scholarly journals The non-equilibrium region of grid-generated decaying turbulence

2014 ◽  
Vol 744 ◽  
pp. 5-37 ◽  
Author(s):  
P. C. Valente ◽  
J. C. Vassilicos

AbstractThe previously reported non-equilibrium dissipation law is investigated in turbulent flows generated by various regular and fractal square grids. The flows are documented in terms of various turbulent profiles which reveal their differences. In spite of significant inhomogeneity and anisotropy differences, the new non-equilibrium dissipation law is observed in all of these flows. Various transverse and longitudinal integral scales are measured and used to define the dissipation coefficient $C_{\varepsilon }$. It is found that the new non-equilibrium dissipation law is not an artefact of a particular choice of the integral scale and that the usual equilibrium dissipation law can actually coexist with the non-equilibrium law in different regions of the same flow.

2016 ◽  
Vol 23 (6) ◽  
pp. 407-417
Author(s):  
Manuel Tijera ◽  
Gregorio Maqueda ◽  
Carlos Yagüe

Abstract. In this work the relation between integral scale and fractal dimension and the type of stratification in fully developed turbulence is analyzed. The integral scale corresponds to that in which energy from larger scales is incoming into a turbulent regime. One of the aims of this study is the understanding of the relation between the integral scale and the bulk Richardson number, which is one of the most widely used indicators of stability close to the ground in atmospheric studies. This parameter will allow us to verify the influence of the degree of stratification over the integral scale of the turbulent flows in the atmospheric boundary layer (ABL). The influence of the diurnal and night cycles on the relationship between the fractal dimension and integral scale is also analyzed. The fractal dimension of wind components is a turbulent flow characteristic, as has been shown in previous works, where its relation to stability was highlighted. Fractal dimension and integral scale of the horizontal (u′) and vertical (w′) velocity fluctuations have been calculated using the mean wind direction as a framework. The scales are obtained using sonic anemometer data from three elevations 5.8, 13 and 32 m above the ground measured during the SABLES 98 field campaign (Cuxart et al., 2000). In order to estimate the integral scales, a method that combines the normalized autocorrelation function and the best Gaussian fit (R2 ≥  0.70) has been developed. Finally, by comparing, at the same height, the scales of u′ and w′ velocity components, it is found that the turbulent flows are almost always anisotropic.


2016 ◽  
Author(s):  
M. Tijera ◽  
G. Maqueda ◽  
C. Yagüe

Abstract. In this work the relation between integral scale and fractal dimension and the type of stratification in fully developed turbulence is analyzed. Integral scale corresponds to that in which energy from larger scales is incoming into turbulent regime. One of the aims of this study is the understanding of the relation between the integral scale and the Bulk Richardson number, which is one the most widely used indicators of stability close to the ground in atmospheric studies. This parameter will allow us to verify the influence of the degree of stratification over the integral scale of the turbulent flows in the Atmospheric Boundary Layer (ABL). The influence of the diurnal and night cycle in the relationship between the fractal dimension and integral scale is also analyzed. Fractal dimension of wind components is a turbulent flow characteristic as it has been shown in previous works, where its relation to stability was highlighted. Fractal dimension and integral scale of the horizontal (u') and vertical (w') velocity fluctuations have been calculated using the mean wind direction as framework. The scales are obtained using sonic anemometer data from three elevations 5.8 m, 13 m and 32 m above the ground measured during the SABLES-98 field campaign. In order to estimate the integral scales a method that combines the normalized autocorrelation function and the best gaussian fit (R2 ≥ 0.70) has been developed. Finally, by comparing, at the same height, the scales of u' and w' velocity components it is found that almost always the turbulent flows are anisotropic.


