English

Closure tests for mean field magnetohydrodynamics using a self consistent reduced model

Astrophysics 2009-01-25 v1

Abstract

The mean electromotive force and alpha effect are computed for a forced turbulent flow using a simple nonlinear dynamical model. The results are used to check the applicability of two basic analytic ansatze of mean-field magnetohydrodynamics - the second order correlation approximation (SOCA) and the tau approximation. In the numerical simulations the effective Reynolds number Re is 2-20, while the magnetic Prandtl number varies from 0.1 to 10710^{7}. We present evidence that the τ\tau approximation may be appropriate in dynamical regimes where there is a small-scale dynamo. Catastrophic quenching of the α\alpha effect is found for high PmP_{m}. Our results indicate that for high PmP_{m} SOCA gives a very large value of the α\alpha coefficient compared with the ``exact'' solution. The discrepancy depends on the properties of the random force that drives the flow, with a larger difference occuring for δ\delta-correlated force compared with that for a steady random force.

Keywords

Cite

@article{arxiv.0712.4311,
  title  = {Closure tests for mean field magnetohydrodynamics using a self consistent reduced model},
  author = {V. V. Pipin and M. R. E. Proctor},
  journal= {arXiv preprint arXiv:0712.4311},
  year   = {2009}
}

Comments

submitted to MNRAS

R2 v1 2026-06-21T09:57:57.894Z