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Drag and Lift Validation of Wing Profiles STAR European Conference 2010 London By: Dr Martin van Staden Aerotherm Computational Dynamics 14 th IAHR Conference December 2009 Outline of Presentation Background Detailed Fan


  1. Drag and Lift Validation of Wing Profiles STAR European Conference 2010 London By: Dr Martin van Staden Aerotherm Computational Dynamics 14 th IAHR Conference – December 2009

  2. Outline of Presentation  Background  Detailed Fan Modelling  2-D Wing Section Modelling  Comparison with Experimental data  Mesh & Turbulence model sensitivity  Summary & Conclusions STAR European Conference 2010

  3. Background  Two large Coal fired power stations are currently being built in South Africa which make use of Air cooled Condensers for cooling.  These ACC’s Consist of 384 fans each with a diameter of 10.4m (34ft).  Detailed fan modelling has become an important part of predicting the thermal performance of such a power station. STAR European Conference 2010

  4. Background….  CFD provides us with the ideal tool to model an ACC in order to understand the complex flows around as well as within the ACC’s A -frames.  One of the most important parts of the ACC modelling process is to understand how the fans react to poor inflow conditions.  Fan performance can therefore be analysed as they will be installed in situ and tested under real operating conditions.  This data can then be used in global ACC models to model the entire ACC in order to evaluate it’s response to changing wind conditions.  An important outcome of the CFD analysis is the predicted fan power for a given blade angle setting. STAR European Conference 2010

  5. Detailed Fan Modelling  Requirements for fan modelling Global ACC model: – Must predict the volume flow rate accurately – Must represent system pressure losses accurately – Must take into account the affect flow rate as a function of varying pressure losses – Must take into account the affect of skewed inflow conditions – Must be able to accurately predict fan power consumption  Accurate prediction of the Fan power is important as the fan power for a given flow rate is a contracted value and has a heavy financial penalty coupled to exceeding of the contract value. STAR European Conference 2010

  6. Detailed Fan Modelling  What is a detailed fan model? – The fan blades are explicitly modelled – Fan is rotated (explicitly or implicitly) – Cell sizes as small as 1mm – All support structures such as the A-frame, I-beams, fan screen supports, steam ducts, fan bridge, motor and gearbox, fan inlet bell etc are explicitly modelled. STAR European Conference 2010

  7. Detailed Fan Modelling  The lift and drag is explicitly calculated based on the 3D flow field and pressure filed which develops around the fan blades as a result of the rotation.  Rotation is achieved through steady state MRF or explicitly rotation of the mesh (transient) i.e. using a sliding mesh.  A test facility was modelled in order to compare the outcome of the CFD results with experimental results STAR European Conference 2010

  8. Outcome of test facility simulation Good agreement was found with Pressure vs. Volume flow rate Power was over predicted by the CFD models by more than 11% STAR European Conference 2010

  9. 2D Wing profile comparison  Tests were conducted on 2D wing sections in order to evaluate the expected accuracy for relatively coarse meshes used in detailed fan models.  The aim of the study was to identify which modelling parameters were the main cause for large discrepancy in fan power predicted by the CFD models. STAR European Conference 2010

  10. Comparison of CFD vs. Experimental data  The laser scanned fan wing section profile was matched with a Wortmann FX60-126 wing section.  Prof. Ewald Krämer from Stuttgart University was kind enough to provide us with the aerodynamic data for comparison with 2D CFD simulations of the lift and drag. STAR European Conference 2010

  11. Initial mesh  Low Rey poly mesh (15 boundary layer cells)  No wake refinement STAR European Conference 2010

  12. Simulation assumptions  Free stream velocity of 50m/s was used (Rey=1.94E+6)  Inlet turbulence intensity of 0.01  Turbulent viscosity ratio of 10  Used all y+ approach in all turbulence models where this option is relevant STAR European Conference 2010

  13. Initial mesh Y+ values STAR European Conference 2010

  14. Comparison of lift curve FX60-126 - Aerofoil data Cl from CFD 2D profile simulation 2.00 1.50 Lift Coefficien Cl 1.00 Stall point 0.50 Cl CFD Coarse k-e Cl Stuttgart : FX 60-126 - Rey=2e6 0.00 -10 -5 0 5 10 15 20 25 -0.50 Angle of attack ( α ) STAR European Conference 2010

