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A trio of simple optimized axisymmetric kinematic dynamos in a sphere

Holdenried-Chernoff, D.; Chen, L.; Jackson, A.

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Authors

D. Holdenried-Chernoff

L. Chen

A. Jackson



Abstract

Planetary magnetic fields are generated by the motion of conductive fluid in the planet's interior. Complex flows are not required for dynamo action; simple flows have been shown to act as efficient kinematic dynamos, whose physical characteristics are more straightforward to study. Recently, Chen et al. (2018, J. Fluid Mech.839, 1–32. (doi:10.1017/jfm.2017.924)) found the optimal, unconstrained kinematic dynamo in a sphere, which, despite being of theoretical importance, is of limited practical use. We extend their work by restricting the optimization to three simple two-mode axisymmetric flows based on the kinematic dynamos of Dudley & James (1989, Proc. R. Soc. Lond. A425, 407–429. (doi:10.1098/rspa.1989.0112)). Using a Lagrangian optimization, we find the smallest critical magnetic Reynolds number for each flow type, measured using an enstrophy-based norm. A Galerkin method is used, in which the spectral coefficients of the fluid flow and magnetic field are updated in order to maximize the final magnetic energy. We consider the t01s01, t01s02 and t02s02 flows and find enstrophy-based critical magnetic Reynolds numbers of 107.7, 142.4 and 125.5 (13.7, 19.6 and 16.4, respectively, with the energy-based definition). These are up to four times smaller than the original flows. These simple and efficient flows may be used as benchmarks in future studies.

Citation

Holdenried-Chernoff, D., Chen, L., & Jackson, A. (2019). A trio of simple optimized axisymmetric kinematic dynamos in a sphere. Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences, 475(2229), Article 20190308. https://doi.org/10.1098/rspa.2019.0308

Journal Article Type Article
Acceptance Date Aug 15, 2019
Online Publication Date Sep 18, 2019
Publication Date Sep 4, 2019
Deposit Date Oct 7, 2019
Publicly Available Date Nov 1, 2019
Journal Proceedings of the Royal Society A: Mathematical, Physical and Engineering Sciences
Print ISSN 1364-5021
Electronic ISSN 1471-2946
Publisher The Royal Society
Peer Reviewed Peer Reviewed
Volume 475
Issue 2229
Article Number 20190308
DOI https://doi.org/10.1098/rspa.2019.0308
Public URL https://durham-repository.worktribe.com/output/1289680

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