A Discussion on The Effect of Mesh Resolution on Convective Boundary Layer Statistics and Structures Generated by Large-Eddy Simulation by Sullivan

Similar documents
Energy partitioning of inland water bodies

Atm S 547 Boundary Layer Meteorology

Note the diverse scales of eddy motion and self-similar appearance at different lengthscales of the turbulence in this water jet. Only eddies of size

Lecture 3. Turbulent fluxes and TKE budgets (Garratt, Ch 2)

Lecture 2. Turbulent Flow

Lecture 12. The diurnal cycle and the nocturnal BL

Direct and Large Eddy Simulation of stably stratified turbulent Ekman layers

Investigating 2D Modeling of Atmospheric Convection in the PBL

Reynolds Averaging. We separate the dynamical fields into slowly varying mean fields and rapidly varying turbulent components.

ESS Turbulence and Diffusion in the Atmospheric Boundary-Layer : Winter 2017: Notes 1

Chapter (3) TURBULENCE KINETIC ENERGY

τ xz = τ measured close to the the surface (often at z=5m) these three scales represent inner unit or near wall normalization

TURBULENT STATISTICS OF NEUTRALLY STRATIFIED FLOW WITHIN AND ABOVE A SPARSE FOREST FROM LARGE-EDDY SIMULATION AND FIELD OBSERVATIONS

LECTURE NOTES ON THE Planetary Boundary Layer

Characteristics of Langmuir Turbulence in the Ocean Mixed Layer

Improving a Turbulence Scheme for the Terra Incognita in a Dry Convective Boundary Layer

Effects of Temporal Discretization on Turbulence Statistics and Spectra in Numerically Simulated Convective Boundary Layers

Wind Flow Modeling The Basis for Resource Assessment and Wind Power Forecasting

Structure of the Entrainment Zone Capping the Convective Atmospheric Boundary Layer

Eddy viscosity. AdOc 4060/5060 Spring 2013 Chris Jenkins. Turbulence (video 1hr):

Turbulence: Basic Physics and Engineering Modeling

1 Introduction to Governing Equations 2 1a Methodology... 2

Before we consider two canonical turbulent flows we need a general description of turbulence.

LECTURE 28. The Planetary Boundary Layer

ESCI 485 Air/sea Interaction Lesson 2 Turbulence Dr. DeCaria

The applicability of Monin Obukhov scaling for sloped cooled flows in the context of Boundary Layer parameterization

Temperature fronts and vortical structures in turbulent stably stratified atmospheric boundary layers

Frictional boundary layers

LES of turbulent shear flow and pressure driven flow on shallow continental shelves.

Rica Mae Enriquez*, Robert L. Street, Francis L. Ludwig Stanford University, Stanford, CA. 0 = u x A u i. ij,lass. c 2 ( P ij. = A k. P = A ij.

Logarithmic velocity profile in the atmospheric (rough wall) boundary layer

Atmospheric Boundary Layers

DNS STUDY OF TURBULENT HEAT TRANSFER IN A SPANWISE ROTATING SQUARE DUCT

14B.2 Relative humidity as a proxy for cloud formation over heterogeneous land surfaces

Buoyancy Fluxes in a Stratified Fluid

Higher-order closures and cloud parameterizations

Wind driven mixing below the oceanic mixed layer


An evaluation of a conservative fourth order DNS code in turbulent channel flow

Lecture Notes on The Planetary Boundary Layer

TURBULENT KINETIC ENERGY

1 The Richardson Number 1 1a Flux Richardson Number b Gradient Richardson Number c Bulk Richardson Number The Obukhov Length 3

Large-Eddy Simulation of the Daytime Boundary Layer in an Idealized Valley Using the Weather Research and Forecasting Numerical Model

Mellor-Yamada Level 2.5 Turbulence Closure in RAMS. Nick Parazoo AT 730 April 26, 2006

Turbulent momentum flux characterization using extended multiresolution analysis

The parametrization of the planetary boundary layer May 1992

Tutorial School on Fluid Dynamics: Aspects of Turbulence Session I: Refresher Material Instructor: James Wallace

