International audienceIn addition to the weak-dipolar state and to the fluctuating-multipolar state, widely discussed in the literature, a third regime has been identified in (Dormy 2016 J. Fluid. Mech. 789 500–13). It corresponds to a strong-dipolar branch which appears to approach, in a numerically affordable regime, the magnetostrophic limit relevant to the dynamics of the Earth's core. We discuss the transitions between these states and point to the relevance of this strong-dipolar state to Geodynamo modelling
International audienceThe parameters regime relevant to dynamo action in astrophysical objects is ou...
Global scale magnetostrophic balance, in which Lorentz and Coriolis forces comprise the leading-orde...
International audienceObservations of surface magnetic fields of cool stars reveal a large diversity...
International audienceIn addition to the weak-dipolar state and to the fluctuating-multipolar state,...
International audienceWe investigate the transition from steady dipolar to reversing multipolar dyna...
Context. Dynamo action in giant planets and rapidly rotating stars leads to a broad variety of magne...
The Earth's magnetic field is generated in its fluid outer core through dynamo action. In this proce...
AbstractWe are using a three-dimensional convection-driven numerical dynamo model without hyperdiffu...
International audienceThe dynamo eect is the most popular candidate to explain the non-primordial ma...
International audienceS U M M A R Y Dynamo action in the Earth's outer core is expected to be contro...
The 2D Parker’s mean-field dynamo equations with a various distributions of the α- and ω-effects are...
Recent studies have demonstrated the possibility of constructing magnetostrophic dynamo models, whic...
International audienceFrom a suite of 56 chemically-driven dynamo simulations with aspect ratio (inn...
International audienceObservations of low-mass stars reveal a variety of magnetic topologies ranging...
International audienceThe parameters regime relevant to dynamo action in astrophysical objects is ou...
Global scale magnetostrophic balance, in which Lorentz and Coriolis forces comprise the leading-orde...
International audienceObservations of surface magnetic fields of cool stars reveal a large diversity...
International audienceIn addition to the weak-dipolar state and to the fluctuating-multipolar state,...
International audienceWe investigate the transition from steady dipolar to reversing multipolar dyna...
Context. Dynamo action in giant planets and rapidly rotating stars leads to a broad variety of magne...
The Earth's magnetic field is generated in its fluid outer core through dynamo action. In this proce...
AbstractWe are using a three-dimensional convection-driven numerical dynamo model without hyperdiffu...
International audienceThe dynamo eect is the most popular candidate to explain the non-primordial ma...
International audienceS U M M A R Y Dynamo action in the Earth's outer core is expected to be contro...
The 2D Parker’s mean-field dynamo equations with a various distributions of the α- and ω-effects are...
Recent studies have demonstrated the possibility of constructing magnetostrophic dynamo models, whic...
International audienceFrom a suite of 56 chemically-driven dynamo simulations with aspect ratio (inn...
International audienceObservations of low-mass stars reveal a variety of magnetic topologies ranging...
International audienceThe parameters regime relevant to dynamo action in astrophysical objects is ou...
Global scale magnetostrophic balance, in which Lorentz and Coriolis forces comprise the leading-orde...
International audienceObservations of surface magnetic fields of cool stars reveal a large diversity...