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Revisiting the two first instabilities of the flow in an annular rotor-stator cavity
The stability of the flow enclosed between a stationary and a rotating disk with a central hub is revisited by experimental visualizations and direct numerical simulations in the case of unmerged boundary layers. The first instability appears as circular rolls, denoted by CRs (type 2 instability), w...
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Published in: | Physics of fluids (1994) 2009-06, Vol.21 (6), p.064106-064106-8 |
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Main Authors: | , , |
Format: | Article |
Language: | English |
Subjects: | |
Citations: | Items that this one cites Items that cite this one |
Online Access: | Get full text |
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Summary: | The stability of the flow enclosed between a stationary and a rotating disk with a central hub is revisited by experimental visualizations and direct numerical simulations in the case of unmerged boundary layers. The first instability appears as circular rolls, denoted by CRs (type 2 instability), which propagate along the stator before vanishing in the vicinity of the hub. The calculations highlight the convective nature of these rolls, which is in agreement with previous experimental results (
P. Gauthier
,
P. Gondret
, and
M. Rabaud
,
J. Fluid Mech.
386
,
105
(
1999
)
). It proves in particular that the CR instability observed in the experiment under permanent conditions is noise sustained. Above a second threshold, spiral rolls, denoted SR1 (type 1 instability), appear at the periphery of the cavity and can coexist with the circular rolls. The DNS shows that they appear through a supercritical Hopf bifurcation. The SR1 patterns appear to be very close to those emitted by the corner vortices obtained by Lopez and Weidman [
J. Fluid Mech.
326
,
373
(
1996
)
] during the spin-down of a rotating disk in a fixed cylinder. |
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ISSN: | 1070-6631 1089-7666 |
DOI: | 10.1063/1.3156859 |