Chaotic magnetic field reversals in turbulent dynamos
arXiv:0904.3343 · doi:10.1209/0295-5075/90/49001
Abstract
We present direct numerical simulations of reversals of the magnetic field generated by swirling flows in a spherical domain. In agreement with a recent model, we observe that coupling dipolar and quadrupolar magnetic modes by an asymmetric forcing of the flow generates field reversals. In addition, we show that this mechanism strongly depends on the value of the magnetic Prandtl number.
4 pages, 5 figures
References in corpus (4)
Cited by in corpus (16)
- Dynamics and symmetries of flow reversals in turbulent convection
- Dynamics of reorientations and reversals of large scale flow in Rayleigh-Benard convection
- Reversals of a large scale field generated over a turbulent background
- Supercriticality to subcriticality in dynamo transitions
- A new deterministic model for chaotic reversals
- A Gaussian Model for Simulated Geomagnetic Field Reversals
- Bistability between equatorial and axial dipoles during magnetic field reversals
- On the Applicability of Low-Dimensional Models for Convective Flow Reversals at Extreme Prandtl Numbers
- Neutron-superfluid vortices and proton-superconductor flux tubes: Development of a minimal model for pulsar glitches
- Dipole-Quadrupole dynamics during magnetic field reversals
- Computing non-equilibrium trajectories by a deep learning approach
- Evidence for crisis-induced intermittency during geomagnetic superchron transitions
- Energy Fluxes during Dynamo Reversals
- Dynamo transition in a five-mode helical model
- Period doubling route to chaos in Taylor-Green dynamo
- Discrete Symmetries in Dynamo Reversals