English

Rotationally induced coherence in turbulent kinematic dynamos

Fluid Dynamics 2018-11-06 v2 Earth and Planetary Astrophysics Solar and Stellar Astrophysics

Abstract

We consider rotating, kinematic dynamos at low magnetic Prandtl number PmPm. We show that the inclusion of rotation leads to an increase in spatio-temporal coherence and a modification of the turbulent spectrum. These effects make the flow more efficient in driving the dynamo, in the sense that the energy injection rate required to reach the critical value of the magnetic Reynolds number RmcRm_c is reduced in comparison with a non-rotating dynamo (Seshasayanan et al. 2017). For random dynamos it is known that the growth-rate would largely be determined by the spectral index of the flow at the resistive scale. Here, however, we demonstrate that the dynamo growth-rate in rotating flows is increased by the rotationally induced long-lived large scale eddies with a coherence time greater than the local turnover time. These eddies play the major role in determining the dynamo growth-rate.

Keywords

Cite

@article{arxiv.1805.02291,
  title  = {Rotationally induced coherence in turbulent kinematic dynamos},
  author = {Vassilios Dallas and Steve Tobias},
  journal= {arXiv preprint arXiv:1805.02291},
  year   = {2018}
}

Comments

12 pages, 8 figures

R2 v1 2026-06-23T01:46:39.426Z