wp6: cd airfoil test-case experimental and numerical data base
DESCRIPTION
WP6: CD Airfoil Test-case Experimental and numerical data base. S. Moreau VEC Manager of the Fan System Core Competencies Manager of the Group Simulation Competency Center. October 200 8. ECL Experimental Set-up, LMFA. RMP. 11. RMP. 26. Thickness 4%. Camber 12°. - PowerPoint PPT PresentationTRANSCRIPT
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WP6: CD Airfoil Test-caseExperimental and numerical data base
October 2008 S. Moreau
VEC Manager of the Fan System Core CompetenciesManager of the Group Simulation Competency Center
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Airfoil chord length ~10 cm smUsm /40/16 0
Valeo CD and NACA12 airfoils, Flat Plate, V2 and V3 airfoils
Nozzle exit section 50 cm x 25 cm
RMP
Camber 12°Thickness 4%
RMP 11
26
Open-Jet Aeroacoustic Experiment in ECL Large Wind Tunnel
ECL Experimental Set-up, LMFA
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CD Airfoil Experimental Data Base
Open-Jet Aeroacoustic Experiment in ECL Large Wind Tunnel
Moreau et al, AIAA J. 2004, 2005, JFE 2005
Valeo CD Airfoil: Re 1.5 105 ; M 0.05 ; several angles of attack (8° focus)Far field noise measurements: Noise spectra and directivities Remote Microphone Probe (RMP) measurements: Wall pressure statistics (Cp, frequency spectra, coherence, phase)Hot wire measurements: Velocity statistics (mean and RMS velocity components, Reynolds stress and frequency spectra)
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CD airfoil in high loading conditions
Flat plate at zero angle of attack
Evidence of 2 mechanisms: vortex-shedding noise and trailing-edge noise
Experimental Far Field Noise
Spectrum
Directivity
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5
70
60
50
40
30
Wal
l pre
ssur
e sp
ectr
a (d
B)
102
2 3 4 5 6 7 8
103
2 3 4 5 6 7 8
104
Frequency (Hz)
RMP 11 RMP 21 RMP 22 RMP 23 RMP 24 RMP 26
Wall pressure fluctuations must be statistically homogeneous
is deduced from coherence measurements
)(l y
d),()(l y
0
2
is deduced from the phase diagrams of streamwise cross spectra
cUGaussian model proposed (Roger & Moreau, AIAA 2002-2460).
Equivalent Corcos’ model
Experimental Wall Pressure Statistics
f-5
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Hot Wire Measurements
Wake Zoom
Overview
Inlet surveyLES bc survey
Shear layer survey
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leading edge
separation line
Reattachment of the
flow
Separation
bubble
Suction side streaklines
Direction of the flow
turbulent
laminar
Flow Visualization on CD Airfoil
« Oil » Flow Tuft Film
MVI_9612.avi
Evidence of laminar flow separation at the leading edge Possible flow separation at the trailing edge
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Two families of results
k-, SST and V2F
k- TL and WL
Numerical Wall Pressure Coefficient
Moreau et al, AIAA J. 2003
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Two families of results
k-, SST and V2F
k- TL and WL
Numerical Wall Friction Coefficient
Moreau et al, AIAA J. 2003
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Comparison of Wall Pressure Coefficients
Good prediction of laminar flow separation at the leading edge No prediction of onset of trailing edge flow separation
SST model
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Broadband Models: Generalized Amiet - 1
3 main mechanisms considered:
Tip and leakage flow are not considered yet
1 - Turbulence-interaction noise
2 - Trailing edge noise
3 - Vortex-shedding noise
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Broadband Models: Generalized Amiet - 2
Turbulence Interaction Noise:
Trailing Edge Noise:
2
0
2
01
0
2
00
2
20
30 ,,),(22
),(
S
xk
UxL
S
xk
U
dU
S
xckxS wwpp
x
yz
)x,x,x(x 321
)y,x(S
0U
2
0
21
0
2
2
20
3 ,,,)(2
),(
S
xk
UxL
S
xkd
S
xckxS ypppp
wall-pressure spectrum
Inflow velocity statistics
Spanwise correlation length
Radiation integrals(including back-scattering
correction)
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Stanford LES Set-up & Averaged Results
Choose the largest jet width (w = 50 cm) LES domain in the jet core, with velocity B.C.'s coming from
RANS (only mean values) Better prediction of leading edge flow (Cp) with LES
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Grid for Stanford LES
• Single block-structured topology• Grid Size: 960 x 84 x 64 5.2 million nodes• Domain Size: (4 x 2.5 x 0.1) x chord (first LES able to resolve the spanwise coherence length)
Very regular, fine and orthogonal grid at LE
Stanford Reference LES grid in 2D slice (2003)
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Grid Quality/Parameters of Stanford LES
• Almost a DNS resolution in the normal direction• Very regular and orthogonal grid near airfoil • Grid independence of the solution verified on pressure spectra• Energy-conserving hybrid finite-difference/spectral code• Dynamic sub-grid-scale model
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Stanford LES Instantaneous Results
