Assesment of a Kinetic Eddy Simulation Turbulence Model for 3D Unsteady Transonic Flows
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Transcript of Assesment of a Kinetic Eddy Simulation Turbulence Model for 3D Unsteady Transonic Flows
American Institute of Aeronautics and Astronautics 092407
1
Assessment of a Kinetic-Eddy Simulation Turbulence Model
for 3D Unsteady Transonic Flows
Jeremy J. Bain1 and Sumit S. Mishra
2
INTECH Software Solutions, Inc.
Lakshmi N. Sankar3 and Suresh Menon
4
School of Aerospace Engineering, Georgia Institute of Technology
The Kinetic-Eddy Simulation (KES) turbulence model has been evaluated for a variety of
unsteady and oscillating wing transonic flows. KES is a two equation VLES/LES model that
solves for the unresolved kinetic energy and the local turbulent length scales without any
dependency on grid spacing. KES was used in OVERFLOW and compared to standard
models. KES showed improved ability to capture the negative lift curve slope and separated
flow of the NACA0036. In dynamic stall, KES improved prediction of peak lift, drag, and
pitching moment. In transonic flows, KES was able to improve modeling of separated flow at
the wing-body connection of the DLR-F6 wing-body configuration but over predicted drag.
Unsteady oscillating transonic flow over a scaled F-5 wing also showed improved prediction
with KES.
I. Introduction
NE of the most difficult challenges in Computational Fluid Dynamics (CFD) is accurately modeling separated,
unsteady, compressible, high Reynolds number flow. Most fixed wing aircraft are designed to avoid large
regions of separated flow but this is often not possible for rotorcraft. Rotorcraft hubs and pylons are often blunt
bodies that are sometimes covered with thick airfoils to reduce separation to a limited degree. They are located in
the unsteady wake of the main rotor further complicating accurate flow prediction. The retreating blade is often
operated at or beyond its stall limit. The motion of the rotor blade is coupled between the aerodynamic forces and
the rotor flap, torsion, and lead-lag motion. Accurate prediction of these flows is extremely challenging. They are
highly unsteady and require time accurate prediction of forces and moments.
Most CFD codes in industry and academia are based on the compressible Reynolds Averaged Navier-Stokes
(RANS) equations and use one or two equation turbulence models. This typically yields acceptable results for
steady, attached flow. RANS turbulence models fail to accurately predict separated flow structures because they
attempt to model all scales and frequencies of turbulence. Direct Numerical Simulation (DNS) can model all scales
of turbulence but requires extremely dense grids and comes at a computational cost that is prohibitive for most flows
of interest. Large-Eddy Simulation (LES) computes the largest turbulence structures and then models the sub-grid
unresolved structures. LES has shown improved predictions but still require too dense of grids for routine
engineering calculations.
Over the past decade, researchers have been working on creating hybrid turbulence models that can capture some
of the benefits of LES models but use standard RANS CFD codes. Spalart extended the Spalart-Allmaras (SA)
model to compute eddy viscosity near the wall using traditional SA model1 and switched to a pseudo Smagorinsky
LES model away from the wall2. This approach, called Detached Eddy Simulation (DES), has been implemented
with other turbulence models like k-ω and Menter’s SST3,4,5,6
.
1Research Engineer, 5655 Peachtree Pkwy., Suite 200 Norcross, GA 30092, Student Member, AIAA
2Proposal Manager, 5655 Peachtree Pkwy., Suite 200 Norcross, GA 30092, Student Member, AIAA
3Regents Professor and Associate Chair (Academic), School of Aerospace Engineering, Georgia Institute of
Technology, Atlanta, GA, 30332-0150, Associate Fellow, AIAA. 4Professor, School of Aerospace Engineering, Georgia Institute of Technology, Atlanta, GA, 30332-0150, Associate
Fellow, AIAA.
