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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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Bibliographic Details
Published in:Physics of fluids (1994) 2009-06, Vol.21 (6), p.064106-064106-8
Main Authors: Poncet, Sébastien, Serre, Éric, Le Gal, Patrice
Format: Article
Language:English
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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.
ISSN:1070-6631
1089-7666
DOI:10.1063/1.3156859