Leading-edge separation leading to transition on suction side Laminar boundary-layer on pressure side
Qualitative agreement with experimental observation
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2D vs 3D LES Instantaneous Results
NACA0012 Re ~ 5-9 105 and M~0.2
Drastic change of flow topology after transition
3D 2D
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#26
Experiment
LES
Stanford Broadband Noise (BBN) Sources
Excellent qualitative and quantitative agreement
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Stanford BBN Prediction
Good agreement of both analogies with experimental data Effect of finite-chord up to 2 kHz
Discrepancy between the two analogies at high frequencies
Acoustic Analogies based on wall pressure statistics (Amiet) and on velocity statistics near the trailing edge (Ffowcs-Williams
and Hall)
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Evaluation of Other Unsteady Methods
Starting from the same “LES domain” with the same RANS boundary conditions and, if possible, the same LES grid:
Unsteady RANS: no unsteadiness was observed
Detached Eddy Simulations (DES-SA within Fluent 6.1)
Lattice Boltzmann (RANS/DNS) > Powerflow (EXA)
LES with Immersed Boundary Technique
Moreau et al, CTR Summer Program 2004
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Grid and Simulation Parameters of SP-2004
Moreau et al, CTR Summer Program 2004
LBM: Powerflow 6.1.22 (3ddp) Grid: 73551 voxels and 1491 surfels in a 2D slice (~1.2 M in 3D)
Smallest cell at LE is similar to body-fitted LESModel: RANS k- in 2D - No model in 3DSimulation parameters: (Re=1.5 105)
Time step: t =2.0e-7
CPU time for 100 time steps: 5 minutes on SGI Octane (1 CPU)
LES-IB: Structured Cartesian (PhD: S. Kang)Grid: 4.8M in 3D (0.15M in a 2D slice)
Smallest cell at LE is ~2.5 larger than body-fitted LESModel: LES + Dynamic ProcedureSimulation parameters: (Re=1.5 105)
Time step: t =1.0e-4
CPU time for 100 time steps: 20 minutes on Linux cluster (8 CPU)
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SP-2004 (Stanford) Grids
Reference LES DES-SA
LBM-DNS LES-IB
1-2 coarsening
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SP-2004 (Stanford) Flow field Results
Reference LES DES-SA
LBM-DNS LES-IB
Instantaneous Velocity Field
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SP-2004 (Stanford) Wall Pressure Coefficient
Moreau et al, CTR Summer Program 2004
2.5
2.0
1.5
1.0
0.5
0.0
-0.5
-1.0
Pre
ssur
e C
oeff
icie
nt
1.00.80.60.40.20.0
Normalized distance
Experiment RANS (v2f) LES DES IB-LES
2.5
2.0
1.5
1.0
0.5
0.0
-0.5
-1.0
Pre
ssur
e C
oeff
icie
nt
1.00.80.60.40.20.0
Normalized distance
Experiment RANS (v2f) LES LB-RANS LB-DNS
Only IB-LES provided a complete flow field close to reference LES
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SP-2004 (Stanford) Wake Velocity Profiles
Moreau et al, CTR Summer Program 2004
Two coarse grids in any of the new simulations to yield good wake
X-wire
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SP-2004 (Stanford) Flow field Results
DES gives unrealistic flow field (over production of k at LE) Grids for IB-LES need to re-visited for better TE prediction
All over estimate the pressure fluctuations at low frequencies
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STAR-CD LES Simulations (2005-2006)Moreau et al, AIAA 2005-2916
PISO algorithm for time discretization
Central differencing and upwind MARS scheme (no stable solution could be obtained even in 2D with CDS for all grid topologies tested).
To keep a CFL number below 1 throughout the computational domain, a maximum allowable time step t = 1.5 10-5 s is used.
5 to 10 time units run to eliminate the transient and collect reliable statistics (based on the free stream velocity of 16 m/s).
Smagorinsky sub-grid scale (SGS) model together with a van Driest near-wall damping and WALE SGS are used.
k- based DES is selected.
Evaluation of different numerical Schemes Evaluation of different SGS models
Re-assessment of the DES model with a different code
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Final MARS LES Grid Topology (2005)
Zoom LE Zoom TE
1,115,000 cells• Similar grid 1-2 coarsening as DES with Fluent 6.1• Only 5% chord span• Good near-surface resolution: x+≤ 20 ; y+≤ 1 ; z+≤ 10
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MARS LES Instantaneous Velocity Field
Stanford Reference LES STAR-CD MARS LES
Similar small structures created after separation convected downstream towards the trailing edge
Larger flow separation at the leading edge in MARS LES.
More coherent structures at the trailing edge in MARS LES.
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MARS LES Wall Pressure Coefficient
Qualitative agreement on the laminar separation bubble (good level of pressure plateau but too large extent of the bubble, 11.2% instead of 3.7%)
First simulation to predict the positive pressure gradient up to mid-chord.
