NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Press Enter or click the Search button to begin your search.

Back to Results
Evolution equations for Taylor vortices in the small-gap limitThe centrifugal instability of the viscous fluid flow between concentric circular cylinders in the small gap limit is considered. The amplitude of the Taylor vortex is allowed to depend on a slow time variable, a slow axial variable, and the polar angle. It is shown that the amplitude of the vortex cannot in general be described by a single amplitude equation. However, if the axial variations are periodic a single amplitude equation can be derived. In the absence of any slow axial variations it is shown that a Taylor vortex remains stable to wavy vortex perturbations. Furthermore, in this situation, stable nonaxisymmeric modes can occur but do not bifurcate from the Taylor vortex state. The stability of these modes is shown to be governed by a modified form of the Eckhaus criterion. Previously announced in STAR as N84-10501
Document ID
19840050507
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Hall, P.
(NASA Langley Research Center Institute for Computer Applications in Science and Engineering, Hampton, VA; Imperial College of Sci, United Kingdom)
Date Acquired
August 11, 2013
Publication Date
May 1, 1984
Publication Information
Publication: Physical Review A - General Physics, 3rd Series
Volume: 29
ISSN: 0556-2791
Subject Category
Fluid Mechanics And Heat Transfer
Report/Patent Number
ISSN: 0556-2791
Accession Number
84A33294
Funding Number(s)
CONTRACT_GRANT: NAS1-17070
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available