O
26th AIAA Applied Aerodynamics Conference18 - 21 August 2008, Honolulu, Hawaii
AIAA 2008-7176
Copyright © 2008 by Jeremy Bain, Sumit Mishra, Lakshmi Sankar, and Suresh Menon. Published by the American Institute of Aeronautics and Astronautics, Inc., with permission.
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The k-ω-SST model has been demonstrated to work well for a number of steady and unsteady applications.
However, in some cases where massively separated flows occur, this model has a tendency to under-predict the flow
separation even on extremely fine grids7. In an attempt to overcome these deficiencies, the present researchers and
their coworkers have been exploring a variety of turbulence models that fall under the classification of “hybrid
RANS-LES (HRLES) models.” One particular version of the HRLES model, called the subgrid Kinetic-Eddy
Simulation (KES) has been implemented in a number of in-house flow solvers at Georgia Tech and in the NASA-
Army flow solver OVERFLOW 2.08,9,10
. The KES model was found to work well in 2-D static stall, 2-D dynamic
stall, and 3-D dynamic stall occurring on helicopter rotors in forward flight.
II. Research Objective
The motivation behind this work to apply the KES model to a variety of steady and unsteady flows is to identify
its strengths and limitations, and to identify areas of future research. The NACA0036 thick airfoil was chosen due to
available computational results with other turbulence models in OVERFLOW. NACA0012 dynamic stall tests were
chosen to be representative of helicopter airfoils. The DLR-F6 wing-body configuration from the 2nd
AIAA CFD
Drag Prediction Workshop was chosen due to the difficulty in prediction of separated flow at the wing-body
connection and to asses the ability of KES to predict a transonic flow. The F-5 wing was chosen to asses the ability
of KES to predict unsteady oscillating transonic flow similar to the advancing rotor blade in high speed forward
flight. In all these simulations, KES results are compared with the Spalart-Allmaras1 (SA) turbulence model. SA is
considered the baseline due to its wide spread use in OVERFLOW and robustness11
.
III. Numerical Formulation
The KES model is briefly described below. The reader is referred to Ref. 8 and 9 for a more complete description
of this model. Kinetic-Eddy Simulation (KES) is a significant departure from the strategies in either HRLES12,13
or DES-k-ω−SST. The KES method directly estimates the local unresolved kinetic energy and the local
characteristic length scale corresponding to this unresolved kinetic energy via the solution of the two transport
equations for k and kl. This model solves for the subgrid ksgs
and klsgs
for the subgrid velocity scale, sgs
k and
the subgrid length scale, lsgs
. The transport equations for ksgs
and klsgs
are
( )3 2
,Pr
sgssgssgs sgs
sgsi i t
ij k sgs
i i i k i
ku k uk kC
t x x l x xε
ρ νρ ντ ρ ρ
σ
∂ ∂∂ ∂ ∂+ = − + +
∂ ∂ ∂ ∂ ∂
ɶ ɶ (1)
( ) ( ) ( ) ( )3 2
,Pr
sgs sgs sgs
sgs sgs sgsi i t
l ij kl
i j i kl i
kl u kl kluC l C k
t x x x xε
ρ ρ νντ ρ ρ
σ
∂ ∂ ∂∂ ∂+ = − + +
∂ ∂ ∂ ∂ ∂
ɶ ɶ (2)
While KES is an LES methodology, in situations where the local grid resolution is inadequate, the KES model
smoothly transitions from LES to Very Large-Eddy Simulation (VLES) with only the very largest scales resolved. In
a very fine grid where the subgrid length scale and subgrid kinetic energy goes to zero, KES asymptotically becomes
a DNS simulation. The ability to smoothly transition from LES to VLES is a unique feature of the KES model,
which can be considered a VLES-LES model. Furthermore, there is no a priori assignment of where VLES or LES
dominates since the transition between the two methods occurs naturally as a part of the solution.
