Nonlinear Aeroelastic Analysis of Flexible High Aspect ...
Transcript of Nonlinear Aeroelastic Analysis of Flexible High Aspect ...
Nonlinear Aeroelastic Analysis of Flexible High
Aspect Ratio Wings Including Correlation With
Experiment
by
Justin W. Jaworski
Department of Mechanical Engineering and Materials ScienceDuke University
Date:
Approved:
Dr. Earl H. Dowell, Chair
Dr. Donald B. Bliss
Dr. Kenneth C. Hall
Dr. Laurens E. Howle
Dr. Lawrence N. Virgin
Dissertation submitted in partial fulfillment of the requirements for the degree ofDoctor of Philosophy in the
Department of Mechanical Engineering and Materials Sciencein the Graduate School of Duke University
2009
Abstract(Aerospace)
Nonlinear Aeroelastic Analysis of Flexible High Aspect Ratio
Wings Including Correlation With Experiment
by
Justin W. Jaworski
Department of Mechanical Engineering and Materials ScienceDuke University
Date:
Approved:
Dr. Earl H. Dowell, Chair
Dr. Donald B. Bliss
Dr. Kenneth C. Hall
Dr. Laurens E. Howle
Dr. Lawrence N. Virgin
An abstract of a dissertation submitted in partial fulfillment of the requirements forthe degree of Doctor of Philosophy in the
Department of Mechanical Engineering and Materials Sciencein the Graduate School of Duke University
2009
Copyright c© 2009 by Justin W. JaworskiAll rights reserved
Abstract
A series of aeroelastic analyses is performed for a flexible high-aspect-ratio wing
representative of a high altitude long endurance (HALE) aircraft. Such aircraft are
susceptible to dynamic instabilities such as flutter, which can lead to large ampli-
tude limit cycle oscillations. These structural motions are modeled by a representa-
tive linear typical section model and by Hodges-Dowell beam theory, which includes
leading-order nonlinear elastic coupling. Aerodynamic forces are represented by the
ONERA dynamic stall model with its coefficients calibrated to CFD data versus wind
tunnel test data. Time marching computations of the coupled nonlinear beam and
ONERA system highlight a number of features relevant to the aeroelastic response
of HALE aircraft, including the influence of a tip store, the sensitivity of the flutter
boundary and limit cycle oscillations to aerodynamic CFD or test data, and the roles
of structural nonlinearity and nonlinear aerodynamic stall in the dynamic stability
of high-aspect-ratio wings.
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To Warren, Melissa, and Bill
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Contents
Abstract iv
List of Tables viii
List of Figures ix
Nomenclature x
Acknowledgements xvii
1 Introduction 1
1.1 Research Questions and Outline . . . . . . . . . . . . . . . . . . . . . 2
2 Structural Models 4
2.1 Typical Section . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 5
2.2 Finite Element Analysis . . . . . . . . . . . . . . . . . . . . . . . . . 6
2.2.1 Step Depth . . . . . . . . . . . . . . . . . . . . . . . . . . . . 8
2.2.2 Ribs . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 9
2.2.3 Balsa Wood Fairings . . . . . . . . . . . . . . . . . . . . . . . 10
2.2.4 Tip Store . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
2.2.5 Combined Effects . . . . . . . . . . . . . . . . . . . . . . . . . 13
2.2.6 Theoretical-Experimental Comparison . . . . . . . . . . . . . 16
2.2.7 Mode Shapes . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
2.2.8 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . 18
2.3 Hodges-Dowell Nonlinear Beam Equations . . . . . . . . . . . . . . . 21
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3 Aerodynamic Models 24
3.1 Slender Body Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . 25
3.2 Theodorsen Theory . . . . . . . . . . . . . . . . . . . . . . . . . . . . 27
3.3 ONERA Dynamic Stall Model . . . . . . . . . . . . . . . . . . . . . . 28
4 Aeroelastic Formulations and Results 33
4.1 Typical Section with Theodorsen Aerodynamics . . . . . . . . . . . . 33
4.1.1 Eigenvalue Analysis . . . . . . . . . . . . . . . . . . . . . . . . 33
4.1.2 Conclusions . . . . . . . . . . . . . . . . . . . . . . . . . . . . 36
4.2 Hodges-Dowell Nonlinear Beam & ONERA Dynamic Stall Model . . 38
4.2.1 Equation Formulation and Time-Marching Scheme . . . . . . 38
4.2.2 Flutter Prediction . . . . . . . . . . . . . . . . . . . . . . . . . 40
4.2.3 Limit Cycle Oscillations . . . . . . . . . . . . . . . . . . . . . 43
4.2.4 Time Estimates for First-Principles Aeroelastic Model . . . . . 47
5 Conclusions 52
5.1 Future Work . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 55
A Time-Domain Computational Fluid Dynamics Solver 57
A.1 Fluid Equations . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 58
A.2 Reynolds Averaging . . . . . . . . . . . . . . . . . . . . . . . . . . . . 63
A.3 Turbulence Modeling . . . . . . . . . . . . . . . . . . . . . . . . . . . 65
B ONERA Model Parameter Identification 68
B.1 Static Lift Curve . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 69
B.2 Unsteady Parameters . . . . . . . . . . . . . . . . . . . . . . . . . . . 70
Bibliography 74
Biography 85
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List of Tables
2.1 Comparison of ANSYS and experimental natural frequencies for dN =0.5 . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 17
4.1 Typical section structural data . . . . . . . . . . . . . . . . . . . . . . 34
4.2 Coefficients for typical section model eigenvalue analysis . . . . . . . 35
4.3 Typical section flutter comparison with HALE wing data . . . . . . . 38
4.4 Experimental wing model data . . . . . . . . . . . . . . . . . . . . . . 41
B.1 Comparison of ONERA lift parameters based on wind tunnel and CFDdata . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 73
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List of Figures
2.1 Schematic of typical section on linear springs . . . . . . . . . . . . . . 5
2.2 ANSYS wing model schematic . . . . . . . . . . . . . . . . . . . . . . 7
2.3 Natural frequencies of a spar with varying step depth . . . . . . . . . 9
2.4 Natural frequency comparison of 2D and 3D spar with ribs, with vary-ing step depth . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 10
2.5 Natural frequencies of a spar with balsa wood fairings, with varyingstep depth . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 12
2.6 Natural frequencies of a spar with tip store, with varying step depth . 13
2.7 Combined structural effects on f1B for varying step depth . . . . . . . 14
2.8 Combined structural effects on f2B for varying step depth . . . . . . . 15
2.9 Combined structural effects on f1C for varying step depth . . . . . . . 15
2.10 Combined structural effects on f1T for varying step depth . . . . . . . 16
2.11 Flapwise mode shape comparison, with tip store . . . . . . . . . . . . 19
2.12 Chordwise mode shape comparison, with tip store . . . . . . . . . . . 20
2.13 Torsion mode shape comparison, with tip store . . . . . . . . . . . . . 20
2.14 Flapwise mode shape comparison, without tip store . . . . . . . . . . 21
2.15 Chordwise mode shape comparison, without tip store . . . . . . . . . 22
2.16 Torsion mode shape comparison, without tip store . . . . . . . . . . . 22
3.1 Schematic of ∆CL . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 30
4.1 V -g plot of HALE typical section model with steady aerodynamics . . 36
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4.2 V -g plot of HALE typical section model with quasi-steady aerodynamics 37
4.3 V -g plot of HALE typical section model with unsteady Theodorsenaerodynamics . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 37
4.4 Dependence of flutter speed on number of panels and aerodynamicevaluation location . . . . . . . . . . . . . . . . . . . . . . . . . . . . 42
4.5 Sensitivity of flutter speed to source data for linear ONERA modelparameters . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 43
4.6 Effect of nonlinear beam stiffness on LCO amplitude and hysteresis . 45
4.7 Bifurcation diagram for computational and experimental LCO results 48
4.8 Time series and FFT spectrum for large-amplitude LCO at U = 40.5m/s . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 49
4.9 Bifurcation diagram comparison of quasi-steady ONERA aerodynamicmodels . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . . 50
A.1 Physical grid for NACA 0012 airfoil . . . . . . . . . . . . . . . . . . . 62
B.1 Piecewise curve fit to CFD static lift data . . . . . . . . . . . . . . . 71
B.2 Comparison of static lift curves from original ONERA model, CFDdata, and experiment . . . . . . . . . . . . . . . . . . . . . . . . . . . 72
B.3 Lift hysteresis comparison of ONERA models with unsteady CFD data 73
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Nomenclature
τ nondimensional time, ωαt
g gravitational constant
H(i)n Hankel function of the ith kind of order n
t time
x, x spanwise position coordinate, x/L
′ d/dx = L−1 d/dx
δ Dirac delta
δij Kronecker delta
˙ d/dt
∗ ωα d/dτ
D/Dt substantial derivative
Structural
An normalization factor
b half chord, c/2
bs spar width
c, c chord length, c/L
Cξφ torsion damping coefficient, 2mK2ξφω1T
Cξv lag damping coefficient, 2mξvω1C
Cξw flapwise damping coefficient, 2mξwω1B
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cSB longitudinal length of slender body
dN notch depth nondimensionalized by bs/2
E modulus of elasticity
e, e distance from elastic axis to center of gravity, positive aft; e/L
EI1 flapwise (out-of-plane) flexural rigidity
EI2 lag (chordwise, in-plane) flexural rigidity
f frequency [Hz]
GJ torsional rigidity
h, h plunge displacement, eigenvalue variable
Iv tip store moment of inertia about axis of lag displacement
Iw tip store moment of inertia about axis of flapwise displacement
Iα second moment of inertia of typical section airfoil about the elastic axis
Iφ tip store moment of inertia about wing elastic axis
K, K wing radius of gyration about spanwise elastic axis, K/L
Kh linear plunge stiffness for typical section
Kα linear torsional stiffness for typical section
M mass of tip store
m wing mass per unit span
Pz fluid momentum in xz-plane due to slender body motion
R slender body radius
rα radius of gyration for typical section airfoil about the elastic axis,√Iα/(mb2)
S slender body cross-sectional area
Sα first moment of inertia of typical section airfoil about the elastic axis
ts spar thickness
v, v lag displacement, v/L
w, w flapwise displacement, w/L
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xα airfoil static unbalance, Sα/(mb)
y length coordinate of slender body
yB pitch axis of slender body
za longitudinal centerline position of slender body
a¯
distance from midchord to elastic axis, positive aft
β dimensional grouping for nonlinear stiffness, (EI2 − EI1)/(mL4)
βn nth torsional eigenvalue
χn nth flapwise eigenvalue
φ geometric twist angle, φ+∫ x
0v′w′′ dx
λn nth bending eigenvalue
ν Poisson ratio
ω frequency [rad/s]
ωh plunge structural frequency for typical section model,√Kh/m
ωα torsional structural frequency for typical section model,√Kα/m
φ twist about deformed elastic axis, positive nose up
ψn nth lag eigenvalue
ρm material density
Θn nth torsional mode shape
ξv modal damping coefficient for lag bending modes
ξw modal damping coefficient for flap bending modes
ξφ modal damping coefficient for torsion modes
–V1 slender body volume
–V2 slender body volume static unbalance
–V3 slender body volume moment of inertia
Aerodynamic
xiii
∆Fv slender body aerodynamic force in lag direction
∆Fw slender body aerodynamic force in flap direction
∆Mx slender body aerodynamic moment
a a nonlinear ONERA load coefficient, a0 + a2(∆CL)2
a0L linear lift curve slope
C(k) Theodorsen function
CD coefficient of drag
CL coefficient of lift
CM coefficient of moment
Cz total ONERA aerodynamic load, Cz1 + Cz2
Czγ circulatory contribution to ONERA aerodynamic load
Cz1 linear ONERA aerodynamic load
Cz2 nonlinear ONERA aerodynamic load contribution from dynamic stall
D drag
dD/dx sectional drag on wing section
dFv/dx sectional aerodynamic force in lag direction
dFw/dx sectional aerodynamic force in flap direction
dL/dx sectional lift on wing section
dM0/dx sectional moment on wing section about the aerodynamic center
dMx/dx sectional aerodynamic moment
e a nonlinear ONERA load coefficient, e0 + e2(∆CL)2
kvz a noncirculatory linear ONERA load coefficient
L lift
M Mach number
Mx pitching moment beam aeroelastic model, positive nose up
My pitching moment for typical section
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r a nonlinear ONERA load coefficient, r0 + r2(∆CL)2
Re Reynolds number based on chord
sz a noncirculatory linear ONERA load coefficient
U uniform flow velocity
wa downwash velocity
yac distance from elastic axis to aerodynamic center, positive aft
α, α angle of attack, eigenvalue variable
αz a circulatory linear ONERA load coefficient
∆CL stalled lift deficit
λz a circulatory linear ONERA load coefficient
ρ fluid density
σz a circulatory linear ONERA load coefficient
θ0 static root angle of attack
Aeroelastic
(CLγ)l ONERA circulatory lift contribution for lth panel
(CL2)l nonlinear ONERA lift contribution for lth panel
xl nondimensional spanwise location for evaluation of aerodynamic loads
∆t time step
Eij =∫ 1
0ψi θj dx
k reduced frequency, ωb/U
Kijk =∫ 1
0ψ′′i ψ
′′j θk dx
NB number of flapwise bending modes
NC number of lag bending modes
NT number of torsion bending modes
NAERO number of aerodynamic panel sections
xv
tτ = b/U
V reduced velocity, 2U∞/(ωαc)
Vj jth lag state variable
Wj jth flap state variable
∆l nondimensional spanwise length of aerodynamic panel, 1/NAERO
κ1 dimensional group, ρ∞U2c/(2mL)
κ2 dimensional group, ρ∞/(mL2)
κ3 dimensional group, ρ∞/(mK2L)
µ typical section mass ratio, m/(πρ∞b2)
φλl inflow angle evaluated at xl, φλ(x = xl)
φλ inflow angle, w/(U + v + wθ0)
Φj jth torsion state variable
Ψj =∫ 1
0ψj dx
Subscripts
∞ freestream condition
deg degrees
F value at flutter point
nB nth flapwise bending mode
nC nth lag bending mode
nT nth torsion mode
ss static stall
ub uniform beam value
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Acknowledgements
First and foremost I would like to thank my advisor, Professor Earl Dowell, for
his introduction to the joy of research during my undergraduate years and for the
fruitful graduate years that followed. His skills as a researcher continue to inspire
me to a higher level of mentorship and scholarship, and to seek deeper insight into
engineering problems.
