63 Unsteady Aerodynamics, Aeroelasticity, & Flutter

Introduction

Aeroelasticity is a specialized field in aerospace engineering that examines the interactions between aerodynamic forces, elastic deformations, and the structural dynamics of aerospace structures. The essence of the field can be described by a Collar Diagram[1], which illustrates the interaction between the structural characteristics and the aerodynamic forces of a flight vehicle or another aeroelastic system. As shown in Figure 1, the Collar Diagram helps assess a structure’s stability and dynamic behavior under aerodynamic loads. This video provides an overview of this fundamental behavior as it affects the wings and tails of different airplanes.

A Collar Diagram illustrates the aeroelastic interplay among elastic, inertial, and aerodynamic effects.

The origins of aeroelasticity date back to the early days of aviation, when unexpected wing failures occurred on the first monoplanes. Many of these failures were traced to a behavior now known as aeroelastic divergence. As a critical airspeed was approached, the increase in aerodynamic forces produced a nose-up pitching moment on the wing, as illustrated in Figure 2. The consequence is excessively large pitch deformations and a further buildup of aerodynamic loads, making a catastrophic structural failure of the wing inevitable unless the airspeed is quickly reduced.

Aeroelastic effects on lifting surfaces can encompass, but are not limited to, phenomena such as structural divergence and flutter.

Flutter, another behavior that can lead to wing or tail surface failure, is a self-excited oscillation arising from the interplay between unsteady aerodynamic forces and the structure’s dynamic response. As also shown in Figure 2, flutter is an oscillatory response that can grow rapidly in amplitude as a critical airspeed is approached. At or near this critical airspeed, a minor disturbance, such as a gust or control input, can trigger the onset of flutter. The flutter can reach a limiting amplitude, but it can also become a divergent oscillatory response in which aerodynamic work feeds energy into the structural motion. In these conditions, structural failure is also likely.

These observations, along with a history of structural failures in early airplanes, revealed that structural elasticity and flutter avoidance could not be ignored during the design process. Understanding aeroelastic phenomena became even more critical with the development of higher-speed and supersonic aircraft, in which aerodynamic forces and structural stresses are significantly more pronounced. Today, all aircraft must be designed for flutter-free operation over their entire flight envelopes, and thorough aeroelastic analyses and flight testing are integral to their design and certification process. This video from Airbus shows how engineers and pilots explore the flutter envelope of a new airplane.

Learning Objectives

  • Understand the basic principles of aeroelasticity and why it is crucial to the design and analysis of flight vehicles.
  • Explore unsteady aerodynamics and how it differs from steady-state aerodynamics.
  • Be able to apply Theodorsen’s theory to calculate the circulatory component of unsteady lift and include the noncirculatory apparent-mass terms separately.
  • Learn about various aeroelastic phenomena, such as divergence, flutter, buffeting, and buzzing, and their relationships to steady and unsteady aerodynamic forces.
  • Appreciate how Computational Fluid Dynamics (CFD) and the Finite Element Method (FEM) can be more comprehensively used to model unsteady aerodynamics and flutter.

History

The origins of aeroelastic behavior can be traced back to the earliest aircraft; see the review paper “Historical Development of Airplane Flutter” by I. E. Garrick and Wilmer H. Reed III. The Wright brothers and other early aviation pioneers sometimes encountered wing oscillations and buzzing. They also observed buzzing at the tips of their propellers, which they addressed by using blades with wider chord lengths. They did not understand these effects at the time, but they were likely aeroelastic in origin, resulting from the interaction between aerodynamic forces and structural dynamics. In 1903, Samuel Langley attempted to fly an aircraft, but his monoplane’s wooden and fabric wings were structurally weak and failed during launch, causing the aircraft to crash into the Potomac River. The episode is often cited as an early warning that aerodynamic loading, structural stiffness, and flight-vehicle stability could not be treated separately. The Wright brothers experimented with various structures and developed a more rigid one in the form of a biplane, which did not suffer as readily from aeroelastic effects. The catastrophic failure of the horizontal tail on a Handley Page O/400 bomber in 1916, caused by an oscillatory aeroelastic phenomenon that would later become known as flutter, suggested that much was still to be learned about aircraft design.

Wing and control surface flutter became an increasingly critical concern as aircraft designs evolved, particularly with the transition to monoplanes. Monoplanes, with their single-wing configuration and lower structural stiffness,[2] highlighted the importance of understanding and mitigating flutter during the design of aircraft. “The Blue Max” is a 1966 film set in WWI that tells the story of a German fighter pilot, Bruno Stachel, who aims to earn the prestigious Pour le Mérite, also known as the “Blue Max,” for outstanding acts of bravery in aerial combat. While wing divergence and flutter are not central themes in the film, it depicts the heightened risks of structural failure that early pilots faced as they transitioned from slow biplanes to faster, more agile monoplanes.

The rapid advancement in aircraft design and increased flight speeds after this period led to more frequent and severe aeroelastic problems. Engineers then systematically studied these issues, developing aeroelastic theories to predict and prevent flutter, often necessitating more rigorous structural design. The work of Theodore Theodorsen, among others, laid the groundwork for modern aeroelastic analyses. The severity of flutter issues in the decade following WWII is underscored by a 1956 state-of-the-art survey conducted by the NACA Subcommittee on Vibration and Flutter, which documented 54 instances of flutter-related difficulties with U.S. military aircraft. The introduction of thin swept wings for supersonic flight in the 1950s increased the challenges of predicting aeroelastic effects at higher Mach numbers. This period saw significant advances in theoretical, wind-tunnel, and flight testing, including a deeper understanding of unsteady aerodynamic effects.

The Lockheed L-188 Electra, a four-engine turboprop airliner introduced in the late 1950s, was found to exhibit a more complex but catastrophic form of flutter known as whirl-mode flutter. Under certain conditions, propeller oscillations were transmitted to the engine mountings, which, in turn, coupled to the wings, creating hazardous vibrations. After two midair breakups in which the wings detached from the airframe, wind tunnel tests (Figure 3) led to design changes, including reinforced engine mounts and thicker wing skins, making the aircraft flutter-free. While these failures damaged the reputation of the airplane and its manufacturer, the modified Electra became a reliable aircraft; the P-3 Orion, in particular, was used extensively by the U.S. Navy until quite recently. While flutter prediction methods continued to advance, wind-tunnel testing of aeroelastic Froude-scaled models remained crucial for validating these methods. Steps were also taken to establish formal criteria for predicting and mitigating the onset of flutter before the aircraft’s first flight.

A 1/8th-scale powered model of the Electra was tested in a wind tunnel. It was determined that the crashes resulted from whirl flutter, which led to catastrophic wing failure.

The development of supersonic aircraft, including military (e.g., SR-71) and civil (e.g., Concorde), as well as hypersonic vehicles that experience thermal heating (e.g., the X-15), has further advanced aeroelastic research. Comprehensive computational methods emerged in the 1980s, enabling more confident predictions of aeroelastic effects and flutter. Today, computational tools such as Computational Fluid Dynamics (CFD) and the Finite Element Method (FEM), which can be coupled to include structural dynamics, are integral to most comprehensive aeroelastic analyses. These methods enable accurate simulations of aeroelastic interactions among airframe components, particularly for complex geometries and high-speed flight conditions. Unlike analytical solutions, which are more limited, CFD and FEM integration enables engineers to analyze the full spectrum of aeroelastic behavior for an entire flight vehicle, including wings, control surfaces, engines, undercarriage, and other components. Aeroelasticity is not solely a concern for airplanes; it also plays a crucial role in the design of helicopter rotors, wind turbines, and even bridges.