The KES model does not depend on non-physical parameters like grid spacing to determine the length scales of
the turbulent eddies. It has relatively few tunable constants, allowing the application of this model to broad variety
of configurations and flows, ranging from airfoils to helicopter rotors to 3-D mixing layers. It has the following
additional features:
• Subgrid length scale is solved locally
• Dissipation of kinetic energy depends on the SGS length as well as length scale gradient
• No wall-distance is employed as in conventional Detached Eddy Simulation schemes
A “law of the wall” type approach is used to specify the ksgs
and lsgs
values at the first point off the wall using
the following equations,
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( )0.5
110.25
sgs
i ik v u u= ∆ɶ ɶ (3)
( )2
10.53
sgs sgsl k v= ∆ (4)
where ∆1 is the grid length scale of the first cells and ν is the kinematic viscosity. These values are based off of
energy dissipation rates at the wall8. At the wall, they are set to zero. At the far field boundary condition, k
sgs is set to
( )2
0.016u∞
and lsgs
is set to the local grid length scale.
The numerical calculations used the compressible Reynolds Averaged Navier-Stokes computational fluid
dynamics code OVERFLOW14,15
. OVERFLOW uses overset structured grids and has been used for a wide variety
of fixed wing and rotorcraft problems16,17
. OVERFLOW has numerous spatial and temporal options. Version 2.0y
with modifications made under the Defense Advanced Research Projects Agency (DARPA) Helicopter Quieting
Program was used18
. These modifications include the addition of HRLES and KES turbulence models as described
in Ref. 10.
OVERFLOW was run on an eight node, dual 2.4 GHZ AMD Athlon Processor cluster. This solver has been
parallelized using the Message Passing Interface (MPI) library, and was run on multiple processors for all
calculations except for the relatively simple NACA0012 calculations. All the simulations reported here were done
with 4th
order central differencing in space, and dual timesteps. It was necessary to use 4-10 Newton sub-iterations.
IV. Numerical Simulations and Discussions
A. NACA0036
The NACA0036 has been the subject of recent computational and experimental studies. Experimental studies
have been performed at the NASA Ames Fluid Mechanic Lab (FLM) 32”x48” low speed open-draft wind-tunnel19
and the California Polytechnic State University – San Luis Obispo (Cal Poly) 3x4 ft low speed, open-return wind
tunnel20,21
. Computational studies of this airfoil are particularly difficult due to the highly separated flow that occurs
at angle of attack. At AFDD, Potsdam studied this airfoil in OVERFLOW with numerous turbulence models in both
2D and 3D studies22
. The 2D grid consists of a 573x81 body fitted O-grid and a 140x80 Cartesian grid to model the
wind tunnel walls with inviscid boundary conditions. In two dimensions, none of the standard RANS one and two
equation turbulence models tested in the OVERFLOW were able to capture the negative lift curve slope. A 3D grid
was created and run with the hybrid RANS/LES (DES) models available in the newest versions of OVERFLOW4,11
.
These models showed improvement in capturing the effects of the separated flow and the wind tunnel wall effects
but at greatly increased computational cost. The 2D grids were run with KES in time accurate mode using the same
nondimentional timestep of 0.001 that was used on the 3D runs by AFDD. KES was able to capture the negative lift
curve slope and had similar results to the SSTDES fine 3D grid results as shown in Figure 1. Instantaneous
streamlines in Figure 2 show the flow highly separated on the upper surface. While KES has higher cost in 2D due
to the requirement for physical time steps and longer convergence time, it is significantly cheaper than the full 3D
runs.