2002 ◽  
Vol 459 ◽  
pp. 429-443 ◽  
Author(s):  
HONGLU WANG ◽  
WILLIAM K. GEORGE

A simple spectral model is used to examine what is required to determine the energy and integral scale in homogeneous isotropic turbulence. The problem is that these are determined in part by the largest scales of the turbulence which are either not simulated at all by DNS or experiments, or cannot be estimated because of an insufficient statistical sample. The absence of scales an order of magnitude below the peak in the energy spectrum is shown to affect the determination significantly. Since this energy peak shifts to lower wavenumbers as the flow evolves, the problem becomes progressively worse during decay. It is suggested that almost all reported integral scales for isotropic decaying turbulence are questionable, and that the power laws fitted to them are seriously in error. Approximate correction using the spectral model shows that recent DNS data which decay as u2 ∝ tn with constant n, are also consistent with L ∝ t1/2.


Author(s):  
Yoshifumi Ogami ◽  
Kazuie Nishiwaki ◽  
Yoshinobu Yoshihara

First, a simple and accurate numerical method is presented to produce velocity fluctuations that are determined by the prescribed physical quantities and qualities of turbulence such as longitudinal and lateral spectra, and integral scales. The fluctuations are obtained by solving a system of nonlinear equations that are derived from the equations of energy spectra and of root mean square of the fluctuations. This method requires as many computer memories and computations as one-dimensional case even for the three dimensional calculations. It is shown that there is a strong resemblance of the simulated velocity fluctuations and experimental data. The energy spectra of these velocity fluctuations are quite accurate with less than 0.01% relative errors to the prescribed spectra. Secondly, these solutions are used to examine the capability of the vortex methods to produce turbulent flows with the prescribed parameters. It is found that although the energy spectra by the vortex method scatter to some extent, they are distributed along the prescribed spectra. It can be said that the vortex methods are able to simulate the target turbulence fairly well. Also it is found that the solutions with the LES model increase and deviate from the target spectrum at the higher frequency regions. This may suggest the nonessentiality of the LES model for the vortex method.


1966 ◽  
Vol 25 (1) ◽  
pp. 97-120 ◽  
Author(s):  
W. G. Rose

An approximately homogeneous turbulent shear flow is generated in an open-return wind tunnel test-section by a plane parallel-rod grid of uniform rod diameter and non-uniform rod spacing. The grid design is based upon an analysis by Owen & Zienkiewicz (1957). Hot-wire measurements taken in this flow include mean velocities, component turbulence intensities, shear and two-point space correlations, and energy spectra. In addition, microscales, obtained both from instantaneous time derivatives of the hot-wire signal and from two-point space correlations, and integral scales, calculated both from correlations and energy spectra, are reported.Based upon these results, it is concluded that, far enough away from the grid and the test-section wall boundary layers:The turbulence intensities are maintained at uniform values by the nearly constant mean shear.The turbulent shear stress approaches an asymptotic value.Measured two-point space correlation coefficients and one-dimensional energy spectra attain self-preserving forms.When distance downstream of the grid is measured in terms of the number of ‘local’ grid rod spacings, (see discussion of microscales obtained from time derivatives), the Taylor microscale defined by the correlation coefficientRuu(rX, 0, 0) grows linearly with this ‘effective’ distance over most of the region measured.The limited number of integral scale determinations and experimental uncertainty allow only the statements that the magnitude of the longitudinal scale is roughly one-eighth the lateral dimension of the square test-section and tends to increase slightly with ‘effective’ distance from the grid.The lateral integral scales are approximately one-half the longitudinal scales and also increases with distance from the grid.The integral scale which characterizes the size of the eddy primarily responsible for momentum transfer is roughly one-tenth the test-section lateral dimension (measured at one point only).


Author(s):  
Yoshifumi Ogami

The energy spectra produced by the vortex method are studied. The strengths of the vortices are determined so that the energy spectra correspond to the given target spectra for two different integral scales. Velocity fluctuations produced by the simulation of vortex shear layer are obtained and energy spectra of these fluctuations are examined. It is found that in the case of the larger integral scale, the spectra almost agree with the target in the range up to the cut-off wave length, and that in the case of the smaller scale, the deviation of the spectra from the target is quite large.