As flight speeds continue to increase and airplane construction evolves toward even lighter and more flexible aerostructures, understanding and controlling aeroelastic effects remain an ongoing engineering challenge. Using active control, either structural or aerodynamic, or both, can help mitigate undesirable aeroelastic effects with lightweight structures. For example, the Boeing 787 has a Flaps-Up Vertical Modal Suppression (F0VMS) system[3] to enhance the damping of a stable but lightly damped low-frequency aeroelastic mode between the engines, wings, and fuselage. This system, which uses differential elevator inputs and flaperons, is designed to provide damping augmentation, rather than suppress a flutter mode. In the FAA special conditions for the 787-10, the agency stated that it was not prepared to accept an active flutter-suppression system that suppresses flutter within the airplane’s operational or design envelope.

Unsteady Airfoil Behavior

Fundamental to predicting flutter is the modeling of unsteady aerodynamics. Unsteady airfoil theory addresses the aerodynamic behavior of airfoils and wings under time-varying boundary conditions, such as oscillations in angle of attack, vertical and horizontal motions, or other situations in which the angle of attack varies with time.

In an unsteady flow, the wake behind an airfoil is time-varying in structure from the shedding of vorticity and circulation, as illustrated in Figure 4, thereby influencing the aerodynamic forces experienced by the airfoil. These wake effects alter the magnitude and phase of the lift response relative to the time-varying boundary conditions. Furthermore, at high angles of attack, the flow may separate from the airfoil surface, causing the leading-edge vortex to shed and resulting in aerodynamic hysteresis, commonly known as dynamic stall. Under these conditions, reduced aerodynamic damping can lead to another form of flutter, known as stall flutter.

 

When the angle of attack changes, the immediate downstream shed wake affects the aerodynamics of the airfoil section.

Several methods exist for quantitatively calculating these unsteady effects. One instructive approach for those first learning about unsteady airfoil behavior is the classic linearized unsteady aerodynamics theories, including Theodorsen’s theory and the indicial response method. Unsteady panel methods discretize the airfoil surface into panels that extend into the wake, thereby capturing the same physical phenomena. The most computationally intensive CFD methods solve the Navier-Stokes equations for unsteady flow, capturing detailed phenomena such as wakes, vortex shedding, and dynamic stall, but at a high computational cost and time.

Reduced Frequency

A nondimensional parameter used to categorize whether a flow is steady or unsteady is the reduced frequency, denoted by the symbol k. The reduced frequency is defined, in general, as

(1)   \begin{equation*} { k = \frac{\omega \, L}{V} } \end{equation*}

where \omega is a characteristic physical frequency of the unsteady flow (in units of radians per second), L is a characteristic length scale, and V is a reference flow velocity. Base units should always be used to obtain the correct numerical value for the reduced frequency.

For a wing or airfoil, such as one oscillating in angle of attack or an oscillatory vertical (heaving) motion as shown in Figure 5, the reduced frequency is often defined in terms of its semi-chord, i.e., L = c/2 = b, and the freestream velocity, {V_{\infty}}, i.e., in this case, it is defined as

(2)   \begin{equation*} k = \frac{\omega \, c}{2 \, V_{\infty}} = \frac{\omega \, b}{V_{\infty}} \end{equation*}

 

Unsteady airfoil motion produces aerodynamic characteristics different from those of steady flow; these effects are encountered in aeroelasticity.

The aerodynamics of non-steady and oscillating airfoil sections and wings must be addressed in the field of aeroelasticity and flutter. If not, flutter predictions will be inadequate. For example, a torsional wing motion introduces a pitching behavior at any wing section. Likewise, a bending motion of the wing introduces a plunging or heaving behavior at the wing section. Both types of motion will alter the effective angle of attack and contribute to the aerodynamic loads, with higher reduced frequencies resulting in greater aerodynamic effects.

For k = 0, the flow is steady, and all the usual steady results will apply regarding the relationships between the aerodynamic quantities and the angle of attack. For 0 \le k \le 0.05, the flow can be considered quasi-steady; that is, unsteady effects are generally minor, and for some problems, they may be neglected completely. Under these conditions, the aerodynamic response is directly related to the instantaneous forcing; therefore, no significant time-history effect is observed. Nevertheless, as will be explained, additional quasi-steady “apparent mass” aerodynamic terms associated with the airfoil section’s velocities and accelerations must be included, potentially affecting both the amplitude and phase of the aerodynamic response.

Flows with characteristic reduced frequencies of 0.05 and above are typically considered as unsteady, so all unsteady terms must be retained in the governing flow equations, including the effects of the shed wake. The manifestation of this is more significant changes in the frequency-dependent amplitude and phase responses of the aerodynamic loads with respect to motion. Such aerodynamic and aeroelastic problems are more challenging to model for two reasons. First, the local flow properties also depend on the previous time, i.e., on the history of the lift and other aerodynamic forces. Second, the effects of compressibility may need to be accounted for even when the freestream flow velocity is low, which introduces additional challenges for modeling the unsteady aerodynamic response.

Quasi-Steady Aerodynamics

In quasi-steady aerodynamics, the behavior can be evaluated by applying the principles of steady flow under the instantaneous boundary conditions of flow tangency to the airfoil surface. Different forcing conditions, such as pure plunge or pitch, pitching, and a combination of pitching and plunging, may be considered, as shown in Figure 6.

At the wing sectional level, unsteady motion displacements can comprise pure plunge, pure pitch, or a combination of pitching and plunging.

For example, for a thin airfoil,[4]the changes in the angle of attack of a harmonically oscillating airfoil can be expressed as

(3)   \begin{equation*} { \alpha (t) = \alpha_0 + \bar{\alpha} \sin \omega \, t } \end{equation*}

where \alpha_0 is the mean angle of attack and \bar{\alpha} is the angle of attack amplitude of the oscillation. If the flow were quasi-steady, in the sense that flow adjustments were to take place instantaneously, the circulatory part of the lift coefficient would be given by

(4)   \begin{equation*} C_l (t) = C_{l_{\alpha}} \left( \alpha + \frac{\overbigdot{\alpha} \, c}{2 \, V_{\infty}} \right) \end{equation*}

recognizing that the pitch rate, i.e., \overbigdot{\alpha}, must affect the lift coefficient because it changes the angle of attack, i.e., to satisfy flow tangency at the rear-neutral point (3/4-chord). This equation then leads to

(5)   \begin{equation*} C_l (t) = C_{l_{\alpha}} \bigg( \alpha_0 + \bar{\alpha} \sin \omega \, t + k \, \bar{\alpha} \cos \omega \, t \bigg) = C_{l_{\alpha}} \alpha_0 + C_{l_{\alpha}} \bar{\alpha} \sqrt{1+k^2} \sin(\omega \, t + \phi) \end{equation*}

where \phi is a frequency-dependent phase angle given by

(6)   \begin{equation*} \phi = \tan^{-1} \big( k \big) \end{equation*}

Therefore, even based on quasi-steady arguments, the harmonic part of the circulatory lift response will no longer be in phase with the angle of attack; it leads by the angle \phi in this case, and its amplitude is larger than the quasi-steady harmonic value by the factor \sqrt{1+k^2}. Notice that because the aerodynamic center is at the 1/4 chord for a thin airfoil, then C_{m_{1/4}} = 0 for the circulatory parts of the quasi-steady aerodynamic response.

Apparent Mass Terms

The apparent mass or “noncirculatory” terms[5] account for the pressure forces required to accelerate the fluid near the airfoil. For example, consider a thin airfoil of chord {c} moving normal to its surface at velocity w(t); the noncirculatory fluid force, F_{\rm nc}, acting on the surface is

(7)   \begin{equation*} F_{\rm nc} = -{\cal{M}}_a \, \frac{dw}{dt} \end{equation*}

The term {{\cal{M}}_a} is often known as the apparent mass or added mass, and in this case is given by

(8)   \begin{equation*} {\cal{M}}_a = \pi \, \varrho \, \frac{c^2}{4} \end{equation*}

Therefore, with the sign convention used here, the noncirculatory lift per unit span for a motion where the airfoil moves normal to its surface with velocity w = \overbigdot{h}, as shown in Figure 7, is written as

(9)   \begin{equation*} L'_{\rm nc} = \pi \, \varrho \, \dfrac{c^2}{4} \overbigddot{h} \end{equation*}

 

Noncirculatory or “apparent mass” terms are related to the airfoil section’s instantaneous translational and angular accelerations.