I am also grateful for the excellent support from my thesis committee: Profes-
sors Don Bliss, Kenneth Hall, Laurens Howle, and Lawrie Virgin. Their thoughtful
criticism and exacting standards have enriched greatly my thesis research and the
enjoyment and value of my graduate education.
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1
Introduction
High-altitude, long-endurance (HALE) aircraft define a unique class of uninhabited
air vehicles (UAV) designed to perform missions for intelligence, surveillance, recon-
naissance, and communications purposes. HALE aircraft employ slender, flexible
wings to reduce weight and enable the high lift-to-drag ratios necessary to achieve
sustained flight for months or years. Increased wing flexibility can lead to large static
structural deformations for trimmed states, which has attracted researchers to the
effects of geometric nonlinearity on the flight dynamics [20, 78, 97] and dynamic
stability [80] of standard unswept wings or more advanced joined-wing vehicle con-
cepts [19]. Most research efforts apply the intrinsic, geometrically-exact beam model
developed by Hodges [50] augmented by intrinsic kinematic equations [78], a combi-
nation which is well-suited for large-deformation finite element analyses. Aeroelastic
analyses are then performed assuming finite state representations of classical two-
dimensional inviscid unsteady aerodynamics [82, 83] sufficient for flutter and flight
dynamic stability predictions. However, the determination of loads for post-flutter
or dynamically unstable situations, such as experienced prior to the mid-flight break
up of the Helios prototype [76], require an integrated understanding of both nonlin-
1
ear structural behavior and of the dynamic fluid loads arising from large unsteady
motions and nonlinear aerodynamic stall effects.
Research efforts by Tang & Dowell [102, 103, 104, 105, 106, 107, 108, 109]
and other researchers [32, 33, 34, 123] describe the nonlinear, unsteady aerody-
namic loads for prismatic wing sections with the semi-empirical ONERA dynamic
stall model [25, 120], which is calibrated to dynamic stall data obtained by exper-
iment [68, 69, 70]. Aeroelastic models including dynamic stall effects successfully
correlate with experimentally observed flutter and limit cycle oscillation (LCO) be-
havior, including hysteresis [108] and chaotic behavior [79]. Theoretical-experimental
comparisons pave the way for computational aeroelastic predictions for HALE air-
craft using computational fluid dynamics (CFD) solver, which at present time are
limited to either the predictions of a static aeroelastic shape [46, 77] or flutter bound-
ary [8] for three-dimensional wings due to the large associated computational cost.
The present research extends the work of Tang & Dowell [106] to include, by approx-
imation within the ONERA model framework, the nonlinear aerodynamic effects
arising from dynamic stall as computed by a CFD solver. The impact of struc-
tural geometric nonlinearity and dynamic stall are isolated and interpreted using
this approach, which provides estimates for the anticipated sensitivity of the flut-
ter boundary and limit cycle oscillation behavior for a fully-coupled, first-principles
nonlinear aeroelastic analysis.
1.1 Research Questions and Outline
The present work seeks answers to the following research questions.
• What level of modeling fidelity is necessary and sufficient for a very flexible
wing structure and its aerodynamic loads to predict accurately flutter and
limit cycle oscillation phenomena?
2
• What are the effects of geometric structural nonlinearity and fluid nonlinearity
due to aerodynamic stall on the aeroelastic behavior of slender wings?
• How sensitive are the flutter boundary and the LCO amplitude and hysteresis
metrics of HALE wings to first-principles-based aerodynamic data versus wind
tunnel data?
Following this Introduction, a range of structural models and aerodynamics models
used for aeroelastic computations are described separately in Chapters 2 and 3, re-
spectively. Chapter 4 integrates the structural and aerodynamic chapters into two
principal aeroelastic models: a linear typical section model with unsteady Theo-
dorsen aerodynamics; and the Hodges-Dowell nonlinear beam equations with the
ONERA dynamic stall lift model. Results from these aeroelastic models and dimi-
nuitive models thereof focus on the effects of flow unsteadiness, beam geometry, and
nonlinearities from structural and aerodynamic origins. Chapter 5 summarizes the
contributions of this research and suggests avenues for future work.
3
2
Structural Models
Very flexible wings may sustain large structural deformations during flight due to
loading, gusts, or fluid-structure instability. This chapter discusses a range of struc-
tural models for aeroelastic analysis to determine the level of physical fidelity to
predict successfully flutter and limit cycle oscillations of an experimental wing rep-
resentative of a HALE-type aircraft.
First, the classical typical section model on linear springs is considered to estab-
lish the simplest scenario for modeling an aeroelastic system with coalescence flutter.
Nondimensional groups for this model are later inferred from full aeroelastic wing
model data to make a posteriori flutter predictions. Second, a finite element analysis
is performed for the experimental aeroelastic wing to determine the individual effects
of its non-uniform components, i.e. spar, ribs, and tip store, on the natural frequen-
cies and mode shapes. Third, the Hodges-Dowell nonlinear beam-torsion equations
are considered to highlight the effects of elastic coupling and second-order geometric
nonlinearities. The removal of these nonlinearities reduces the Hodges-Dowell equa-
tions to Euler-Bernoulli beam theory and thus enables the systematic investigation
of structural nonlinear effects on flutter and limit cycle oscillations.
4
Mid Chord
c
+h
+α
b
a b
Elastic Axis
α
b
Mean Position Mass Center
K
x b
αK
h
Figure 2.1: Schematic of typical section on linear springs (courtesy of J.P. Thomas).
2.1 Typical Section
The typical airfoil section model [13, 29] shown in Figure 2.1 allows for the direct
study of aerodynamic interaction with a representative elastic structure constrained
to pitch, α, and plunge, h, motions only. Despite the simplicity of this model, it
continues to be a test bed for investigations of nonlinear stiffness [7, 9, 27, 26, 56, 57,
73], control surface free-play [10, 21, 28, 40, 47, 58, 73, 101, 110, 121], flutter and limit
cycle oscillations [9, 10, 27, 26, 40, 47, 58, 73, 95, 110], dynamic stall [44, 45, 105],
and stochastic [7, 88] and transonic aerodynamics [22, 28, 36, 58, 66, 73, 95]. The
present work restricts the structural model to linear stiffness behavior in pitch and
plunge motions modeled by the following set of equations.
mh+Kh h+ Sα α = −L (2.1)
Sα h+ Iα α+Kα α = My (2.2)
These equations can be recast into a nondimensional form that requires only the
5
external lift and moment forces as determined by an aerodynamic model.
(∗ ∗h/b) + (ωh/ωα)2 (h/b) + xα
∗ ∗α= − V
2
π µCL (2.3)
xα (∗ ∗h/b) + r2
α
∗ ∗α +r2
α α =2V 2
π µCM (2.4)
2.2 Finite Element Analysis
Materials of various densities and stiffnesses typically constitute the experimental
slender wing structures designed for flutter and limit cycle oscillation experiments
of HALE aircraft. Therefore, it is necessary to determine the effects of structural
nonuniformity on the natural frequencies and mode shapes of very flexible beams,
which are frequently used in geometrically nonlinear structural analyses of HALE
wings [32, 106, 107, 108, 109]. Jaworski and Dowell [54] demonstrated that such a
beam-like structure with spanwise discontinuities could be represented modally as
a uniform beam for sufficiently small spanwise discontinuities. However, determin-
ing the set of natural frequencies requires knowledge of any such discontinuities or
variations.
This section addresses the effects of these nonuniformities on the four lowest nat-
ural frequencies of a cantilevered HALE-type wing [53]. Here, the experimental wing
model used by Tang and Dowell [106, 107, 108] is analyzed using the commercial
finite element program ANSYS. As shown in Fig. 2.2, the HALE wing is composed
of a steel spar with multiple steps, periodically-spaced aluminum ribs, balsa wood
fairings to fill the space between ribs, and a tip store. Specifically, the effects ex-
amined herein are the step depth for the particular step distribution used by Tang
and Dowell [106, 107, 108]; the addition of periodically-spaced ribs; the presence of
balsa wood fairings with varying levels of rigid connection to the central spar; and
the addition of a tip store. For this study the total spar length, maximum width,
6
(a)
(b)
Figure 2.2: (a) Aeroelastic wing model; (b) Schematic of ANSYS wing model. Tipmass spanwise location indicated by ?. Dimensions in millimeters.
7
thickness, step distribution, and step width are held constant; only the step depth
varies. Step depth is defined as the chordwise dimension of the symmetrical material
removed from the spar, which is 3.17mm for the experimental model in Fig. 2.2(b).
The step depth is scaled by the spar half-width, and the natural frequencies by their
uniform beam values of the spar alone, fub. The four natural frequencies of interest
(f1B, f2B, f1C , f1T ) are tracked as the nondimensional step depth dN varies.
The physical parameters used in the finite element computations for balsa wood,
aluminum, and steel are ρm = 138.5, 2664, 7850 kgm−3; E = 2.34, 60.6, 200GPa; and
ν = 0.3, 0.33, 0.3, respectively. The densities are calculated from total mass and
dimensional data of material specimens, and the elastic moduli are calibrated to
their first flapwise resonance using classical beam theory. Standard handbook values
are assumed for the Poisson ratios.
All figures herein indicate actual finite element data with symbols unless otherwise
noted, and the curves between these symbols are interpolated using piecewise cubic
splines [67]. The results are analyzed for individual additions of ribs, fairings, and a
tip store, as well as their combined effects on natural frequencies.
2.2.1 Step Depth
The spar is modeled using two-dimensional, 8-node structural shell elements (shell-
93) [5]. The finite element meshes are generated by the “SmartSizing” free-meshing
function within ANSYS, set to the highest possible resolution.
The natural frequency results in Fig. 2.3 show that the first two out-of-plane
bending mode trends are virtually coincident, and that the torsion mode follows a
very similar trend. This similarity is anticipated because both torisonal and out-of-
plane bending stiffnesses scale as bst3. The frequency trend for the in-plane bending
mode is an almost linear function of the step depth, as expected from uniform beam
theory where the in-plane stiffness scales as b3st.
8
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
1.1
dN
f/f u
b
Figure 2.3: Spar natural frequencies as step depth is varied: , f1B; ♦, f2B; 4,f1C ; , f1T .
2.2.2 Ribs
The effect of adding aluminum ribs with a NACA 0012 profile [1] is evaluated using
both two-dimensional shell (SHELL93) and three-dimensional solid (SOLID45) finite
element models. As shown in Fig. 2.4, the two- and three-dimensional finite element
models are in close agreement, which suggests that three-dimensional effects at the
constraints between the ribs and spars may be neglected.
A comparison between Figs. 2.3 and 2.4 indicates that rib addition does not
change the qualitative frequency trends observed for the stepped spar, but rather
the ribs change the magnitude of the results. The bending mode results are roughly
85% of those for the spar alone, whereas the torsion mode results are reduced by
nearly 40%. Clearly, the main contribution of the ribs is an increase in torsional
inertia.
9
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
dN
f/f u
b
Figure 2.4: Natural frequencies of spar with ribs as step depth is varied: solid line,2D; dashed line, 3D. , f1B; ♦, f2B; 4, f1C ; , f1T .
2.2.3 Balsa Wood Fairings
The addition of balsa wood fairings and the constraint conditions between the spar
and fairings are modeled by three-dimensional solid elements. Figure 2.5 shows that
the fairings dominate the torsion and out-of-plane bending modes and that the step
depth has virtually no effect. Therefore, the balsa wood addition acts effectively as
a stiffness increase for the out-of-plane bending modes and an inertial increase for
the torsion mode.
The particular distribution of balsa wood provides a modest 5% change in the
natural frequency of the in-plane bending mode for zero step depth. The in-plane
bending mode trend resembles that of the spar alone but approaches a nonzero
frequency as dN → 1; the other modes also have nonzero frequencies in this limit
because the balsa wood holds the structure together. It is also inferred from the
limit dN → 1 that the presence of the balsa wood accounts for a quarter of the
10
effective in-plane bending stiffness, recalling f 2∼EI2.
The computations for the results shown in Fig. 2.5 assume that the balsa wood
and spar are perfectly joined, i.e. the interfacial node displacements are identical.
To investigate the influence of the compatibility condition, three alternative con-
straint conditions are considered in the computational model for single- and double-
component segments of the full structure.
