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Journal ArticleDOI

Inertial waves in a rotating annulus with inclined inner cylinder: comparing the spectrum of wave attractor frequency bands and the eigenspectrum in the limit of zero inclination

01 Jun 2013-Theoretical and Computational Fluid Dynamics (Springer-Verlag)-Vol. 27, Iss: 3, pp 397-413
TL;DR: In this paper, the authors investigate theoretically inertial waves inside a liquid confined between two co-rotating coaxial cylinders of finite length, and they consider the case of small viscosity and high angular velocity (i.e., small Ekman numbers).
Abstract: We investigate theoretically inertial waves inside a liquid confined between two co-rotating coaxial cylinders of finite length. We consider the case of small viscosity and high angular velocity (i.e., small Ekman numbers), a parameter range of interest for many geophysical applications. In this case, inertial waves propagating in the container show multiple reflections at the walls before the waves can be damped by weak diffusion. We allow for the inner cylinder wall to be parallel or inclined with respect to the annulus’ vector of rotation (truncated cone). For the limit of zero viscosity, the wave propagation is governed by a boundary value problem that is composed of a linear second-order hyperbolic partial differential equation and the impermeability boundary conditions. For the special case of vertical cylinder walls (no inclination of the inner cylinder), this boundary value problem is separable, the corresponding eigenmodes can analytically be found and they are regular. However, when the inner cylinder wall is inclined, the hyperbolicity of the governing equation leads to internal shear layers (corresponding to singularities for the inviscid case). The geometrical structure of the shear layers can be explained by inertial waves, trapped on limit cycles denoted as wave attractors. The shape of the limit cycles depends on the wave frequency. In fact, the spectrum of regular modes, existing for the case of vertical cylinder walls, vanishes almost completely when the inner wall is inclined. Instead of a spectrum of discrete frequencies and regular eigenmodes, a spectrum of wave attractor frequency bands and singular eigenmodes exist. The question addressed here is whether the spectrum of wave attractor intervals collapses to the discrete frequency spectrum when the inclination angle of the inner cylinder goes to zero. To answer this question, the attractor frequency intervals are evaluated numerically for a series of decreasing cylinder inclination angles and are compared with the analytically found eigenspectrum for the case of zero inclination. Goal is to better understand the asymptotic behavior of the problem for decreasing inclination angles. This understanding helps to interpret results from laboratory experiments with geometries that differ from the perfect annulus with parallel cylinder walls.
Citations
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Journal ArticleDOI
TL;DR: In this article, the authors investigated the mechanism of localized inertial wave excitation and its efficiency for an annular cavity rotating with. Meridional symmetry is broken by replacing the inner cylinder with a truncated cone (frustum). Waves are excited by individual longitudinal libration of the walls.
Abstract: The mechanism of localized inertial wave excitation and its efficiency is investigated for an annular cavity rotating with . Meridional symmetry is broken by replacing the inner cylinder with a truncated cone (frustum). Waves are excited by individual longitudinal libration of the walls. The geometry is non-separable and exhibits wave focusing and wave attractors. We investigated laboratory and numerical results for the Ekman number , inclination and libration amplitudes within the inertial wave band . Under the assumption that the inertial waves do not essentially affect the boundary-layer structure, we use classical boundary-layer analysis to study oscillating Ekman layers over a librating wall that is at an angle to the axis of rotation. The Ekman layer erupts at frequency , where is the effective Coriolis parameter in a plane tangential to the wall. For the selected inclination this eruption occurs for the forcing frequency . For the librating lids eruption occurs at . The study reveals that the frequency dependence of the total kinetic energy of the excited wave field is strongly connected to the square of the Ekman pumping velocity that, in the linear limit, becomes singular when the boundary layer erupts. This explains the frequency dependence of non-resonantly excited waves. By the localization of the forcing, the two configurations investigated, (i) frustum libration and (ii) lids together with outer cylinder in libration, can be clearly distinguished by their response spectra. Good agreement was found for the spatial structure of low-order wave attractors and periodic orbits (both characterized by a small number of reflections) in the frequency windows predicted by geometric ray tracing. For ‘resonant’ frequencies a significantly increased total bulk energy was found, while the energy in the boundary layer remained nearly constant. Inertial wave energy enters the bulk flow via corner beams, which are parallel to the characteristics of the underlying Poincare problem. Numerical simulations revealed a mismatch between the wall-parallel mass fluxes near the corners. This leads to boundary-layer eruption and the generation of inertial waves in the corners.