In terms of lift coefficient, then

(10)   \begin{equation*} C_{l_{\rm nc}} = \left( \dfrac{\pi \, \varrho \, \dfrac{c^2}{4}}{\dfrac{1}{2} \varrho \, V_{\infty}^2 \, c} \right) \overbigddot{h} = \left( \frac{\pi \, c}{2 V_{\infty}^2} \right) \overbigddot{h} \end{equation*}

As also shown in Figure 7, an additional contribution arises from rotational acceleration when the airfoil undergoes pitching motion. For the sign convention used here, consider pitching with angular acceleration {\overbigddot{\theta}}; then the noncirculatory lift coefficient contribution may be written as

(11)   \begin{equation*} C_{l_{\rm nc, \, \theta}} = \left( \frac{\pi \, c^2}{4 \, V_{\infty}^2} \right) \overbigddot{\theta} \end{equation*}

where \theta is defined as positive in the same sense as the pitching motion used in the later worked examples. Therefore, the total noncirculatory lift contribution from a combination of pitch and plunge generally contains terms proportional to plunge acceleration, pitch rate, and pitch acceleration. For a two-dimensional airfoil section, this may be written in the form

(12)   \begin{equation*} L'_{\rm nc} = \pi \, \varrho \, b^2 \left( \overbigddot{h} + V_{\infty}\overbigdot{\theta} - a b \, \overbigddot{\theta} \right) \end{equation*}

where b=c/2, and a locates the pitch axis relative to the mid-chord in semi-chord units. The precise signs depend on the adopted sign convention for positive plunge, positive pitch, positive lift, and the definition of a. In coefficient form, this gives

(13)   \begin{equation*} C_{l_{\rm nc}} = \left( \frac{\pi \, c}{2 V_{\infty}^2} \right)\overbigddot{h} + \left( \frac{\pi \, c}{2 V_{\infty}} \right)\overbigdot{\theta} - \left( \frac{\pi \, a c^2}{4 V_{\infty}^2} \right)\overbigddot{\theta} \end{equation*}

with the same sign-convention qualifications.

The corresponding moment about the leading edge from the pitching motion is

(14)   \begin{equation*} M'_{\rm nc, \, LE} = -\dfrac{\pi}{8} \varrho \, c^4 \, \overbigddot{\theta} \end{equation*}

In terms of the moment coefficient, then

(15)   \begin{equation*} C_{m_{\rm nc, \, LE}} = \frac{M'_{\rm nc, \, LE}}{\tfrac{1}{2} \varrho \, V_{\infty}^2 \, c^2} = -\left( \frac{\pi \, c^2}{4 \, V_{\infty}^2} \right) \overbigddot{\theta} \end{equation*}

The moment about the 1/4-chord is related to the leading-edge moment by the application of statics using

(16)   \begin{equation*} C_{m_{\rm nc, \, 1/4}} = C_{m_{\rm nc, \, LE}} + \left( \frac{1}{4} \right) C_{l_{\rm nc}} \end{equation*}

Therefore, it is apparent that incorporating the apparent mass or noncirculatory effects introduces additional terms that are proportional to the airfoil’s acceleration, including translation (plunge), i.e., \overbigddot{h}, and rotation (pitch), i.e., \overbigddot{\theta}. Unlike the circulatory air loads, which depend on the instantaneous angle of attack and its rate of change, the noncirculatory forces depend directly on acceleration. These effects are most pronounced in high-frequency oscillations where \overbigddot{h} and \overbigddot{\theta} are large. They are also essential for predicting unsteady airloads in transient motions, such as airplanes undergoing rapid pitch maneuvers.

Quasi-Steady Aerodynamics, Including Apparent Mass

Using the previous oscillatory pitching example and identifying the angle-of-attack variation with a small pitching motion, the noncirculatory contribution to the lift is associated with angular acceleration. Therefore, it is proportional to the harmonic part of the motion, not to the mean angle of attack. For

(17)   \begin{equation*} \alpha(t)=\alpha_0+\bar{\alpha}\sin\omega t \end{equation*}

then

(18)   \begin{equation*} \overbigddot{\alpha}(t) = -\omega^2\bar{\alpha}\sin\omega t \end{equation*}

so the noncirculatory contribution may be written as

(19)   \begin{equation*} C_{l_{\text{nc}}}(t) = -\pi \left( \frac{\omega c}{2V_{\infty}} \right)^2 \bar{\alpha}\sin\omega t \end{equation*}

Adding this term to the previous quasi-steady circulatory lift expression gives

(20)   \begin{equation*} C_l(t) = C_{l_{\alpha}} \left( \alpha + \frac{\overbigdot{\alpha} \, c}{2 \, V_{\infty}} \right) - \pi \left( \frac{\omega c}{2V_{\infty}} \right)^2 \bar{\alpha}\sin\omega t \end{equation*}

Substituting {\alpha (t) = \alpha_0 + \bar{\alpha} \sin \omega \, t } leads to {\overbigdot{\alpha} = \omega \bar{\alpha} \cos \omega \, t} and {\overbigddot{\alpha} = -\omega^2 \bar{\alpha} \sin \omega \, t}. Therefore, using k=\omega c/(2V_{\infty}), the total lift coefficient is

(21)   \begin{equation*} C_l(t) = C_{l_{\alpha}} \alpha_0 + \left(C_{l_{\alpha}} - \pi \, k^2\right)\bar{\alpha} \sin \omega \, t + C_{l_{\alpha}} k \bar{\alpha} \cos \omega \, t \end{equation*}

which, after some rearrangement, becomes

(22)   \begin{equation*} C_l(t) = C_{l_{\alpha}} \alpha_0 + C_{l_{\alpha}} \bar{\alpha} \sqrt{ k^2 + \left(1 - \frac{\pi \, k^2}{C_{l_{\alpha}}}\right)^2 } \sin(\omega t + \phi') \end{equation*}

where

(23)   \begin{equation*} \phi' = \tan^{-1} \left( \frac{k}{1 - \dfrac{\pi \, k^2}{C_{l_{\alpha}}}} \right) \end{equation*}

These results show that the apparent mass effect modifies the amplitude and induces a phase shift in the lift response, depending on the reduced frequency. The upshot is that the aerodynamic forces will differ depending on whether the angle of attack increases or decreases over time. Indeed, measurements suggest that the unsteady lift on an airfoil or wing is often attenuated (diminished) by unsteady effects and not amplified as the quasi-steady theory would suggest. Still, there can be a lag or a lead in the aerodynamic response with respect to the angle of attack.

Frequency Domain Theories

Although an extensive literature exists on unsteady airfoil aerodynamics, a physically correct theory must account for the vorticity shed from the trailing edge and convected downstream, which feeds back into the airfoil loads and introduces a history-dependent response. When the motion or excitation is harmonic in time, all unsteady quantities vary as e^{i\omega t}, and the governing equations reduce to algebraic relations in the frequency domain. The effects of the shed wake then appear through the use of complex functions with frequency-dependent transfer functions. Within thin-airfoil theory, this framework leads to two classical results: Theodorsen’s function for harmonic airfoil motion and Sears’s function for a convected sinusoidal gust.