First, the constraint between the fairings and spar is relaxed (i.e. stiffness due to
shear flow is eliminated) along the thin edges of the spar; this effect is very small
(∼1%) for all modes. Second, the constraint along the wide edges of the spar is
relaxed instead. The in-plane bending mode is relatively unchanged, but the out-
of-plane bending and torsion values decrease by roughly 5-10%. However, the com-
parison of component results suggests that the first out-of-plane natural frequency
becomes progressively lower than the corresponding perfectly joined cases, whereas
the second out-of-plane bending and torsion natural frequencies have a relative in-
crease. The stiffening of the second bending mode for the double-component case is
thought to explain its trend difference from the first out-of-plane mode.
Third, the balsa wood fairings are connected to the spar only at its outermost
corner points using constraint equations to relate node displacements. The net ef-
fect is a limiting case where the balsa wood is solely a mass addition. The in-plane
bending and torsion results are most affected. The change in out-of-plane natural
frequencies is roughly 5-10%, though more data would be needed to deduce a trend
because the constraint locations and node lines of the bending modes factor signif-
icantly into the analysis. This was a lesser concern for the other cases because the
constraint was applied over an area instead of at a small number of points.
Overall, the effect of varying the compatibility conditions is modest for the in-
and out-of-plane bending modes, but more pronounced for the torsion mode.
11
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
1.1
dN
f/f
ub
Figure 2.5: Natural frequencies of 3D spar with balsa wood fairings as step depthis varied: , f1B; ♦, f2B; 4, f1C ; , f1T .
2.2.4 Tip Store
This section examines the three-dimensional spar when fitted with a tip store. The
store is modeled as two identical point masses positioned such that the effective
mass and torsional inertia match the measured values of M = 36.95 g and Iφ =
8.314× 10−5 kgm2, respectively.
The results in Fig. 2.6 show that the tip store inertia renders the torsional mode
almost insensitive to step depth. Also, the bending mode trends are similar to those
of the spar alone. For the first time, the out-of-plane bending mode curves do not
overlap because the frequency results depend on the tip store placement relative to
the nodes of the particular mode shape.
12
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
dN
f/f
ub
Figure 2.6: Natural frequencies of 3D spar with a tip store as step depth is varied:, f1B; ♦, f2B; 4, f1C ; , f1T .
2.2.5 Combined Effects
The modeling variations analyzed herein are now combined to observe their net effect
on the natural frequencies. Figures 2.7–2.10 describe the frequency behavior of the
stepped spar as the ribs, balsa wood fairings, and tip store are added in sequence.
The trends are similar for the out-of-plane bending and torsion modes. The
addition of the ribs reduces the magnitude of the stepped spar frequency results to
varying degrees, which indicates that the ribs essentially contribute more inertia than
stiffness. Balsa wood fairings flatten the curve and increase the frequency values,
indicating that the fairing stiffness dominates and that step depth effects become
less important. The tip store affects the curves such that the final configuration has
out-of-plane bending and torsion frequencies lower than those of the spar alone. The
resulting out-of-plane bending and torsion modes are effectively independent of step
depth.
13
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
dN
f/f u
b
Figure 2.7: Combined effects on f1B for varying step depth: solid line, spar alone;, with ribs; , with ribs and balsa; 4, with ribs, balsa, and tip store.
The change in the in-plane bending mode frequency behavior in Fig. 2.9 is less
pronounced than for the other modes. The rib addition changes the uniform spar
frequency by 15%, a difference that diminishes as the step depth is increased. The
subsequent balsa wood addition retains the uniform spar trend but changes the
frequency for dN → 1 to a non-zero value as with the other modes. The tip store
scales down the magnitude of previous results as seen with the other modes.
The results shown in Figs. 2.7–2.10 support the hypothesis that an aeroelastic
wing could be designed by varying the tip store properties and step depth alone.
Explicitly, the out-of-plane bending modes depend primarily on the tip store mass;
the tip store mass and step depth tune the in-plane bending frequency; and tip store
torsional inertia controls the torsion frequency. The next section correlates such
computational results against experiment.
14
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
dN
f/f u
b
Figure 2.8: Combined effects on f2B for varying step depth: solid line, spar alone;, with ribs; , with ribs and balsa; 4, with ribs, balsa, and tip store.
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
dN
f/f
ub
Figure 2.9: Combined effects on f1C for varying step depth: solid line, spar alone;, with ribs; , with ribs and balsa; 4, with ribs, balsa, and tip store.
15
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 10
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
1.1
dN
f/f u
b
Figure 2.10: Combined effects on f1T for varying step depth: solid line, spar alone;, with ribs; , with ribs and balsa; 4, with ribs, balsa, and tip store.
2.2.6 Theoretical-Experimental Comparison
The HALE-type wing [106, 107, 108] natural frequencies were measured using a
transducer-fitted impact hammer (Bruel & Kjær (B&K) type 8204) and an ac-
celerometer (B&K type 4374). The signal from the accelerometer is boosted by
a charge amplifier (B&K type 2635), and the transfer function between the hammer
and accelerometer is measured by the B&K pulse data acquisition system [16]. Each
transfer function is averaged linearly over five impacts at the spar tip. Every impact
is sampled at 256Hz for eight seconds, yielding a frequency resolution of 125mHz.
Table 2.1 compares the results for the three-dimensional finite element model
both with and without the tip store with observed values for the HALE-type wing.
Without the tip store, the finite element model agrees to within 15-30% of comparable
experimental values for the bending modes. Lesser agreement is observed for the
torsion mode. The full model with tip store overestimates the experimental values
16
Table 2.1: Comparison of ANSYS and experimental natural frequencies for dN = 0.5.
ANSYS ExperimentMode
w/o Store w/ Store w/o Store w/ Storef1B 4.598 (3.968)† 2.882 (2.658) 4.000 2.625f2B 28.76 (24.83) 22.37 (19.87) 22.38 17.88f1C 25.82 (22.29) 15.86 (14.93) 23.13 14.13f1T 145.3 (140.9) 25.75 (25.71) 102.9 22.88
† total mass matched to experiment for parentheses values
by roughly 10-25%; the second out-of-plane mode has the largest overestimate.
The results for the mass-corrected model are placed in parentheses for Table 2.1.
The ANSYS bending mode results agree to within 11% of experiment using the mass
correction. The torsion mode is virtually unaffected because the assumed radius of
gyration of the added mass is small.
2.2.7 Mode Shapes
This section compares the mode shapes of uniform beam theory to those from the
finite element wing model for dN =0.5, which corresponds to the experimental wing
in Ref. [106] (cf. Fig. 2.2). This comparison demonstrates how accurately the present
three-dimensional HALE wing finite element model with its many nonuniformities
can be approximated by classical beam theory.
Figures 2.11-2.13 compare the wing mode shapes with the tip store. The ANSYS
modal deflections are recorded for 18 spanwise locations at the midchord, and a least-
squares tenth-order polynomial curve fit is drawn through the data. The classical
bending modes are described by
χn(x), ψn(x) = An
[(cosλnx− coshλnx)−
(cosλn + coshλn
sinλn + sinhλn
)(sinλnx− sinhλnx)
],
(2.5)
where An is a scaling factor to normalize the mode shape, and λn are solutions to
17
the transcendental equation [52]
1 + cosλn coshλn = λn
(M
mL
)(sinλn coshλn − cosλn sinhλn). (2.6)
The torsion mode shape is Θn(x)=An sin(βnx), where βn satisfies [52, 13]
βn tan βn =mLK2
Iφ. (2.7)
To compare the mode shapes directly, the values M/mL= 0.4032 and mLK2/Iφ =
9.496×10−2 follow from the ANSYS model. Classical theory closely approximates
the resulting ANSYS mode shapes when including tip store effects, especially for
the higher-order flapwise modes in Fig. 2.11. Figures 2.14–2.16 indicate that the
first modes remain virtually coincident without the tip store, but the maximum
percentage differences between the second-, third-, and fourth-order flapwise modes
grow to 5.38%, 9.72%, and 13.5%, respectively.
Overall, the finite element mode shapes of the considered nonuniform HALE
wing model are well-described by classical uniform beam theory. The addition of
a tip store improves the approximation of the computed mode shapes by classical
theory.
2.2.8 Conclusions
A computational structural analysis is performed for a high-aspect-ratio, experimen-
tal aeroelastic wing model using the commercial finite element program ANSYS.
The computational results quantify the effects of spanwise nonuniformities such as
ribs, fairings, and a tip store on the first four wing modes. The mode shapes of the
nonuniform finite element wing model are shown to be well-approximated by classical
beam modes, which are typically assumed as trial functions for nonlinear aeroelastic
analyses of slender wings. In addition, the computed natural frequency results are
18
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
χ1(x
)
(a)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ2(x
)
(b)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ3(x
)
(c)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ4(x
)
(d)
Figure 2.11: Flapwise mode shapes for HALE wing with tip store: a) χ1; b) χ2; c)χ3; d) χ4. , ANSYS data; solid line, least-squares polynomial fit of ANSYS data;dashed line, uniform beam theory.
compared with those from experiment and shown to be in reasonable agreement.
The agreement between computational and experimental results without resorting
to empiricism supports the use of ANSYS as a design tool for aeroelastic analyses
of HALE-type wings. Also, the close agreement of the computed mode shapes and
those from classical beam theory enbales and validates the use of a more sophisticated
homogeneous and isotropic continuum beam model.
19
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
ψ1(x
)
Figure 2.12: First chordwise mode shape for HALE wing with tip store: , ANSYSdata; solid line, least-squares polynomial fit of ANSYS data; dashed line, uniformbeam theory.
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
Θ1(x
)
Figure 2.13: First torsion mode shape for HALE wing with tip store: , ANSYSdata; solid line, least-squares polynomial fit of ANSYS data; dashed line, uniformbeam theory.
20
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
χ1(x
)
(a)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ2(x
)
(b)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ3(x
)
(c)
0 0.2 0.4 0.6 0.8 1−1
−0.5
0
0.5
1
x
χ4(x
)
(d)
Figure 2.14: Flapwise mode shapes for HALE wing without tip store: a) χ1; b)χ2; c) χ3; d) χ4. , ANSYS data; solid line, least-squares polynomial fit of ANSYSdata; dashed line, uniform beam theory.
2.3 Hodges-Dowell Nonlinear Beam Equations
The Hodges-Dowell equations [51] describe the nonlinear interactions between elastic
bending and torsion motions for a slender, straight, homogeneous, and isotropic beam
without cross-sectional warping. Originally developed to investigate the importance
of nonlinearity on the aeroelastic stability and behavior of hingeless helicopter rotor
blades, these equations reduce to expressions suitable for the nonlinear analysis of
the slender wings of HALE-type aircraft. Hodges-Dowell theory features nonlinear
elastic coupling between the bending and torsion motions arising from a nonlinear
strain-displacement relationship, which enables an ordering scheme for geometrically
21
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
ψ1(x
)
Figure 2.15: First chordwise mode shape for HALE wing without tip store: ,ANSYS data; solid line, least-squares polynomial fit of ANSYS data; dashed line,uniform beam theory.
0 0.2 0.4 0.6 0.8 10
0.2
0.4
0.6
0.8
1
x
Θ1(x
)
Figure 2.16: First torsion mode shape for HALE wing without tip store: , ANSYSdata; solid line, least-squares polynomial fit of ANSYS data; dashed line, uniformbeam theory.
22
nonlinear stiffness effects based on the assumptions that the squares of the bending
slopes, twist, thickness to length, and aspect ratio are small compared to unity.
For the present investigation, the Hodges-Dowell equations describe flap, lag, and
twist motions under gravitational loading and include second-order geometrical strain
effects.
EI2 v(IV ) + (EI2 − EI1)[φw
′′]′′ +mv + Cξ v + (Mv + Ivv′) δ(x− L) =
dFv
dx+ ∆Fv − [Mg δ(x− L) +mg] sin θ0 (2.8)
EI1w(IV ) + (EI2 − EI1)[φv
′′]′′ +mw −meφ+ Cξ w + (Mw + Iww′) δ(x− L) =
dFw
dx+ ∆Fw − [Mg δ(x− L) +mg] cos θ0 (2.9)
−GJ φ′′ + (EI2 − EI1)w′′v′′ + Iφ δ(x− L) +mK2
mφ+ Cξ φ−mew =
dMx
dx+ ∆Mx (2.10)
These continuum equations are well-suited for the presently considered experimen-
tal aeroelastic wing as supported by the finite element mode shape comparisons in
Section 2.2.7.
The right-hand sides of Eqns. 2.8–2.10 include the aerodynamic conributions
from the wing surface, dFv/dx, dFw/dx, and dMx/dx, as well as from the slender
body at the wing tip, ∆Fv, ∆Fw, and ∆Mx [106]. As a consequence of the second-
order geometrical accuracy, the projection of the deformed twist angle, φ, onto the
twisting plane of the undeformed axis is defined as the geometric angle, φ [31].
This relationship will be necessary to properly determine the angle of attack at a
prescribed spanwise location within strip-theory aerodynamic assumptions.
φ = φ+
∫ x
0
v′w′′ dx (2.11)
23
3
Aerodynamic Models
High-aspect-ratio wings achieve high aerodynamic efficiency by virtue of their large
spans. Except for the regions influenced by the vortices generated at the ends of these
wings, the flow over most of the inboard wing section remains two-dimensional. This
observation supports the assumption of strip-theory aerodynamics, where the aerody-
namic loads at a particular spanwise location are dependent strictly on the geometric
angle of attack at that location and are independent of the (three-dimensional) aero-
dynamic influence of other spanwise locations [42].