37 citations


Cites background from "Inertial waves in a rotating annulu..."

  • ...This rather shallow angle permits investigation of focusing reflections over a wide range of frequencies (cf. Borcia & Harlander 2012)....

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  • ...The geometry of the annular cavity suggests to write the dimensionless (2.2) and (2.3) in cylindrical coordinates (see Borcia & Harlander 2012, and references therein)....

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  • ...Symmetry permits us to consider only the (r, z)-plane, where it was shown by Borcia & Harlander (2012) that characteristics c± are described by c± = z± r √ 4 ω2 − 1....

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  • ...By fulfilling cp + cg = ±2Ω0/|k|, the waves show anomalous reflection from oblique boundaries (Phillips 1963; Maas 2001; Manders & Maas 2003; Harlander & Maas 2007b; Borcia & Harlander 2012)....

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Journal ArticleDOI
TL;DR: In this article, an experimental investigation of the flow induced in a rotating spherical shell is presented, where the velocity of the shell is measured by a zonal jet on the cylinder tangent to the inner sphere and parallel to the axis of rotation.

33 citations

Journal ArticleDOI
TL;DR: In this article, the influence of the libration amplitude and frequency on linear and nonlinear inertial waves in a spherical shell with a radius ratio of 2.5 on the Kalliroscope visualisation in a meridional laser plane and quantitative particle image velocimetry (PIV) data in a horizontal plane was analyzed.
Abstract: We experimentally study linear and nonlinear inertial waves in a spherical shell with a radius ratio of . The shell rotates with a mean angular velocity around its vertical axis. This rotation is overlaid by a time-periodic libration of the inner sphere in the range to excite inertial waves with a defined frequency. In the first part, we investigate linear inertial waves. The influence of the libration amplitude and the libration frequency on the waves and further the efficiency of the forcing to excite linear inertial waves will be discussed. For this, qualitative data from Kalliroscope visualisation in a meridional laser plane, as well as quantitative particle image velocimetry (PIV) data in a horizontal plane, have been analysed. A simple two-dimensional ray-tracing model is applied for the meridional plane to interpret the visualisations with respect to energy focusing and wave attractors. For sufficiently high/low libration amplitudes/frequencies, the Stewartson layer, a vertical shear layer tangential to the inner sphere’s equator, becomes unstable. This so-called ‘supercritical’ regime, where centrifugal and shear instabilities occur, allows for nonlinear wave coupling. PIV analyses in the horizontal laser plane in the corotating frame show low-frequency structures that correspond to Rossby-wave instabilities of the Stewartson layer. Some of these are travelling retrograde and are trapped near the Stewartson layer, others are travelling prograde filling the whole gap outside the Stewartson layer. Since libration can be viewed as a time-periodic variation of differential rotation, we assume that these two different structures are related to either the retrograde or the prograde phase of the libration cycle. The experimental results confirm theoretical, numerical as well as other experimental studies on Stewartson-layer instabilities.

26 citations


Cites background or methods or result from "Inertial waves in a rotating annulu..."

  • ...In spite of the present mean zonal flow, we found that the inertial wave shear layers are approximately straight lines, in accordance to findings e.g. by Tilgner (1999), Harlander & Maas (2006) or Borcia & Harlander (2013)....

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  • ...This method is common for hyperbolic boundary value problems (Maas 2001; Manders & Maas 2003; Harlander & Maas 2007a,b; Borcia & Harlander 2013)....

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  • ...Of special interest is the wave-reflection behaviour at inclined walls, which can be studied using simple ray models (Greenspan 1968; Tilgner 1999; Harlander & Maas 2006; Borcia & Harlander 2013; Koch et al. 2013)....

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  • ...The wave rays can be approximated by straight lines (Tilgner 1999; Harlander & Maas 2006; Borcia & Harlander 2013)....

