FLOW IN A CYLINDER DRIVEN BY ROTATING SPLIT-DISK ENDWALLS

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Flow of an incompressible viscous fluid contained in a cylindrical vessel (radius R, height H) is considered. Each of the cylinder endwalls is split into two parts which rotate steadily about the central axis with different rotation rates: the inner disk (r < r1) rotating at OMEGA1, and the outer annulus (r, < r < R) rotating at OMEGA2. Numerical solutions to the axisymmetric Navier-Stokes equations are secured for small system Ekman numbers E (= nu/(OMEGAH-2)). In the linear regime, when the Rossby number Ro ( = 2(OMEGA2 - OMEGA1)/(OMEGA1, + OMEGA2)) much less than 1, the numerical results are shown to be compatible with the theoretical prediction as well as the available experimental measurements. Emphasis is placed on the results in the nonlinear regime in which Ro is finite. Details of the structures of azimuthal and meridional flows are presented by the numerical results. For a fixed Ekman number, the gross features of the flow remain qualitatively unchanged as Ro increases. The meridional flows are characterized by two circulation cells. The shear layer is a region of intense axial flow toward the endwall and of vanishing radial velocity. The thicknesses of the shear layer near r = r1 and the Ekman layer on the endwall scale with E1/4 and E1/2, respectively. The numerical results are consistent with these scalings.
Publisher
ELSEVIER SCIENCE BV
Issue Date
1994-06
Language
English
Article Type
Article
Citation

FLUID DYNAMICS RESEARCH, v.13, no.6, pp.317 - 327

ISSN
0169-5983
URI
http://hdl.handle.net/10203/67127
Appears in Collection
ME-Journal Papers(저널논문)
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