Relaminarisation of turbulent stratified flow Bas van de Wiel Moene, Steeneveld, Holtslag.

Slides:



Advertisements
Similar presentations
Introduction Irina Surface layer and surface fluxes Anton
Advertisements

Turbulent flow over groups of urban-like obstacles
Section 2: The Planetary Boundary Layer
Training course: boundary layer IV Parametrization above the surface layer (layout) Overview of models Slab (integral) models K-closure model K-profile.
Non-Universal Turbulence in Planetary Boundary Layers
ON WIDTH VARIATIONS IN RIVER MEANDERS Luca Solari 1 & Giovanni Seminara 2 1 Department of Civil Engineering, University of Firenze 2 Department of Environmental.
Stability of MHD Buoyancy Driven Flows Presented by Naveen Vetcha (UCLA) With contribution from: Sergey Smolentsev (UCLA) Rene Moreau (Prof., Lab. EPM,
Free Convection: General Considerations and Results for Vertical and Horizontal Plates Chapter 9 Sections 9.1 through 9.6.2, 9.9.
Boundary Layer Flow Describes the transport phenomena near the surface for the case of fluid flowing past a solid object.
Hans Burchard Leibniz Institute for Baltic Sea Research Warnemünde From the Navier-Stokes equations via the Reynolds decomposition.
Generalities Separated Flows Wakes and Cavities. 1.1 What is separation ? A streamline leaves the body and turns into the interior of the fluid 2D separation.
Sensitivity of High-Resolution Simulations of Hurricane Bob (1991) to Planetary Boundary Layer Parameterizations SCOTT A. BRAUN AND WEI-KUO TAO PRESENTATION.
THE PARAMETERIZATION OF STABLE BOUNDARY LAYERS BASED ON CASES-99 Zbigniew Sorbjan Marquette University, Milwaukee Zbigniew Sorbjan Marquette University,
Reading: Text, (p40-42, p49-60) Foken 2006 Key questions:
Direct numerical simulation study of a turbulent stably stratified air flow above the wavy water surface. O. A. Druzhinin, Y. I. Troitskaya Institute of.
Convection Convection Matt Penrice Astronomy 501 University of Victoria.
Large-eddy simulation of flow and pollutant dispersion in urban street canyons under different thermal stratifications W. C. Cheng and Chun-Ho Liu * Department.
Stable Boundary Layers over Land Bert Holtslag Wageningen University, NL Towards a better representation of the Atmospheric Boundary Layer in Weather and.
Baroclinic Instability in the Denmark Strait Overflow and how it applies the material learned in this GFD course Emily Harrison James Mueller December.
James Sprittles ECS 2007 Viscous Flow Over a Chemically Patterned Surface J.E. Sprittles Y.D. Shikhmurzaev.
Introduction to Convection: Flow and Thermal Considerations
Training course: boundary layer II Similarity theory: Outline Goals, Buckingham Pi Theorem and examples Surface layer (Monin Obukhov) similarity Asymptotic.
Review of the Boundary Layer
Observed Structure of the Atmospheric Boundary Layer Many thanks to: Nolan Atkins, Chris Bretherton, Robin Hogan.
Convection Prepared by: Nimesh Gajjar. CONVECTIVE HEAT TRANSFER Convection heat transfer involves fluid motion heat conduction The fluid motion enhances.
Momentum Heat Mass Transfer
Introduction to Convection: Flow and Thermal Considerations
Monin-Obukhoff Similarity Theory
The representation of stratocumulus with eddy diffusivity closure models Stephan de Roode KNMI.
A control algorithm for attaining stationary statistics in LES of thermally stratified wind-turbine array boundary layers Adrian Sescu * and Charles Meneveau.
The Nature of the Wind.
Enhancement of Heat Transfer P M V Subbarao Associate Professor Mechanical Engineering Department IIT Delhi Invention of Compact Heat Transfer Devices……
Contact Line Instability in Driven Films