Theodorsen’s Theory

One of these frequency-domain unsteady theories is called Theodorsen’s theory. Theodorsen’s theory[6] provides a linearized, small-disturbance solution for oscillating airfoils in an incompressible flow. Therefore, it should be regarded as a low-Mach-number baseline theory; at appreciable Mach numbers, compressibility modifies both the circulatory wake response and the noncirculatory apparent-mass response. The theory is based on the assumption of small oscillation amplitudes. It provides an exact analytical theory (within the stated assumptions and limitations of thin-airfoil theory) for describing the unsteady airloads on a thin airfoil. Theodorsen’s problem was to determine the bound-vorticity distribution, {\gamma_b}, on the airfoil surface under harmonic forcing, as shown in the flow model in Figure 8.

The flow model used for Theodorsen’s theory is used to find the unsteady loading on a thin airfoil, accounting for the effects of circulation shed into the downstream wake.

Governing Equation

The governing integral equation is

(24)   \begin{equation*} w(x_0,t) = \frac{1}{2\pi} \int_0^c \frac{\gamma_b(x,t)}{x_0-x} \, dx + \frac{1}{2\pi}\int_c^{\infty} \frac{\gamma_w(x,t)}{x_0-x} \, dx \end{equation*}

where w is the downwash on the airfoil surface. This equation must be solved subject to flow tangency on the airfoil chord and by invoking the Kutta condition at the trailing edge, i.e., \gamma_b (c,t) = 0. There is also a connection between the change in circulation about the airfoil and the circulation shed into the wake. Conservation of circulation (Kelvin’s theorem) requires that

(25)   \begin{equation*} \gamma_w(c,t) \, dx = -\frac{d\Gamma(t)}{dt} \, dt \end{equation*}

Assuming that the vorticity in the shed wake is convected at the freestream velocity, {V_{\infty}}, this gives {dx = V_{\infty} \, dt}, and so

(26)   \begin{equation*} V_{\infty} \, \gamma_w(c,t) = -\frac{d\Gamma(t)}{dt} \end{equation*}

where the total circulation about the airfoil, \Gamma(t) is given by

(27)   \begin{equation*} \Gamma(t) = \int_0^c \gamma_b(x,t) \, dx \end{equation*}

Because this wake vorticity is near the airfoil, it alters the downwash velocity, thereby affecting the airfoil loads. Suppose the net circulation about the airfoil is changing harmonically with respect to time, as in Theodorsen’s problem. In that case, circulation will be shed harmonically into the wake and will continuously affect the airfoil’s aerodynamic loads. In the limit, as the changing boundary conditions end, the shed wake vorticity cast off the trailing edge of the airfoil becomes zero, and the remaining circulation in the wake convects downstream to infinity, thereby recovering the classic thin airfoil theory.

Theodorsen Function

The unsteady problem posed above is certainly not trivial to solve. Still, for a simple harmonic motion, the solution is given by Theodorsen in a form that represents a transfer function between the forcing (angle of attack) and the aerodynamic response (i.e., the chordwise loading distribution, lift, and pitching moment). The solution, which is given in terms of the Theodorsen function, denoted by C(k), is a complex-valued function that captures the instantaneous effect of the circulation shed into the wake on the unsteady aerodynamic response and is given by

(28)   \begin{equation*} C(k) = F(k) + i G(k) = \frac{H_1^{(2)}(k)}{H_1^{(2)}(k) + i H_0^{(2)}(k)} \end{equation*}

where H_0^{(2)} and H_1^{(2)} are Hankel functions of the second kind, and k is the reduced frequency. The Hankel function is defined as H_{\rm v}^{(2)} = J_{\rm v} - i Y_{\rm v}, with {J_{\rm v}} and {Y_{\rm v}} being Bessel functions of the first and second kind, respectively. Therefore, the C(k) function can be viewed as an aerodynamic transfer function that relates the input (forcing) to the response.

Recognizing that each Bessel function has an argument k, then the real or in-phase (\Re) part and imaginary or out-of-phase part (\Im) of the Theodorsen function can be written as

(29)   \begin{equation*} \Re C(k) = F = \frac{J_1 ( J_1 + Y_0 ) + Y_1 (Y_1 - J_0)}{(J_1 + Y_0)^2 + (J_0 - Y_1)^2} \end{equation*}

and

(30)   \begin{equation*} \Im C(k) = G = -\frac{Y_1 \, Y_0 + J_1 \, J_0}{(J_1 + Y_0)^2 + (J_0 - Y_1)^2} \end{equation*}

Despite its apparent mathematical complexity, the Theodorsen function can be readily computed numerically in MATLAB and is plotted in Figure 9.

Theodorsen’s function plotted in terms of its real and imaginary parts.

Another way of interpreting the Theodorsen function, which is perhaps more tangible in the first instance, is in terms of the amplitude, | C(k) |, and phase angle, \phi, of the response, which are given by

(31)   \begin{equation*} | C(k)| = \sqrt{ F^2 + G^2} \quad \mbox{and} \quad \phi = \tan^{-1} \left( \frac{G}{F} \right) \end{equation*}

MATLAB code to calculate the Theodorsen function

Show the code/hide the code.

function theodorsen_function_plot_and_save
% Calculate, plot, and save Theodorsen’s function C(k).

% Define the range of reduced frequencies.
k = linspace(0.01, 10, 500);

% Preallocate arrays for real and imaginary parts.
Ck_real = zeros(size(k));
Ck_imag = zeros(size(k));

% Calculate Theodorsen’s function for each value of k.
for i = 1:length(k)
[Ck_real(i), Ck_imag(i)] = theodorsen_function(k(i));
end

% Plot the real part.
figure;
subplot(2, 1, 1);
plot(k, Ck_real, ‘b-‘, ‘LineWidth’, 1.5);
xlabel(‘Reduced Frequency, k’);
ylabel(‘Real Part of C(k)’);
title(‘Real Part of Theodorsen Function’);
grid on;

% Plot the imaginary part.
subplot(2, 1, 2);
plot(k, Ck_imag, ‘r-‘, ‘LineWidth’, 1.5);
xlabel(‘Reduced Frequency, k’);
ylabel(‘Imaginary Part of C(k)’);
title(‘Imaginary Part of Theodorsen Function’);
grid on;

% Save the data to a file.
data = [k.’, Ck_real.’, Ck_imag.’];
save(‘theodorsen_function_data.txt’, ‘data’, ‘-ASCII’, ‘-double’);

end

function [Ck_real, Ck_imag] = theodorsen_function(k)
% Calculate Theodorsen’s function C(k) and return its real and
% imaginary parts. The reduced frequency is k.

% Bessel functions of the first kind.
J0 = besselj(0, k);
J1 = besselj(1, k);

% Bessel functions of the second kind.
Y0 = bessely(0, k);
Y1 = bessely(1, k);

% Hankel functions of the second kind.
H0 = J0 – 1i * Y0;
H1 = J1 – 1i * Y1;

% Theodorsen’s function.
Ck = H1 ./ (H1 + 1i * H0);

% Separate into real and imaginary parts.
Ck_real = real(Ck);
Ck_imag = imag(Ck);

end

It will be apparent that Theodorsen’s theory is a frequency domain theory; even though the results for the aerodynamic response may be expressed as a function of time, the unsteady forcing must be oscillatory, which is expressed in terms of the reduced frequency. Recall that the reduced frequency is a dimensionless parameter representing the unsteadiness of the flow, defined by

(32)   \begin{equation*} k = \frac{\omega c}{2\, V_\infty} \end{equation*}

Physically, the reduced frequency can be interpreted as the ratio of the oscillation frequency to the convective time of the flow. Airfoils respond differently to different values of k. Low k values imply a quasi-steady behavior, while high k values indicate highly unsteady conditions. Quasi-steady means that the flow responds almost immediately to changes in the angle of attack; therefore, the aerodynamic response is in phase with the motion of the airfoil.

