-09-06 C. S. Ng , A. Bhattacharjee

When magnetohydrodynamic turbulence evolves in the presence of a large-scale mean magnetic field, an anisotropy develops relative to that preferred direction. The well-known tendency is to develop stronger gradients perpendicular to the…

等离子体物理 · 物理学 2020-07-15 Rohit Chhiber , William H. Matthaeus , Sean Oughton , Tulasi N. Parashar

We present a new analysis of the anisotropic spectral energy distribution in incompressible magnetohydrodynamic (MHD) turbulence permeated by a strong mean magnetic field. The turbulent flow is generated by high-resolution pseudo-spectral…

等离子体物理 · 物理学 2015-05-19 Roland Grappin , Wolf-Christian Müller

Recent numerical and observational studies contain conflicting reports on the spectrum of magnetohydrodynamic turbulence. In an attempt to clarify the issue we investigate anisotropic incompressible magnetohydrodynamic turbulence with a…

天体物理学 · 物理学 2010-11-11 Jean Carlos Perez , Stanislav Boldyrev

Magnetic field fluctuations in MHD turbulence can be viewed as current sheets that are progressively more anisotropic at smaller scales. As suggested by Loureiro & Boldyrev (2017) and Mallet et al (2017), below a certain critical thickness…

等离子体物理 · 物理学 2017-08-09 Stanislav Boldyrev , Nuno F. Loureiro

We present a numerical analysis of an incompressible decaying magnetohydrodynamic turbulence run on a grid of 1536^3 points. The Taylor Reynolds number at the maximum of dissipation is ~1100, and the initial condition is a superposition of…

天体物理学 · 物理学 2009-06-23 P. D. Mininni , A. Pouquet

The problem of anomalous scaling in magnetohydrodynamics turbulence is considered within the framework of the kinematic approximation, in the presence of a large-scale background magnetic field. The velocity field is Gaussian,…

混沌动力学 · 物理学 2009-10-31 N. V. Antonov , A. Lanotte , A. Mazzino

High Reynolds number isotropic magneto-hydro-dynamic turbulence in the presence of large scale magnetic fields is investigated as a function of the magnetic field strength. For a variety of flow configurations the energy dissipation rate…

流体动力学 · 物理学 2012-09-20 Alexandros Alexakis

The transition from weak to strong turbulence when passing from large to small scales in magnetohydrodynamic (MHD) turbulence with guide field is a cornerstone of anisotropic turbulence theory. We present the first check of this transition,…

太阳与恒星天体物理 · 物理学 2015-06-04 Andrea Verdini , Roland Grappin

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 describes the time evolution of the anisotropic…

天体物理学 · 物理学 2009-11-13 Benjamin D. G. Chandran

We report a numerical investigation of three dimensional, incompressible, Hall magnetohydrodynamic turbulence with a relatively strong mean magnetic field. Using helicity decomposition and cross-bicoherence analysis, we observe that the…

混沌动力学 · 物理学 2018-09-19 Romain Meyrand , Khurom H. Kiyani , Ozgur D. Gurcan , Sebastien Galtier

One of the most important predictions in magnetohydrodynamics (MHD) is that in the presence of a uniform magnetic field $\textbf{b}_{0}$ a transition from weak to strong wave turbulence should occur when going from large to small…

流体动力学 · 物理学 2016-03-23 Romain Meyrand , Sebastien Galtier , Khurom H. Kiyani

A heuristic model is given for anisotropic magnetohydrodynamics (MHD) turbulence in the presence of a uniform external magnetic field $B_0 {\bf {\hat e}_{\pa}}$. The model is valid for both moderate and strong $B_0$ and is able to describe…

等离子体物理 · 物理学 2009-11-11 Sebastien Galtier , Annick Pouquet , Andre Mangeney

We propose a phenomenological theory of incompressible magnetohydrodynamic turbulence in the presence of a strong large-scale magnetic field, which establishes a link between the known anisotropic models of strong and weak MHD turbulence We…

等离子体物理 · 物理学 2012-09-21 Roland Grappin , Wolf-Christian Müller , Özgür Gürcan

Motivated by recent analytic predictions, we report numerical evidence showing that in driven incompressible magnetohydrodynamic turbulence the magnetic- and velocity-field fluctuations locally tend to align the directions of their…

天体物理学 · 物理学 2007-05-23 Joanne Mason , Fausto Cattaneo , Stanislav Boldyrev

We analyze 3D numerical simulations of driven incompressible magnetohydrodynamic (MHD) turbulence in a periodic box threaded by a moderately strong external magnetic field. We sum over nonlinear interactions within Fourier wavebands and…

天体物理学 · 物理学 2011-05-10 Jungyeon Cho , Alex Lazarian , Ethan Vishniac

We compare the properties of ordinary strong magnetohydrodynamic (MHD) turbulence in a strongly magnetized medium with the recently discovered viscosity-damped regime. We focus on energy spectra, anisotropy, and intermittency. Our most…

天体物理学 · 物理学 2009-11-07 Jungyeon Cho , A. Lazarian , Ethan T. Vishniac

We present numerical simulations and explore scalings and anisotropy of compressible magnetohydrodynamic (MHD) turbulence. Our study covers both gas pressure dominated (high beta) and magnetically dominated (low beta) plasmas at different…

天体物理学 · 物理学 2011-05-05 Jungyeon Cho , A. Lazarian
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