Xin Xi. 1946: Obukhov Length, as a universal length scale for exchange processes in surface layer. 1954: Monin-Obukhov Similarity Theory, as a starting.
Effects of Upwind Roughness Changes and Impacts on Hub-Height Winds Peter A. Taylor 1,2, Wensong Weng 1 and James R. Salmon 2 1 Centre for Research in.
Understanding the USEPA’s AERMOD Modeling System for Environmental Managers Ashok Kumar Abhilash Vijayan Kanwar Siddharth Bhardwaj University of Toledo.
Momentum Equations in a Fluid (PD) Pressure difference (Co) Coriolis Force (Fr) Friction Total Force acting on a body = mass times its acceleration (W)
Turbulent properties: - vary chaotically in time around a mean value - exhibit a wide, continuous range of scale variations - cascade energy from large.
50 Years of the Monin-Obukhov Similarity Theory Thomas Foken University of Bayreuth, Bayreuth, Germany.
CEE 262A H YDRODYNAMICS Lecture 15 Unsteady solutions to the Navier-Stokes equation.
Xin Xi Feb. 28. Basics  Convective entrainment : The buoyant thermals from the surface layer rise through the mixed layer, and penetrate (with enough.
How Small-Scale Turbulence Sets the Amplitude and Structure of Tropical Cyclones Kerry Emanuel PAOC.
Chapter 6 Introduction to Forced Convection:
A canopy model of mean winds through urban areas O. COCEAL and S. E. BELCHER University of Reading, UK.
USE THESE VALUES. e(T) = e s (T Dew ) PRACTICE WITH STABILITY.
1 Equations of Motion Buoyancy Ekman and Inertial Motion September 17.
EMS Sep Reading UK Evaluating modelled surface long wave downward radiation with Cabauw observations: The GABLS3 SCM case. Fred Bosveld (KNMI)
Analysis of Turbulence Development in the Morning
Large-Eddy Simulations of the Nocturnal Low-Level Jet M.A. Jiménez Universitat de les Illes Balears 4th Meso-NH user’s meeting, Toulouse April 2007.
Next The evening boundary layer: turbulence or no turbulence? Bas van de Wiel, Ivo van Hooijdonk & Judith Donda in collaboration with: Fred Bosveld, Peter.
1 Large Eddy Simulation of Stable Boundary Layers with a prognostic subgrid TKE equation 8 th Annual Meeting of the EMS, Amsterdam, 2008 Stephan R. de.
The simplifed momentum equations Height coordinatesPressure coordinates.
Compressible Frictional Flow Past Wings P M V Subbarao Professor Mechanical Engineering Department I I T Delhi A Small and Significant Region of Curse.
SOES6002 Module A, part 2: Multiple equilibria in the THC system: Governing equation Tim Henstock.
NATO ASI Conference, Kyiv MODELING AND SIMULATION OF TURBULENT PENETRATIVE CONVECTION AND POLLUTANT DISPERSION ABOVE THE URBAN HEAT ISLAND IN STABLY.
INTRODUCTION TO CONVECTION
Modeling and Evaluation of Antarctic Boundary Layer
Observed Structure of the Atmospheric Boundary Layer
Heat Transfer Su Yongkang School of Mechanical Engineering # 1 HEAT TRANSFER CHAPTER 9 Free Convection.
A revised formulation of the COSMO surface-to-atmosphere transfer scheme Matthias Raschendorfer COSMO Offenbach 2009 Matthias Raschendorfer.
Development of the two-equation second-order turbulence-convection model (dry version): analytical formulation, single-column numerical results, and.
Boris Galperin Univ. South Florida
Similarity theory 1. Buckingham Pi Theorem and examples
Vertical resolution of numerical models
Fundamentals of Convection
A hybrid model for the wind profile
Lecture 1: Introduction
Turbulent Kinetic Energy (TKE)
Large-eddy simulation of an observed evening transition boundary layer
Turbulent properties:
Presentation transcript:

Relaminarisation of turbulent stratified flow Bas van de Wiel Moene, Steeneveld, Holtslag

Overview 1)Motivation 2)A simple Couette flow analogy 3)Pressure driven flow: comparison with DNS 4)Conclusion and perspectives

(1) Motivation Why does the wind drop in the evening?