Unsteady Aerodynamic Response

The effect of the Theodorsen function, which emulates a physical wake lag response, can be appreciated if a pure oscillatory variation in the angle of attack is considered, as before, i.e., \alpha (t) = \alpha_0 + \bar{\alpha} \sin \omega \, t,[7] where \alpha_0 is the mean angle of attack and \bar{\alpha} is the angle of attack amplitude of the oscillation. If the flow were quasi-steady, in the sense that flow adjustments were to take place instantaneously, the lift coefficient would be given by

(33)   \begin{equation*} C_l (t) = C_{l_{\alpha}} \alpha = C_{l_{\alpha}} \left( \alpha_0 + \bar{\alpha} \, \sin \omega \, t \right) \end{equation*}

where C_{l_{\alpha}}  = 2 \pi for a thin-airfoil in incompressible flow. In the unsteady case, this circulatory part of the airfoil lift coefficient becomes

(34)   \begin{equation*} C_l(t) = C_{l_{\alpha}}\alpha_0 + C_{l_{\alpha}} |C(k)| \, \bar{\alpha} \sin ( \omega \, t + \phi ) \end{equation*}

or in terms of the real and imaginary parts, then

(35)   \begin{equation*} C_l(t) = C_{l_{\alpha}}\alpha_0 + C_{l_{\alpha}}\bar{\alpha} \,\Im\!\left\{ C(k) \, e^{i\omega t} \right\} \end{equation*}

or equivalently

(36)   \begin{equation*} C_l(t) = C_{l_{\alpha}}\alpha_0 + C_{l_{\alpha}}\bar{\alpha} \left[ F(k)\sin\omega t + G(k)\cos\omega t \right] \end{equation*}

The amplitude ratio and phase angle of the harmonic circulatory lift response are then obtained from the Theodorsen function, i.e.,

(37)   \begin{equation*} |C(k)| = \sqrt{F^2+G^2} \quad \mbox{and} \quad \phi = \tan^{-1}\left(\frac{G}{F}\right) \end{equation*}

so that the harmonic lift amplitude is reduced from its quasi-steady value by the factor |C(k)|.

Representative results from the Theodorsen theory are shown in Figure 10 in terms of lift coefficient C_l versus angle of attack, {\alpha}. Notice that the Theodorsen function introduces an amplitude reduction and phase lag effect on the circulatory part of the lift response compared to the result obtained under quasi-steady conditions.

Representative unsteady lift coefficient versus angle of attack on an airfoil when oscillating at different reduced frequencies.

For k = 0, the steady-state lift behavior is obtained, i.e., C_l is linearly proportional to {\alpha}. However, as k is increased, the lift plots develop into hysteresis loops, and these loops rotate such that the amplitude of the lift response (slope of the lift curve) decreases with increasing values of reduced frequency. Notice also that these loops are circumvented in a counterclockwise direction such that the lift is lower than the steady value when {\alpha} is increasing with time and higher than the steady value when {\alpha} is decreasing with time, i.e., there is a phase lag accounted for by \phi. Notice also that for infinite reduced frequency, the circulatory part of the lift amplitude is half that at k=0, and there is no phase lag angle.

These concepts can be readily extended to more complex boundary conditions, including the effects of pitch rate and combinations of frequencies. Because the method is fundamentally a potential-flow solution, linear superposition can be used to obtain results for more general forcing functions, such as a Fourier series.

It should also be appreciated that Theodorsen’s theory applies only to the “circulatory” component of the lift, i.e., the aerodynamic response associated with the creation and shedding of circulation. Additional non-circulatory forces (and moments) are produced by inertial effects or “apparent mass” in an unsteady flow. These effects must be included to round out the unsteady aerodynamic theory if it is to be used in any predictive sense.

Circulatory & Noncirculatory Contributions

Theodorsen’s function applies only to the circulatory part of the unsteady airloads, i.e., the part associated with bound circulation on the airfoil and vorticity shed into the wake. The shed wake introduces the amplitude attenuation and phase lag represented by the complex function C(k). However, this circulatory contribution is not the entire unsteady aerodynamic response.

There is also a noncirculatory contribution, often called the apparent-mass or added-mass contribution. This part of the airload is associated with the pressure field required to accelerate the fluid near the airfoil. It is instantaneous in the sense that it is tied directly to the velocity and acceleration of the airfoil motion, rather than to the history of vorticity shed into the wake. Therefore, these terms are not multiplied by Theodorsen’s function.

For a thin airfoil undergoing small-amplitude plunge h(t) and pitch \theta(t), the unsteady lift coefficient may be written as the sum of circulatory and noncirculatory parts, i.e.,

(38)   \begin{equation*} C_l = C_{l_c}+C_{l_{\rm nc}} \end{equation*}

Theodorsen’s function modifies the circulatory part. In a simplified form, the effective angle of attack contains contributions from pitch, plunge velocity, and pitch rate, so that

(39)   \begin{equation*} C_{l_c} = 2\pi \, C(k) \left[ \theta + \frac{\overbigdot{h}}{V_{\infty}} + \frac{\overbigdot{\theta}c}{2V_{\infty}} \right] \end{equation*}

where C(k) accounts for the wake-induced amplitude attenuation and phase shift.

The noncirculatory or apparent-mass contribution is added separately. With the sign convention used in the following pitching example, the pitch contribution is written as

(40)   \begin{equation*} C_{l_{\rm nc,\theta}} = \left( \frac{\pi c^2}{4V_{\infty}^2} \right)\overbigddot{\theta} \end{equation*}

so that for \theta(t)=\theta_0 \, e^{i\omega t}, then

(41)   \begin{equation*} C_{l_{\rm nc,\theta}} = -\pi \, k^2\theta_0 \, e^{i\omega t} \end{equation*}

where k=\omega c/(2V_{\infty}). A plunge contribution may be included in the same way, with its sign depending on the convention used for positive h and positive lift. These noncirculatory terms depend directly on the accelerations of the airfoil section and are not multiplied by C(k) because they do not arise from circulation shed into the wake.

For harmonic motion, differentiation converts the time dependence into algebraic factors. If

(42)   \begin{equation*} h(t)=h_0 \, e^{i\omega t} \quad \mbox{and} \quad \theta(t)=\theta_0 \, e^{i\omega t} \end{equation*}

then

(43)   \begin{equation*} \overbigdot{h}=i\omega h_0 \, e^{i\omega t}, \quad \overbigddot{h}=-\omega^2h_0 \, e^{i\omega t} \qquad \text{and} \qquad \overbigdot{\theta}=i\omega \theta_0 \, e^{i\omega t}, \quad \overbigddot{\theta}=-\omega^2\theta_0 \, e^{i\omega t} \end{equation*}

Therefore, in the frequency domain, the circulatory velocity terms introduce factors proportional to i\, \omega, while the apparent-mass acceleration terms introduce factors proportional to -\omega^2. Using k = \omega \, c/(2 \, V_{\infty}), the pitching apparent-mass term becomes

(44)   \begin{equation*} \left( \frac{\pi \, c^2}{4 \, V_{\infty}^2} \right)\overbigddot{\theta} = -\pi \, k^2 \theta_0\, e^{i\omega t} \end{equation*}

for harmonic pitching motion. This result shows explicitly how the apparent-mass contribution enters the same frequency-domain framework as the Theodorsen circulatory term, but as an additive acceleration-dependent contribution rather than as a term multiplied by C(k).

Check Your Understanding #1 – Theodorsen’s theory

An airfoil is undergoing harmonic pitching motion about its quarter-chord in a freestream with velocity V_{\infty} = 50 m/s. The pitching motion is described as \theta(t) = \theta_0 \, e^{i\omega \, t} where the amplitude of motion is \theta_0 = 5^\circ, and the oscillation frequency is \omega = 10 rad/s. The airfoil has a chord length of {c} = 1 m. Using Theodorsen’s theory, compute the unsteady lift coefficient, including its magnitude and phase angle.

