A Mixing-Length Formulation for the Turbulent Prandtl Number in Wall-Bounded flows with Bed Roughness and Elevated Scalar Sources ͒ John P
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CFD-Driven Symbolic Identification of Algebraic Reynolds-Stress Models
CFD-driven Symbolic Identification of Algebraic Reynolds-Stress Models Isma¨ılBEN HASSAN SA¨IDIa,∗, Martin SCHMELZERb, Paola CINNELLAc, Francesco GRASSOd aInstitut A´erotechnique, CNAM, 15 Rue Marat, 78210 Saint-Cyr-l'Ecole,´ France bFaculty of Aerospace Engineering, Delft University of Technology, Kluyverweg 2, Delft, The Netherlands cInstitut Jean Le Rond D'Alembert, Sorbonne Universit´e,4 Place Jussieu, 75005 Paris, France dLaboratoire DynFluid, CNAM, 151 Boulevard de l'Hopital, 75013 Paris, France Abstract A CFD-driven deterministic symbolic identification algorithm for learning ex- plicit algebraic Reynolds-stress models (EARSM) from high-fidelity data is de- veloped building on the CFD-free SpaRTA algorithm of [1]. Corrections for the Reynolds stress tensor and the production of transported turbulent quantities of a baseline linear eddy viscosity model (LEVM) are expressed as functions of tensor polynomials selected from a library of candidate functions. The CFD- driven training consists in solving a blackbox optimization problem in which the fitness of candidate EARSM models is evaluated by running RANS simula- tions. A preliminary sensitivity analysis is used to identify the most influential terms and to reduce the dimensionality of the search space and the Constrained Optimization using Response Surface (CORS) algorithm, which approximates the black-box cost function using a response surface constructed from a limited number of CFD solves, is used to find the optimal model parameters within a realizable search space. The resulting turbulence models are numerically robust and ensure conservation of mean kinetic energy. Furthermore, the CFD-driven procedure enables training of models against any target quantity of interest com- putable as an output of the CFD model. -
Turbulence and Vertical Fluxes in the Stable Atmospheric Boundary Layer. Part II: a Novel Mixing-Length Model
1528 JOURNAL OF THE ATMOSPHERIC SCIENCES VOLUME 70 Turbulence and Vertical Fluxes in the Stable Atmospheric Boundary Layer. Part II: A Novel Mixing-Length Model JING HUANG* AND ELIE BOU-ZEID Department of Civil and Environmental Engineering, Princeton University, Princeton, New Jersey JEAN-CHRISTOPHE GOLAZ NOAA/Geophysical Fluid Dynamics Laboratory, Princeton, New Jersey (Manuscript received 13 June 2012, in final form 3 January 2013) ABSTRACT This is the second part of a study about turbulence and vertical fluxes in the stable atmospheric boundary layer. Based on a suite of large-eddy simulations in Part I where the effects of stability on the turbulent structures and kinetic energy are investigated, first-order parameterization schemes are assessed and tested in the Geophysical Fluid Dynamics Laboratory (GFDL)’s single-column model. The applicability of the gradient-flux hypothesis is first examined and it is found that stable conditions are favorable for that hy- pothesis. However, the concept of introducing a stability correction function fm as a multiplicative factor into the mixing length used under neutral conditions lN is shown to be problematic because fm computed a priori from large-eddy simulations tends not to be a universal function of stability. With this observation, a novel mixing-length model is proposed, which conforms to large-eddy simulation results much better under stable conditions and converges to the classic model under neutral conditions. Test cases imposing steady as well as unsteady forcings are developed to evaluate the performance of the new model. It is found that the new model exhibits robust performance as the stability strength is changed, while other models are sensitive to changes in stability. -
Turbulence Momentum Transport and Prediction of the Reynolds Stress in Canonical Flows