An Introduction to Theories of Turbulence. James Glimm Stony Brook University

Model Studies on Slag-Metal Entrainment in Gas Stirred Ladles

Buoyancy and Wind-Driven Convection at Mixed Layer Density Fronts

A closer look at boundary layer inversion. in large-eddy simulations and bulk models: Buoyancy-driven case

Introduction to Turbulence and Turbulence Modeling

6.3 EFFECT OF HORIZONTAL SURFACE TEMPERATURE HETEROGENEITY ON TURBULENT MIXING IN THE STABLY STRATIFIED ATMOSPHERIC BOUNDARY LAYER

Large eddy simulation studies on convective atmospheric boundary layer

SIMULATION OF STRATOCUMULUS AND DEEP CONVECTIVE CLOUDS WITH THE DYNAMIC RECONSTRUCTION TURBULENCE CLOSURE

Meteorology 6150 Cloud System Modeling

Calculating equation coefficients

Atm S 547 Boundary Layer Meteorology

Homogeneous Turbulence Dynamics

Eulerian models. 2.1 Basic equations

PENETRATIVE TURBULENCE ASSOCIATED WITH MESOSCALE SURFACE HEAT FLUX VARIATIONS

IMPROVEMENT OF THE MELLOR YAMADA TURBULENCE CLOSURE MODEL BASED ON LARGE-EDDY SIMULATION DATA. 1. Introduction

Atm S 547 Boundary Layer Meteorology

Improved Atmospheric Stable Boundary Layer Formulations for Navy Seasonal Forecasting

Multiscale Computation of Isotropic Homogeneous Turbulent Flow

Numerical simulation of marine stratocumulus clouds Andreas Chlond

DYNAMIC SUB-GRID MODELLING OF AN EVOLVING CBL AT GREY-ZONE RESOLUTIONS

Needs work : define boundary conditions and fluxes before, change slides Useful definitions and conservation equations

Part III: Modeling atmospheric convective boundary layer (CBL) Evgeni Fedorovich School of Meteorology, University of Oklahoma, Norman, USA

3-Fold Decomposition EFB Closure for Convective Turbulence and Organized Structures

Non-local Momentum Transport Parameterizations. Joe Tribbia NCAR.ESSL.CGD.AMP

Unified Cloud and Mixing Parameterizations of the Marine Boundary Layer: EDMF and PDF-based cloud approaches

Modified PM09 parameterizations in the shallow convection grey zone

The Stable Boundary layer

From small-scale turbulence to large-scale convection: a unified scale-adaptive EDMF parameterization

A new source term in the parameterized TKE equation being of relevance for the stable boundary layer - The circulation term

Reynolds Averaging. Let u and v be two flow variables (which might or might not be velocity components), and suppose that. u t + x uv ( ) = S u,

The Planetary Boundary Layer and Uncertainty in Lower Boundary Conditions

Horizontal buoyancy-driven flow along a differentially cooled underlying surface

SIMULATION OF GEOPHYSICAL TURBULENCE: DYNAMIC GRID DEFORMATION

Large-Eddy Simulations of Radiatively Driven Convection: Sensitivities to the Representation of Small Scales

The atmospheric boundary layer: Where the atmosphere meets the surface. The atmospheric boundary layer:

Characteristics of the night and day time atmospheric boundary layer at Dome C, Antarctica

PALM - Cloud Physics. Contents. PALM group. last update: Monday 21 st September, 2015

(Wind profile) Chapter five. 5.1 The Nature of Airflow over the surface:

Impact of Typhoons on the Western Pacific Ocean (ITOP) DRI: Numerical Modeling of Ocean Mixed Layer Turbulence and Entrainment at High Winds

The Role of Splatting Effect in High Schmidt Number Turbulent Mass Transfer Across an Air-Water Interface

Energy Cascade in Turbulent Flows: Quantifying Effects of Reynolds Number and Local and Nonlocal Interactions

Multi-Scale Modeling of Turbulence and Microphysics in Clouds. Steven K. Krueger University of Utah