This chapter identifies a range of aerodynamic models to describe the aerody-
namic loads of the wing store and the spanwise ‘strips’ constituting the aeroelastic
wing surface. Slender body theory is first described to model the aerodynamics of the
store at the wing tip. Subsequent sections discuss the classical Theodorsen thin air-
foil theory for incompressible flow and the ONERA dynamic stall model. By design,
the semi-empirical, nonlinear, large motion ONERA model is calibrated to provide
steady and unsteady aerodynamic loads for a particular airfoil section and reduces
to an equivalent Theodorsen-like state-space model for small motions. The present
work uses a computational fluid dynamics (CFD) code to generate the aerodynamic
24
calibration data and identify a new ONERA dynamic stall model for the NACA 0012
airfoil based on first-principles information.
3.1 Slender Body Theory
A body is considered aerodynamically ‘slender’ if its crosswise dimensions such as
span and thickness are small compared to its length [61]. Specifically, slender body
theory assumes that the disturbed flow is two-dimensional in planes normal to the
flight direction [13, 55, 72], which renders the theory valid for any Mach number
so long as the flow normal to the flight direction is effectively incompressible. The
present model follows the inviscid flow derivation of Ref. [13] for a rigid body of
revolution that is restricted to pitching and plunging motions with small incidence
angles.
Consider a longitudinal centerline of the slender body defined by za(y, t), where
y is the freestream flow direction and the length coordinate of the slender body with
a pitch axis at yB.
za = −h(t)− α(t)[y − yB] (3.1)
The assumption of small incidence angles allows the generated downwash, wa, to be
expressed as wa = Dza/Dt. The fluid momentum contained in xz-planes separated
by distance dy can then be expressed as
dPz = ρ∞ S wa dy
= ρ∞ S
[dza
dt+ U
dza
dy
]dy, (3.2)
where the cross-section is circular with area distribution S(y) = πR2(y). The momen-
tum flux of displaced fluid in the xz-plane produces a lift reaction on the differential
25
length segment dy of the slender body.
dL
dy= − D
Dt
[dPz
dy
](3.3)
= ρ∞U(h+ Uα)dS
dy+ ρ∞Uα(y − yB)
dS
dy+ ρ∞(h+ 2Uα)S + ρ∞α(y − yB)S
(3.4)
Total lift and moment are calculated by direct integration of Eqn. 3.4 over the body,
noting that S(y = 0, cSB) = 0.
L =
∫ cSB
0
dL
dydy (3.5)
= ρ∞(h+ Uα) –V1 + ρ∞α –V1 (3.6)
Mx = −∫ cSB
0
(y − yB)dL
dydy (3.7)
= ρ∞U(h+ Uα) –V1 − ρ∞h –V2 − ρ∞α –V3 (3.8)
The slender body volume, volume static unbalance, and volume moment of inertia
are constant-valued coefficients defined respectively by the following integrals.
–V1 =
∫ cSB
0
S dy (3.9)
–V2 =
∫ cSB
0
(y − yB)S dy (3.10)
–V3 =
∫ cSB
0
(y − yB)2S dy (3.11)
Aerodynamic forces from the slender body relate to the wing motions of Eqns. 2.8–
2.10 through the definitions h = −w|x=L and α = φ|x=L. Also, within the small inci-
dence angle approximation a lag force appears by tipping the lift vector; viscous drag
effects that would also act in this direction are not accounted for in this framework.
26
The final expressions for the slender body aerodynamic loads follow [103, 106, 107].
∆Fw = ρ∞
[(U
˙φ− w) –V1 +
¨φ –V2
]δ(x− L) (3.12)
∆Fv = (θ0 + φ− φλ)∆Fw (3.13)
∆Mx = ρ∞
[U(Uφ− w) –V1 + w –V2 − ¨
φ –V3
]δ(x− L) (3.14)
3.2 Theodorsen Theory
Theodorsen [113] first published the solution for unsteady aerodynamic loads on a
thin airfoil in incompressible flow. The circulatory and non-circulatory contributions
to sectional lift and moment can be expressed directly by assuming simple harmonic
motion of the airfoil and wake [13].
L = πρ∞b2[h+ Uα− ba α] + 2πρ∞UbC(k)[h+ Uα+ b (1/2− a) α] (3.15)
My = πρ∞b2[bah− Ub (1/2− a) α− b2 (1/8 + a2) α]
+ 2πρ∞Ub2 (a+ 1/2)C(k)[h+ Uα + b (1/2− a) α] (3.16)
The Theodorsen function,
C(k) =H
(2)1 (k)
H(2)1 (k) + iH
(2)0 (k)
(3.17)
quantifies the dependence of the circulatory lift on the vorticity shed unsteadily into
the wake, and may be physically regarded as the lag in the development of bound
circulation due to the influence of shed wake vortices [61]. Flutter analyses using the
original Theodorsen function are valid only at the flutter point due to the assumption
of undamped harmonic motion.
Aeroelastic calculations rearrange Eqns. 3.15 and 3.16 typically into independent
load coefficients due to pitch and plunge motions, which may then be expressed in
27
their frequency-domain forms for eigenvalue computations.
CLh/b= πV −2[(
∗ ∗h/b) + 2V C(k) (
∗h/b)] (3.18)
CLα = πV −2[V∗α −a ∗ ∗
α +2C(k) (V 2α+ V (1/2− a)∗α)] (3.19)
CMh/b= πV −2/4 [a (
∗ ∗h/b) + 2 (a+ 1/2)V C(k) (
∗h/b)] (3.20)
CMα = πV −2/4[− V (1/2− a)∗α −(1/8 + a2)
∗ ∗α
+ 2 (a+ 1/2)C(k) (V 2α+ V (1/2− a)∗α)] (3.21)
3.3 ONERA Dynamic Stall Model
Early dynamic stall studies looked to experimental programs [17, 68, 70, 71] to inves-
tigate the effects of airfoil shape, Mach and Reynolds numbers, mean and unsteady
angles of attack, and reduced frequency on the aerodynamic loads in response to
prescribed harmonic motion. These data led to the development of a semi-empirical
model by Tran & Petot [120] and Dat & Tran [25] at l’Office National d’Etudes et
Recherches Aerospatiales (ONERA) designed to predict the loads on helicopter ro-
tor blades encountering large unsteady motions and dynamic stall phenomena. The
ONERA dynamic stall model consists of a set of differential equations with nonlinear
coefficients but linear operators, which enable the convenient and simultaneous up-
date of structural motion and aerodynamic forces in state-space for a fully-coupled
aeroelastic computation. Moreover, the model equations of the model can be lin-
earized about a nonlinear state for use in traditional dynamic analysis and stability
programs [81].
Despite the immediate utility of the ONERA equations for both fixed and rotating
blades, the original model had no basis in first-principles physics and had relatively
little in common with classical aerodynamic theory. Researchers sought to improve
the consistency of the ONERA model with classical theory [81, 87] and to overcome
28
its limitations when applied to extreme unsteady behavior, such as numerical insta-
bility for large angles of attack involving reversed flow [81]. Peters [81] reformulated
the model to fix this deficiency and enable the reproduction of Theodorsen [113]
and Greenberg (pulsatile freestream) [48] aerodynamics in a logical manner. Fur-
thermore, Peters [81] and Rogers [93] worked to isolate the effects of pitching and
plunging motions on dynamic stall [18, 35, 41], whose distinctions affect the circula-
tory lift and apparent mass terms.
The final form of the ONERA equations investigated here follows from Dunn [32,
33, 34] and has been used extensively in aeroelastic investigations using the NACA
0012 airfoil section [32, 102, 104, 105, 106, 107, 108, 110].
Cz = Cz1 + Cz2 (3.22)
Cz1 = tτszα+ t2τkvz¨φ+ Czγ (3.23)
tτ Czγ + λzCzγ = λz(a0zα+ tτσz˙φ) + αz(tτa0zα+ t2τσz
¨φ) (3.24)
t2τ Cz2 + atτ Cz2 + r Cz2 = −r[∆Cz + tτe
∂∆Cz
∂αα
](3.25)
The ONERA model separates the total lift (z = L) or moment (z = M) coefficient
into linear and nonlinear contributions to be solved independently; the ONERA
model describes only the unsteady lift in this work. The linear aerodynamics of
Eqns. 3.23 and 3.24 constitute a state-space representation of Theodorsen-like airfoil
aerodynamics for a particular airfoil geometry and flow condition. Effects due to
fluid viscosity, compressibility, and airfoil geometry are embedded into the constant
coefficients of each equation by the parameter identification of given aerodynamic
data.
Nonlinearity in the ONERA model arises from Eqn. 3.25 due to the dependence of
its coefficients on ∆CL [69, 84, 86], the force deficit measured between the unstalled
29
Figure 3.1: Schematic of ∆CL.
static lift coefficient and the actual static lift coefficient including stall (cf. Fig. 3.1).
a = a0 + a2(∆CL)2 (3.26)
r = r0 + r2(∆CL)2 (3.27)
e = e0 + e2(∆CL)2 (3.28)
The static lift deficiency, ∆CL, also forces the nonlinear lift equation, which would
otherwise represent a damped oscillator. Therefore, the ONERA model does not
predict any kind of nonlinear or dynamic stall behavior unless the effective angle
of attack exceeds that of static stall, α > αss, when ∆CL > 0. The right-hand
side (RHS) of Eqn. 3.25 also includes lag effects that are apparent in deep stall,
where the aerodynamic loads are sensitive to the generation and convection of vor-
tices interacting with the time-dependent motion of the structure. Debate exists
as to how these lag effects are best incorporated into the ONERA model, as dis-
cussed at length by Dunn [34]. Early forms of the model included an explicit lag
30
term [85], which has been replaced in modern versions by a dependence on the terms
r and e from Eqns. 3.27 and 3.28. The model selection depends on a balance be-
tween the retention of physical behavior in the modeling effort and the convenience
to its particular application of the ONERA model. For example, Dunn [34] chose
the form RHS=[−r∆CL + tτe(∂∆CL/∂α)α] to simplify a harmonic balance analysis.
The present RHS of Eqn. 3.25 follows from Petot & Dat [87], where the phase-lag
is expressed in direct relation to the force deficit ∆CL [34] to facilitate physical
interpretation of aerodynamic lag.
Here, the ONERA dynamic stall model determines the two-dimensional lift co-
efficients for each NACA 0012 spanwise wing section. The sectional lift, drag, and
moment values of each wing section are defined by the following.
dL
dx=
1
2ρ∞c U
2CL (3.29)
dD
dx=
1
2ρ∞c U
2CD (3.30)
dM0
dx=
1
2ρ∞c
2U2CM (3.31)
The moment about the aerodynamic center is determined by a simpler form of
the ONERA equations with a quasi-static nonlinear stall contribution for α > αss,
∆CM = −0.08 sgn(α) [103].
CM = CM1 + CM2 (3.32)
CM1 = tτsM α+ tτσM˙φ+ t2τkvM
¨φ (3.33)
CM2 = −∆CM (3.34)
Values for the unsteady moment coefficients follow from thin airfoil theory: sM ,
σM = −π/4; kvM = −3π/16. A curve fit to static experimental data [1] defines the
drag dependence on the instantaneous angle of attack.
CD = 0.008 + 1.7α2deg (3.35)
31
To be consistent with the Hodges-Dowell equations, the quasi-steady inflow angle,
φλ, and effective angle of attack, α, must incorporate the root pretwist of the wing,
the geometric twist angle, and kinematic effects of three-dimensional wing motion.
φλ ≈ w/(U + v + wθ0) (3.36)
α = θ0 + φ− φλ (3.37)
Thus, the sectional aerodynamic loads for the Hodges-Dowell equations can now be
written explicitly.
dFw
dx=dL
dx+ (θ0 − φλ)
dD
dx(3.38)
dFv
dx= −dD
dx+ (θ0 − φλ)
dL
dx(3.39)
dMx
dx=dM0
dx− yac
dFw
dx(3.40)
32
4
Aeroelastic Formulations and Results
The structural and aerodynamic models of Chapters 2 and 3 are integrated to per-
form a range of aeroelastic analyses for the HALE experimental wing. The aeroelas-
tic models investigate the effects of beam geometry modeling, structural nonlinearity
arising from elastic coupling among the degrees of freedom, and dynamic stall aero-
dynamic nonlinearity on the flutter and limit cycle oscillation behavior. Also, the
two ONERA dynamic stall models based on wind tunnel or first-principles CFD data
are compared with regard to their impact on the dynamic behavior on the aeroelastic
wing. The goal of the present chapter is to establish the role of structural and aero-
dynamic modeling fidelity on the simulated linear and nonlinear dynamic response
of a HALE wing, and to benchmark the agreement between experimental data and
simulated results based on aerodynamic data computed by a CFD solver.
4.1 Typical Section with Theodorsen Aerodynamics
4.1.1 Eigenvalue Analysis
The typical section model on linear springs is combined with Theodorsen unsteady
thin airfoil theory to perform an a posteriori flutter analysis using structural param-
33
Table 4.1: Typical section data representative of a HALE-type wing [106].
xα -0.005rα 0.3682ωh/ωα 0.7815µ 103.1
eters adapted from the experimental HALE wing, which are identified in Table 4.1
from data in Ref. [106]. Note that the plunge-to-pitch frequency ratio, ωh/ωα, is
tuned to the known second-bending/first-torsion coalescence flutter mode.