Turbulence Momentum Transport and Prediction of the Reynolds Stress in Canonical Flows T.-W. Lee Mechanical and Aerospace Engineering, Arizona State University, Tempe, AZ, 85287 Abstract- We present a unique method for solving for the Reynolds stress in turbulent canonical flows, based on the momentum balance for a control volume moving at the local mean velocity. A differential transform converts this momentum balance to a solvable form. Comparisons with experimental and computational data in simple geometries show quite good agreements. An alternate picture for the turbulence momentum transport is offered, as verified with data, where the turbulence momentum is transported by the mean velocity while being dissipated by viscosity. The net momentum transport is the Reynolds stress. This turbulence momentum balance is verified using DNS and experimental data. T.-W. Lee Mechanical and Aerospace Engineering, SEMTE Arizona State University Tempe, AZ 85287-6106 Email: [email protected] 0 Nomenclature C1 = constants Re = Reynolds number based on friction velocity U = mean velocity in the x direction Ue = free-stream velocity V = mean velocity in the y direction u’ = fluctuation velocity in the x direction urms’ = root-mean square of u’ u’v’ = Reynolds stress = boundary layer thickness m = modified kinematic viscosity Introduction Finding the Reynolds stress has profound implications in fluid physics. Many practical flows are turbulent, and require some method of analysis or computations so that the flow process can be understood, predicted and controlled. This necessity led to several generations of turbulence models including a genre that models the Reynolds stress components themselves, the Reynolds stress models [1, 2]. -
2.29 Numerical Fluid Mechanics Lecture 25 Slides
2.29 Numerical Fluid Mechanics η NW N y n ne iη Spring 2015 – Lecture 25 n ξ nw iξ e E n P n n REVIEW Lecture 24: w W S se sw • Finite Volume on Complex geometries n SE j S – Computation of convective fluxes: i x xy • For mid-point rule:Fe (.) vn dS fSee ( vn .)eeeeeeeeee S m() S u S v Image by MIT OpenCourseWare. Se – Computation of diffusive fluxes: mid-pointpoint rule for complex geometries often used • Either use shape function (x, y), with mid-point rule: Fd ( k .) nS k Sx Sy e ee e ee xye e • Or compute derivatives at CV centers first, then interpolate to cell faces. Option include either: xi – Gauss Theorem: dV dV c Sc dV x xxiiP P CV i 4c faces old Fd kSEP kS ni – Deferred-correction approach: e ee eee rrEP old old – Comments on 3D where is interpolated from ,e.g. Sxi dV eP c c xi P 4c faces 2.29 Numerical Fluid Mechanics PFJL Lecture 25, 1 2.29 Numerical Fluid Mechanics Spring 2015 – Lecture 25 REVIEW Lecture 24, Cont’d: • Turbulent Flows and their Numerical Modeling η (Kolmogorov microscale) – Properties of Turbulent Flows LO/ ~ (Re3/4 ) • Stirring and Mixing L ReL UL • Energy Cascade and Scales Image by MIT OpenCourseWare. • Turbulent Wavenumber Spectrum and Scales S SK( ,) A2/3 K 5/3 L 1 1 K 1 – Numerical Methods for Turbulent Flows: Classification ε = turbulent energy dissipation • Direct Numerical Simulations (DNS) for Turbulent Flows • Reynolds-averaged Navier-Stokes (RANS) – Mean and fluctuations – Reynolds Stresses – Turbulence closures: Eddy viscosity and diffusivity, Mixing-length Models, k-ε Models – Reynolds-Stress Equation Models • Large-Eddy Simulations (LES) – Spatial filtering – LES subgrid-scale stresses 2.29 • Examples Numerical Fluid Mechanics PFJL Lecture 25, 2 References and Reading Assignments • Chapter 9 on “Turbulent Flows” of “J. -
A Generalized Mixing Length Closure for Eddy‐Diffusivity Mass‐Flux
RESEARCH ARTICLE A Generalized Mixing Length Closure for Eddy‐Diffusivity 10.1029/2020MS002161 Mass‐Flux Schemes of Turbulence and Convection Key Points: Ignacio Lopez‐Gomez1 , Yair Cohen1 , Jia He1, Anna Jaruga1,2 , and Tapio Schneider1,2 • EDMF schemes represent boundary layer (BL) turbulence and 1Department of Environmental Science and Engineering, California Institute of Technology, Pasadena, CA, USA, convection separately yet 2 consistently Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA • A mixing length model based on kinetic energy constraints represents turbulent fluxes in EDMF schemes Abstract Because of their limited spatial resolution, numerical weather prediction and climate models well have to rely on parameterizations to represent atmospheric turbulence and convection. Historically, • The resulting EDMF scheme captures dynamic regimes ranging largely independent approaches have been used to represent boundary layer turbulence and convection, from stable BLs to neglecting important interactions at the subgrid scale. Here we build on an eddy‐diffusivity mass‐flux ‐ stratocumulus topped BLs (EDMF) scheme that represents all subgrid‐scale mixing in a unified manner, partitioning subgrid‐scale fluctuations into contributions from local diffusive mixing and coherent advective structures and allowing them to interact within a single framework. The EDMF scheme requires closures for the interaction Correspondence to: between the turbulent environment and the plumes and for local mixing. A second‐order equation for T. Schneider, turbulence kinetic energy (TKE) provides one ingredient for the diffusive local mixing closure, leaving a [email protected] mixing length to be parameterized. Here, we propose a new mixing length formulation, based on constraints derived from the TKE balance. It expresses local mixing in terms of the same physical processes in all Citation: regimes of boundary layer flow. -
