Spectral solution of the Navier-Stokes equations for rotating flows (Q2737511)

From MaRDI portal





scientific article; zbMATH DE number 1645709
Language Label Description Also known as
English
Spectral solution of the Navier-Stokes equations for rotating flows
scientific article; zbMATH DE number 1645709

    Statements

    0 references
    0 references
    0 references
    0 references
    18 June 2002
    0 references
    Navier-Stokes equations
    0 references
    Ekman layer
    0 references
    Bödewadt layer
    0 references
    direct numerical simulation
    0 references
    three-dimensional Chebyshev-Fourier collocation method
    0 references
    projection scheme
    0 references
    cylindrical domains
    0 references
    forced throughflow
    0 references
    rotating cavity
    0 references
    rotor-stator cavity
    0 references
    perturbations
    0 references
    instabilities
    0 references
    Spectral solution of the Navier-Stokes equations for rotating flows (English)
    0 references
    Direct numerical simulation by spectral methods are used to study the instabilities in Ekman and Bödewadt layers at the transition to time-dependent regimes. The physical phenomena are characteristic of rotating flows with walls, and the cavities possess elementary geometries that are relevant to turbine applications and to typical configurations studied in fundamental investigations and in experiments. The three-dimensional Chebyshev-Fourier collocation method is based on a projection scheme to solve the coupled equations for velocity and pressure. The method developed earlier for annular domains is extended to fully cylindrical domains with an axis of rotation. A special development is required to deal with singular behaviour of coefficients when the radius tends to zero. The investigation is carried out for two generic configurations: forced throughflow in a rotating cavity, and the confined flow driven by differential rotation inside a rotor-stator cavity. Depending on the aspect ratio and on Reynolds number, counter-rotating rolls can superimpose spiral structures on the boundary layer near the disks. The characteristic parameters of perturbations (wavelength, frequency, phase velocity, inclination of the spiral) are shown to be relevant to instabilities in rotating flows.
    0 references
    0 references

    Identifiers

    0 references
    0 references
    0 references
    0 references
    0 references