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2000, Theoretical and Computational Fluid Dynamics
The effects of Rossby wave-turbulence interactions on particle dispersion are investigated in a Lagrangian analysis of the potential vorticity equation. The analysis produces several exact statistical results for fluid particle dispersion in barotropic turbulence on a β-plane. In the inviscid problem the first integral time scale of the meridional velocity is found to be zero, as might occur in pure wave processes, and the meridional particle dispersion is bounded. The second integral time scale, which determines the magnitude of the bound, is shown to depend explicitly on β, the enstrophy and the energy of the meridional velocity. Expressions relating the autocorrelation of the vorticity to the autocorrelation of the meridional velocity are derived and the Lagrangian integral time scale of the relative vorticity is diagnostically related to the meridional velocity correlation. The applicability of these predictions is verified in a series of numerical simulations. For a range of β values, the meridional extent of quasisteady alternating zonally averaged jets occurring in the numerical solutions scales with a length scale given by the the standard deviation of the meridional particle dispersion.
Physical review letters, 2004
The dynamics of passive Lagrangian tracers in three-dimensional quasigeostrophic turbulence is studied numerically and compared with the behavior of two-dimensional barotropic turbulence. Despite the different Eulerian properties of the two flows, the Lagrangian dynamics of passively advected tracers in three-dimensional quasigeostrophic turbulence is very similar to that of barotropic turbulence. In both systems, coherent vortices play a major role in determining the mixing and dispersion properties. This work indicates that recent results on particle dynamics in barotropic, two-dimensional turbulence carry over to more realistic baroclinic flows, such as those encountered in the large-scale dynamics of the atmosphere and ocean.
1984
The theory of homogeneous barotropic beta-plane turbulence is here extended to include effects arising from spatial inhomogeneity in the form of a zonal shear flow. Attention is restricted to the geophysically important case of zonal flows that are barotropically stable and are of larger scale than the resulting transient eddy field. Because of the presumed scale separation, the disturbance enstrophy is approximately conserved in a fully nonlinear sense, and the (nonlinear) w a v e mean-flow interaction may be characterized as a shear-induced spectral transfer of disturbance enstrophy along lines of constant zonal wavenumber k. In this transfer the disturbance energy is generally not conserved. The nonlinear interactions between different disturbance components are turbulent for scales smaller than the inverse of Rhines's cascade-arrest scale K~ = (/3,,/2u,,,)~, and in this regime their leading-order effect may be characterized as a tendency to spread the enstrophy (and energy) along contours of constant total wavenumber K = (k2+Z2)4. Insofar as this process of turbulent isotropization involves spectral transfer of disturbance enstrophy across lines of constant zonal wavenumber k, it can be readily distinguished from the shear-induced transfer which proceeds along them. However, an analysis in terms of total wavenumber K alone, which would be justified if the flow were homogeneous, would tend to mask the differences. The foregoing theoretical ideas are tested by performing direct numerical simulation experiments. It is found that the picture of classical beta-plane turbulence is altered, through the effect of the large-scale zonal flow, in the following ways: (i) while the turbulence is still confined to K > K~, the disturbance field penetrates to the largest scales of motion; (ii) the larger disturbance scales K < K~ exhibit a tendency to meridional rather than zonal anisotropy, namely towards w2 > u2 rather than vice versa; (iii) the initial spectral transfer rate away from an isotropic intermediate-scale source is significantly enhanced by the shear-induced transfer associated with straining by the zonal flow. This last effect occurs even when the large-scale shear appears weak to the energy-containing eddies, in the sense that dU/dy 4 K U , , , for typical eddy length and velocity scales. TUNQ, K. K. 1983 Initial-value problems for Rossby waves in a shear flow with critical level.
Dynamics of Atmospheres and Oceans, 1992
Interaction of a zonal jet and small-amplitude Rossby-wave turbulence is studied within the framework of the barotropic r-plane model. It is demonstrated that turbulent-laminar interaction in this case transfers energy from the wave turbulence to the laminar flow (the effect of negative friction). We derive a conclusion that, as the geophysical turbulence is determined partly by wave turbulence and none of the traditional heuristic models can adequately describe the effect of negative friction associated with wave turbulence, the application of these models to the 'real' ocean and atmosphere is unreliable. It is also demonstrated that, as they are affected by the turbulence, all westward jets slowly expand without strengthening. Each jet has a core, within the limits of which the velocity of the fluid is constant. In some cases, the core expands faster than the jet periphery, resulting in jumps on the profile of the flow. All eastward jets are steady irrespective of their profiles.