The eigenvalue forms h = h epτ and α = α epτ are substituted into Eqns. 2.3–2.4
and combined with Eqns. 3.18–3.21 to arrive at following expression. A(p)
h/(αb)
1
= 0 (4.1)
Setting the determinant of the coefficient matrix A to zero determines the aeroelastic
characteristic equation for the typical section model.
A4 p4 + A3 p
3 + A2 p2 + A1 p+ A0 = 0 (4.2)
Table 4.2 identifies these polynomial coefficients for the full unsteady Theodorsen
aerodynamic model, in addition to the standard steady and quasi-steady aerody-
namic models. The steady and quasi-steady approximations include only circulatory
lift based on the instantaneous effective angles of attack of α and (α + h/U), re-
spectively [30]. The eigenvalue solution of Eqn. 4.2 can be computed directly by a
complex root solver for the steady and quasi-steady aerodynamic approximations.
For the general unsteady case, the reduced frequency must be iterated for each value
of reduced velocity until the frequency ratio determined by these values matches the
frequency ratio of the least stable eigenvalue.
Figures 4.1–4.3 plot the real and imaginary parts of the eigenvalue parameter,
p = pR + i(ω/ωα), for each aerodynamic model over a range of reduced velocities.
34
Tab
le4.
2:C
oeffi
cien
tsfo
rty
pic
alse
ctio
nm
odel
eige
nva
lue
anal
ysi
s.
Aer
odynam
icM
odel
Coeffi
cien
tsSte
ady
Quas
i-Ste
ady
Unst
eady
A4
µ(r
2 α−x
2 α)
µ(r
2 α−x
2 α)
µ(r
2 α−x
2 α)+r2 α
+2ax
α
+(1/8
+a
2)+
1/(8µ)
A3
02V
[r2 α
+(a
+1/
2)x
α]
2VC
(k)[r2 α
+a(a
+2x
α)−
1/4−
1/(8µ)]
+V
[1/(
2µ)−x
α+
(1/2−a)]
A2
µr2 α
[1+
(ωh/ω
α)2
]µr2 α
[1+
(ωh/ω
α)2
]µr2 α
[1+
(ωh/ω
α)2
]−
2V2[x
α+
(a+
1/2)
]−
2V2[x
α+
(a+
1/2)
]−
2V2C
(k)[x
α+
(a+
1/2)−
1/(2µ)]
+r2 α
+(1/8
+a
2)(ω
h/ω
α)2
A1
02r
2 αV
2VC
(k)[r2 α
+(a
2−
1/4)
(ωh/ω
α)2
]+V
(1/2−a)(ω
h/ω
α)2
A0
(ωh/ω
α)2
[µr2 α−
2V2(a
+1/
2)]
(ωh/ω
α)2
[µr2 α−
2V2(a
+1/
2)]
(ωh/ω
α)2
[µr2 α−
2V2C
(k)(a
+1/
2)]
35
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5−100%
−50%
0%
50%
100%
pR
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 50
0.2
0.4
0.6
0.8
1
V = 2 U∞/(ωαc)
ω/ω
α
Figure 4.1: V -g plot of HALE typical section model with steady aerodynamics:stable mode (dashed line); unstable mode (solid line).
Each aerodynamic model predicts a different behavior of dynamic instability for the
structural data from Table 4.1. The steady aerodynamic model predicts divergence,
whereas the quasi-steady model is dynamically unstable for all flow velocities. By
contrast, only the complete unsteady model predicts the flutter behavior observed ex-
perimentally for the HALE wing; these flutter results are compared against available
data in Table 4.3. Despite tailoring the typical section analysis to the experimental
wing and its known flutter mode, the reduced frequency and reduced velocity at the
flutter point differ from the experimental values by factors of 2.9 and 0.58, respec-
tively. The flutter frequency is in relatively good agreement with a prediction 16%
lower than experiment.
4.1.2 Conclusions
The unsteady and non-circulatory contributions to lift and moment are necessary to
predict the flutter behavior of the linear typical section representation of the HALE
36
0 0.25 0.5 0.75 1 1.25 1.5 1.75 2−3%
−2%
−1%
0%
1%
2%
3%
pR
0 0.25 0.5 0.75 1 1.25 1.5 1.75 20
0.2
0.4
0.6
0.8
1
V = 2 U∞/(ωαc)
ω/ω
α
Figure 4.2: V -g plot of HALE typical section model with quasi-steady aerodynam-ics: stable mode (dashed line); unstable mode (solid line).
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5−3%
−2%
−1%
0%
1%
2%
3%
pR
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 50
0.2
0.4
0.6
0.8
1
V = 2 U∞/(ωαc)
ω/ω
α
Figure 4.3: V -g plot of HALE typical section model with unsteady Theodorsenaerodynamics: stable mode (dashed line); unstable mode (solid line).
37
Table 4.3: Typical section flutter comparison with HALE wing data.
Parameters Present Analysis Tang & Dowell [106]k 0.305 0.105V 2.72 4.72ω/ωα 0.829 0.989h/(αb) 1.127 + 5.852i –
experimental wing. A reduction of the aerodynamic model to steady and quasi-steady
approximations leads to drastically different instability behavior, as corroborated by
other flutter studies, e.g. Ref. [64]. However, the poor numerical agreement between
experiment and the typical section model using Theodorsen unsteady aerodynamics
suggests the need for more sophisticated structural and/or aerodynamic modeling to
represent the HALE wing configuration.
4.2 Hodges-Dowell Nonlinear Beam & ONERA Dynamic Stall Model
4.2.1 Equation Formulation and Time-Marching Scheme
The Hodges-Dowell nonlinear beam equations of Section 2.3 and the ONERA aerody-
namic model in Section 3.3 are combined to create a fully-coupled nonlinear aeroelas-
tic system. This time-marching formulation extends beyond the modeling capacity of
the typical section model to include the effects of beam geometry, nonlinear stiffness,
and nonlinear stall aerodynamics on aeroelastic stability and limit cycle oscillations.
The aeroelastic model is cast into the following set of ordinary differential equa-
tions in time by assuming modal forms of the generalized coordinates and integrating
the equations over the wing span.
38
NC∑p=1
δip(Vp + 2 ξv ω1C Vp + ω2
pCVp
)+ β
NB∑q=1
NT∑r=1
KiqrWqΦr
+Vp ψi(x = 1)
[(M
mL
)ψp(x = 1) +
(IvmL2
)ψ′p(x = 1)
]
= κ1
NAERO∑l=1
∆l ψi(x = xl) [−CDl + (θ0 − φλl)CLl]
+ κ2ψi(x = 1)∆Fv(x = 1)−( gL
sin θ0
) [(M
mL
)ψi(x = 1) + Ψi
](4.3)
NB∑q=1
δiq(Wq + 2 ξw ω1BWq + ω2
qBWq
)+ β
NC∑p=1
NT∑r=1
KpirVpΦr − e
NT∑r=1
EirΦr
+Wq ψi(x = 1)
[(M
mL
)ψq(x = 1) +
(IwmL2
)ψ′q(x = 1)
]
= κ1
NAERO∑l=1
∆l ψi(x = xl) [CLl + (θ0 − φλl)CDl]
+ κ2 ψi(x = 1)∆Fw(x = 1)−( gL
cos θ0
) [(M
mL
)ψi(x = 1) + Ψi
](4.4)
NT∑r=1
δir(Φr + 2 ξφ ω1T Φr + ω2
rT Φr
)+
β
K2
NC∑p=1
NB∑q=1
KpqiVpWq
− e
K2
NB∑q=1
EqiWq +
(Iφ
mK2L
)Θi(x = 1)
NT∑r=1
ΦrΘr(x = 1)
= κ1c
K2
NAERO∑l=1
∆lΘi(x = xl) CMl − (yac/c) [CLl + (θ0 − φλl)CDl]
+ κ3 Θi(x = 1)∆Mx(x = 1) (4.5)
Let q be a state vector defined as
q =Vp, Vp, Wq,Wq, Φr,Φr, (CL2)l, (CL2)l, (CLγ)l
T
, (4.6)
39
such that Eqns. 4.3–4.5 can be expressed as a state-space matrix equation to which
a time-marching scheme can be readily applied. The present work employs the
standard fourth-order Runge-Kutta time-marching scheme [15, 59, 60, 91, 94] using
a fixed time step interval.
[A] q + [B]q = F0 + FN (4.7)
Coefficient matrices [A] and [B] depend on the flow velocity and structural parame-
ters, and the force vectors F0 and FN represent respectively the gravity effects and
the nonlinear forces due to structural and aerodynamic stall nonlinearities [106].
All simulations performed herein use the experimentally obtained data from Ta-
ble 4.4 with a time step of ∆t = 8192−1 s assuming ten spanwise aerodynamic strips,
NAERO = 10. The numbers of assumed modes for the flap, lag, and twist directions
are NC = 1, NB = 4, and NT = 1, respectively. All comparisons between simulation
and experiment assume a representative root angle of θ0 = 1.
4.2.2 Flutter Prediction
Setting the force vectors F0 and FN of Eqn. 4.7 to zero determines the strictly linear
flutter boundary, which does not include the effects of initial conditions, static defor-
mation, or nonlinearity. Figure 4.4 illustrates the sensitivity of the flutter boundary
to both the number of specified aerodynamic panels and the spanwise location on
each of the panels at which the aerodynamic loads are evaluated. As the number of
panels increases, the evaluation location has a weaker influence on the flutter speed.
However, Fig. 4.4 also suggests that an accurate flutter prediction is possible for
only a few panels with a proper choice of evaluation location. The flutter speed
using the 65%-span location agrees well for a number of panels greater than or equal
to two, suggesting that at least two panels are required to describe appropriately the
second-bending flap motion of the flutter and LCO response of the present HALE
40
Table 4.4: Experimental wing model data (adapted from Ref. [106]).
Property Value
WingSpan L 0.4508 mChord c 0.0508 mMass per unit length m 0.2351 kg/mMoment of inertia (50% chord) mK2
m 2.056×10−5 kgmSpanwise elastic axis 50% chordCenter of gravity 49% chordFlap bending rigidity EI1 0.4186 N m2
Lag bending rigidity EI2 18.44 Nm2
Torsional rigidity GJ 0.9539 N m2
Flap structural modal damping ξw 0.02Lag structural modal damping ξv 0.025Torsional structural modal damping ξφ 0.031First flap natural frequency ω1B 3.675 HzSecond flap natural frequency ω2B 23.03 HzThird flap natural frequency ω3B 64.50 HzFourth flap natural frequency ω4B 126.3 HzFirst lag natural frequency ω1C 24.39 HzFirst torsional natural frequency ω1T 119.5 Hz
Slender BodyRadius R 4.762×10−2 mChord length cSB 0.1406 mMass M 0.0417 kgMoment of inertia Iw 0.9753×10−4 kgm2
Moment of inertia Iv 0.3783×10−4 kgm2
Moment of inertia Iφ 0.9753×10−4 kgm2
Volume –V1 1.001×10−5 m3
Volume static unbalance –V2 0.0 m4
Volume moment of inertia –V3 1.64×10−8 m5
41
0 0.1 0.2 0.3 0.4 0.5 0.6 0.7 0.8 0.9 120
22
24
26
28
30
32
34
36
38
40
Normalized Evaluation Location on Panel
UF
[m/s]
12451020
Figure 4.4: Dependence of flutter speed on the number of panels and the spanwiseaerodynamic evaluation location on each panel for the HALE wing configuration.Assumes the ONERA lift model coefficients from Tang & Dowell [106].
model. Also, the agreement of flutter speeds at the 65%-span location of each panel
is the equivalent ‘3/4 span rule’ typically used to reduce beam flutter problems to
equivalent typical sections.
The observed second-bending/first-torsion coalescence flutter mode is predicted
using the linear beam model with linear unsteady aerodynamics. Also, the converged
flutter speed of UF = 34.5m/s in Fig. 4.4 is in good agreement with the experimental
value of UF = 33.5m/s. Therefore, the simplest model required to make a useful
flutter prediction for a HALE-type wing must include beam geometry and fully
unsteady, linear aerodynamics.
Figure 4.5 compares the source data used for ONERA lift model identification
with respect to their impact on the flutter speed. Despite the close numerical agree-
ment between the ONERA models based on wind tunnel or CFD unsteady data (cf.
42
2.8 3 3.2 3.4 3.6 3.8 4 4.234
35
36
37
38
39
40
a0L · αL
UF
Wind Tunnel DataCFD Data
Figure 4.5: Sensitivity of flutter speed to source data for the linear ONERA liftmodel and to the product of parameters a0L and αL.
Table B.1), the flutter speed is notably sensitive to the product of the two parameters
with the largest variation: the static lift curve slope, a0L; and the unsteady ONERA
parameter αL. The product of these terms varies from 2.83 to 3.45 to 4.2 for the
linear ONERA models considered by Dunn [32, 33, 34], Tang & Dowell [106], and the
CFD-based model identified in the present work. The sensitivity to these parameters
yields a flutter speed variation of up to 14% relative to the observed flutter speed.
The cumulative effect of the differences between the rest of the other linear ONERA
coefficients in Table B.1 amounts to a much smaller variation in flutter speed of
nearly a percent.
4.2.3 Limit Cycle Oscillations
Flutter can lead to an exponential growth of unsteady motion into a limit cycle os-
cillation, which by definition must embody a nonlinear feature in the structure, the
aerodynamic flow, or both. The sensitivity of the computed limit cycle oscillation
43
amplitude and hysteresis to these nonlinearities and to the source data of the ON-
ERA dynamic stall model is compared against experimental results from Ref. [106].
