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The effect on dynamo action of an anisotropic electrical conductivity conjugated to an anisotropic magnetic permeability is considered. Not only is the dynamo fully axisymmetric, but it requires only a simple differential rotation, which…

等离子体物理 · 物理学 2021-02-09 Franck Plunian , Thierry Alboussière

A milestone of dynamo theory is Cowling's theorem, known in its modern form as the impossibility for an axisymmetric velocity field to generate an axisymmetric magnetic field by dynamo action. Using an anisotropic electrical conductivity we…

流体动力学 · 物理学 2020-04-20 Franck Plunian , Thierry Alboussière

We consider a fluid dynamo model generated by the flow on both sides of a moving layer. The magnetic permeability of the layer is larger than that of the flow. We show that there exists an optimum value of magnetic permeability for which…

流体动力学 · 物理学 2014-11-04 Johann Herault , François Pétrélis

Planetary and stellar dynamos likely result from turbulent motions in magnetofluids with kinematic viscosities that are small compared to their magnetic diffusivities. Laboratory experiments are in progress to produce similar dynamos in…

天体物理学 · 物理学 2009-11-11 P. D. Mininni

In the limit of large magnetic Reynolds numbers, it is shown that a smooth differential rotation can lead to fast dynamo action, provided that the electrical conductivity or magnetic permeability is anisotropic. If the shear is infinite,…

流体动力学 · 物理学 2022-07-11 Franck Plunian , Thierry Alboussière

We perform numerical experiments to study the shear dynamo problem where we look for the growth of large--scale magnetic field due to non--helical stirring at small scales in a background linear shear flow, in previously unexplored…

星系天体物理 · 物理学 2015-09-16 Nishant K. Singh , Naveen Jingade

We compute numerically the threshold for dynamo action in Taylor-Green swirling flows. Kinematic calculations, for which the flow field is fixed to its time averaged profile, are compared to dynamical runs for which both the Navier-Stokes…

流体动力学 · 物理学 2016-08-16 Yannick Ponty , Pablo Mininni , Jean-François Pinton , Hélène Politano , Annick Pouquet

Recently Ricca and Maggione [MHD (2008)] have presented a very simple and interesting model of stretch-twist-fold dynamo in diffusive media based on numerical simulations of Riemannian flux tubes. In this paper we present a yet simpler way…

流体动力学 · 物理学 2009-04-13 Garcia de Andrade

(abridged) Aims: Three-dimensional numerical simulations of penetrative compressible convection with uniform horizontal shear are used to study dynamo action and the generation of large-scale magnetic fields. Methods: We consider cases…

天体物理学 · 物理学 2008-11-10 P. J. Käpylä , M. J. Korpi , A. Brandenburg

Using direct numerical simulations, we verify that "flow IV" of Roberts (1972) exhibits dynamo action dominated by horizontally averaged large-scale magnetic field. With the test-field method we compute the turbulent magnetic diffusivity…

太阳与恒星天体物理 · 物理学 2013-08-09 Ebru Devlen , Axel Brandenburg , Dhrubaditya Mitra

The dynamo effect is a class of macroscopic phenomena responsible for generation and maintaining magnetic fields in astrophysical bodies. It hinges on hydrodynamic three-dimensional motion of conducting gases and plasmas that achieve high…

强关联电子 · 物理学 2018-10-31 Victor Galitski , Mehdi Kargarian , Sergey Syzranov

We study dynamo action in a convective layer of electrically-conducting, compressible fluid, rotating about the vertical axis. At the upper and lower bounding surfaces, perfectly-conducting boundary conditions are adopted for the magnetic…

太阳与恒星天体物理 · 物理学 2011-11-23 Benjamin F. N. Favier , Paul J. Bushby

The dynamo mechanism is a process of magnetic field self-excitation in a moving electrically conducting fluid. One of the most interesting applications of this mechanism related to the astrophysical systems is the case of a random motion of…

太阳与恒星天体物理 · 物理学 2021-08-04 E. A. Illarionov , D. D. Sokoloff

Many astrophysical bodies harbor magnetic fields that are thought to be sustained by a dynamo process. However, it has been argued that the production of large-scale magnetic fields by mean-field dynamo action is strongly suppressed at…

星系天体物理 · 物理学 2013-01-22 Fabio Del Sordo , Gustavo Guerrero , Axel Brandenburg

Boozer addressed the role of magnetic helicity in dynamos [Phys Fluids \textbf{B},(1993)]. He pointed out that the magnetic helicity conservation implies that the dynamo action is more easily attainable if the electric potential varies over…

等离子体物理 · 物理学 2009-11-23 Garcia de Andrade

We numerically examine dynamo action generated by a flow of an electrically conducting fluid in a precessing cylindrical cavity. We compare a simplified kinematic approach based on the solution of the magnetic induction equation with a…

流体动力学 · 物理学 2025-04-07 André Giesecke , Mike Wilbert , Ján Šimkanin , Rainer Grauer , Frank Stefani

The onset of dynamo action is investigated within the context of a newly developed low Rossby, low magnetic Prandtl number, convection-driven dynamo model. This multiscale model represents an asymptotically exact form of an $\alpha^2$ mean…

We analyze the nature of dynamo action that produces horizontally averaged magnetic fields in two particular flows that were studied by Roberts (1972, Phil. Trans. R. Soc. A 271, 411), namely his flows II and III. They have zero kinetic…

太阳与恒星天体物理 · 物理学 2014-04-25 Matthias Rheinhardt , Ebru Devlen , Karl-Heinz Rädler , Axel Brandenburg

We consider kinematic dynamo action in rapidly rotating Boussinesq convection just above onset. The velocity is constrained to have either a square or a hexagonal pattern. For the square pattern, large-scale dynamo action is observed at…

流体动力学 · 物理学 2015-06-17 B. Favier , M. R. E. Proctor

We address magnetic-field generation by dynamo action in systems with inhomogeneous electrical conductivity and magnetic permeability. More specifically, we first show that the Taylor-Couette kinematic dynamo undergoes a drastic reduction…

流体动力学 · 物理学 2021-12-29 Florence Marcotte , Basile Gallet , Francois Pétrélis , Christophe Gissinger
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