Add to ORKGnamo involve usually complex configurations of fluid flow and magnetic field, designed to achieve the critical magnetic Reynolds number (Rm) sufficient for magnetic self-excitation, but with minimum energy input and at scales manage-able in a laboratory. Computer simulations that could be used to optimize th
Nowadays, it is widely accepted that the magnetic fields of planets, stars, and galaxies are generat...
Context. A crucial step in the numerical investigation of small-scale dynamos in the solar atmospher...
International audienceWe numerically investigate the efficiency of a spherical Couette flow at gener...
Magnetic fields of planets, stars, and galaxies result from self-excitation in moving electroconduct...
There is no sufficient condition telling that a given flow is able to generate magnetic energy throu...
Abstract.Magnetic dynamo experiments are being performed in many laboratories throughout the world. ...
Introduction. The theory of large-scale (mean field) and small-scale (tur-bulent) dynamos is mainly ...
We report on hybrid numerical simulations of a turbulent magnetic dynamo. The simulated set-up mimic...
The process, in which a magnetic field is amplified by the flow of an electrically conducting fluid,...
Planetary and stellar dynamos likely result from turbulent motions in magnetofluids with kinematic v...
The lecture gives a short review on recent developments in the MHD-dynamo problem, including theory,...
We present results from numerical simulations of nonlinear MHD dynamo action produced by three-dimen...
Coherent structures in turbulent flows consisting of vorticity filaments may generate small-scale ma...
This report summarises work carried out during the 2007 Summer School in Multiscale Modeling in Simu...
Direct numerical simulations of turbulent Hall dynamos are presented. The evolution of an initially ...
Nowadays, it is widely accepted that the magnetic fields of planets, stars, and galaxies are generat...
Context. A crucial step in the numerical investigation of small-scale dynamos in the solar atmospher...
International audienceWe numerically investigate the efficiency of a spherical Couette flow at gener...
Magnetic fields of planets, stars, and galaxies result from self-excitation in moving electroconduct...
There is no sufficient condition telling that a given flow is able to generate magnetic energy throu...
Abstract.Magnetic dynamo experiments are being performed in many laboratories throughout the world. ...
Introduction. The theory of large-scale (mean field) and small-scale (tur-bulent) dynamos is mainly ...
We report on hybrid numerical simulations of a turbulent magnetic dynamo. The simulated set-up mimic...
The process, in which a magnetic field is amplified by the flow of an electrically conducting fluid,...
Planetary and stellar dynamos likely result from turbulent motions in magnetofluids with kinematic v...
The lecture gives a short review on recent developments in the MHD-dynamo problem, including theory,...
We present results from numerical simulations of nonlinear MHD dynamo action produced by three-dimen...
Coherent structures in turbulent flows consisting of vorticity filaments may generate small-scale ma...
This report summarises work carried out during the 2007 Summer School in Multiscale Modeling in Simu...
Direct numerical simulations of turbulent Hall dynamos are presented. The evolution of an initially ...
Nowadays, it is widely accepted that the magnetic fields of planets, stars, and galaxies are generat...
Context. A crucial step in the numerical investigation of small-scale dynamos in the solar atmospher...
International audienceWe numerically investigate the efficiency of a spherical Couette flow at gener...