English

Mean-field dynamos: the old concept and some recent developments

Solar and Stellar Astrophysics 2014-02-27 v1

Abstract

This article reproduces the Karl Schwarzschild lecture 2013. Some of the basic ideas of electrodynamics and magnetohydrodynamics of mean fields in turbulently moving conducting fluids are explained. It is stressed that the connection of the mean electromotive force with the mean magnetic field and its first spatial derivatives is in general neither local nor instantaneous and that quite a few claims concerning pretended failures of the mean-field concept result from ignoring this aspect. In addition to the mean-field dynamo mechanisms of α2\alpha^2 and α\alpha Ω\Omega type several others are considered. Much progress in mean-field electrodynamics and magnetohydrodynamics results from the test-field method for calculating the coefficients that determine the connection of the mean electromotive force with the mean magnetic field. As an important example the memory effect in homogeneous isotropic turbulence is explained. In magnetohydrodynamic turbulence there is the possibility of a mean electromotive force that is primarily independent of the mean magnetic field and labeled as Yoshizawa effect. Despite of many efforts there is so far no convincing comprehensive theory of α\alpha quenching, that is, the reduction of the α\alpha effect with growing mean magnetic field, and of the saturation of mean-field dynamos. Steps toward such a theory are explained. Finally, some remarks on laboratory experiments with dynamos are made.

Keywords

Cite

@article{arxiv.1402.6557,
  title  = {Mean-field dynamos: the old concept and some recent developments},
  author = {K. -H. Rädler},
  journal= {arXiv preprint arXiv:1402.6557},
  year   = {2014}
}

Comments

11 pages, 3 figures, submitted to Astronomische Nachrichten

R2 v1 2026-06-22T03:16:18.553Z