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A New Wall Function for Complex Turbulent Flows T. J. Craft, S. E. Gant, H. Iacovides, B. E. Launder and C. M. E. Robinson UMIST, Manchester, UK.

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Presentation on theme: "A New Wall Function for Complex Turbulent Flows T. J. Craft, S. E. Gant, H. Iacovides, B. E. Launder and C. M. E. Robinson UMIST, Manchester, UK."— Presentation transcript:

1 A New Wall Function for Complex Turbulent Flows T. J. Craft, S. E. Gant, H. Iacovides, B. E. Launder and C. M. E. Robinson UMIST, Manchester, UK

2 Contents Introduction Overview of new wall function Results in 2-D/Axisymmetric flows –channel –impinging jet –spinning disc Generalization to 3-D curvilinear grids –Ahmed body flow –Rotor-stator flows Conclusions

3 Near-Wall Treatments in RANS Simulations Low-Reynolds-Number Model Integrate transport equations across the viscous sublayer to the wall using a fine near-wall grid +Good accuracy and conceptually simple –High computational cost due to highly elongated cells, high storage requirement Two main options in handling the wall boundary condition in turbulent flows: Standard Wall Functions Large near-wall cell in which profiles of velocity, temperature and turbulence parameters are assumed +Fast solution (typically 10 x faster than low-Re) low storage –Poor performance in complex flows and sensitive to near- wall cell size (difficult to obtain grid-independent result)

4 Summary of “Standard” Wall Functions Assumed log-law profiles for velocity and temperature Wall shear stress,, and average source terms (e.g., ) applied within wall-adjacent cell “Local equilibrium” between turbulence production and dissipation –Shear stress,, assumed constant/linear –Kinetic energy, k, assumed linear/quadratic –Length scale,, assumed linear

5 Wall-Function Research at UMIST Two new approaches recently developed at UMIST: Analytical WF: Adopts a simple prescribed viscosity (not velocity) that enables analytical integration of momentum and energy equations over the near-wall cell (Gerasimov et al.). Numerical WF: The present approach A simple prescribed viscosity is inadequate for really complex flows (e.g. recirculating flows)

6 Overview of Numerical Wall Function Near-wall control volume divided into subgrid volumes Wall-normal V-velocity from continuity within subgrid (and scaled) Upwind convection scheme used with saved subgrid values Transport equations solved across the subgrid for: –Mean-flow parameters: U, W, T –Turbulence parameters (e.g. k, )

7 Overview of Numerical Wall Function (cont.) Wall-parallel pressure gradient (dP/dx) calc’d from main-grid and assumed constant across subgrid and average source terms applied to main-grid as in standard wall-function treatments and average source terms ( ) calculated from subgrid solution

8 Subgrid Transport Equations Simplified low-Re transport equations for U, k, and T in plane Cartesian coordinates (convection terms in non-conservative form).

9 Numerical Solution of Subgrid Equations Similar to 1-D convection-diffusion problem Finite-volume method Central differences for diffusion, upwind for convection Tri-diagonal matrix algorithm (TDMA) Under-relaxation factors (U, k, , T) = (1.0, 0.9, 0.9, 1.0) One iteration of subgrid solver performed for each main-grid iteration: subgrid solution converges as main- grid converges Number of subgrid nodes must be sufficient for grid- independent result.

10 TEAM Code Finite-volume 2D/axisymmetric Cartesian grid Staggered velocity/scalar nodes SIMPLE pressure-correction algorithm Quadratic upstream-weighted (QUICK) or upwind differences for convection Central differences for diffusion

11 Channel Flow Results (Re = 100,000) Log-law predictions using the subgrid wall function with two different near- wall cell sizes:

12 Impinging Jet: grid and velocity vectors High-Re grid and velocity vectors, Re = 70,000, H/D = 4

13 Impinging Jet: low-Re and wall-function grids Close-up of near-wall grids: high-Re (left) and low-Re (right) DX=1 Low-Re Grid (90 x 70: grid-independent) wall Wall-Function Grids (45 x 70: four different near-wall cell sizes) DX=250DX=500

14 Impinging Jet Nusselt Number: Linear Numerical wall functionChieng & Launder wall function (Launder & Sharma model, Re = 70,000, H/D = 4)

15 Impinging Jet Nusselt Number: NLEVM Numerical wall functionChieng & Launder wall function (Craft et al. two-equation NLEVM, Re = 70,000, H/D = 4)

16 Computational Costs NLEVM (Craft et al.), axisymmetric impinging jet (Re = 70,000, H/D = 4), running on Silicon Graphics O 2 with same levels of under-relaxation and compiler optimisation in each case. Wall FunctionsLow-Re Craft et al. Chieng & Launder Numerical Number of Nodes 45 x 7045(+40) x 7090 x 70 CPU Time per Iteration (s) 0.1580.2600.324 No. of Iterations142613809116 Total CPU Time (s)2263592955 Relative CPU Time11.613.1

17 Spinning Free-Disc Flow Turbulent kinetic energy contours “Natural” transition from laminar to turbulent b.l. at Near-wall peak in radial velocity Tangential velocity exhibits log-law profile Linear model used in simulations

18 Free –Disc Computational Grids Low-Re grid 70 x 120 (axial x radial) Wall-function grid 22 x 120 (axial x radial)

19 Free-Disc Integral Nusselt Number Numerical wall function Chieng & Launder wall function

20 Free-Disc Radial Wall Shear Stress Numerical wall function Chieng & Launder wall function

21 Free-Disc Radial Velocity (Re  = 10 6 ) Low-Re Launder & Spalding WF Chieng & Launder WF Numerical WF “universal” log-lawexperiment