2.3 The Turbulent Flat Plate Boundary Layer

Large-eddy simulation of a neutrally stratified boundary layer: A comparison of four computer codes

Accretion Disks I. High Energy Astrophysics: Accretion Disks I 1/60

The Johns Hopkins Turbulence Databases (JHTDB)

The Atmospheric Boundary Layer. The Surface Energy Balance (9.2)

Numerical Methods in Aerodynamics. Turbulence Modeling. Lecture 5: Turbulence modeling

A Simple Turbulence Closure Model

A Note on the Estimation of Eddy Diffusivity and Dissipation Length in Low Winds over a Tropical Urban Terrain

A Simple Turbulence Closure Model. Atmospheric Sciences 6150

Vertical resolution of numerical models. Atm S 547 Lecture 8, Slide 1

Mostafa Momen. Project Report Numerical Investigation of Turbulence Models. 2.29: Numerical Fluid Mechanics

Transcription:

耶鲁 - 南京信息工程大学大气环境中心 Yale-NUIST Center on Atmospheric Environment A Discussion on The Effect of Mesh Resolution on Convective Boundary Layer Statistics and Structures Generated by Large-Eddy Simulation by Sullivan Journal Of the Atmospheric Sciences, 2011 Reporter: Wang Kefei 2015.10.23 1

Outline Introduction LES equations Design of LES experiment Overall results Results: a. Inertial subrange scaling b. Temperature profile and entrainment statistics c. Convergence of variance statistics d. Spectra analysis e. High-order moments f. Flow visualization Summary 2

Introduction Large-Eddy simulations (LES) has important role in studying boundary layer dynamics since large-scale parallel computing with increased computer power enables it. The applications include: Atmosphere-land interactions; Boundary layers with surface water wave effects; Weakly stable nocturnal flows; Flow in complex terrain and so on 3

It s important to examine the quality of LES solutions: Solution quality Grid mesh Subgrid-scale(SGS) parameterizations Numerical discretizations Boundary conditions Here, the paper investigate the sensitivity and convergence of LES solutions as the grid mesh is substantially varied for a certain choice of SGS model, and the physical problem investigated is a very weakly sheared daytime convective PBL. 4

LES equations and symbol description Typical LES model equations for a dry atmospheric PBL under the Boussinesq approximation include: u t + u u = f u U g a transport equation for momentum: π + kβ θ T (1) b transport equation for a conserved buoyancy variable (e. g., virtual potential temperature θ) θ t + u θ = B (2) c closure expressions for SGS variables(e. g., TKE e) e t + u e = P + B + D ε (3) 5

Total velocity u = u + u where () and () denote resolved and subgrid fields respectively. Resolved turbulence fluctuation f = is vertical velocity, w w. where denotes ensemble average. f f and a special case The SGS momentum and scalar fluxes and SGS energy are T = u i u j u i u j B = u i θ u i θ e = u iu i u i u i 2 4a 4b (4c) which represent the SGS influence on the resolved field. 6

Design of LES experiments Computation domain is L x, L y, L z = 5120,5120,2048 m and the initial inversion height z i ~1024m. Coarse Table 1. Simulation grid spacings. Run Grid points ( x, y, z)(m) f(m) A 32 3 (160,160,64) 154 B 64 3 (80,80,32) 77.2 C 128 3 (40,40,16) 38.6 D 256 3 (20,20,8) 19.3 E 512 3 (10,10,4) 9.6 F 1024 3 (5,5,2) 4.8 Fine Characteristic subgird length scale or LES filter width used in 2D filter f 3 = x y z, and ( x, y)=3( x, y)/2 7

The initial sounding of virtual potential temperature θ has a three-layer structure: θ z = 300K 0 < z < 974m. 300K + z 974m 0.08 Km 1 974 < z < 1074m. 308K + z 1074m 0.003 Km 1 : z > 1074m. (5) A sharp jump in temperature of 8K is imposed over a depth of 100m near the top of the PBL. All simulations are started from small random seed perturbations in temperature near the surface. The PBL is driven by a constant surface buoyancy flux Q and weak geostrophic winds and a fully rough lower boundary. The simulations are carried forward for about 25 large eddy turnover time T. 8