Chapter 119 Numerical Simulation of Turbulent
CHAPTER 119 NUMERICAL SIMULATION OF TURBULENT WAVE BOUNDARY LAYERS J. H. Trowbridge1, A.M.ASCE, C. N. Kanetkar2 and N. T. Wu3 ABSTRACT: This paper reports numerical computations of fully rough turbulent boundary layers produced by first and second order Stokes waves. The computations are based on a mixing length turbulence closure and on a slightly more sophisticated turbulent kinetic energy closure. The first order results compare well with existing laboratory results. Reversal of the second order steady streaming under relatively long waves, which has been predicted analytically, is also predicted in the numerical results, The steady second order velocity field is found to become fully established only after a development time on the order of a few hundred wave periods. Both the first and second order results indicate that advection and diffusion of turbulent kinetic energy play a minor role in determining the Reynolds averaged velocity field. INTRODUCTION A quantitative understanding of turbulent wave boundary layers is necessary for coastal engineers concerned with dissipation of wave energy, wave-induced sediment transport, and the effect of waves on large-scale, slowly varying currents. This study is confined to the case of fully turbulent boundary layers produced by weakly nonlinear waves near fixed hydrodynamically rough boundaries. The boundary roughness elements are assumed to be small compared to the boundary layer thickness. Previous analytical studies (Kajiura, 1968; Grant and Madsen, 1979; Brevik, 1981; Myrhaug, 1982; Trowbridge and Madsen, 1984a), numerical studies (Bakker, 1974; Johns, 1975; Bakker and van Doom, 1978), experimental studies (Jonsson, 1966; Jonsson and Carlsen, 1976; Bakker and van Doom, 1978; Kamphuis, 1975) and semi-empirical analyses (Jonsson, 1966) have clarified the physics of the first-order problem. -
Two-Equation Models (The K -E Model)
INTRODUCTION TO TURBULENCE MODELING Goodarz Ahmadi Department of Mechanical and Aeronautical Engineering Clarkson University Potsdam, NY 13699-5725 In this section, an introduction to the historical development in turbulence modeling is provided. Outline · Viscous Fluid · Turbulence · Classical Phenomenological models (Mixing Length) · One-Equation Models · Two-Equation Models (The k -e Model) · Stress Transport Models · Material-Frame Indifference · Continuum Approach · Consistency of the k -e Model · Rate-Dependent Model ME637 1 G. Ahmadi VISCOUS FLOW The conservation laws for a continuous media are: Mass ¶r + Ñ × (ru) = 0 ¶t Momentum du r = rf + Ñ × t dt Angular Momentum t T = t Energy re& = t : Ñu + Ñq + rh Entropy Inequality q rh r h& - Ñ ×( ) - > 0 T T Constitutive Equation Experimental evidence shows that for a viscous fluid, the stress is a function of velocity gradient. That is tkl = -pd kl + G kl (u i, j ) The velocity gradient term may be decomposed as ui, j = dij + wij where d ij is the deformation rate tensor and wij is the spin tensor. These are given as 1 1 d = (u + u ), w = (u - u ) kl 2 k,l l,k kl 2 k,l l,k ME637 2 G. Ahmadi The principle of Material Frame-Indifference of continuum mechanics implies that the stress is generated only by the deformation rate of media and the spin has no effect. This is because both stress and deformation rate tensors are frame-indifferent while spin is not. Thus, the general form of the constitutive equation is given as tkl = -pdkl + Fkl (dij ) For a Newtonian fluid, the constitutive equation is linear and is given as tkl = (-p + lu i,i )dkl + 2md kl The entropy inequality imposed the following restrictions on the coefficient of viscosity: 3l + 2m > 0 , m >0 , Using the constitutive equation in the balance of momentum leads to the celebrated Navier-Stokes equation. -
7. Turbulence Turbulent Jet
