Abstract

Numerical simulations of the kinematic induction equation are performed on a model configuration of the Cadarache von-Kármán-sodium dynamo experiment. The effect of a localized axisymmetric distribution of relative permeability μr that represents soft iron material within the conducting fluid flow is investigated. The critical magnetic Reynolds number Rmc for dynamo action of the first non-axisymmetric mode roughly scales like Rmcμr − Rmc∞∝μ−1/2r, i.e. the threshold decreases as μr increases. This scaling law suggests a skin effect mechanism in the soft iron discs. More important with regard to the Cadarache dynamo experiment, we observe a purely toroidal axisymmetric mode localized in the high-permeability discs which becomes dominant for large μr. In this limit, the toroidal mode is close to the onset of dynamo action with a (negative) growth rate that is rather independent of the magnetic Reynolds number. We qualitatively explain this effect by paramagnetic pumping at the fluid/disc interface and propose a simplified model that quantitatively reproduces numerical results. The crucial role of the high-permeability discs in the mode selection in the Cadarache dynamo experiment cannot be inferred from computations using idealized pseudo-vacuum boundary conditions (H × n = 0).

Highlights

  • This scaling law suggests a skin effect mechanism in the soft iron discs

  • The toroidal mode is close to the onset of dynamo action with a growth rate that is rather independent of the magnetic Reynolds number

  • We investigate the impact of a localized disc-like permeability distribution embedded in a conducting axisymmetric fluid flow on the growth rates of the axisymmetric and first non-axisymmetric magnetic eigenmodes

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Summary

Introduction

More important with regard to the Cadarache dynamo experiment, we observe a purely toroidal axisymmetric mode localized in the high-permeability discs which becomes dominant for large μr. In this limit, the toroidal mode is close to the onset of dynamo action with a (negative) growth rate that is rather independent of the magnetic Reynolds number. We investigate the influence of the concentrated high permeability on the axisymmetric field modes Even though they are always damped, according to Cowling’s theorem (Cowling 1933, Hide and Palmer 1982), for large μr we find a dominant toroidal mode very close to the onset of dynamo action. This term is responsible for the suction of the magnetic field into the regions with large permeability and involves a (non-divergence-free) velocity-like field that we call ‘pumping velocity’

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