Show solution/hide solution.

The reduced frequency is given by

    \[ k = \frac{\omega c}{2V_{\infty}} = \frac{10 \times 1}{2 \times 50} = 0.1 \]

From Theodorsen’s function for k = 0.1, then

    \[ C(0.1) \approx 0.832 - 0.172i \]

The effective angle of attack is

    \[ \alpha(t) = \theta(t) + \frac{\overbigdot{\theta}(t) c}{2 V_{\infty}} \]

Using Theodorsen’s equation for the unsteady lift coefficient:

    \[ C_l = 2\pi \, C(k) \alpha(t) = 2\pi \, C(k) \left( \theta(t) + \frac{\overbigdot{\theta}(t)c}{2V_{\infty}} \right) \]

Substituting \theta_0 = 5^\circ = 0.0873 rad, \theta(t) = \theta_0 \, e^{i\omega \, t}, and \overbigdot{\theta}(t) = i\, \omega \theta_0 \, e^{i\omega \, t}, then

    \[ C_l = 2\pi (0.832 - 0.172i)(1 + 0.1i)(0.0873) \, e^{i\omega \, t} \]

or

    \[ C_l = 2\pi(0.0873)(0.849 - 0.089i) \, e^{i\omega t} = (0.466 - 0.049i) \, e^{i\omega t} \]

Therefore,

    \[ C_l = 0.468\,e^{i(\omega t - 5.99^\circ)} \]

This represents an attenuation of the lift amplitude compared to the quasi-steady result, with a phase lag of about 6.0^\circ for the convention used here.

The preceding example computed only the circulatory part of the unsteady lift response, i.e., the part modified by Theodorsen’s function. The next example adds the noncirculatory apparent-mass contribution to obtain the total unsteady lift coefficient.

Check Your Understanding #2 – Theodorsen’s theory plus apparent mass terms

Using conditions in the previous Check Your Understanding #1, determine the total unsteady lift coefficient, including Theodorsen’s circulatory and non-circulatory (added mass) lift components.

Show solution/hide solution.

The non-circulatory (apparent mass) lift coefficient for this motion is

    \[ C_{l_{\rm nc}} = \left( \frac{\pi \, c^2}{4V_{\infty}^2} \right) \overbigddot{\theta}(t) \]

Because \overbigddot{\theta}(t) = -\omega^2 \theta_0 \, e^{i\omega \, t}, then

    \[ C_{l_{\rm nc}} = -\left( \frac{\pi \, c^2 \omega^2}{4V_{\infty}^2} \right) \theta_0 \, e^{i\omega \, t} \]

Using k = \omega c/(2V_{\infty}), this becomes

    \[ C_{l_{\rm nc}} = -\pi \, k^2 \theta_0 \, e^{i\omega \, t} \]

For k = 0.1 and \theta_0 = 5^\circ = 0.0873 rad, then

    \[ C_{l_{\rm nc}} = -\pi (0.1)^2(0.0873) \, e^{i\omega \, t} = -0.00274 \, e^{i\omega \, t} \]

which is 180^\circ out of phase with the prescribed pitching displacement. From Check Your Understanding #1, the circulatory contribution is

    \[ C_{l_c} = (0.466 - 0.049i) \, e^{i\omega t} \]

Summing the circulatory and non-circulatory contributions gives

    \[ C_l = C_{l_c} + C_{l_{\rm nc}} = \left[(0.466 - 0.049i) - 0.00274 \right] \, e^{i\omega t} \]

or

    \[ C_l = (0.463 - 0.049i) \, e^{i\omega t} \]

Therefore,

    \[ C_l = 0.465\,e^{i(\omega t - 6.03^\circ)} \]

Sinusoidal Gust: Sears’s Problem

Von Kármán & Sears[8] analyzed the unsteady lift of a thin airfoil encountering a sinusoidal vertical gust convected by the free stream, as shown in Figure 11. The gust is represented as a prescribed upwash velocity field of the form

(45)   \begin{equation*} w_g(x,t)=w_0 \,\sin\!\left(\omega_g t-\frac{\omega_g x}{V}\right) \end{equation*}

where w_0 is the gust amplitude, \omega_g is the gust (temporal) frequency, and V is the free-stream speed. The corresponding gust wavelength is

(46)   \begin{equation*} \lambda_g=\frac{2\pi \, V}{\omega_g} \end{equation*}

The flow model used for a thin airfoil encountering a sinusoidal vertical gust (Sears’s problem) to find the unsteady aerodynamic loading.

Using the identity \sin(A-B)=\sin A \cos B-\cos A \sin B, then Eq. 45 may be written as

(47)   \begin{equation*} \frac{w_g(x,t)}{w_0} = \sin(\omega_g t)\cos\!\left(\frac{\omega_g x}{V}\right) -\cos(\omega_g t)\sin\!\left(\frac{\omega_g x}{V}\right) \end{equation*}

Two reference conventions are common. If the gust is referenced to the leading edge, then x=0 and Eq. 45 reduces to w_g(t)=w_0\sin(\omega_g t). If the gust is referenced to the mid-chord, then x = b = c/2 and the forcing becomes w_g(t)=w_0\sin(\omega_g t-k_g), i.e., a frequency-dependent phase shift, where the (dimensionless) gust reduced frequency is

(48)   \begin{equation*} k_g \equiv \frac{\omega_g b}{V} = \frac{\omega_g c}{2V} = \frac{\pi \, c}{\lambda_g} \end{equation*}

The mid-chord convention was used in the original work of von Kármán & Sears, and their use of the mid-chord reference point has caused much confusion in the literature. For a thin airfoil, the harmonic lift response to the convected gust may be written in transfer-function form as

(49)   \begin{equation*} C_l(t)=2\pi\left(\frac{w_0}{V}\right)\,\Im\!\left\{ S(k_g)\,e^{i\omega_g t}\right\} \end{equation*}

where S(k_g) is called Sears’s function. An exact representation is

(50)   \begin{equation*} S(k_g)=\big(J_0(k_g)-iJ_1(k_g)\big)\,C(k_g)+iJ_1(k_g) \end{equation*}

where J_0 and J_1 are Bessel functions of the first kind and C(k) is Theodorsen’s function. Writing S=\Re S+i\,\Im S, and C=F+i\,G, Eq. 50 gives

(51)   \begin{eqnarray*} \Re S(k_g) &=& F(k_g)\,J_0(k_g)+G(k_g)\,J_1(k_g)\\[6pt] \Im S(k_g) &=& G(k_g)\,J_0(k_g)-F(k_g)\,J_1(k_g)+J_1(k_g) \end{eqnarray*}

as plotted in Figure 12. The results can be calculated numerically, as in the case of the Theodorsen function. Sears’s function describes the circulatory lift response of a fixed airfoil to a convected gust. Unlike the pitching or plunging airfoil problem, the standard Sears problem does not introduce separate apparent-mass terms because the airfoil itself is not undergoing prescribed acceleration; the unsteadiness is imposed by the flow field rather than by the motion of the airfoil.

Real and imaginary parts of Sears’s function, referenced to the mid-chord and to the leading edge.

If the gust is instead referenced to the leading edge, which is much more intuitive, then the transfer function differs by a pure convective phase shift over the distance b=c/2, i.e.,

(52)   \begin{equation*} S_{\mathrm{LE}}(k_g)=S_{\mathrm{MC}}(k_g)\,e^{i k_g} \end{equation*}

Equivalently, if S_{\mathrm{MC}}=\Re S+i\,\Im S and S_{\mathrm{LE}}=\Re S'+i\,\Im S', then

(53)   \begin{eqnarray*} \Re S'(k_g) &=& \Re S \cos k_g - \Im S \sin k_g \\[6pt] \Im S'(k_g) &=& \Re S \sin k_g + \Im S \cos k_g \end{eqnarray*}

This reference-point issue is frequently mishandled in the literature. The two conventions agree closely for small k_g, but the discrepancy becomes significant once k_g \gtrsim 0.2.