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Proceedings ArticleDOI
01 Nov 2017
TL;DR: In this paper, the spectral element method is used to solve the Navier-Stokes equations in rotating fluid, with the non-slip boundary conditions at all rigid walls, and a prescribed vertical velocity field at the upper lid.
Abstract: Internal (inertial) waves in a uniformly stratified (rotating) fluid obey a highly specific dispersion relation that admits their propagation in form of oblique beams, which preserve their inclination to the distinguished direction (prescribed by gravity for internal waves and the angular velocity vector for the inertial waves) upon reflection In confined domains with sloping walls, repeated reflections of the wave beams lead to concentration of the wave energy at closed loops called wave attractors The dynamics of wave attractors is best studied in essentially two-dimensional problems (plane or axisymmetric), progressing from the ideal-fluid concept to more realistic ones, with consideration of viscous effects, energy balance and cascades of wave-wave interactions Development of fully three-dimensional highly nonlinear regimes has not yet been unexplored The present paper considers direct numerical simulations of inertial wave attractors in an axisymmetric rotating annulus having a trapezoidal cross section and a vertical axis of revolution The rotating fluid volume is confined between two vertical co-axial cylinders, with truncated cone as a bottom surface The large-scale forcing is applied to the fluid volume by specific motion of the upper lid The spectral element method (based on Nek5000 open solver) is used to solve the Navier-Stokes equations in rotating fluid, with the non-slip boundary conditions at all rigid walls, and a prescribed vertical velocity field at the upper lid We consider two types of forcing The first one simulates a small-amplitude nutation (Euler-disk-type motion) of the rigid lid, where the vector normal to the lid undergoes precession in such a way that the tip of the vector describes a horizontal circle of small radius around the axis of rotation of the annulus This motion is modelled by prescribing the vertical velocity field with cosine-shaped running wave in azimuthal direction and linear variation in the radial direction The response to such forcing mimics some essential features of tidal excitation We show that attractors are formed only when the sense of nutation in azimuthal direction (in rotating coordinate system) is opposite to the sense of the background rotation (in a fixed laboratory system) In a horizontal cross-section of the flow we see then a rotating pattern with `Yin-Yang' interplay in laminar mode, and when instability occurs with growth of the amplitude of external forcing, we see the interplay between the large- and small-scale `Yin-Yang' patterns The second type of forcing is purely axisymmetric At the upper lid we prescribe the vertical velocity profile in radial direction, with the amplitude in form of half-wave of the Bessel function, and simple harmonic time dependence Such forcing excites a purely axisymmetric motion in linear regime As the forcing increases, the axial symmetry of the inertial-wave motion is broken: in the horizontal cross-section we observe the development of fine-scale `Mandala' patterns possessing rotational symmetry whose complexity grow with time In both cases of forcing the triadic resonance is responsible for development of instability, and at sufficiently large forcing we observe a transition to three-dimensional wave turbulence We show thus for the first time that fully three-dimensional simulations are necessary to capture the essential features of nonlinear regimes in inertial wave attractors in a rotating fluid annulus

15 citations


Cites background from "Inertial waves in a rotating annulu..."

  • ...A reader interested in this subject is referred to recent papers on this subject [5]–[7], Figure 8....

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Journal ArticleDOI
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Journal ArticleDOI
07 Aug 1997-Nature
TL;DR: In this paper, it was shown that internal-wave attractors, rather than eigenmodes, determine the response of a confined, stably stratified fluid over a broad range of vibration frequencies.
Abstract: When a container of water is vibrated, its response can be described in terms of large-scale standing waves—the eigenmodes of the system. The belief that enclosed continuous media always possess eigenmodes is deeply rooted. Internal gravity waves in uniformly stratified fluids, however, present a counterexample. Such waves propagate at a fixed angle to the vertical that is determined solely by the forcing frequency, and a sloping side wall of the container will therefore act as a lens, resulting in ray convergence or divergence. An important consequence of this geometric focusing is the prediction1 that, following multiple reflections, these waves will evolve onto specific paths—or attractors—whose locations are determined only by the frequency. Here we report the results of laboratory experiments that confirm that internal-wave attractors, rather than eigenmodes, determine the response of a confined, stably stratified fluid over a broad range of vibration frequencies. The existence of such attractors could be important for mixing processes in ocean basins and lakes, and may be useful for analysing oscillations of the Earth's liquid core and the stability of spinning, fluid-filled spacecraft.

200 citations