Physics of Fluids, 2003
The governing equations of a surface wave field and a coexisting roll-streak circulation typical of Langmuir circulations or submesoscale frontal circulations are derived to better describe their two-way interactions. The gradients and vertical velocities of the roll-streak circulation induce wave refraction, amplitude modulation and higher-order waves. These changes then produce wave-wave nonlinear forces and divergence of the wave-induced mass transport, both of which in turn affect the circulation. To accurately represent these processes, both a wave theory and a wave-averaged theory are developed without relying on any extrapolation, any spatiotemporal mapping or an approximation that treats the wave-induced mass divergence as being concentrated at the surface. This wave theory finds seven types of current-induced higher-order wave motions. It also determines the wave dynamics such as the governing equation of the wave action density valid in the presence of the complex circulation. The evolution of the wave action density is clearly affected by the upwelling or downwelling. The new wave-averaged theory presents the governing equations of the wave-averaged circulation which satisfies the wave-averaged mass conservation. This circulation is different from the circulation considered to satisfy the mass conservation in the Craik-Leibovich theory, and the difference becomes critical when the wave field evolves due to refraction. In this case, compared to the Craik-Leibovich theory, long waves are more important and also the rolls are more weakly forced.
Journal of Fluid Mechanics, 2001
We investigate the performance of standard stochastic models of single-particle dispersion in two-dimensional turbulence. Owing to the presence of coherent vortices, particle dispersion in two-dimensional turbulence is characterized by a non-Gaussian velocity distribution and a non-exponential velocity autocorrelation, and it cannot be properly captured by either linear or nonlinear stochastic models with a single component process. Based on physical and dynamical considerations, we introduce a family of two-process stochastic models that provide a better parameterization of turbulent dispersion in rotating barotropic flows.
Nonlinear Processes in Geophysics
We study numerically the comparison between Lagrangian experiments on turbulent particle dispersion in 2-D turbulent flows performed, on the one hand, on the basis of direct numerical simulations (DNS) and, on the other hand, using kinematic simulations (KS). Eulerian space-time structure of both DNS and KS dynamics are not comparable, mostly due to the absence of strong coherent vortices and advection processes in the KS fields. The comparison allows to refine past studies about the contribution of nonhomogeneous space-time 2-D Eulerian structure on the turbulent absolute and relative particle dispersion processes. We particularly focus our discussion on the Richardson's regime for relative dispersion.
International Journal of Multiphase Flow, 2000
A physical model for the dynamics of a dispersion of solid spherical particles in an incompressible viscous¯uid is outlined and used to calculate the turbulence modulation in a stationary, homogeneous and isotropic turbulent¯ow with particles. Starting from a postulated¯uid turbulence spectrum in the absence of particles, the physical model predicts the corresponding¯uid turbulence spectrum in the presence of particles and the particles turbulence spectrum as function of frequency and wavenumber. There are two versions of the model. The ®rst one uses a point-force approximation for the particles and takes into account the hydrodynamic interaction between the particles. The second version accounts for the detailed¯ow around the (®nite-diameter) particles, but does not consider their hydrodynamic interaction. The spectra, calculated with the two versions, are used to determine the turbulence intensity of the¯uid and particles as function of three relevant dimensionless groups. It is found that in general the dierences between the results of the point-particle model and the ®nite-diameter-particle model are signi®cant. So one has to be careful with point-particle models. The eect of the hydrodynamic interaction between the particles is up to a volume fraction of 0.1 still mostly negligible.