At low reduced frequencies, S(k_g)\rightarrow 1 and the gust response becomes quasi-steady. At high reduced frequencies, Sears’s function decays in magnitude, with the asymptotic behavior given by

(54)   \begin{equation*} |S(k_g)| \ \propto \ \frac{1}{\sqrt{2\pi \, k_g}} \quad \text{when} \ k_g\rightarrow\infty \end{equation*}

with a phase that depends on the chosen reference point. Notice again that the mid-chord convention contains the additional convective phase accumulation that produces the characteristic spiral locus in the complex plane, whereas the leading-edge-referenced function accounts for this phase shift through the factor e^{ik_g} in Eq. 52.

The Theodorsen and Sears functions describe different physical problems and are not interchangeable. Theodorsen’s function applies to airfoil motion (pitching or plunging), whereas Sears’s function applies to a convected gust acting on a stationary airfoil. In one case, the unsteadiness is generated by the airfoil; in the other, it is imposed by the flow. This distinction matters because the amplitude and phase of the lift response differ between the two cases. However, because the underlying unsteady airfoil theory is linear, the unsteady lift responses predicted by Theodorsen’s and Sears’s functions can be added by superposition when both airfoil motion and a convected gust are present simultaneously.

Check Your Understanding #3 – Use of the Sears function versus the Theodorsen function

An airfoil of chord length c = 1.2 m is moving at a steady freestream speed {V_{\infty}} = 60 m/s in incompressible flow. Consider the following two cases: (a) The airfoil undergoes a small-amplitude harmonic pitching motion about the quarter-chord, i.e.,

    \[ \theta(t) = \theta_0 \, e^{i\omega t} \]

where \theta_0 = 2^{\circ} and \omega = 8 rad/s. (b) The airfoil is fixed but encounters a convected sinusoidal vertical gust, i.e.,

    \[ w_g(x,t) = w_0 \,\sin\!\left(\omega t - \frac{\omega x}{V_{\infty}}\right) \]

where w_0 = 1.5 m/s and \omega = 8 rad/s. For each case: (i) Identify whether the unsteadiness is generated by airfoil motion or imposed by the flow field, and state which transfer function (Theodorsen’s or Sears’s) is appropriate. (ii) Compute the reduced frequency. (iii) Using the value of k, state whether the lift response is expected to be essentially quasi-steady or appreciably unsteady.

Show solution/hide solution.

(a) The unsteadiness is generated by prescribed airfoil motion, so the appropriate transfer function is Theodorsen’s function.
(b) The unsteadiness is imposed by a convected gust acting on a fixed airfoil, so the appropriate transfer function is Sears’s function.
(ii) The reduced frequency is the same in both cases:

    \[ k = \frac{\omega c}{2V_{\infty}} = \frac{8 \times 1.2}{2 \times 60} = \frac{9.6}{120} = 0.08 \]

(iii) Because k = 0.08 is still small but above the usual quasi-steady range, the lift response in both cases is expected to show modest unsteady effects, including some amplitude attenuation and phase shift relative to the quasi-steady prediction. It would not usually be considered strongly unsteady, but it should no longer be treated as strictly quasi-steady.

Time-Domain: The Indicial Response

The indicial aerodynamic response method provides a time-domain framework for calculating unsteady aerodynamic forces and moments. The indicial response refers to the system’s response to a unit step input applied at t = 0 and held constant thereafter. Like all classic thin-airfoil theories, the response relies on the linearization of aerodynamic forces. For a change in angle of attack, \Delta \alpha, from an initial angle \alpha_0, then

(55)   \begin{equation*} \Delta C_l(t) = C_{l_{\alpha}} \, \Delta \alpha \end{equation*}

The indicial response is given by

(56)   \begin{equation*} C_l(t) = C_l(t=0) + C_{l_{\alpha}} \, \phi(t) \, \Delta \alpha \end{equation*}

where {\phi(t)} is called the indicial response function.

For arbitrary variations in \alpha(t), Duhamel’s convolution integral applies, i.e.,

(57)   \begin{equation*} C_l(t) = C_{l_{\alpha}} \alpha(0) \phi(t) + C_{l_{\alpha}} \int_0^t \frac{d\alpha(\sigma)}{d\sigma} \, \phi(t-\sigma) \, d\sigma \end{equation*}

where \sigma is a dummy time variable of integration. In this dimensional-time form, the indicial response function \phi is understood to depend on the elapsed convective time after the disturbance. Therefore, the solution to the Duhamel integral accounts for the time-history effects of arbitrary forcing. However, it requires repeated evaluation of the indicial aerodynamic functions, so one challenge in solving the integral is determining them in a form suitable for numerical solution.

Non-Dimensional Time

The nondimensional or reduced time is always used for transient problems where the reduced frequency becomes ambiguous. The reduced time is defined as

(58)   \begin{equation*} s = \frac{1}{b}\int_0^t V_{\infty} \, dt = \frac{2}{c} \int_0^t V_{\infty} \, dt \end{equation*}

where {V_{\infty}} is the freestream velocity, so that s represents the relative distance traveled by the airfoil through the flow in units of semi-chords. This parameter facilitates the analysis of unsteady flow problems that discrete frequencies cannot characterize. It will be apparent that the reduced time variable is the same as the distance traveled by the airfoil through the flow expressed in semi-chords.

Wagner’s Problem

Wagner determined the transient lift response to a step change in angle of attack.[9] In Wagner’s problem, the airfoil experiences a sudden change in angle of attack caused by its own motion. The response accounts for the effects of the shed wake through Wagner’s function, \phi(s), where

(59)   \begin{equation*} s = \frac{2 \, V_{\infty} \, t}{c} \end{equation*}

is the reduced time, i.e., the distance traveled by the airfoil through the flow in units of semi-chords.

For a step change in angle of attack, \Delta \alpha, the lift coefficient increment may be written formally as the sum of a noncirculatory impulsive term and a circulatory term, i.e.,

(60)   \begin{equation*} \Delta C_l(s) = \pi \, \Delta \alpha \, \delta(s) + 2\pi \, \Delta \alpha \, \phi(s) \end{equation*}

where \delta(s) is the Dirac delta function in nondimensional time. The first term is a distributional impulse associated with the apparent-mass response at the instant of the step; it is not a finite sustained lift coefficient and contributes only when integrated through the impulse. The second term represents the circulatory lift increment that develops as vorticity is shed into the wake.

The Wagner function can be calculated exactly in terms of special functions and is shown in Figure 13. Because \phi(s) builds asymptotically from 0.5 to 1 as s \to \infty, the circulatory component of the lift increment increases from \Delta C_l^c(0^+) = \pi \, \Delta \alpha to \Delta C_l^c(\infty) = 2\pi \, \Delta \alpha. The impulsive contribution at s = 0 is separate and represents the noncirculatory apparent-mass response. Otherwise, Wagner’s function represents the gradual growth of circulatory lift as the starting vortex is shed into the downstream wake and circulation develops around the airfoil.

The Wagner indicial response function is the circulatory lift response to a step change in angle of attack.

