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Research Papers: Fundamental Issues and Canonical Flows

A Numerical Investigation on the Onset of the Various Flow Regimes in a Spherical Annulus

[+] Author and Article Information
Lalaoua Adel

Laboratory of Thermodynamic and
Energetic Systems,
Faculty of Physics,
USTHB,
Bab Ezzouar 16111, Algeria
e-mail: lalaouaadel@gmail.com

Bouabdallah Ahcene

Laboratory of Thermodynamic and
Energetic Systems,
Faculty of Physics,
USTHB,
Bab Ezzouar 16111, Algeria
e-mail: bouabdallah.usthb@gmail.com

Contributed by the Fluids Engineering Division of ASME for publication in the JOURNAL OF FLUIDS ENGINEERING. Manuscript received June 20, 2015; final manuscript received April 13, 2016; published online July 15, 2016. Assoc. Editor: Samuel Paolucci.

J. Fluids Eng 138(11), 111201 (Jul 15, 2016) (11 pages) Paper No: FE-15-1414; doi: 10.1115/1.4033489 History: Received June 20, 2015; Revised April 13, 2016

The spherical Couette system, consisting of the flow in the annular gap between two concentric rotating spheres, is a convenient problem for studying the laminar–turbulent transition. Many of the transitional phenomena encountered in this flow are of fundamental relevance for the understanding of global processes in the planetary atmospheres as well as in astrophysical and geophysical motions. Furthermore, the study of spherical Couette flow (SCF) is of basic importance in the field of hydrodynamic stability. This paper focuses principally on the numerical prediction of various transitions between flow regimes in a confined spherical gap between a rotating inner sphere and a fixed outer spherical shell. The finite-volume-based computational fluid dynamics, FLUENT software package, is adopted to investigate numerically the flow of a viscous incompressible fluid in the closed spherical gap. Two important dimensionless parameters completely define the flow regimes: the Reynolds number, Re = 1R12/ν, for the rotation of the inner sphere and the gap width, β = (R2 − R1)/R1 = 0.1, for the geometry. The numerical calculations are carried out over a range of Reynolds number from two until 60,000. The numerical results are compared with the experimental data available in the literature, and the agreement between the two approaches is very good. The laminar–turbulent transition, the onset of different instabilities, the formation mechanisms of various structures, and the flow behavior are examined and described in detail by the pressure field, meridional streamlines, circumferential velocity, and skin friction coefficient. In addition, the velocity time series and the corresponding power spectral density are considered and analyzed over a large range of Reynolds number. Three kinds of fundamental frequencies expressed by F0, F1, and F2 are obtained corresponding to the spiral mode associated with the wavy mode (SM + WM), the wavy mode (WVF), and the chaotic fluctuation (CF), respectively. However, no sharp fundamental frequency components are observed for the turbulent regime.

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Figures

Grahic Jump Location
Fig. 1

Spherical coordinate system

Grahic Jump Location
Fig. 3

Convergence studies on the profile of circumferential velocity at Re = 60,000 and θ = π/2

Grahic Jump Location
Fig. 4

Successive transitions to turbulent flow in the spherical Couette system/static pressure distribution

Grahic Jump Location
Fig. 5

Meridional streamlines of narrow gap-size SCF in (r, θ) plane

Grahic Jump Location
Fig. 6

Laminar turbulent transition/evolution of the skin friction coefficient for different Reynolds numbers

Grahic Jump Location
Fig. 7

Dimensionless circumferential velocity distributions versus Reynolds numbers

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