Each simulated limit cycle analysis begins at a sufficiently low flow velocity such
that the wing achieves a static steady state, after which the velocity is increased by
∆U = 0.1m/s. The aeroelastic model simulates 200 seconds of time at each velocity,
and the root-mean-squared (rms) amplitude of the unsteady motion is determined
by data from the final 10 seconds. The flow velocity increases until a critical veloc-
ity is reached, beyond which a numerical or possibly a physical divergence occurs
in the theoretical model, which is supported by observations for the present aeroe-
lastic model in previous researches, e.g. [106, 109]. The simulated flow velocity is
then decreased incrementally until the limit cycle oscillation disappears and a static
aeroelastic state is recovered.
Figure 4.6 investigates the effect of structural nonlinearity arising from elastic
coupling between the the flap, lag, and twist motions. The aeroelastic model used
by Tang & Dowell [106] including both structural and aerodynamic stall nonlineari-
ties is in relatively good agreement with experiment with respect to LCO amplitude
and hysteresis. Without the structural nonlinearity, the limit cycle amplitude curve
is reversible with respect to flow velocity. Therefore, the existence of hysteresis is
a direct consequence of structural nonlinearity arising from elastic coupling. Also,
the effect of structural nonlinearity increases the limit cycle amplitude at the flut-
ter point. However, elastic coupling leads to an anticipated stiffening effect and
comparatively lower LCO amplitudes at higher flow velocities.
Figure 4.7 shows the impact of the aerodynamic model on the flutter and limit
cycle oscillation behavior of the HALE wing. The ONERA model used by Tang &
Dowell [106] agrees well with experiment with respect to flutter speed, hysteresis
bandwidth, and LCO amplitude; note that the flutter speed for the statically de-
formed wing is only slightly lower than the speed predicted by the strictly linear
44
30 32 34 36 38 40 420
5
10
15
20
25
Flow Velocity, U [m/s]
Mid
span
rms
Am
plitu
de
[mm
]
Without Nonlinear StiffnessWith Nonlinear StiffnessExperiment
Figure 4.6: Comparison of computational results with and without nonlinear beamstiffness, including experimental data from Ref. [106]. Solid/dashed lines denoteincreasing/decreasing flow velocity.
calculation. When the linear ONERA lift coefficients based on wind tunnel data are
replaced with those identified by CFD data in Table B.1, the flutter speed increases
from 34.3m/s to 39.8m/s and the predicted LCO amplitude is roughly 20% larger.
Thus, the linear aerodynamic coefficients are significant for quantitative accuracy of
both flutter speed and LCO amplitude. The non-smooth bifurcation curve for this
aeroelastic response is due to the assumption of a sinusoidal response at a single fre-
quency in the rms amplitude calculation. Figure 4.8 depicts the unsteady oscillation
at U = 40.5m/s and its frequency spectrum, which includes low-frequency content
that effects the rms amplitude computation.
Conversely, an ONERA model is also constructed from the linear ONERA coef-
ficients from Ref. [106] and the nonlinear aerodynamic terms and static stall curve
45
identified by CFD. Because the nonlinear ONERA coefficients of the wind tunnel and
CFD models are virtually identical, a comparison of the nonlinearity in these two
models is effectively a comparison of their static lift curves. Recall that these static
lift curves prescribe the forcing function for the nonlinear component of the ONERA
lift model. The new prediction for LCO amplitude also increases but with a lesser
sensitivity of the amplitude to the flow velocity. The hysteresis bandwidth doubles
for the new nonlinear model in comparison to the original aeroelastic computation,
as it did for the new linear coefficients. Therefore, the aerodynamic nonlinearity
due to dynamic stall, which for the ONERA model also depends on its linear coeffi-
cients, and the structural geometric nonlinearity are both important in quantifying
hysteresis behavior.
Both modified aerodynamic models, identified as Case 1 and Case 2 in Fig. 4.7,
hinder the ability to simulate limit cycle oscillations at flow velocities much greater
than the flutter speed. When using the ONERA aerodynamic model with both linear
and nonlinear parts identified by CFD data, the simulation diverges at the flutter
speed. The sensitivity of the aeroelastic model based on the Hodges-Dowell equations
and ONERA dynamic stall aerodynamics is noted in the literature [106, 109], where
small parametric variations in the flow scenario can lead to divergent behavior that
may be rooted in either numerical or physical instability. It should also be noted that
the limit cycle calculations shown in Figs. 4.6 and 4.7 are strictly divergent when the
aerodynamic nonlinearity is removed.
The divergent nature of the nonlinear aeroelastic system is further investigated by
considering a quasi-steady approximation of the aerodynamic model. For this model
the aerodynamic lift is computed from the static lift curve and the effective angle
of attack, which includes the instantaneous incidence angle and the quasi-steady in-
flow angle. Figure 4.9 compares the bifurcation curves of the ONERA models based
on wind tunnel of CFD static lift data. The flutter speeds and resulting LCO am-
46
plitudes are much smaller than the results predicted by unsteady aerodynamics and
experimental observation. Hysteresis is also observed for quasi-steady aerodynamics;
however, the bandwidth is narrower, noting the difference in scales in comparison
with Fig. 4.7. The bifurcation curves for the quasi-steady cases can be extended to
greater flow velocities beyond the flutter point than for the comparable unsteady
computations, up to 48.9 and 50.0m/s for the CFD- and wind-tunnel-based models,
respectively. When the aerodynamic nonlinearity due to stall is removed, both quasi-
steady model simulations diverge as also observed for the unsteady cases. Therefore,
the present aeroelastic model is exquisitely sensitive to input parameter combinations
and suggests that a stable limit cycle oscillation is not possible without the presence
of the aerodynamic nonlinearity associated with dynamic stall. Moreover, the aeroe-
lastic simulations indicate that unsteadiness in the aerodynamic model is essential
to the accurate flutter and LCO prediction of HALE wings, but this unsteadiness
may also be the source of the divergent computational behavior for post-flutter cal-
culations.
4.2.4 Time Estimates for First-Principles Aeroelastic Model
Application of the ONERA dynamic stall model to aeroelastic analyses enables rapid
time-marching and stability computations. For example, the simulated bifurcation
curves for Figs. 4.6 and 4.7 require computational times of less than half an hour
on a single processor. However, as with other reduced-order models, the ONERA
nonlinear lift model is limited by the data used for its parameter identification and
by the ability of the model equations to approximate this data appropriately over
a range of flow situations. Also, the ONERA model represents only the integrated
load on a particular airfoil section and does not provide any information about the
physics of the unsteady flow field. Thus, a natural extension of the present work is
to couple the Hodges-Dowell nonlinear beam equations instead with a CFD solver
47
3032
3436
3840
42051015202530
Flo
wV
eloci
ty,U
[m/s]
MidspanrmsAmplitude[mm]
E
xper
imen
t:U
↑E
xper
imen
t:U
↓T
ang
&D
owel
l(2
001)
:U
↑
Tan
g&
Dow
ell(2
001)
:U
↓C
ase
1:U
↑C
ase
1:U
↓C
ase
2:U
↑C
ase
2:U
↓
Fig
ure
4.7
:B
ifurc
atio
ndia
gram
com
par
ison
offu
lly
non
linea
rco
mputa
tion
alre
sult
san
dex
per
imen
tal
dat
afr
omR
ef.
[106
].C
ases
1/2
den
ote
ON
ER
Aae
rodynam
icm
odel
susi
ng
linea
rpar
amet
ers
bas
edon
CFD
/win
dtu
nnel
dat
aan
da
non
linea
rst
atic
lift
curv
efr
omw
ind
tunnel
/CFD
resu
lts.
48
0 5 10 15 20−50
−40
−30
−20
−10
0
10
20
30
40
50
Time [s]
Mid
span
Am
plitu
de
[mm
]
(a)
0 5 10 15 20 25 300
5
10
15
20
25
Frequency [Hz]
Am
plitu
de
[mm
]
(b)
Figure 4.8: Limit cycle oscillations at U = 40.5 m/s for aeroelastic model usinglinear ONERA coefficients based on CFD data and a nonlinear static lift curve fromRef. [106]: (a) time series; (b) frequency spectrum.
49
20 20.5 21 21.5 22 22.5 230
0.5
1
1.5
2
2.5
3
3.5
4
4.5
5
Flow Velocity, U [m/s]
Mid
span
rms
Am
plitu
de
[mm
]
Wind TunnelCFD
Figure 4.9: Bifurcation diagram comparison of quasi-steady ONERA aerodynamicmodels using static lift curves based on wind tunnel or CFD data.
to create a complete first-principles aeroelastic model to gain greater insight into the
nonlinear dynamics of HALE wings.
The tradeoff for this improvement in the aerodynamic model is a large increase in
the computational cost required to determine a stable limit cycle oscillation, as well as
the long transients of the fluid-structure system near the flutter point. Using the CFD
code OVERFLOW, a parametrically-converged period of LCO for a two-dimensional
section of the experimental HALE wing requires 26.5 hours of computational time
for a limit cycle frequency of fLCO = 21.5Hz at a reduced frequency of k = 0.1. The
present work and Ref. [106] suggest that nearly 15 simulated seconds are necessary
to capture the transition from flutter to a stable limit cycle at the flutter speed,
which would take nearly a year of computational time to compute a single point
on the bifurcation diagram. By using results from the present work to prescribe
50
initial conditions for a limit cycle, the required simulated time could be reduced
to one or two seconds to capture a stable limit cycle oscillation using 47.5 days of
computational time for each value of the flow velocity.
These computational costs may be reduced by roughly an order of magnitude
using the harmonic balance technique developed by Hall et al. [49], which was recently
extended to convert existing time-domain codes to the frequency domain [23, 24,
114]. A first-principles aeroelastic model in the frequency domain would inform
the companion time-marching analysis to facilitate rapid agreement between the
two models. Thomas et al. [115, 116] have demonstrated the ability of a harmonic
balance CFD solver to predict accurate limit cycle oscillations for the linear typical
section in nonlinear transonic flow. An extension of this work to nonlinear dynamic
stall aerodynamics at low subsonic Mach numbers for a nonlinear beam model would
create the first fully nonlinear aeroelastic model for the HALE configuration based
entirely on first-principles physics.
51
5
Conclusions
The objective of this research is to perform predictive aeroelastic analyses for the
flutter and limit cycle oscillation behaviors of flexible wing representative of HALE
aircraft using a range of structural and aerodynamic models. These models include
the effects of beam geometry, nonlinear structural stiffness due to elastic coupling
between the degrees of freedom, and nonlinear aerodynamics associated with dynamic
stall. A new ONERA dynamic stall model is identified from steady and unsteady
data computed by the CFD code OVERFLOW, which is compared to the standard
model based on wind tunnel data. The range of structural and aerodynamic models
considered enables a gradual increase in the sophistication of the aeroelastic model to
determine which modeling features are essential to the prediction of flutter and LCO
behaviors for HALE wings via correlation with the experimental data of Ref. [106].
The present work also establishes the roles of structural and aerodynamic nonlinearity
on the aeroelastic system and the impact of aerodynamics based on first-principles
rather than wind tunnel data.
The non-uniform design of the HALE experimental wing is first analyzed us-
ing finite element analysis to quantify the effects of periodically-spaced elements of
52
various materials, material removal, and the presence of a tip store on the natural fre-
quencies and mode shapes. The natural frequencies of interest are affected by these
non-uniformities, and these results are reduced to design curves for the construction
of similar HALE aeroelastic wings. However, the mode shapes are well-approximated
by uniform beam modes, whose agreement improves with the addition of the tip store.
This result demonstrates the appropriate use of uniform beam modes to approximate
nonuniform wings with a beam-like structure, a result which is typically assumed to
be true in aeroelastic analyses similar to the present work. Moreover, the valid-
ity of continuous beam modes enables their use as trial functions for the Galerkin
projections of continuum beam models, such as the Hodges-Dowell nonlinear beam
equations, to describe the HALE wing structure for aeroelastic analyses.
A typical section aeroelastic model is first considered to make a posteriori es-
timates of the flutter speed using representative structural data and flutter mode
information from experiment. This system describes the lift and moment with stan-
dard steady, quasi-steady, and full unsteady Theodorsen aerodynamics models. Each
aerodynamic model predicts a different instability behavior. Only the unsteady
Theodorsen aerodynamic model is able to identify correctly the flutter instability
but with noticable disagreement between the predicted flutter speed and mode re-
sults and the experimental results. An accurate predictive model for HALE wing
flutter is found to require the additional feature of beam geometry, which is modeled
by the linear beam reduction of the Hodges-Dowell equations in conjuction with the
Theodorsen-like linear aerodynamics of the ONERA aerodynamic model.
Flutter instability leads to limit cycle oscillations for the cantilevered aeroelas-
tic wing considered in this work. The nonlinear aeroelastic model, comprised of the
Hodges-Dowell nonlinear beam equations and the ONERA dynamic stall model, sug-
gests that the aerodynamic nonlinearity due to dynamic stall is essential to predict
a stable limit cycle oscllation. Both the structural and aerodynamic nonlinearities
53
effect the hysteresis bandwidth of the limit cycle motions, but the hysteresis vanishes
when the structural nonlinearity is removed from the aeroelastic model. The nonlin-
ear elastic coupling is identifed as the key feature necessary to model the hysteresis
of HALE wing LCO and is the mechanism by which the aerodynamic nonlinearity
effects this hysteresis bandwidth.
