The electromotive force in multi-scale flows at high magnetic Reynolds number

Author:

Tobias Steven M.,Cattaneo Fausto

Abstract

Recent advances in dynamo theory have been made by examining the competition between small- and large-scale dynamos at high magnetic Reynolds number $\mathit{Rm}$. Small-scale dynamos rely on the presence of chaotic stretching whilst the generation of large-scale fields occurs in flows lacking reflectional symmetry via a systematic electromotive force (EMF). In this paper we discuss how the statistics of the EMF (at high $\mathit{Rm}$) depend on the properties of the multi-scale velocity that is generating it. In particular, we determine that different scales of flow have different contributions to the statistics of the EMF, with smaller scales contributing to the mean without increasing the variance. Moreover, we determine when scales in such a flow act independently in their contribution to the EMF. We further examine the role of large-scale shear in modifying the EMF. We conjecture that the distribution of the EMF, and not simply the mean, largely determines the dominant scale of the magnetic field generated by the flow.

Publisher

Cambridge University Press (CUP)

Subject

Condensed Matter Physics

Cited by 7 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. A Physical Interpretation of Asymmetric Growth and Decay of the Geomagnetic Dipole Moment;Geochemistry, Geophysics, Geosystems;2022-03

2. On magnetic helicity generation and transport in a nonlinear dynamo driven by a helical flow;Journal of Plasma Physics;2020-08

3. Convection-driven kinematic dynamos with a self-consistent shear flow;Geophysical & Astrophysical Fluid Dynamics;2018-09-11

4. What is a large-scale dynamo?;Monthly Notices of the Royal Astronomical Society: Letters;2016-09-23

5. SHEAR-DRIVEN DYNAMO WAVES IN THE FULLY NONLINEAR REGIME;The Astrophysical Journal;2016-06-28

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