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Figure 2. Instantaneous Streamlines with KES of NACA0036 at 10 degrees Angle of Attack
B. NACA0012
The NACA0012 is a common airfoil in helicopters for its moderately high maximum lift and low pitching
moment. Dynamic stall is a dominating factor in forward flight and can limit the operational envelope of a
helicopter. In forward flight, the advancing blade encounters additional velocity due to the free stream and the
retreating blade encounters a reduced velocity. The lift generated on the advancing and retreating side needs to be
balanced to avoid a large rolling moment necessary to trim the vehicle. This leads to the retreating blade operating
near its maximum lift capability while the advancing blade is at low or negative incidence. This causes the blade to
undergo dynamic stall cycles as the blade rapidly goes from low to high incidence causing large negative pitching
moments, high vibration, and buffeting. The high negative pitching moment that occurs causes an elastic
deformation in the rotor blade that causes further pitch changes. This presents significant challenges in modeling due
to the effect of leading and trailing edge shedding. In the experiment of McCroskey et al23
, several airfoils are
studied in light, moderate and deep stall. A C-grid was generated to have y+=1, 547 chordwise points, and 105
Figure 1. KES 2D Results Compared to 2D (Left) and 3D (Right) Results using Various Turbulence
Models (Ref 22)
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points in the normal. The static CL was calculated using SA and KES compared for a slowly increasing angle of
attack (k=0.001) with 150,000 timesteps in Figure 3. KES captures the maximum lift of 1.29 at 13.4° that is within
the experimental scatter. SA predicts a maximum lift of 1.43 at 14.8°. After the stall, SA smoothly decreases
smoothly while KES shows the unsteady fluctuation of vortex shedding. To capture the unsteady effects of dynamic
stall, 35000 timesteps per cycle were run for 2.5 cycles. Figure 4 compares SA and KES results for deep stall. At
low angles of attack, the two models have similar results as expected. The SA model overestimates the peak lift,
drag, and pitching moment while the KES model does a significantly better job predicting these critical quantities.
Figure 4. NACA0012 Dynamic Stall M=0.3, k=0.1, αααα=15° + 10° sin(ωωωωt)
Figure 3. Static NACA0012 Lift with SA and KES
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Table 1. Results for CL=0.5, Mach 0.75
CL CD CM
Experiment 0.500 0.0275 -0.121
SA 0.501 0.0284 -0.0907
KES 0.4999 0.0347 -0.0923
Figure 5. 2
nd AIAA CFD Drag Prediction Workshop Wing Body Medium Grid
C. Drag Prediction Workshop Wing Body Configuration
Since 2000, the AIAA has organized four CFD Drag Prediction Workshops to test the ability of a variety of CFD
solvers to calculate the drag on generic transport aircraft configurations24
. OVERFLOW was used extensively on the
various configurations on a series of progressively finer grids25,26
. The DLR-F6 wing-body configuration from the
second workshop was selected for further study with KES. This configuration had separated flow at the wing-body
juncture that was over predicted using the SA1 and Baldwin-Barth turbulence models
27.
The flight condition selected represents the cruise design point of Mach number = 0.75, CL = 0.5, and Reynolds
number of 3 million. An initial run was completed using the SA turbulence model and the medium grid provided to
the authors. The medium grid consists of twelve overset grids and approximately 6.8 Million points, shown in
Figure 5, created following accepted best practices28,29
. The grids were created using Chimera Grid Tools and
PEGASUS30,31,32
. More details of the grid generation can be found in Ref. 28. KES was run with the same
computational options as the SA baseline but with a physical time step of 0.01 nondimensionalized by freestream
velocity and no multigrid acceleration. The physical time step is required by KES. The KES run took approximately
twice as long to run due to the greater number of physical time steps required for convergence.
As shown in Table 1, KES overestimates the drag. Figure 6 has the surface pressure contours and Figure 7 has
the locations of supersonic flow. The shock location using KES occurs upstream of the SA prediction. The suction
peak was also under predicted compared to SA. The separation bubble at the wind body connection was better
predicted with KES. The width of the bubble is shown in Table 2 and instantaneous streamlines in Figure 8.