The ONERA dynamic stall models identified by first-principles CFD data or wind
tunnel data compare the influence of aerodynamic source information on both flutter
and LCO. The standard model based on wind tunnel data is in excellent agreement
with experiment with respect to flutter speed, LCO amplitude, and hysteresis band-
width [106]. When the linear coefficients of this model are changed to those of the
CFD model, the flutter speed increases by 16% and the predicted LCO amplitude
increases by roughly 20%. A more complex frequency spectrum is observed for this
model, which includes many frequencies lower than the predominant single limit
cycle frequency found in other simulations. The dynamic stall contribution of the
CFD-based model is found to increase the LCO amplitude and hysteresis bandwidth
similarly as compared to the wind tunnel model. The close agreement between the
nonlinear ONERA coefficients for the wind tunnel and CFD models indicates that
the principal difference between dynamic stall behavior of the two models is due to
the static stall characteristics that drive the nonlinear lift dynamics.
The aeroelastic model of the Hodges-Dowell nonlinear beam equations and the
semi-empirical ONERA dynamic stall model based on CFD data is intended to
approximate and anticipate the effects of nonlinear, first-principles, computational
aeroelastic modeling for a simple HALE wing configuration. The present work may
used as a benchmark for more complex geometrical configurations and complete first-
principles analyses where the aerodynamic loads are computed by a CFD solver.
54
5.1 Future Work
The present work invites a number of natural research extensions to improve the
fidelity of the aeroelastic computation and the realism of the modeling effort for
modern HALE wing configurations.
First, the structural model may be modified to include the rigid body modes,
which are known to be important to the gust response of slender wings. A compan-
ion wind tunnel test with a cantilevered wing mounted on a tunable spring would
account for the symmetric aeroelastic effects of a HALE wing in the limit of zero
spring stiffness, which is an attractive alternative to a much more difficult free-flying
experimental setup.
Second, flow field measurements using techniques such as particle image velocime-
try (PIV) may be used to capture the dynamic interaction of the elastic wing with
vortex generation and dynamic stall events. This investigation would extend the
modest amount of published work regarding the distinction between pitching and
plunging motions for large unsteady motions, for which much more is known than
about the flow dynamics for a wing structure in a limit cycle oscillation. Experimen-
tal LCO flow field measurements would also provide benchmark data for aeroelastic
analyses using a CFD code.
And third, the present analysis may be extended to a fully-coupled aeroelastic
analysis using the existing nonlinear beam model with a computational fluid dynam-
ics solver. This may be implemented with a time domain [37, 62] or frequency domain
code [23, 24, 49, 115, 116], the latter of which may offer a significant reduction in
computational cost by avoiding the long transients of aeroelastic simulations near
the flutter point. It should be noted that the flutter speed observed for the experi-
mental wing by Tang & Dowell [106] occurs at Re = 1.15× 105, which is an order of
magnitude smaller than the Reynolds numbers associated with the data used for the
55
ONERA model parameter identification. The Reynolds number of the experiment
is sufficiently low such that transitional flow effects may become important, and a
suitable CFD code may elucidate these effects on the dynamic stability of flexible
wings to provide further insight into the complex fluid-structure interactions that
may be encountered by HALE aircraft.
56
Appendix A
Time-Domain Computational Fluid DynamicsSolver
The computational fluid dynamics code OVERFLOW 2.1 was developed by Nichols
and Buning [74] at NASA Langley Research Center to enable high-fidelity, unsteady
aerodynamic modeling for complex geometries using Chimera overset grid techniques.
OVERFLOW performs implicit time-domain analyses and employs a suite of dis-
cretization schemes and turbulence models to suit the needs of a particular flow
situation. Custer [23] reviewed recently the development of OVERFLOW and ex-
tended its capabilities to nonlinear frequency-domain analysis, including the use of
overset grids for sufficiently small motions [24, 114].
The present work uses OVERFLOW in its original time-domain form to com-
pute unsteady aerodynamic loads for prescribed motion at large angles of attack.
This Appendix summarizes the fundamental equations and assumptions made in
the computational model to identify a new ONERA dynamic stall model based on
first-principles aerodynamic data obtained from OVERFLOW.
57
A.1 Fluid Equations
The compressible, three-dimensional Navier-Stokes equations are presented in strong
form as a result of conserving mass, momentum, and energy for an arbitrary volume
of a calorically-perfect, Newtonian gas.
The mass conservation expression for a fluid, or continuity equation,
Dρ
Dt+ ρ(∇ ·V) = 0, (A.1)
relates the time rate of change of the density of a fluid particle to the divergence of the
velocity field, where this divergence can be interpreted physically as the volumetric
time rate of change of a moving fluid element [4].
Cauchy’s equation of motion represents the conservation of momentum for any
continuum substance subjected to an arbitrary distribution of body forces and surface
tractions [2].
ρDV
Dt= ρ f +∇ ·Π (A.2)
The properties of a Newtonian fluid are invoked to establish a constituitive relation-
ship for the stress tensor, Π. By definition, a fluid cannot sustain a shear stress at
rest [39], and although fluids can resist shear, they are unable to withstand a defor-
mation [96]. Furthermore, a Newtonian fluid assumes a linear relationship between
stress and the rate-of-strain. These simplifying assumptions allow for the stress ten-
sor to be separated into a hydrostatic pressure (normal stress) term and a deviatoric
stress component to account strictly for viscous shear [11].
Πij = −p δij + τij (A.3)
The isotropic fluid assumption [6, 65] simplifies the deviatoric stress tensor, τ , and
further reduces the constituitive description for a Newtonian fluid to two independent
58
fluid coefficients: the dynamic viscosity, µ, and the second (dilitational) coefficient
of viscosity, λ [43].
τij = µ (ui,j + uj,i) + λ δij(∇ ·V) (A.4)
The quantities µ and (λ + 2µ/3) must be non-negative to satisfy the second law of
thermodynamics [43]. Stokes [100] assumed the relationship (λ+ 2µ/3) = 0 to force
the mechanical pressure to be equal to the thermodynamic pressure, which differ for
nonequilibrium thermodynamic processes. However, the Stokes hypothesis holds for
most flow investigations of aeronautical interest. The result of the hypothesis on the
fluid equations is exact for inviscid flows and incompressible flows, and valid within
boundary layer approximations where the normal viscous stresses are much smaller
in comparison to the shear stresses [43]. The application of Stokes’s hypothesis to
Eqn. A.4 enables Eqn. A.2 to be rewritten as the famous Navier-Stokes equation [111].
ρDV
Dt= ρ f −∇p +
∂
∂xj
[µ
(∂ui
∂xj
+∂uj
∂xi
)− 2
3δijµ
∂uk
∂xk
](A.5)
Energy conservation can be expressed simply by direct application of the first law
of thermodynamics to a fixed infinitesimal control volume [111].
∂Et
∂t+∇ · (EtV) =
∂Q
∂t−∇ · q + ρ f ·V +∇ · (Π ·V) (A.6)
The total energy per unit volume is expressed as Et = ρ[e + (V · V)/2]. The two
terms on the left-hand side of Eqn. A.6 denote respectively the time rate of change
of total fluid energy per unit volume, and the convection of heat energy away from
the control volume. The first term on the right-hand side (RHS) represents heat
generation within the fluid, for example, from electrical power dissipation [12]. The
second RHS term describes the conduction of heat of away from the control surface,
which can be expressed in terms of temperature by Fourier’s law, q = −k∇T . The
remaining two terms denote the increase in total energy due to body forces and
59
surface forces, respectively. A final energy equation follows by incorporating Fourier’s
law, Eqn. A.4, and Stokes’s hypothesis into Eqn. A.6.
ρDe
Dt=∂Q
∂t+∇ · (k∇T )− p(∇ ·V) + Φ (A.7)
The viscous dissipation function, Φ, is defined as
Φ = ∇ · (τ ·V)− (∇ · τ ) ·V. (A.8)
Lastly, an equation of state is required to render the fluid equations well-posed
with respect to the number of equations and unknown variables. A calorically-perfect
gas obeys the expression
p = ρRT, (A.9)
with constant-valued specific heats. The calorically-perfect gas assumption allows
Eqn. A.9 to be written alternatively as p = (γ − 1)ρe or T = (γ − 1)e/R, where
γ ≡ cp/cv and cp = γR/(γ − 1).
The fluid equations from Eqns. A.1, A.5, A.7, and A.9 combine into a compact
vector form that enables the direct application of finite differencing scheme. Thus, the
compressible Navier-Stokes equations in a Cartesian coordinate system are expressed
as [111]
dU
dt+dE
dx+dF
dy+dG
dz= 0, (A.10)
60
where
U =
ρρuρvρwEt
(A.11)
E =
ρu
ρu2 + p− τxx
ρuv − τxy
ρuw − τxz
(Et + p)u− uτxx − vτxy − wτxz + qx
(A.12)
F =
ρv
ρuv − τxy
ρv2 + p− τyy
ρvw − τyz
(Et + p)v − uτxy − vτyy − wτyz + qy
(A.13)
G =
ρw
ρuw − τxz
ρuv − τyz
ρw2 + p− τzz
(Et + p)w − uτxz − vτyz − wτzz + qz
(A.14)
The Cartesian vector form of the Navier-Stokes equations must be converted to a
generalized coordinate system that will allow for the computation of aerodynamic
flows on complex grids. Figure A.1 shows the computational grid for the NACA
0012 airfoil considered in this work, which was designed specifically for unsteady
aerodynamic analyses by clustering high-resolution regions at the leading and trailing
edge region where large gradients are expected. The physical domain of Fig. A.1 can
be transformed to a regular computational domain in a generalized coordinate system
(ξ,η,ζ).
ξ = ξ(x, y, z) (A.15)
η = η(x, y, z) (A.16)
ζ = ζ(x, y, z) (A.17)
61
(a) (b)
Figure A.1: Physical C-grid for NACA 0012 airfoil with 401×75 resolution and19c outer radius: a) far view; b) near view.
Eqns. A.10–A.14 can be rewritten in the generalized coordinate system of the com-
putational domain by the chain rule. The Jacobian for this transformation is defined
as
J =∂(ξ, η, ζ)
∂(x, y, z)=
∣∣∣∣∣∣ξx ξy ξzηx ηy ηz
ζx ζy ζz
∣∣∣∣∣∣ , (A.18)
where the transformation metrics are computed numerically [38]. The transformed
fluid equations retain the original vector form of Eqn. A.10 with modest changes to
the vector expressions [111].
dU
dt+dE
dx+dF
dy+dG
dz= 0, (A.19)
62
U =1
JU (A.20)
E =1
J(ξxE + ξyF + ξzG) (A.21)
F =1
J(ηxE + ηyF + ηzG) (A.22)
G =1
J(ζxE + ζyF + ζzG) (A.23)
These equations enable the direct application of finite-differencing schemes for fixed
grid geometries. Deforming grid geometries require further consideration of the trans-
formation metrics by the geometric conservation law [117, 118] to be consistent and
prevent errors in the solution. All unsteady aerodynamic computations were per-
formed using solid body rotation and translation of the physical grid.
In the present work, the temporal and spatial derviatives are represented by
the Symmetric Successive Over-Relaxation (SSOR) Unfactored Method [75] and the
HLLC upwind method [119], respectively, which have proven to be robust algorithms
within OVERFLOW for large unsteady motions over a range of reduced frequencies.
A.2 Reynolds Averaging
The use of direct simulations of the Navier-Stokes equations for practical engineering
flows is precluded by the phenomenon of turbulence. Turbulence is inherently three-
dimensional and is characterized by a broad and continuous spectum of length scales.
Larger turbulent eddies break down and transfer their kinetic energy to smaller
eddies in a cascading process that continues until the energy smallest eddy dissipates
into heat through the action of molecular viscosity [122]. The size of the smallest
eddy sets the minimum length scale for a physical grid for direct Navier-Stokes
(DNS) simulations. The smallest eddy is much larger than the molecular length
scale [112] but is extremely small compared to the greater computational grid and
63
solid bodies of interest. However, most aerodynamic flows of engineering interest
do not require the turbulent structure to be fully resolved to provide useful and
accurate results. Computations for high Reynolds number flows typical of aerospace
applications focus on the impact of turbulent flow on the force distribution over
a solid body. Comparatively rapid numerical solutions rely on averaged forms of
the Navier-Stokes equations to reduce the computational dependence on predicting
turbulent structures in favor of approximating the gross effects of turbulence on the
flow field.
Reynolds [92] approached turbulence by time-averaging the Navier-Stokes equa-
tions to eliminate all unsteadiness under the premise that all unsteadiness is due to
turbulence [38]. For a statistically steady flow, every variable can be expressed as a
time-averaged value and a time-dependent fluctuation about that value.
uj(x, t) = uj(x) + u′j(x, t) (A.24)
uj(x) ≡ lim∆t→∞
1
∆t
∫ t0+∆t
t0
uj(x, t) dt (A.25)
This averaging concept can be extended to unsteady flows by instead considering
an ensemble average of the desired variable, where the amount of ensemble data is
sufficiently large to eliminate the effects of the fluctuations [38].
uj(x, t) = limN→∞
1
N
N∑n=1
uj(x, t) (A.26)
Both methods in Eqns. A.25 and A.26 are referred to as Reynolds averaging, which
when applied to the fluid equations results in the Reynolds-Averaged Navier-Stokes
(RANS) equations [111].