Overall Results Table 2. Bulk simulation properties. Run z i (m) z i / f z i /C s f w (m s 1 ) w e /w Re l u /w (δ b, δ t )/z i A 1132 7.2 40 2.07 9.56 238 0.084 (0.74,1.22) B 1118 14.5 80 2.06 8.45 554 0.091 (0.75,1.18) C 1099 28.5 158 2.05 6.84 1300 0.090 (0.77,1.12) D 1092 56.6 314 2.05 5.23 3178 0.087 (0.80,1.09) E 1088 113.3 630 2.04 5.27 8050 0.084 (0.80,1.07) F 1099 229.0 1272 2.05 5.16 20600 0.079 (0.80,1.05) No variant PBL depth z i, Deardorff convective velocity scale w, entrainment rate w e, large-eddy Reynolds number at mid-pbl Re l, friction velocity u, bottom and top of the entrainment zone (δ b, δ t )/z i 9

Results a.inertial subrange scaling A fundamental basis of high Reynolds number LES is that the resolved (large eddy) turbulence is independent of SGS influence, namely the SGS viscosity ν t and scalar diffusivity ν H. Define Re l for LES of a convective PBL based on the SGS viscosity ν t and character velocity and length scale (w, z i ) Re l = w z i ν t = w z i C k Δf e (6) and ε = C εe 3/2 f, w = g θ 0 Q z i, C s = C k 3 4 C ε 1 4 (7) 10

Leads to Re l = z i f 4 3 C ε 3 C g Q k θ 0 ε 1 3 = z i C s f 4 3 g Q θ 0 ε 1 3 (8) 0.5 0.1 0.9 mesh > 256 3 Re l f z i 4/3 constant if Δf or C s Δf lies in the inertial subrange. Coarse Fine Fig.1 Variation of large-eddy Reynolds number Re l with mesh resolution at heights z = z i 0.1,0.5 and 0.9 11

Results b.temperature profiles & entrainment statistics inversion layer entrainment zone Fig.2 Vertical profile of mean virtual potential temperature θ and normalized total turbulent temperature flux w θ + B k /Q for varying mesh resolution. 12

Use the maximum vertical gradient in temperature method to determine the PBL height z i. A critical parameter, the entrainment rate w e = dz i /dt, is then a function of mesh resolution. Fig.3 Variation of the boundary layer height z i with nondimensional time t/t. 13

To further expose the coupling between the mean temperature field and turbulence in the entrainment zone, the paper examine the average budget equations for the resolved vertical temperature flux and temperature variance. >0, M term acts as a sink t w θ = z w 2 θ w 2 θ + g θ z θ 2 1 π θ 0 ρ z T M B P 1 2 t θ 2 = 1 2 <0 >0 θ z w θ 2 w θ +S z θ T M S +F S (9a) (9b) In these equations, T is turbulent transport, M is mean-gradient production, B is buoyant production, P is pressure destruction, and S is a SSG term. 14

It is the mean temperature gradient that influences mean temperature flux and temperature variance, and in turn impact the entrainment prediction as well as itself. To illustrate the influence of θ / z, additional simulations are added: Simulation D1 uses a 256 3 mesh but sets the filter width Δf equal to the value for the 64 3 with other settings still. (open circle marker in Fig.3) Simulation B1 uses a 64 3 mesh but with no monotone vertical temperature flux. (open square marker in Fig.3) Results show that insufficient vertical resolution weakens the inversion and increases the entrainment rate while maintaining nearly the same minimum temperature flux. 15

Results c. Convergence of variances statistics Fig.4 Effect of mesh resolution on the total(resolved plus SGS contributions) TKE(left),total variance of the vertical(middle) and horizontal(right) velocities. TKE is normalized by w 2. 16