7. Turbulence Turbulent Jet Instantaneous Mean Turbulent Boundary Layer y U(y) Instantaneous Mean What is Turbulence? • A “random”, 3-d, time-dependent eddying motion with many scales, superposed on an often drastically simpler mean flow • A solution of the Navier-Stokes equations • The natural state at high Reynolds numbers • An efficient transporter and mixer • A major source of energy loss • A significant influence on drag: ‒ increases frictional drag in non-separated flow ‒ delays, or sometimes prevents, boundary-layer separation on curved surfaces, so reducing pressure drag. ● “The last great unsolved problem of classical physics” Momentum Transfer in Laminar and Turbulent Flow • Laminar: ‒ smooth ‒ no mixing of fluid ‒ momentum transfer by viscous forces • Turbulent: ‒ chaotic ‒ mixing of fluid ‒ momentum transfer mainly by the net effect of intermingling ρ푈퐿 푈퐿 Regime determined by Reynolds number: Re = = μ ν “Low” Re laminar; “high” Re turbulent “High” or “low” depends on the flow and the choice of 푈 and 퐿 Reynolds’ Decomposition v u + mean fluctuation 푢 = 푢ത + 푢′ 푣 = 푣ҧ + 푣′ 푝 = 푝ҧ + 푝′ Alternative Notations • Overbar for mean, prime for fluctuation: 푢 + 푢′ −ρ푢′푣′ • Upper case for mean, lower case for fluctuation: 푈 + 푢 −ρ푢푣 Reynolds Averaging of a Product 푢 = 푢 + 푢′ 푢′ = 0 cf statistics: σ 푢2 2 2 ′2 σ2 = 푢′2 = − 푢ത2 푢 = 푢 + 푢 Variance 푁 σ 푢푣 푢푣 = 푢 푣 + 푢′푣′ ρ ≡ 푢′푣′ = − 푢ത푣ҧ Covariance 푁 푢푣 = (푢 + 푢′)(푣 + 푣′) = 푢 푣 + 푢푣′ + 푢′푣 + 푢′푣′ 푢푣 = 푢 푣 + 푢푣ഥ′ + 푢ഥ′푣 + 푢′푣′ 푢푣 = 푢 푣 + 푢′푣′ Effect of Turbulence on the Mean Flow (i) Mass vA Mass flux: ρ푣퐴 Average mass flux: ρ푣퐴 The mean velocity satisfies the same continuity equation as the instantaneous velocity Effect of Turbulence on the Mean Flow (ii) Momentum vA (푥-)momentum flux: (ρ푣퐴)푢 = ρ(푢푣)퐴 u Average momentum flux : (ρ푣퐴)푢 = ρ(푢 푣 + 푢′푣′)퐴 extra term Net rate of transport of momentum per unit area ρ푢′푣′ from LOWER to UPPER .. -
Intrinsic Plasma Rotation and Reynolds Stress at the Plasma
Measurements of Reynolds Stress and its Contribution to the Momentum Balance in the HSX Stellarator by Robert S. Wilcox A dissertation submitted in partial fulfillment of the requirements for the degree of Doctor of Philosophy (Electrical Engineering) at the University of Wisconsin–Madison 2014 Date of final oral examination: 12/2/2014 The dissertation is approved by the following members of the Final Oral Committee: David T. Anderson, Professor, Electrical Engineering Amy E. Wendt, Professor, Electrical Engineering Chris C. Hegna, Professor, Engineering Physics Paul W. Terry, Professor, Physics Joseph N. Talmadge, Associate Scientist, Electrical Engineering c Copyright by Robert S. Wilcox 2014 All Rights Reserved i ABSTRACT In a magnetic configuration that has been sufficiently optimized for quasi-symmetry, the neoclas- sical transport and viscosity can be small enough that other terms can compete in the momentum balance to determine the plasma rotation and radial electric field. The Reynolds stress generated by plasma turbulence is identified as the most likely candidate for non-neoclassical flow drive in the HSX stellarator. Using multi-tipped Langmuir probes in the edge of HSX in the quasi-helically symmetric (QHS) configuration, the radial electric field and parallel flows are found to deviate from the values calculated by the neoclassical transport code PENTA using the ambipolarity con- straint in the absence of externally injected momentum. The local Reynolds stress in the parallel and perpendicular directions on a surface is also measured using the fluctuating components of floating potential and ion saturation current measurements. Although plasma turbulence enters the momentum balance as the flux surface averaged radial gradient of the Reynolds stress, the locally measured quantity implies a significant contribution to the momentum balance. -
Computational Fluid Dynamics Techniques for Flows in Lapple Cyclone Separator
COMPUTATIONAL FLUID DYNAMICS TECHNIQUES FOR FLOWS IN LAPPLE CYCLONE SEPARATOR A. F. Lacerda, L. G. M.Vieira, A. M. Nascimento, S. D. Nascimento, J. J. R. Damasceno and M. A. S. Barrozo. Federal University of Uberlândia, Faculty of Chemical Engineering -FEQUI, Block K, Campus Santa Mônica, Uberlândia-MG - Brazil. ZIP: 38400-902 – Fax: 55-034-32394188 E-mail: [email protected] Keywords: Separation; Lapple; Cyclones; Computational Fluid Dynamics; Fluent Abstract A two-dimensional fluidynamics model for turbulent flow of gas in cyclones is used for available the importance of the anisotropic of the Reynolds stress components. This study presents consisted in to simulate through computational fluid dynamics (CFD) package the operation of the Lapple cyclone. Yields of velocity obtained starting from a model anisotropic of the Reynolds stress are compared with experimental data of the literature, as form of validating the results obtained through the use of the Computational fluid dynamics (Fluent). The experimental data of the axial and swirl velocities validate numeric results obtained by the model. 