∂ρ
∂t+
∂
∂xj
(ρuj + ρ′u′j) = 0 (A.27)
64
∂
∂t(ρui+ρ′u′i)+
∂
∂xj
(ρuiuj+uiρ′u′j) = − ∂p
∂xi
+∂
∂xj
(τij−ujρ′u′i−ρu′iu′j−ρ′u′iu′j) (A.28)
∂
∂t(cpρT + cpρ′T ′) +
∂
∂xj
(ρcpT uj) =
∂p
∂t+ uj
∂p
∂xj
+ u′j∂p′
∂xj
+∂
∂xj
(k∂T
∂xj
− ρcpT ′u′j − cpρ′T ′u′j
)+ Φ (A.29)
Note that the internal heat generation has been dropped from Eqn. A.29, which is
neglected for most fluid analyses of aerodynamic systems. The ensemble-averaged
deviatoric stress and viscous dissipation tensors are defined by Eqns. A.30 and A.31.
τij = µ
[(∂ui
∂xj
+∂uj
∂xi
)− 2
3δij∂uk
∂xk
](A.30)
Φ = τij∂ui
∂xj
+ τ ′ij∂u′i∂xj
(A.31)
The averaging process to formulate the RANS equations generates additional un-
knowns dependent on turbulent fluctuations for which there are no additional equa-
tions. Boussinesq [14] first approximated these Reynolds stress terms by introducing
the concept of turbulent eddy viscosity, which enables the effects of turbulence to be
modeled by a single laminar-like molecular viscosity.
− ρu′iu′j = µT
(∂ui
∂xj
+∂uj
∂xi
)− 2
3δij
(µT∂uk
∂xk
+ ρk
)(A.32)
The Boussinesq eddy viscosity assumption reduces the closure problem for the RANS
equations to a calculation of an effective turbulent viscosity, µT , to be determined
by a turbulence model.
A.3 Turbulence Modeling
Prandtl [89] developed the first model for the turbulent eddy viscosity based on his
mixing-length hypothesis, which used a scaling argument to relate mathematically
65
the momentum transfer of a turbulent eddy to an equivalent viscosity (µT ) or diffu-
sivity (νT = µT/ρ). The mixing length itself is unknown and varies from one type of
flow to another [12], thus relying on experimental data to calibrate the turbulence
model for each flow situation. Algebraic or zero-equation turbulence models such
as the mixing-length model are computationally attractive as they do not require
additional transport equations to be solved along with the conservation equations
for mass, momentum, and energy [122]. Prandtl later developed a physically more
realistic mathematical turbulence model where the turbulent stresses depended on
the kinetic energy of the turbulent fluctuations [90]. The addition of a transport
equation for the turbulent kinetic energy accounts for the fact that eddy viscosity is
dependent upon flow history. Turbulence models of this type are referred to as one-
equation models, which like the algebraic models are inherently incomplete because
they do not predict the turbulent length scale. In other words, something must be
known a priori about the flow other than initial and boundary conditions to ob-
tain a solution [122]. However, modern zero- and one-equation turbulence models
have proven to be both popular and useful for computational simulations of many
engineering applications.
For the present work, the Spalart-Allmaras one-equation turbulence model [98]
was selected for use in computational simulations with OVERFLOW. This selection
was based on good agreement between dynamic stall computations and available
experimental data, which was corroborated by computational-experimental compar-
isons in the literature, e.g. Ref. [99]. However, it should be noted that the Spalart-
Allmaras and other turbulence models are calibrated with steady flow data, and their
application to unsteady flow phenomena has been moderately successful although not
warranted rigorously by the model assumptions.
The Spalart-Allmaras turbulence model without trip line specification obeys the
66
transport equation,
Dν
Dt= σ−1∇ · [(ν + νT )∇ν] + cb2|∇ν|2+ cb1Sν − cw1fw
(ν
d
)2
, (A.33)
where the kinematic eddy viscosity, νT , is related to the Spalart-Allmaras variable,
ν, by νT = νfv1. Here it is important to note the distinction between the kine-
matic eddy viscosity, a theoretical construction from the Boussinesq approximation,
and the molecular viscosity, which is a fluid property [12]. The closure coefficients
and auxiliary relations necessary to complete the turbulence model are given by
Eqns. A.34–A.35 and Eqns. A.36–A.38, respectively.
cb1 = 0.1355, cb2 = 0.622, cv1 = 7.1, σ = 2/3 (A.34)
cw1 = cb1/κ2 + (1 + cb2)/σ, cw2 = 0.3, cw3 = 2, κ = 0.41 (A.35)
fv1 = χ3/(χ3 + c3v1), fv2 = 1− χ/(1 + χfv1), fw = g[
1+c6w3
g6+c6w3
]1/6(A.36)
χ = νν, g = r + cw2(r
6 − r), r = ν/(Sκ2d2) (A.37)
S = S + fv2ν/(κ2d2), S =
√2ΩijΩij, Ωij = 1
2( ∂ui
∂xj− ∂uj
∂xi) (A.38)
The tensor Ω is the fluid rotation tensor, and d is the distance to the closest surface.
67
Appendix B
ONERA Model Parameter Identification
Parameter identification of the ONERA model coefficients began largely as a trial-
and-error effort to determine which values for the assumed model form were well-
behaved and embodied the gross features of lift hysteresis loops (cf. Refs. [25, 85,
120]). McAlister et al. [69] systematized the identification process by linearizing
the ONERA equations about a steady-state angle of attack, at which the flow field
could be either linear or nonlinear. A large set of data for small-amplitude, har-
monic pitching motions about the quarter-chord location, performed over a range
of reduced frequencies and mean angles of attack, was then used both to identify
the ONERA coefficients computationally and to refine the formulation of the model.
Petot [86] later discovered that fewer experimental data sets were necessary to iden-
tify the model coefficients when using large-amplitude hysteresis loops. This method
determines the linear and nonlinear coefficients together and is most efficient for
data sets where the airfoil goes in and out of dynamic stall over a period of mo-
tion [3]. Alternatively, one could use aerodynamic data sets that are either only
stalled or unstalled to determine independently the nonlinear and linear coefficients,
68
respectively.
The present work employs Petot’s method [86] to create a new set of ONERA
parameter coefficients based on first-principles aerodynamic data computed by a com-
putational fluid dynamics (CFD) code. The CFD code OVERFLOW described in
Appendix A computes the aerodynamic forces on an isolated NACA 0012 section un-
dergoing large-amplitude motion representative of the experimentally-observed limit
cycle oscillation of the HALE aeroelastic wing [106]. From these CFD data and pa-
rameter identification, the salient features of the aerodynamic data are highlighted
and interpreted with respect to the sensitivity of the ONERA model to its provided
data, and to the changes in the flutter (linear) and LCO (nonlinear) behaviors of the
aeroelastic model.
B.1 Static Lift Curve
Parameter identification of the ONERA model begins with the static lift curve, which
determines the forcing function ∆CL for the dynamic stall aerodynamics. Static lift
CFD computations were performed at M = 0.3 and Re = 3.66×106 to be consistent
with the experimental data used to identify the original ONERA coefficients for
the NACA 0012 section [70]. These computational results were approximated by a
piecewise continuous curve with linear, parabolic, and exponential decay segments,
which are compared against the original CFD data in Fig. B.1.
(CL)CFD =
6.2486α 0 ≤ αdeg < 11.18
−62.43 (α− 0.24514)2 + 1.3755 11.18 ≤ αdeg ≤ 18.01
0.75715 e−11.412 (α−0.31435) + 0.31931 αdeg > 18.01(B.1)
Tang & Dowell [106] used a piecewise linear curve with discontinuous slopes to de-
scribe the static lift curve for aeroelastic computations with the ONERA model
69
originally based on wind tunnel test data.
(CL)TD =
2πα 0 ≤ αdeg < 10
1.096− 0.313 [αdeg − 10] αdeg > 10(B.2)
Both static lift curves agree well in the unstalled portion, with slope values near
the thin airfoil result of 2π. Abbott & von Doenhoff [1] corroborate this result
experimentally for the NACA 0012 section, whose additional lift due to its thickness
is balanced by the lift reduction due to boundary layer effects on the shed vorticity
necessary to satisfy the Kutta condition [63].
The static lift curves of Eqns. B.1 and B.2 also agree well with the inception
of stall at αss = 11.2 and 10, respectively, but differ for stalled flow. Figure B.2
compares the force deficit for Eqns. B.1 and B.2 against the discrete CFD steady
data and experimental data from Ref. [1], which was measured at Re = 3.00 × 106
and corrected for M ≈ 0. The CFD and experimental data suggest that ∆CL is small
and nonzero within the linear portion of the lift curve, where ∆CL = 0 is an assumed
feature of the approximate static lift curves. Also, the CFD and experimental data
indicate a smooth transition to stalled flow for the NACA 0012 section for the given
conditions. The better agreement between the discrete data and the CFD curve fit
suggests that the new curve fit is an improved and more realistic nonlinear forcing
function for the ONERA aerodynamic model.
B.2 Unsteady Parameters
The unsteady model coefficients are determined from a single hysteresis loop for
prescribed pitching motion α = 12 sin(kτ) about the quarter-chord for k = 0.1.
This scenario represents the most severe condition at a spanwise location on the
aeroelastic wing in Ref. [106]. To create a new set of coefficients, a lift hysteresis
loop is simulated numerically for the same prescribed motion using the existing
70
0 2 4 6 8 10 12 14 16 18 200
0.2
0.4
0.6
0.8
1
1.2
1.4
α [deg]
CL
Figure B.1: Piecewise curve fit to CFD static lift data: curve fit (solid line); data,.
ONERA coefficients [32, 33, 34]. A residual based on the mean-square difference
between the simulated lift and the discrete, unsteady CFD data determines the
error of the initial set of coefficients. MATLAB nonlinear optimization tools update
the unsteady ONERA coefficients and iterate the residual procedure until a set of
parameters converges.
Table B.1 compares the new set of ONERA coefficients against the original NACA
0012 coefficients used by Dunn [32, 33, 34], which are labeled as ‘wind tunnel’ results
to distinguish the impact of the data source on the model parameters. The sets
of parameters determined from wind tunnel and CFD data are strikingly similar,
particularly the nonlinear terms. Figure B.3 compares the lift hysteresis loops for
α = 12 sin(kτ), k = 0.1 using both sets of parameters and includes discrete lift
data from the CFD simulation. The elliptical loops of the CFD simulation and cor-
responding ONERA model suggest that the flow is weakly nonlinear, which may be
due to the unsteady airfoil motion maintaining attached flow. Therefore, the param-
71
−20 −15 −10 −5 0 5 10 15 20−1.5
−1
−0.5
0
0.5
1
1.5
α [deg]
∆C
L
CFD Curve FitTang & Dowell (2001)CFD DataExperiment
Figure B.2: Comparison of static lift curves from original ONERA model (Tang &Dowell (2001), Ref. [106]), CFD data, and experiment [1].
eter identification effects principally the linear aerodynamic terms. Because most
spanwise sections of the wing undergo smaller unsteady motions than the prescribed
CFD airfoil motion, the CFD data and reported experimental data [106] suggest that
linear aerodynamics may be sufficient to model LCO of the actual HALE aeroelastic
wing.
72
Table B.1: Comparison of ONERA lift parameters based on wind tunnel and CFDdata.
Data SourceParameter
Wind Tunnel [32, 33, 34] CFDa0L 5.9† 6.22sL 0.09 (180/π) 0.092 (180/π)kvL π/2 (0.504)πλL 0.15 0.146αL 0.55† 0.455σL 5.9 5.75a0 0.25 0.261a2 0.4 0.400r0 0.2 0.213r2 0.23 0.233e0 0.0 1.34×10−4
e2 -2.7 -2.74
† a0L = 6.28 and αL = 0.67 for computations in Ref. [106].
−12 −9 −6 −3 0 3 6 9 12−1.2
−0.8
−0.4
0
0.4
0.8
1.2
α [deg]
CL
Original ONERANew ONERACFD
Figure B.3: Lift hysteresis loops for two sets of ONERA model parameters forα = 12 sin(kτ), k = 0.1: ONERA model from wind tunnel data (dashed line);ONERA model from CFD data (solid line); CFD data, .
73
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Biography
Justin W. Jaworski was born on May 28, 1981 in Ft. Wayne, IN, the firstborn child of
Melissa and Warren Jaworski. He graduated from H.B. Plant High School in Tampa,
FL in 1999 and matriculated to Duke University the fall of the same year. As an
undergraduate, Justin received a number of named merit-based awards including the
Peggie C. Cleveland Scholarship, T.R. Mullen, Jr. Scholarship, and the Pratt Un-
dergraduate Fellowship. In 2003, Justin graduated with a Bachelor of Engineering
degree magna cum laude with distinction and was awarded the Mechanical Engineer-
ing and Materials Science Faculty Award for the highest scholastic average among
mechanical engineering graduates.
From 2003 to 2004, Justin worked as a research assistant on the Silent Air-
craft Initiative within the Aero/Astro Department at the Massachusetts Institute of
Technology. In August 2004, he returned to Duke to pursue graduate research with
Professor Earl Dowell, and completed a Master’s degree in May 2006. As a graduate
student, Justin has published three journal papers and has received external grants
from the North Carolina Space Grant Consortium and Sigma Xi to support his re-
search activities. He was awarded the Dean’s Award for Excellence in Mentoring
by the Graduate School and has served as a graduate student representative on the
Duke University Board of Trustees Facilities and Environment Committee.
Justin is a member of AIAA and ASME, and the honor societies of Sigma Xi, Pi
Tau Sigma, and Tau Beta Pi. He is also an avid classical singer and pianist.
85