2003 ◽  
Vol 56 (6) ◽  
pp. 615-632 ◽  
Author(s):  
RA Antonia ◽  
P Orlandi

Previous reviews of the behavior of passive scalars which are convected and mixed by turbulent flows have focused primarily on the case when the Prandtl number Pr, or more generally, the Schmidt number Sc is around 1. The present review considers the extra effects which arise when Sc differs from 1. It focuses mainly on information obtained from direct numerical simulations of homogeneous isotropic turbulence which either decays or is maintained in steady state. The first case is of interest since it has attracted significant theoretical attention and can be related to decaying turbulence downstream of a grid. Topics covered in the review include spectra and structure functions of the scalar, the topology and isotropy of the small-scale scalar field, as well as the correlation between the fluctuating rate of strain and the scalar dissipation rate. In each case, the emphasis is on the dependence with respect to Sc. There are as yet unexplained differences between results on forced and unforced simulations of homogeneous isotropic turbulence. There are 144 references cited in this review article.


2012 ◽  
Vol 706 ◽  
pp. 150-172 ◽  
Author(s):  
P. A. Davidson ◽  
N. Okamoto ◽  
Y. Kaneda

AbstractWe consider freely decaying, anisotropic, statistically axisymmetric, Saffman turbulence in which $E(k\ensuremath{\rightarrow} 0)\ensuremath{\sim} {k}^{2} $, where $E$ is the energy spectrum and $k$ the wavenumber. We note that such turbulence possesses two statistical invariants which are related to the form of the spectral tensor ${\Phi }_{ij} (\mathbi{k})$ at small $k$. These are ${M}_{\parallel } = {\Phi }_{\parallel } ({k}_{\parallel } = 0, {k}_{\perp } \ensuremath{\rightarrow} 0)$ and ${M}_{\perp } = 2{\Phi }_{\perp } ({k}_{\parallel } = 0, {k}_{\perp } \ensuremath{\rightarrow} 0)$, where the subscripts $\parallel $ and $\perp $ indicate quantities parallel and perpendicular to the axis of symmetry. Since ${M}_{\parallel } \ensuremath{\sim} { u}_{\parallel }^{2} { \ell }_{\perp }^{2} {\ell }_{\parallel } $ and ${M}_{\perp } \ensuremath{\sim} { u}_{\perp }^{2} { \ell }_{\perp }^{2} {\ell }_{\parallel } $, $u$ and $\ell $ being integral scales, self-similarity of the large scales (when it applies) demands ${ u}_{\parallel }^{2} { \ell }_{\perp }^{2} {\ell }_{\parallel } = \text{constant} $ and ${ u}_{\perp }^{2} { \ell }_{\perp }^{2} {\ell }_{\parallel } = \text{constant} $. This, in turn, requires that ${ u}_{\parallel }^{2} / { u}_{\perp }^{2} $ is constant, contrary to the popular belief that freely decaying turbulence should exhibit a ‘return to isotropy’. Numerical simulations performed in large periodic domains, with different types and levels of initial anisotropy, confirm that ${M}_{\parallel } $ and ${M}_{\perp } $ are indeed invariants and that, in the fully developed state, ${ u}_{\parallel }^{2} / { u}_{\perp }^{2} = \text{constant} $. Somewhat surprisingly, the same simulations also show that ${\ell }_{\parallel } / {\ell }_{\perp } $ is more or less constant in the fully developed state. Simple theoretical arguments are given which suggest that, when ${ u}_{\parallel }^{2} / { u}_{\perp }^{2} $ and ${\ell }_{\parallel } / {\ell }_{\perp } $ are both constant, the integral scales should evolve as ${ u}_{\perp }^{2} \ensuremath{\sim} { u}_{\parallel }^{2} \ensuremath{\sim} {t}^{\ensuremath{-} 6/ 5} $ and ${\ell }_{\perp } \ensuremath{\sim} {\ell }_{\parallel } \ensuremath{\sim} {t}^{2/ 5} $, irrespective of the level of anisotropy and of the presence of helicity. These decay laws, first proposed by Saffman (Phys. Fluids, vol. 10, 1967, p. 1349), are verified by the numerical simulations.


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