Physical Review E, 1998
We numerically study the time evolution of coherent vortices in decaying turbulence described by the Charney-Hasegawa-Mima equation with the weak dissipation. Self-organized coherent vortices develop through the mutual advection and the vortex merging. The dimensional analysis provides the dynamical scaling law of structure function of the potential vorticity field S(k,t)ϭE 5/4 1/2 t 1/2 G"k/ k(t)… ͓ k(t)ϳE Ϫ1/8 3/4 t Ϫ1/4 ͔ with a scaling function G(x), which turns out to be in good agreement with numerical experiments. In physical space, quantities related to coherent vortices develop algebraically with time. The dimensional analysis predicts that the total number N of vortices decreases as Nϳt Ϫ with exponent ϭ1/2. Moreover, it is found that the remarkable feature of this system is the approximate conservation of the area of the coherent region in the potential vorticity field. ͓S1063-651X͑98͒01802-9͔
Physical Review E, 2004
The influence of Eulerian and Lagrangian scales on the turbulent relative dispersion is investigated through a three-dimensional Eulerian consistent Lagrangian stochastic model. As a general property of this class of models, it is found to depend solely on a parameter  based on the Kolmogorov constants C K and C 0. This parameter represents the ratio between the Lagrangian and Eulerian scales and is related to the intrinsic inhomogeneity of the relative dispersion process. In particular, the quantity g*ϭg/C 0 ͑where g is the Richardson constant͒ and the temporal extension of the t 3 regime are found to be strongly dependent on the value adopted for .
Physics of Fluids, 2000
We study the statistical properties of the velocity and velocity gradient distributions in barotropic turbulence. At large enough Reynolds number, the velocity distribution becomes non-Gaussian outside the vortex cores, and its characteristics are completely determined by the properties of the far field induced by the coherent vortices. The velocity gradients are always non-Gaussian inside coherent vortices, due to the spatial velocity correlations associated with the ordered flow in the vortex cores, and become non-Gaussian also in the background turbulence at large enough Reynolds number.
Physics of Fluids, 2005
The statistical geometry of dispersing Lagrangian clusters of four particles (tetrahedra) is studied by means of high-resolution direct numerical simulations of three-dimensional homogeneous isotropic turbulence. We give the first evidence of a self-similar regime of shape dynamics characterized by almost two-dimensional, strongly elongated geometries. The analysis of four-point velocity-difference statistics and orientation shows that inertial-range eddies typically generate a straining field with a strong extensional component aligned with the elongation direction and weak extensional/compressional components in the orthogonal plane.
Journal Homepage: http://pof.aip.org/ Journal Information: http://pof.aip.org/about/about_the_journal Top downloads: http://pof.aip.org/features/most_downloaded Information for Authors: http://pof.aip.org/authors Downloaded 22 Jul 2013 to 143.215.126.126. This article is copyrighted as indicated in the abstract. Reuse of AIP content is subject to the terms at: http://pof.aip.org/about/rights_and_permissions A wide range of relative two-particle dispersion statistics from the Lagrangian Kinematic Simulation KS model, which contains turbulent-like flow structures, compares well with Yeung's Phys. Fluids 6, 3416 1994 DNS results. In particular, the Lagrangian flatness factor 4 (t) compares excellently better than Heppe's J. Fluid Mech. 357, 167 1998 nonlinear stochastic model. For higher Reynolds numbers the results from KS show that 4 (t) is significantly greater than 3 over a wide range of times within the inertial range of time scales.
ESAIM: Proceedings, 1996
A wide parameter space is spanned to check the in uence of numerical parameters on selforganized jets in rotating, turbulent shallow-water ows. It is found that, even in harsh physical (strongly ageostrophic) and numerical (ltered, hyperviscous, high-resolution) environments, the basic morphogenesis of steady jets, qualitatively re ecting the Rhines scale, is robust. However, detailed features of the jet pattern, such as the amplitude, the width, and the location can be substantially a ected by n umerical parameters for a xed set of physical parameters. In general, while the amount of energy lost seems to be a good predictor of maximum jet amplitude and width, a nonmonotonic dependence of these features on the numerical parameters is observed. The most acute sensitivity is associated with the use of a r 16 hyperdissipation operator in conjunction with a Robert-Asselin lter, which leads to substantial meridional shifts of the entire jet pattern as the viscosity coe cient i s v aried.
Physical Review Fluids, 2018
We present models for single-particle dispersion in vertical and horizontal directions of stably stratified flows. The model in the vertical direction is based on the observed Lagrangian spectrum of the vertical velocity, while the model in the horizontal direction is a combination of a continuoustime eddy-constrained random walk process with a contribution to transport from horizontal winds. Transport at times larger than the Lagrangian turnover time is not universal and dependent on these winds. The models yield results in good agreement with direct numerical simulations of stratified turbulence, for which single-particle dispersion differs from the well studied case of homogeneous and isotropic turbulence.
