International audienceWe investigate the transition from steady dipolar to reversing multipolar dynamos. The Earth has been argued to lie close to this transition, which could offer a scenario for geomagnetic reversals. We show that the transition between dipolar and multipolar dynamos is characterized by a three terms balance (as opposed to the usually assumed two terms balance), which involves the nongradient parts of inertial, viscous and Coriolis forces. We introduce from this equilibrium the sole parameter RoE-1/3≡ReE2/3, which accurately describes the transition for a wide database of 132 fully three-dimensional direct numerical simulations of spherical rotating dynamos (courtesy of U. Christensen). This resolves earlier contradiction...
The magnetic elds of the planets are generated by dynamo action in their electrically conducting int...
We show that the modes involved in the dynamics of reversals of the magnetic field generated by the ...
We investigate polarity reversals in the geodynamo using a rotating, convection-driven dynamo model....
International audienceThe parameters regime relevant to dynamo action in astrophysical objects is ou...
The Earth's magnetic field is generated in its fluid outer core through dynamo action. In this proce...
Context. Dynamo action in giant planets and rapidly rotating stars leads to a broad variety of magne...
International audienceS U M M A R Y Dynamo action in the Earth's outer core is expected to be contro...
International audienceWe review some of the recent progress on modeling planetary and stellar dynamo...
International audienceObservations of surface magnetic fields of cool stars reveal a large diversity...
International audienceThe dynamo eect is the most popular candidate to explain the non-primordial ma...
In numerical simulations of planetary dynamos there is an abrupt transition in the dynamics of both ...
The objective of this thesis is to understand more about the role of inertia in the Earth’s dynamo. ...
International audienceIn addition to the weak-dipolar state and to the fluctuating-multipolar state,...
AbstractWe are using a three-dimensional convection-driven numerical dynamo model without hyperdiffu...
The magnetic elds of the planets are generated by dynamo action in their electrically conducting int...
We show that the modes involved in the dynamics of reversals of the magnetic field generated by the ...
We investigate polarity reversals in the geodynamo using a rotating, convection-driven dynamo model....
International audienceThe parameters regime relevant to dynamo action in astrophysical objects is ou...
The Earth's magnetic field is generated in its fluid outer core through dynamo action. In this proce...
Context. Dynamo action in giant planets and rapidly rotating stars leads to a broad variety of magne...
International audienceS U M M A R Y Dynamo action in the Earth's outer core is expected to be contro...
International audienceWe review some of the recent progress on modeling planetary and stellar dynamo...
International audienceObservations of surface magnetic fields of cool stars reveal a large diversity...
International audienceThe dynamo eect is the most popular candidate to explain the non-primordial ma...
In numerical simulations of planetary dynamos there is an abrupt transition in the dynamics of both ...
The objective of this thesis is to understand more about the role of inertia in the Earth’s dynamo. ...
International audienceIn addition to the weak-dipolar state and to the fluctuating-multipolar state,...
AbstractWe are using a three-dimensional convection-driven numerical dynamo model without hyperdiffu...
The magnetic elds of the planets are generated by dynamo action in their electrically conducting int...
We show that the modes involved in the dynamics of reversals of the magnetic field generated by the ...
We investigate polarity reversals in the geodynamo using a rotating, convection-driven dynamo model....