Evolution equations for Taylor vortices in the small-gap limit

Philip Hall
Phys. Rev. A 29, 2921 – Published 1 May 1984
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Abstract

We consider the centrifugal instability of the viscous fluid flow between concentric circular cylinders in the small-gap limit. The amplitude of the Taylor vortex is allowed to depend on a slow time variable, a slow axial variable, and the polar angle θ. It is shown that the amplitude of the vortex cannot, in general, be described by a single amplitude equation. In the absence of any slow axial variations it is shown that a Taylor vortex remains stable to wavy vortex perturbations.

  • Received 21 October 1983

DOI:https://doi.org/10.1103/PhysRevA.29.2921

©1984 American Physical Society

Authors & Affiliations

Philip Hall*

  • Department of Mathematics, Imperial College of Science of Technology, University of London, London SW7 2AZ, England

  • *Address until October 1984: Institute for Computer Applications in Science and Engineering, NASA Langley Research Center, National Aeronautics and Space Administration, Hampton, VA 23665.

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Vol. 29, Iss. 5 — May 1984

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