Classical picture of continuous turbulent quasi-steady SBL: z pot. T t=0t=3t=2t=1 (Nieuwstadt, 1984) Quasi-steady: Shape profiles cst. Linear heat flux profile

Central question: what happens for low pressure gradients? Continuous turbulent, quasi-steady nocturnal boundary layer only observed for strong pressure gradient conditions (high geostrophic winds)

Observational example (Cabauw, KNMI, Netherlands): Clear sky conditions Little wind near surface Collapse of turbulence→ decoupling of the surface from the atmosphere

z Temperature profiles Quasi-steady T

Rationale present work “Yet not every solution of the equations of motion, even if it is exact, can actually occur in nature. The flows that occur in nature must not only obey the equations of fluid dynamics but also be stable.” Landau and Lifschitz (1959) We hypothesize that: 1)The continuous turbulent SBL is hydrodynamically stable for high pressure gradient and are therefore observed in nature. 2)The continuous turbulent SBL is hydrodynamically unstable for low pressure gradient and are therefore not observed in nature. Instead a SBL with collapsed turbulence is observed. In fact we aim to find the transition T-L!

(2) A simple Coutte flow model Some characteristics: First order turbulence closure based on Ri No radiative divergence Rough flow using Z0=0.1 [m] BC’s: Top:Wind speed and temperature fixed Bottom:No slip and fixed surface heat flux Van de Wiel et al. (2006) Flows, Turbulence and Combustion, submitted

Turbulence closure First order closure: Two major elements controlling dominant eddie size: stratification and presence solid boundary Non-trivial in a sense that collapse of system as whole occurs way before Rc! Support locality of TKE in strongly stratified flow e.g.: Nieuwstadt ’84, Lenshow, ’88, Duynkerke ’91(Observations) Mason and Derbyshire ’90, Galmarini ’98, Basu ’05 (LES) Coleman et al (DNS); also recall presentation by Clercx

Results

Continuous turbulent case

Collapse case

Positive feedback mechanism: (following Van de Wiel et al. 2002, J. Atmos. Sc.). Increasing gradient:

Equilibrium solutions: bifurcation analysis

Linear stability analysis (i.e. on logarithmic profiles e.g. not linear!) Ansatz: (1-D!) BC’s

Criterion for instability Agreement between theory and numerical results! 0.55 Previous example: =0.52 Continuous turbulent cases Relaminarised cases

Thus: Collapse of SBL turbulence explained naturally from a linear stability analysis on the governing equations (assuming local closure) The crucial question: how close is our model in comparison with reality (here say reality~DNS)

(3) Comparison with DNS results from Nieuwstadt (2005) Pressure force Cooling BC’s Top: stress free, fixed T Bottom: no slip, prescribed heat extraction Smooth flow; Re*= 360

(3) Comparison with DNS results from Nieuwstadt (2005) We used a priori:(smooth flow) Remarkable in view of origin model

(3) Comparison with DNS results from Nieuwstadt (2005) A posteriori

DNS shows collapse at h/L~1.23 [-] Note: TKE normalised with u*^2

Our model shows collapse at h/L~1.45 [-] A priori threshold h/L~1.55

Predicting relaminarisation: Generalisation of the results Note: Continuous turbulent cases Relaminarised cases

Summary/conclusions: Relaminarization of turbulent stratified shear flows is predicted from linear stability analysis on parameterized equations In this way relaminarization critically depends on two dimensionless parameters: Re* (or Z0/h) and h/L The results seem to be confirmed by recent DNS results (at least in a qualitative sense)

z Wind speed profiles Quasi-steady U