Θ 2 z = θ 2 + φ /θ 2 (10a) and the SGS variance contribution is diagnosed from: φ ~ 2l fb k θ (10b) C θ e z There s no prognostic equation for the SGS temperature variance. Fig.5 Total temperature variance Θ 2 on different mesh resolution. The temperature variance is normalized by Θ = Q /w. The weaker temperature gradient that develops on the coarse mesh greatly reduces the temperature variance. 17

Results d. Spectral analysis k h 5/3 slope Fig.6 Two-dimensional energy spectra of vertical (left) and horizontal (right) velocity in the PBL for varying meshes. The groups of spectra at the top, middle and bottom are height at 0.9,0.5 and 0.1. 18

k h 5/3 slope Fig.7 Two-dimensional energy spectrum of vertical(left) and horizontal(right) velocity near the lower boundary at various heights z z i =0.1,0.2,0.3 and 0.5 for a simulations with 1024 3 grid points. 19

Results e. High-order moments Identify the vertical velocity skewness S w as a critical parameter in boundary layer dynamics, and it is formed by high-order moments. S w = w3 w 2 3/2 (11) With decreasing grid resolution, S w becomes larger and shows a obvious maximum below the inversion. near the surface S w decrease and eventually becomes unrealistically negative on the coarse meshes. Fig.8 Resolved vertical velocity skewness on different 20 mesh resolution with observations compared.

The interpretation of Fig.8 hinges on the behavior and modeling of the SGS fluxes in LES, since typical LES uses Smagorinsky closures that parameterized fluxes at the second moment level, so there s no clear definition of SGS skewness in LES. S w = S w 1 ψ (1 φ) 3 2 SGS correction (12) F Ff B =1 Fig.9 (a)skewness from simulation F, Ff and B, and (b) SGS moments from Ff. 21

Hunt et al.(1988) note that Smagorinsky closures assume SGS third-order moment φ = 0, as a consequence, coarse-mesh LES results predict erroneous values of skewness. When Smagorinsky type closures are used with LES, the resolution ratio z i /C s f needs to be greater than 630 to obtain mesh-independent estimates of S w.(see Fig.8 simulation E and F) For other third-order moments γ a = w 2 θ and γ b = w θ 2 There is also a clear mesh dependence in the inversion layer and near the surface. Fig.10 Resolved third-order moments on different 22 mesh resolution.

Results f. Flow visualization Coarse-mesh LES hints at coherent vortices but fine-resolution simulations allow a detailed examination of their dynamics within the larger-scale flow. Fig.11 Visualization of the vertical velocity field in a convective PBL at different heights from the F simulation: z/z i =0.04(top left), 0.1(top right),0.5 and 0.9. The fine-resolution simulation clearly illustrates the classical formation of plumes in a convective PBL, which represents one aspect of large- and small-scale interaction. 23

Summary This code is to carry out a grid sensitivity study of a daytime convective PBL for a wide range of meshes varying from 32 3 to 1024 3. Based on the variation of the second-order statistics, spectra and entrainment statistics we find that the 3D time-dependent LES solutions numerically converge as the mesh is refined. For our mesh of 256 3, the ratio z i / f>60 or z i /(C s f) > 310,in this regime, the LES solutions show clear Kolmogorov inertial subrange scaling, which is the basis of most high-reynolds number subgrid-scale modeling. (results a and d) The LES estimates of entrainment velocity become mesh independent when the vertical grid resolution is able to capture both the mean structure of the overlying inversion and the turbulence. (result b) 24

Near the rough lower surface and in the entrainment zone, the total (resolved plus subgrid) temperature variance increases with mesh refinement, which is partly a consequence of the SGS model that does not employ a prognostic equation for SGS temperature variance. (result c) The mesh dependence of S w is a consequence of a Smagorinsky closure that neglects third-order SGS moments of vertical velocity. Simulation with 512 3 mesh points or more are needed to estimate vertical velocity and higher-order moments from the resolved LES flow field. (result e) The criterion z i /(C s f)>310 proposed here for simulations of convective boundary layers needs to be tested under other meteorological conditions. 25

Thank you 26