TY - GEN A1 - Ghasemi, Abouzar A1 - Klein, Marten A1 - Harlander, Uwe A1 - Kurgansky, Michael V. A1 - Schaller, Eberhard A1 - Will, Andreas T1 - Mean flow generation by Görtler vortices in a rotating annulus with librating side walls T2 - Physics of Fluids N2 - Time periodic variation of the rotation rate of an annulus induces in supercritical regime an unstable Stokes boundary layer over the cylinder side walls, generating Görtler vortices in a portion of a libration cycle as a discrete event. Numerical results show that these vortices propagate into the fluid bulk and generate an azimuthal mean flow. Direct numerical simulations of the fluid flow in an annular container with librating outer (inner) cylinder side wall and Reynolds-averaged Navier–Stokes (RANS) equations as diagnostic equations are used to investigate generation mechanism of the retrograde (prograde) azimuthal mean flow in the bulk. First, we explain, phenomenologically, how absolute angular momentum of the bulk flow is mixed and changed due to the propagation of the Görtler vortices, causing a new vortex of basin size. Then we investigate the RANS equations for intermediate time scale of the development of the Görtler vortices and for long time scale of the order of several libration periods. The former exhibits sign selection of the azimuthal mean flow. Investigating the latter, we predict that the azimuthal mean flow is proportional to the libration amplitude squared and to the inverse square root of the Ekman number and libration frequency and then confirms this using the numerical data. Additionally, presence of an upscale cascade of energy is shown, using the kinetic energy budget of fluctuating flow. KW - Direct Numerical Simulation KW - Fluid Mechanics KW - Mean Flow KW - Rotation KW - Cylinder KW - Centrifugal KW - Instability KW - Mechanism KW - Vortex Y1 - 2016 U6 - https://doi.org/10.1063/1.4948406 VL - 28 IS - 056603 SP - 1 EP - 23 ER - TY - THES A1 - Ghasemi, Abouzar T1 - Mean flow generation mechanisms in a rotating annular container with librating walls N2 - The current work aims to contribute to our understanding of mean flow generation mechanisms in rotating fluids. The focus is on the mean flow generation mechanisms by: 1) centrifugally unstable Görtler vortices and 2) resonant excitation of inertial waves in a stable regime. Direct numerical simulations (DNS) of the fluid flow in a rotating annular container with longitudinally librating walls are used to investigate the mechanisms. Longitudinal libration of the cylinder side walls of an annulus induces in supercritical regime an unstable Stokes boundary layer which generates Görtler vortices in a portion of a libration cycle, as a discrete event. DNS results show that these vortices propagate into the fluid bulk and generate an azimuthal mean flow. Reynolds-averaged Navier–Stokes (RANS) equations are used as a diagnostic tool to investigate generation mechanism of the azimuthal mean flow in the bulk. First, we explain, phenomenologically, how absolute angular momentum of the bulk flow is mixed and changed due to the propagation of the Görtler vortices, causing a new vortex of basin scale size. Then we investigate the RANS equations for an intermediate time scale of the development of the Görtler vortices, and for a long time scale of the order of several libration periods. The former exhibits sign selection of the azimuthal mean flow. Investigating the latter, we predict that the azimuthal mean flow is proportional to the libration amplitude squared and to the inverse square root of the Ekman number and libration frequency. We confirm this using the numerical data. Additionally, the presence of an upscale cascade of energy is shown, using the kinetic energy budget of fluctuating flow. In the second part of the current study, we investigate the mean flow generation mechanism by intrinsic nonlinearity of the inertial wave beams and normal modes in a rotating annular cavity with longitudinally librating top and bottom lids in a stable regime. We confirm the generation of progressive inertial waves as localized shear layer and normal modes as standing waves at and close to the resonance frequencies. We focus on the low order inertial normal modes. Using the DNS results, we show that when the low order normal modes are excited, a non-geostrophic azimuthal mean flow is generated in the bulk. Following Tilgner (2007) and using analytical and DNS solutions, we identify the source terms responsible for the generation of the azimuthal mean flow. We show that the helical property of the inertial waves and normal modes causes the source terms. Using the analytical solution, we separate the inertial wave beams from the DNS solution. We show that at and close to the resonance frequency, libration phase of the normal modes is always following that of the inertial wave beam, and their phase lag depends on the libration frequency. Analogy to classical mechanics is commented. The generation efficiency of the mean flow is discussed with respect to the phase lag. Additionally, we address wave-wave and wave-boundary layer interactions, and dependency of the mean flow on the dimensionless parameters. We show that the results obtained are valid for small inclination of the inner cylinder side wall. KW - Fluid Mechanics KW - Rotation KW - Coriolis Force KW - Inertial Wave KW - Centrifugal KW - Instability KW - Direct Numerical Simulation KW - Geophysical Fluid Dynamics Y1 - 2016 PB - Brandenburgische Techn. Univ. CY - Cottbus ER -