International Journal of Multiphase Flow, 2005
Comparisons are made between the Advection-Diffusion Equation (ADE) approach for particle transport and the two-fluid model approach based on the PDF method. In principle, the ADE approach offers a much simpler way of calculating the inertial deposition of particles in a turbulent boundary layer than that based on the PDF approach. However the ADE equations that have recently been used are only strictly valid for a simple Gaussian process when particle inertia is small. Using a prescribed, but in general non-Gaussian random particle velocity field, it is shown that the net particle mass flux contains a drift term in addition to that from the mean velocity of the particle velocity field, associated with the compressibility of the velocity field. Furthermore the diffusive flux in general depends not only upon the gradient of the mean concentration (true only for a Gaussian random flow field) but also upon higher order derivatives whose relative contribution depends on diffusion coefficients D ijk. . . etc. These coefficients depend upon the statistical moments associated with random displacements and compressibility of the particle flow field along particle trajectories which in turn depend upon particle inertia. In contrast the PDF approach offers the advantage of using a simple gradient (Gaussian) approximation in particle phase space which can lead to a non-Gaussian spatial dispersion process when particle inertia is important. Conditions based on the particle mean free path are derived for which a simple ADE is appropriate. Some of the features of particle transport in an inhomogeneous turbulent flow are illustrated by examining particle dispersion in a random flow field composed of pairs of counter rotating vortices which has an rms velocity which increase linearly from a stagnation point.
Physical Review E, 2012
In this paper we present a new model for modeling the diffusion and relative dispersion of particles in homogeneous isotropic turbulence. We use an Heisenberg-like Hamiltonian to incorporate spatial correlations between fluid particles, which are modeled by stochastic processes correlated in time.
Nonlinear Processes in Geophysics, 2007
We study numerically the comparison between Lagrangian experiments on turbulent particle dispersion in 2-D turbulent flows performed, on the one hand, on the basis of direct numerical simulations (DNS) and, on the other hand, using kinematic simulations (KS). Eulerian space-time structure of both DNS and KS dynamics are not comparable, mostly due to the absence of strong coherent vortices and advection processes in the KS fields. The comparison allows to refine past studies about the contribution of nonhomogeneous space-time 2-D Eulerian structure on the turbulent absolute and relative particle dispersion processes. We particularly focus our discussion on the Richardson's regime for relative dispersion.
Physics of Fluids, 2004
A beta-plane approximation of the two-dimensional quasigeostrophic model describes a single layer ͑barotropic͒ fluid subjected to a latitudinally varying Coriolis parameter or topography. Rhines ͑1975͒ initiated the study of beta-plane turbulence. He predicted the inverse energy cascade into predominantly zonal modes, hence an array of eastward-westward jets, and estimated the jet number ͑celebrated Rhines scale͒. He also proposed a k Ϫ5 scaling law of zonal energy spectra. Our paper reexamines scaling, spectra, and zonal structure of beta-plane turbulence, based on theoretical predictions and numeric experiments. We show that the inverse cascade gives rise to strong organized zonal jets that evolve a peculiar frontal-band ͑''saw-tooth''͒ vorticity profile. Such structure affects all spectral properties of the system, by creating organized sequences of spectral peaks, and thus confounds any putative ''scaling behavior.'' The frontal-band structure appears consistently in all stochastically forced beta-plane flows, independent of dissipation and/or other details. But the resulting turbulent quasiequilibrium is not unique, its gross parameters ͑jets number, mean vorticity gradient͒ retain memory of the initial state and/or history.
Journal of the Atmospheric Sciences, 2011
The eddy-driven jet is located in the midlatitudes, bounded on one side by the pole and often bounded on the opposite side by a strong Hadley-driven jet. This work explores how the eddy-driven jet and its variability persist within these limits. It is demonstrated in a barotropic model that as the jet is located at higher latitudes, the eddy length scale increases as predicted by spherical Rossby wave theory, and the leading mode of variability of the jet changes from a meridional shift to a pulse. Looking equatorward, a similar change in eddy-driven jet variability is observed when it is moved equatorward toward a constant subtropical jet. In both the poleward and equatorward limits, the change in variability from a shift to a pulse is due to the modulation of eddy propagation and momentum flux. Near the pole, the small value of beta (the meridional gradient of absolute vorticity) and subsequent lack of wave breaking near the pole account for the change in variability, whereas on t...
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