The presence of chaotic transients in a nonlinear dynamo is investigated through numerical simulations of the 3D magnetohydrodynamic equations. By using the kinetic helicity of the flow as a control parameter, a hysteretic blowout bifurcation is conjectured to be responsible for the transition to dynamo, leading to a sudden increase in the magnetic energy of the attractor. This high-energy hydromagnetic attractor is suddenly destroyed in a boundary crisis when the helicity is decreased. Both the blowout bifurcation and the boundary crisis generate long chaotic transients that are due, respectively, to a chaotic saddle and a relative chaotic attractor
The generation of magnetic fields in space plasmas and in astrophysics is usually described within t...
International audienceMagnetohydrodynamic dynamo action is often invoked to explain the existence of...
Large-scale dynamo action is well understood when the magnetic Reynolds number (Rm) is small, but be...
Nonlinear mean-field models of the solar dynamo show long-term variability, which may be relevant to...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
Turbulent dynamo phenomena, observed almost everywhere in astrophysical objects and also in the labo...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
Context.We present results from non linear MHD dynamo experiments with a three-dimensional steady an...
This paper gives new results concerning magnetic field generation leading to a steady equilibrated s...
Context. We present results from non linear MHD dynamo experiments with a three-dimensional steady a...
A model planetary dynamo based on the Boussinesq approximation along with homogeneous boundary condi...
We report successive bifurcations in direct numerical simulations (DNSs) of a Taylor–Green flow, in ...
Magnetohydrodynamic dynamo action is often invoked to explain the existence of magnetic fields in se...
The generation of magnetic fields in space plasmas and in astrophysics is usually described within t...
International audienceMagnetohydrodynamic dynamo action is often invoked to explain the existence of...
Large-scale dynamo action is well understood when the magnetic Reynolds number (Rm) is small, but be...
Nonlinear mean-field models of the solar dynamo show long-term variability, which may be relevant to...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
A three-dimensional numerical computation of magnetohydrodynamic dynamo behavior is described. The d...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
Turbulent dynamo phenomena, observed almost everywhere in astrophysical objects and also in the labo...
11 pagesInternational audienceA three-dimensional numerical computation of magnetohydrodynamic dynam...
Context.We present results from non linear MHD dynamo experiments with a three-dimensional steady an...
This paper gives new results concerning magnetic field generation leading to a steady equilibrated s...
Context. We present results from non linear MHD dynamo experiments with a three-dimensional steady a...
A model planetary dynamo based on the Boussinesq approximation along with homogeneous boundary condi...
We report successive bifurcations in direct numerical simulations (DNSs) of a Taylor–Green flow, in ...
Magnetohydrodynamic dynamo action is often invoked to explain the existence of magnetic fields in se...
The generation of magnetic fields in space plasmas and in astrophysics is usually described within t...
International audienceMagnetohydrodynamic dynamo action is often invoked to explain the existence of...
Large-scale dynamo action is well understood when the magnetic Reynolds number (Rm) is small, but be...