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MARS LES Wake Velocity Profiles
Excellent agreement in the near wake for the MARS LES
Too large diffusion and deflection of the wake in the DES.
-0.2
-0.1
0.0
0.1
0.2
y/c
1.00.90.80.70.6
x-velocity
Experiment present LES
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MARS LES Wall Pressure Spectra
Too high levels everywhere
No homogeneous statistics close to TE
P2
P8
P14P60
P60: mid-chord (-60 mm)P14: -14 mmP8: -8 mmP2: -2 mm
Origin: TE
• Too large structures and coherence at the trailing edge• Fluctuations are getting damped towards TE (MARS upwinding)
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MARS Fine Scale Structures
Turbulent re-attach.Turbulent T.E.Separation
Laminar L.E. separation
Iso-values of normalized Q colored by the streamwise vorticity
Larger structures than reference LES
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DES Simulation Issue
Velocity Field Sub-grid Turbulent Viscosity
Well attached flow field all the way to the trailing edge as in RANS simulations
Short laminar separation bubble is not captured
Transition occurs at the stagnation point (local turbulent kinetic energy overproduction in k- model).
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Conclusions Summer 2005
The STAR-CD MARS LES reproduces all qualitative features of the flow encountered in the ECL experiment and simulated in the reference LES (Wang et al, Stanford 2004).
A short laminar separation bubble is formed, reattaches and sheds small vortices that are convected towards the trailing edge.
Evolution of the boundary layer seems to be well captured, especially the experimental positive pressure gradient up to mid-chord.
Yet the laminar separation bubble is too wide and the wall pressure fluctuations are damped at the trailing edge (most likely due to MARS upwind scheme). No use for self-noise prediction.
All DES found inadequate for this attached flow (transitional airfoil with a short laminar bubble).
Further grid optimization required to remove instabilities with Central Differencing Scheme (CDS).
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Final CDS LES Grid Topology (2006)
690,000 cells
• 3-4 grid coarsening in all directions• 10% chord span• Good near-surface resolution: x+~ 2.5 ; y+~ 2 ; z+~ 3.6
3-4 coarsening
Stability of CD scheme without significant oscillationsOnly a small jump in the turbulent viscosity
D. Laurence, VKI Lecture Series 2005Y. Addad, PhD UMIST
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CDS LES Wall Pressure Coefficient
Same qualitative agreement on the laminar separation bubble
No significant differences between the two SGS models
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CDS LES Wake Velocity Profiles
Same excellent agreement in the near wake for the CDS-LES
No significant differences between the two SGS models
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CDS LES Wall Pressure Spectra
Good overall predicition with the CD SGS model has only a moderate effect on spectra
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Iso-values of normalized Q colored by the streamwise vorticity
t = 0.07 s
t = 0.25 s
CDS Fine Scale Structures
Smaller structures than with MARS scheme
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SP-2006 (Stanford) Unstructured LES
Excellent agreement with both structured LES and experimental data
Comparison of Urms
0.000
0.020
0.040
0.060
0.080
0.100
0.120
0.140
0.160
0.180
-0.100 -0.080 -0.060 -0.040 -0.020 0.000 0.020 0.040 0.060 0.080 0.100 0.120
y/C
Urm
s/U
ref
2005 Wake Data (18 Jan) @ x/C = 0.057356
2003 LES (M. Wang) Wake Data @ x/C = 0.057356
2006 LES (CDP 2.3) Wake Data @ x/C = 0.05736
103
104
-110
-100
-90
-80
-70
-60
-50
-40
f (Hz)
Pow
er S
pect
ral D
ensi
ty (
dB)
Wake Spectra at x/c = 0.057356
EXP (y/H = 0.00038238)
LES (y/H = -0.00045381)
x/C = 0.057356
0,0
0,2
0,4
0,6
0,8
1,0
1,2
-0,100 -0,080 -0,060 -0,040 -0,020 0,000 0,020 0,040 0,060 0,080 0,100
y/C
Vm
ag/U
ref
2005 ECL Experiment
2003 RANS-V2F
2004 LES (M. Wang)
2006 LES (CDP 2.3)
<4% difference
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Conclusions Summer 2006
The STAR-CD CDS LES improves the MARS LES significantly (over dissipative in the TE region) and compares favorably with the ECL experiment and the reference LES (Wang et al, Stanford 2004).
A regular grid with smooth jumps is required if coarsening is to be used to yield numerical stability and limited oscillations. (3-4) coarsening as suggested by Laurence seems to provide the best compromise and still yield reasonable grid sizes (< 1 Million nodes).
Different SGS models do not yield significant differences
Unstructured LES solver (CDP, Stanford) with the same numerical schemes and SGS as the reference structured LES yields similar results .
But all LES still show weaknesses in the laminar flow recirculation and especially in the transition process (we have as many bubble sizes as LES)
Yet in the trailing edge region, similar statistics are achieved and consequently same broadband noise prediction