1 - Introduction Cyclones are equipment used for the separation and suspended solid collection in gaseous chains. Its popularity if must mainly to the its simplicity of construction, absence of mobile parts, what it guarantees a low necessity of maintenance. Cyclones are among the oldest of industrial particulate control equipment and air sampling device. The primary advantages of cyclones are economy and simplicity in construction and designs. By using suitable materials and methods of construction, cyclones may be adapted for use in extreme operating conditions: high temperature, high pressure, and corrosive gases. Therefore, cyclones have found increasing utility in the field of air pollution [1]. -
Reynolds Number Effects on the Reynolds-Stress Budgets In
PHYSICS OF FLUIDS 20, 101511 ͑2008͒ Reynolds number effects on the Reynolds-stress budgets in turbulent channels ͒ ͒ Sergio Hoyasa and Javier Jiménezb School of Aeronautics, Universidad Politécnica, 28040 Madrid, Spain ͑Received 28 December 2007; accepted 10 June 2008; published online 31 October 2008͒ Budgets for the nonzero components of the Reynolds-stress tensor are presented for numerical channels with Reynolds numbers in the range Re =180–2000. The scaling of the different terms is + Ϸ discussed, both above and within the buffer and viscous layers. Above x2 150, most budget 3 4 components scale reasonably well with u /h, but the scaling with u / is generally poor below that level. That is especially true for the dissipations and for the pressure-related terms. The former is traced to the effect of the wall-parallel large-scale motions, and the latter to the scaling of the pressure itself. It is also found that the pressure terms scale better near the wall when they are not separated into their diffusion and deviatoric components, but mostly only because the two terms tend to cancel each other in the viscous sublayer. The budgets, together with their statistical uncertainties, are available electronically from http://torroja.dmt.upm.es/channels. © 2008 American Institute of Physics. ͓DOI: 10.1063/1.3005862͔ I. INTRODUCTION nolds stress is found not to hold. As determinants, it is clear that failures in the scaling of the energy equations, or in the The interest of the budget equations for the normal and budget of the tangential Reynolds stress, bear directly on the tangential Reynolds stresses in turbulent shear flows extends dynamics of the flow. -
On Reynolds Stresses and Turbulent Flows in Circular Ducts
ON REYNOLDS STRESSES AND TURBULENT FLOWS IN CIRCULAR DUCTS A THESIS Presented to The Faculty of the Division of Graduate Studies and Research . *y • Kenneth Alan Williams In Partial Fulfillment of the Requirements for the Degree Master of Science in Mechanical Engineering Georgia Institute of Technology June, 1974 ON REYNOLDS STRESSES AND TURBULENT FLOWS IN CIRCULAR DUCTS Approved: Novak Zuber, Chairman Ward 0. Winer /f) ~ K PV^V. Desai- Charles W. Gorton Date approved by Chairman: ""7 7 ' ^ / 11 ACKNOWLEDGMENTS The author wishes to express his deep appreciation to his advisor, Dr. Novak Zuber, for suggesting the thesis area and for his devoted assistance which made the success of this work possible. The author is also grateful for the valuable career guidance given him by his advisor. It is a pleasure to thank Drs. Winer and Desai of the School of Mechanical Engineering and Dr. Gorton of the School of Chemical Engineering, for their interest in the work and for their meaningful comments and suggestions. Finally the author wishes to express his gratitude toward his entire family, whose continued encouragement and support made his education possible. TABLE OF CONTENTS Page ACKNOWLEDGMENTS. ..... .... ... ii LIST OF ILLUSTRATIONS. .,. ,-. • • • • v NOMENCLATURE . „ . .... .., ..... vi SUMMARY. ..... ........ ... ..... viii Chapter I. INTRODUCTION. .... ... ..... 1 1.1 Significance of the Problem 1.2 Purpose of the Tlvesas II. BASIC FORMULATION AND DISCUSSION . ... 2 2.1 Analytical Formulation of Basic Relationships 2; 1.1 Shear. Stress Distribution 2.1.2 Reynolds Equation 2.1.3 Closure Problem 2.2 Present Methods 2.3 General Observations Concerning Turbulent Flows 2.4 Comments and Conclusions III.