Table 2. Separation Bubble Width
Separation
Size (mm)
∆mm
Experiment (Ref 25) 90.9 -
SA 96.8 5.9
KES 89.4 -0.6
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Figure 6. Upper Surface CP Distribution with SA (left) and KES (right) for CL=0.5
Figure 7. Predicted Locations of Supersonic Flow (Grey) near the wingtip with SA (left) and KES (right)
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Figure 8. Instantaneous Streamlines near Wing Body Connection with SA (left) and KES (right)
Figure 9. F-5 Grid (Every 2
nd Point in each direction removed)
D. F-5 Wing
A scaled F-5 wing has been tested for a variety of transonic steady and unsteady conditions. The experiment of
Tijdeman et al. had eight spanwise stations instrumented to capture steady and unsteady pressures33,34
. The wing has
a semi-span of 0.6476m, a taper ratio of 0.281, leading edge sweep of 31° and a modified NACA 65-A-004.8 airfoil.
A variety of types of solvers have studied this configuration including potential flow35
, Euler36
, Navier-Stokes37,38
,
and hybrid Navier-Stokes/Full-Potential39,40
solvers.
The F-5 grid was created utilizing best practices in OVERFLOW grid generation including those established
during the Drag Prediction Workshop28,29
. The grid corresponds to a medium grid and consists of approximately 3
million points and is shown in Figure 9. For hole cutting, xrays were used30
.
To simulate the combined bending and torsion aeroelastic response of the F-5 wing, grid deformation routines
were added to OVERFLOW. The method used followed the method of Morton41
that was used by previous
researches and the authors in OVERFLOW42,43
. The deformed surface is calculated using the measured mode
shapes44
. The points in the normal direction are then calculated to maintain grid orthogonality. As the distance from
the surface increases, a cubic spline is used to blend the deformed grid and the original grid. This maintains the grid
spacing and outer boundary of the original grid.
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Figure 10. Surface Pressure Contours over the Upper Surface of the F-5 Wing using SA (left) and KES
(right) at Zero degrees Angle of Attack and Mach 0.9
Figure 11. Surface Pressure Distribution over F-5 Wing at 35.2% Span (left) and 72.1% Span (right) at Zero
Angle of Attack, Mach 0.9
Steady runs were done at zero degrees angle of attack at Mach 0.9. The upper surface pressures are shown in
Figure 10 and compared with experimental data at two span stations in Figure 111. The real and imaginary
components of surface pressure during a 20Hz oscillation are shown in Figure 12. The SA results show a stronger
shock than the experimental and KES data. The unsteady results using KES show good correlation with
experimental data. The SA results showed the effect of overestimating the shock around x/c=0.6.
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V. Conclusions
The Kinetic Eddy Simulation turbulence model has been evaluated for a variety of unsteady low speed and
transonic flows. In areas of separated flows, KES showed improved predictions over standard RANS turbulence
models while smoothly transitioning between VLES and LES. In transonic flows, KES overestimated drag from
improper shock placement. This deficiency may stem for specifying the ksgs
and lsgs
at the first point off the wall.
The HRKES45
model overcomes this problem by using k-ω-SST near the wall and then smoothly transitioning to
KES away from the wall. Work is also ongoing to reduce and eventually eliminate the six empirical constants in
KES.
Acknowledgements
This work was funded under a NASA SBIR project entitled “Advanced Turbulence Models for Unsteady and
Stalled flows.” Ethan Romander is the technical monitor. The authors would like to thank Mark Potsdam of AFDD
for providing the NACA 0036 grids and Joe Morrison of NASA Langley for access to the AIAA CFD Drag
Prediction Workshop grids. The authors also thank Mina Zaki for discussions on KES and the HRKES model.
References
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Synthetic Jet Flow Control,” AIAA 24th Applied Aerodynamics Conference, San Francisco, CA June 2006, AIAA 2006-3157 22 Potsdam, M., Le Pape, A., “CFD Investigations on a NACA0036 Airfoil with Active Flow Control” 4th AIAA Flow
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