  15. Comparison of drag curve FX60-126 - Aerofoil data Cl and Cd from CFD 2D profile simulation 0.06 Cd CFD Coarse k-e 0.05 Cl Stuttgart : FX 60-126 - Rey=2e6 0.04 Drag Coefficient Cd 0.03 0.02 0.01 0 -10 -5 0 5 10 15 20 25 Angle of attack ( α ) STAR European Conference 2010

  16. Finer mesh STAR European Conference 2010

  17. Finer mesh y+ values STAR European Conference 2010

  18. Flow field at 10º & 15º angle of attack Onset of stall 10º 15º STAR European Conference 2010

  19. Turbulence models - lift FX60-126 - Aerofoil data Cl and Cd from CFD 2D profile simulation 2.50 15º 2.00 10º 1.50 Lift Coefficien Cl 1.00 Cl CFD Coarse k-e Cl Stuttgart : FX 60-126 - Rey=2e6 0.50 k-e low Rey mesh k-w low Rey mesh Spalat-Almaris RS-2l 0.00 k-e_V2-f -10 -5 0 5 10 15 20 25 k-w_trans -0.50 Angle of attack ( α ) STAR European Conference 2010

  20. Turbulence models - drag FX60-126 - Aerofoil data Cl and Cd from CFD 2D profile simulation 0.06 Cd CFD Coarse k-e Cl Stuttgart : FX 60-126 - Rey=2e6 0.05 k-e low Rey mesh k-w low Rey mesh-refine1 15º Spalat-Almaris 0.04 Drag Coefficient (Cd) RS-2l 10º k-e_V2-f k-w_trans 0.03 0.02 0.01 0 -10 -5 0 Angle of attack ( α ) 5 10 15 20 25 STAR European Conference 2010

  21. Pressure Coefficient Pressure Coefficient 5000 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 -5000 k-e low rey -10000 Skin Friction Coef. k-w -15000 Spalat-Almaris -20000 RST_2l -25000 k-e v2f -30000 -35000 Position (m) STAR European Conference 2010

  22. Skin Friction Coefficient Skin Friction Coefficient 300 250 k-e low rey 200 k-w Skin Friction Coef. Spalat-Almaris 150 RST_2l 100 k-e v2f 50 0 0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 1 Position (m) STAR European Conference 2010

  23. Summary Pressure vs. Shear Pressure vs. Shear drag @ 10deg & 15deg angle of attack 120% 15deg Pressure 15deg Shear Pressure Shear 10 deg Average 68% 32% 10deg Pressure 10deg Shear 100% 15 deg Average 86% 14% 80% 60% 40% 20% 0% k-e low Rey RS_2l k-e_V2-f k-w low Rey k-w_sst Spalat-Almaris mesh mesh STAR European Conference 2010

  24. Pressure vs. Shear  On average at 15º angle of attack the drag due to pressure accounts for 86% of the drag as opposed to 68% for an angle of attack of 10º.  This leads one to suspect that the pressure drag may be the component which is mainly to blame  Further mesh refinement studies could confirm and/or quantify this assumption.  Better definition of the profile geometry could reduce the shear drag.  Sensitivity to inlet turbulence levels still has to be investigated STAR European Conference 2010

  25. Summary and Conclusions  Lift and stall point are predicted with a high degree of accuracy even with relatively coarse meshes using the Realizable κ - ε turbulence model with an all Y+ wall function formulation.  Drag however is highly over predicted with all turbulence models that were tested. This coincides with the higher power predicted in detailed fan simulations.  Further work has to be performed on mesh sensitivity studies as only 2 mesh sizes have presently been investigated.  Experimental work is underway at Universities to evaluate drag and lift forces explicitly in order to obtain a further set of independent aerodynamic data STAR European Conference 2010

  26. Thank you for your time ! Questions? 14 th IAHR Conference – December 2009

  27. 14 th IAHR Conference – December 2009

  28. Mesh Sensitivity on Detailed Fan COARSE MESH (1.7 million cells) FINE MESH (5.3 million cells) STAR European Conference 2010

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