Intermittent magnetic field excitation by a turbulent flow of liquid sodium
arXiv:physics/0606239 · doi:10.1103/PhysRevLett.97.044503
Abstract
The magnetic field measured in the Madison Dynamo Experiment shows intermittent periods of growth when an axial magnetic field is applied. The geometry of the intermittent field is consistent with the fastest growing magnetic eigenmode predicted by kinematic dynamo theory using a laminar model of the mean flow. Though the eigenmodes of the mean flow are decaying, it is postulated that turbulent fluctuations of the velocity field change the flow geometry such that the eigenmode growth rate is temporarily positive. Therefore, it is expected that a characteristic of the onset of a turbulent dynamo is magnetic intermittency.
arXiv comment5 pages, 7 figures
References in corpus (4)
Cited by in corpus (19)
- Magnetohydrodynamic experiments on cosmic magnetic fields
- On the magnetic fields generated by experimental dynamos
- Laboratory Space Physics: Investigating the Physics of Space Plasmas in the Laboratory
- The Small-Scale Dynamo at Low Magnetic Prandtl Numbers
- Subcritical dynamo bifurcation in the Taylor Green flow
- Zonal shear and super-rotation in a magnetized spherical Couette flow experiment
- Do Androids Dream of Magnetic Fields? Using Neural Networks to Interpret the Turbulent Interstellar Medium
- Bypassing Cowling's theorem in axisymmetric fluid dynamos
- The Catalogue for Astrophysical Turbulence Simulations (CATS)
- Applications of a finite-volume algorithm for incompressible MHD problems
- Wave-driven dynamo action in spherical MHD systems
- The onset of turbulent rotating dynamos at the low limit
- Magnetic structure, dipole reversals, and 1/f noise in resistive MHD spherical dynamos
- Two-Loop Turbulent Helical Magnetohydrodynamics: Large-Scale Dynamo and Energy Spectrum
- High dimensional tori and chaotic and intermittent transients in magnetohydrodynamic Couette flows
- Identification of vortexes obstructing the dynamo mechanism in laboratory experiments
- The integral equation approach to kinematic dynamo theory and its application to dynamo experiments in cylindrical geometry
- Diagnosing Turbulence in the Neutral and Molecular Interstellar Medium of Galaxies
- Effect of electromagnetic boundary conditions on the onset of small-scale dynamos driven by convection