Self-Sustaining Nonlinear Dynamo Process in Keplerian Shear Flows

F. Rincon, G. I. Ogilvie, and M. R. E. Proctor
Phys. Rev. Lett. 98, 254502 – Published 19 June 2007

Abstract

A three-dimensional nonlinear dynamo process is identified in rotating plane Couette flow in the Keplerian regime. It is analogous to the hydrodynamic self-sustaining process in nonrotating shear flows and relies on the magnetorotational instability of a toroidal magnetic field. Steady nonlinear solutions are computed numerically for a wide range of magnetic Reynolds numbers but are restricted to low Reynolds numbers. This process may be important to explain the sustenance of coherent fields and turbulent motions in Keplerian accretion disks, where all its basic ingredients are present.

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  • Received 16 March 2007

DOI:https://doi.org/10.1103/PhysRevLett.98.254502

©2007 American Physical Society

Authors & Affiliations

F. Rincon*, G. I. Ogilvie, and M. R. E. Proctor

  • Department of Applied Mathematics and Theoretical Physics, Centre for Mathematical Sciences, University of Cambridge, Wilberforce Road, Cambridge CB3 0WA, United Kingdom

  • *F.Rincon@damtp.cam.ac.uk

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Issue

Vol. 98, Iss. 25 — 22 June 2007

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