22 Free-Disc Computational Costs Linear k-  model for the spinning free-disc (Re   = 3.3  x 10 6 ) running on a single processor of an Origin 2000 with the same levels of under-relaxation and compiler optimisation. Model TestedNo. of NodesTime per Iter (s) No. of Iterations Total CPU Time (s) Relative CPU Time Launder & Spalding WF 120 x 28 0.0720091361 Chieng & Launder WF 120 x 28 0.0722081541.1 Numerical WF 120 x 28(+30) 0.1423633392.2 Low-Re 120 x 70 0.2019928399629.4

23 3-D Flows: STREAM Code Lien & Leschziner 1994 Finite-volume Curvilinear structured multi-block grids Collocated storage with Rhie-Chow interpolation SIMPLE pressure-correction TVD version of QUICK scheme for convection terms Central differences for diffusion Fully-implicit or Crank-Nicolson Time scheme

24 Wall Function Generalization to 3-D Flows where (U, V, W) are grid-aligned contravariant subgrid velocity components in the (  directions, J is the Jacobian (equivalent to cell volume), g ii and g jj are metric tensors and the source term C includes pressure gradient, turbulence-equation sources and geometric terms. Generic form of subgrid transport equations  U, V, k  : Multi-block implementation using subgrid halo cells Efficient interpolation scheme to minimize cost of calculating geometric terms Same under-relaxation as for 2-D version x y z   

25 Ahmed Body Simplified car body with interchangeable rear slant angles. Previously studied at UMIST as part of EU project and subject of two ERCOFTAC workshops.

26 Ahmed body: flow regimes Flow features drag “crisis” at approx 30 o slant: < 30 o : flow attached on slant (high drag) > 30 o : flow separated at leading edge of slant (low drag)

27 Ahmed Body: flow domain Symmetry plane used No stilts Block decomposition (22 blocks)

28 Ahmed Body: standard WF’s Simulations using log-law wall functions at UMIST showed: -Linear k-  model attached for 25 o -Non-linear k-  model fully-separated for 25 o -Both models fully- separated for 35 o Aim: to see whether curvature of streamlines near surface of body has influential effect on formation of vortices and hence separation.

29 Ahmed Body: results

30 Ahmed body: rear slant Arrows indicate direction of velocity vector at near-wall main-grid node and subgrid nodes Significant skewing of velocity vector across near-wall cell due to side-edge vortex This effect would be ignored by log-law wall functions

31 Ahmed Body: Conclusions Numerical wall function successfully applied in complex 3D grid. However, no significant improvement in linear k-  results. Similar results have been obtained using full low-Re model treatments (from other research groups at ERCOFTAC workshops). Unable to get fully-converged results using non-linear k-  model with the new wall function, possible causes: -Unsteady flow behaviour -Problem with highly skewed near-wall cells -Positive feedback inherent with non-linear model Challenging test-case: at workshops none of the RANS or LES models correctly predicted flow patterns over rear slant.

32 Rotor-Stator Cavity Aim: to reproduce coherent structures observed experimentally by Czarny et al. using URANS. H R  Bottom disc rotates Top disc and walls stationary No through-flow

33 Rotor-Stator: 2D Simulations Itoh et al. test case: Re=  R 2 /    H/R  Numerical wall function results agree well with full low-Re model No problem with internal corner cells.

34 Rotor-Stator: 3D Simulations STREAM code parallelized using domain decomposition and MPI: -2-block axisymmetric grids running on local linux cluster -8-block version running on SGI Origin/Altix at CSAR Number of main-grid nodes in (R,  = (60,50,37) plus 30 subgrid nodes on each wall. Reynolds Number Re=  RH/  Disc spacing H/R=0.126

35 Rotor-Stator: Quasi-LES Using laminar viscosity only (deactivating turbulence model) Radial velocity isocontours (scale:  R max = 1.0) Axial velocity contours near stator surface

36 Rotor-Stator: URANS Eddy-viscosity contours: (red, yellow, green)  (40 , 30 , 20  ) Axial velocity contours near stator surface (scale:  R max = 1.0) Realizable k-  model

37 Rotor-Stator: URANS/LES Only OES shows continued presence of eddy structures Future work: examine filter-based (LES/URANS) approach using finer grids. Models tested: Linear k-  with/without Yap Realizable k-  Cubic non-linear k-  Linear Production (LP) (Laurence & Guimet) Organized Eddy Simulation (OES) (Braza) Filter-based URANS (Johansen et al.) (Using different initial turbulence levels for each case.)

38 Overall Conclusions The 2D test-cases showed that the new numerical wall function results agree well with full low-Re model treatments, in contrast to standard log- law wall functions. In 2D/axisymmetric flow the computational cost is approx. twice that of standard wall functions but an order-of-magnitude less than low-Re models. Storage requirements are roughly equivalent to a low-Re model. Changing the size of the near-wall main-grid cell has little/no effect (provided that there are sufficient subgrid cells). It can be applied to flows with internal/external corners (e.g. pipe expansion) and to 3D curvilinear grids.

39 Future Work Simplify the 3D-curvilinear wall function to use a local Cartesian grid instead of contravariant velocity components: -Easier mathematics -Simpler to code and debug -Fewer problems with skewed cells -Faster to compute and lower storage Investigate wall functions for LES: -Extensions to Balaras & Benocci wall function Continue rotor-stator calculations


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