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相关论文: Electrodynamics of turbulent fluids with fluctuati…

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A mean-field theory of the electrodynamics of a turbulent fluid is formulated under the assumption that the molecular electric conductivity is correlated with the turbulent velocity fluctuation in the (radial) direction, $\mathbf{g}$. It is…

流体动力学 · 物理学 2023-05-03 Oliver Gressel , Günther Rüdiger , Detlef Elstner

We consider the generation of magnetic field by the flow of a fluid for which the electrical conductivity is nonuniform. A new amplification mechanism is found which leads to dynamo action for flows much simpler than those considered so…

流体动力学 · 物理学 2016-05-04 Francois Petrelis , Alexandros Alexakis , Christophe Gissinger

It is shown that the turbulent dynamo $\alpha$-effect converts magnetic helicity from the turbulent field to the mean field when the turbulence is electromagnetic while the magnetic helicity of the mean-field is transported across space…

天体物理学 · 物理学 2008-11-26 Hantao Ji

An effect of rotation on a developed turbulent stratified convection is studied. Dependencies of the hydrodynamic helicity, the alpha-tensor and the effective drift velocity of the mean magnetic field on the rate of rotation and an…

天体物理学 · 物理学 2009-11-07 N. Kleeorin , I. Rogachevskii

In systems where the standard $\alpha$ effect is inoperative, one often explains the existence of mean magnetic fields by invoking the `incoherent $\alpha$ effect', which appeals to fluctuations of the mean kinetic helicity at a mesoscale.…

太阳与恒星天体物理 · 物理学 2023-10-24 Kishore Gopalakrishnan , Nishant Singh

The mean electromotive force caused by turbulence of an electrically conducting fluid, which plays a central part in mean--field electrodynamics, is calculated for a rotating fluid. Going beyond most of the investigations on this topic, an…

流体动力学 · 物理学 2013-05-29 Karl-Heinz Readler , Rodion Stepanov

This article is focused on the dynamics of a rotating electrically conducting fluid in a turbulent state. As inside the Earth's core or in various industrial processes, a flow is altered by the presence of both background rotation and a…

流体动力学 · 物理学 2011-04-01 Benjamin F. N. Favier , Fabien S. Godeferd , Claude Cambon

This article presents a calculation of the mean electromotive force arising from general small-scale magnetohydrodynamical turbulence, within the framework of the second-order correlation approximation. With the goal of improving…

高能天体物理现象 · 物理学 2015-11-23 Jonathan Squire , Amitava Bhattacharjee

The mean electromotive force in the framework of mean--field magnetohydrodynamics is found with a particular attention to the effect of a mean rotation of the fluid on the mean electromotive force. Anisotropy of the turbulence due to…

天体物理学 · 物理学 2009-11-07 K-H. Raedler , N. Kleeorin , I. Rogachevskii

Mean-field dynamo theory has important applications in solar physics and galactic magnetism. We discuss some of the many turbulence effects relevant to the generation of large-scale magnetic fields in the solar convection zone. The…

太阳与恒星天体物理 · 物理学 2023-11-23 Axel Brandenburg , Detlef Elstner , Youhei Masada , Valery Pipin

The magnetic field of planets or stars is generated by the motion of a conducting fluid through a dynamo instability. The saturation of the magnetic field occurs through the reaction of the Lorentz force on the flow. In relation to this…

流体动力学 · 物理学 2009-11-13 Michael Berhanu , Basile Gallet , Nicolas Mordant , Stephan Fauve

Various approaches to estimate turbulent transport coefficients from numerical simulations of hydromagnetic turbulence are discussed. A quantitative comparison between the averaged magnetic field obtained from a specific three-dimensional…

天体物理学 · 物理学 2009-11-07 Axel Brandenburg , Dmitry Sokoloff

In mean-field magnetohydrodynamics the mean electromotive force due to velocity and magnetic field fluctuations plays a crucial role. In general it consists of two parts, one independent of and another one proportional to the mean magnetic…

太阳与恒星天体物理 · 物理学 2010-01-03 K. -H. Rädler , A. Brandenburg

The turbulent diffusion tensor describing the evolution of the mean concentration of a passive scalar is investigated for non-helically forced turbulence in the presence of rotation or a magnetic field. With rotation, the Coriolis force…

太阳与恒星天体物理 · 物理学 2009-05-09 Axel Brandenburg , Andreas Svedin , Geoffrey M. Vasil

(abridged) Aims: To study turbulent transport coefficients that describe the evolution of large-scale magnetic fields in turbulent convection. Methods: We use the test field method together with 3D numerical simulations of turbulent…

天体物理学 · 物理学 2009-07-29 P. J. Käpylä , M. J. Korpi , A. Brandenburg

We calculate the mean electromotive force in plane Couette flows of a nonrotating conducting fluid under the influence of a large-scale magnetic field for driven turbulence. A vertical stratification of the turbulence intensity results in…

太阳与恒星天体物理 · 物理学 2014-08-12 G. Ruediger , A. Brandenburg

Turbulence with a large magnetic Reyonolds number, generically leads to rapidly growing magnetic noise over and above any mean field. We revisit the dynamics of this fluctuating field, in homogeneous, isotropic, helical turbulence. Assuming…

天体物理学 · 物理学 2007-05-23 K. Subramanian

We study one-point statistics of spiral turbulent pulsations on the background of three-dimensional large-scale vortex in a rotating fluid. Assuming that the helical flow is created by a statistically axially symmetric random force with…

流体动力学 · 物理学 2023-10-31 Leon L. Ogorodnikov , Sergey S. Vergeles

Small magnetic fluctuations ($B_1/B_0 \sim 10^{-4}$) are intrinsically present in a magnetic confinement plasma due to turbulent currents. While the perpendicular transport of particles and heat is typically dominated by fluctuations of the…

等离子体物理 · 物理学 2025-01-10 Kaiyu Zhang , Wladimir Zholobenko , Andreas Stegmeir , Konrad Eder , Frank Jenko

An effect of sheared large-scale motions on a mean electromotive force in a nonrotating turbulent flow of a conducting fluid is studied. It is demonstrated that in a homogeneous divergence-free turbulent flow the alpha-effect does not…

天体物理学 · 物理学 2009-11-07 I. Rogachevskii , N. Kleeorin
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