For arbitrary variations in angle of attack, the circulatory lift can be computed using Duhamel’s integral. In terms of nondimensional time s, the circulatory lift coefficient is

(61)   \begin{equation*} C_l^c(s) = 2\pi \left[ \alpha(0)\,\phi(s) + \int_0^s \frac{d\alpha(\sigma)}{d\sigma} \,\phi(s-\sigma)\,d\sigma \right] \end{equation*}

where \sigma is a dummy reduced-time variable. This expression gives only the circulatory part of the lift, i.e., the part associated with the gradual development of circulation and the shed wake. The noncirculatory apparent-mass terms are added separately as local velocity- or acceleration-dependent terms. For practical calculations, Wagner’s function is often approximated using a two-term exponential form, i.e.,

(62)   \begin{equation*} \phi(s) \approx 1.0 - 0.165\,e^{-0.0455s} - 0.335\,e^{-0.3s} \end{equation*}

or, more generally,

(63)   \begin{equation*} \phi(s) = 1 - A_1e^{-b_1s} - A_2e^{-b_2s} \end{equation*}

where, for the common two-term approximation,

(64)   \begin{equation*} A_1=0.165, \quad b_1=0.0455, \qquad A_2=0.335, \quad b_2=0.3 \end{equation*}

Therefore, Wagner’s function is the time-domain indicial response for airfoil-motion forcing. Recall that the corresponding frequency-domain response for harmonic airfoil motion is Theodorsen’s function.

Sharp-Edged Gust: Küssner’s Problem

The gust-response counterpart to Wagner’s problem is Küssner’s problem.[10] In Wagner’s problem, the unsteadiness is generated by airfoil motion. In Küssner’s problem, the airfoil is fixed and encounters a sharp-edged vertical gust convected by the freestream, i.e., the unsteadiness is imposed by the flow field rather than generated by the motion of the airfoil.

For a sharp-edged gust of vertical velocity w_g, the effective gust angle is

(65)   \begin{equation*} \alpha_g = \frac{w_g}{V_{\infty}} \end{equation*}

for small angles. The corresponding circulatory lift response may be written as

(66)   \begin{equation*} \Delta C_l^g(s) = 2\pi \, \alpha_g \, \psi(s) \end{equation*}

where \psi(s) is Küssner’s function and s=2V_{\infty}t/c is the nondimensional time. Unlike Wagner’s function, which begins at \phi(0^+)=0.5, Küssner’s function begins at \psi(0) = 0 and approaches unity as s\to\infty, i.e., \psi(\infty) = 1. Therefore, the circulatory lift response to a sharp-edged gust builds from zero to the quasi-steady value, i.e.,

(67)   \begin{equation*} \Delta C_l^g(\infty) = 2\pi \frac{w_g}{V_{\infty}} \end{equation*}

The Küssner function can be obtained from the classical incompressible thin-airfoil gust problem and is shown in Figure 14.

The Küssner indicial response function is the circulatory lift response to a sharp-edged gust.

For engineering calculations, Küssner’s function is often represented by a two-term exponential approximation of the form

(68)   \begin{equation*} \psi(s) \approx 1 - A_1 e^{-b_1s} - A_2 e^{-b_2s} \end{equation*}

with constants chosen to match the exact or tabulated response over the range of reduced times of interest. A simple approximation is

(69)   \begin{equation*} \psi(s) \approx 1 - 0.5\,e^{-0.13s} - 0.5\,e^{-s} \end{equation*}

which satisfies the correct limiting values at s=0 and s\to\infty, but more accurate coefficient sets may be used when better agreement with the classical Küssner function is required.

For an arbitrary gust history, the gust-induced circulatory lift can be computed by applying Duhamel’s integral to the gust angle, i.e.,

(70)   \begin{equation*} C_l^g(s) = 2\pi \left[ \alpha_g(0)\psi(s) + \int_0^s \frac{d\alpha_g(\sigma)}{d\sigma} \,\psi(s-\sigma)\,d\sigma \right] \end{equation*}

where

(71)   \begin{equation*} \alpha_g(s)=\frac{w_g(s)}{V_{\infty}} \end{equation*}

and \sigma is again a dummy reduced-time variable.

Therefore, it will be appreciated that Küssner’s function is the time-domain indicial response for a gust input, just as Wagner’s function is the time-domain indicial response for a sudden change in airfoil angle of attack. The corresponding frequency-domain response for a sinusoidal gust is Sears’s function. The two viewpoints are complementary: Küssner’s function is used for arbitrary gust histories in the time domain, whereas Sears’s function is used for harmonic gusts in the frequency domain.

Connection Between Apparent Mass & Indicial Response

The distinction between circulatory and noncirculatory lift can also be understood from the indicial-response viewpoint. Previously, the noncirculatory or apparent-mass terms were introduced as local velocity- and acceleration-dependent contributions that are added to the circulatory lift. These terms are not multiplied by Theodorsen’s function because they are not wake-memory effects. In the time domain, the same physical contribution appears as the impulsive part of the indicial response.

In Wagner’s problem, the circulatory lift following a step change in angle of attack develops gradually as vorticity is shed into the wake. This gradual development is represented by Wagner’s function, \phi(s), where s is the usual nondimensional time. The noncirculatory response, by contrast, is instantaneous because it is associated with the pressure field required to accelerate the fluid around the airfoil. Therefore, it appears mathematically as an impulse.

The point can be made explicitly by considering a sudden step change in angle of attack, i.e.,

(72)   \begin{equation*} \alpha(s)=\Delta\alpha\,H(s) \end{equation*}

where H(s) is the Heaviside step function. This function is zero before the step and one after the step, i.e.,

(73)   \begin{equation*} H(s)= \begin{cases} 0, & s<0\\ 1, & s>0 \end{cases} \end{equation*}

Therefore, \Delta\alpha H(s) represents an angle of attack that jumps suddenly from zero to \Delta\alpha at s=0. The derivative of the Heaviside function is the Dirac delta function, so

(74)   \begin{equation*} \frac{d\alpha}{ds} = \Delta\alpha\,\delta(s) \end{equation*}

The delta function is not an ordinary finite function at s=0. It is defined by its integral, namely

(75)   \begin{equation*} \int_{-\epsilon}^{+\epsilon}\delta(s)\,ds=1 \end{equation*}

for any \epsilon>0. Therefore,

(76)   \begin{equation*} \int_{-\epsilon}^{+\epsilon} \frac{d\alpha}{ds}\,ds = \int_{-\epsilon}^{+\epsilon} \Delta\alpha\,\delta(s)\,ds = \Delta\alpha \end{equation*}

which recovers the finite jump in angle of attack. This is the mathematical meaning of an impulsive response: the instantaneous value is singular, but the integrated effect through the impulse is finite.

It is important to distinguish between an indicial-response kernel and the lift itself. Let the noncirculatory part of the indicial-response kernel be written as

(77)   \begin{equation*} K_{\rm nc}(s)=A\,\delta(s) \end{equation*}

where A is the appropriate apparent-mass coefficient for the motion being considered. The symbol K_{\rm nc} denotes the kernel, not the lift coefficient. The corresponding noncirculatory lift coefficient is obtained from Duhamel’s integral, i.e.,

(78)   \begin{equation*} C_{l_{\rm nc}}(s) = \int_0^s K_{\rm nc}(s-\sigma) \frac{d\alpha(\sigma)}{d\sigma} \,d\sigma \end{equation*}

Substituting K_{\rm nc}(s-\sigma)=A\,\delta(s-\sigma) gives

(79)   \begin{equation*} C_{l_{\rm nc}}(s) = A \int_0^s \delta(s-\sigma) \frac{d\alpha(\sigma)}{d\sigma} \,d\sigma \end{equation*}

Using the sifting property of the delta function,

(80)   \begin{equation*} \int_0^s \delta(s-\sigma) \frac{d\alpha(\sigma)}{d\sigma} \,d\sigma = \frac{d\alpha(s)}{ds} \end{equation*}

so that

(81)   \begin{equation*} C_{l_{\rm nc}}(s) = A\,\frac{d\alpha}{ds} \end{equation*}

This result shows how the impulsive part of the indicial response becomes a local derivative term for a general smooth motion.

The angle-of-attack example shows how a delta-function kernel becomes a local derivative term. For an actual airfoil section, the same mechanism acts on the motion variables that create normal velocity on the airfoil. Therefore, for a two-dimensional airfoil with semi-chord b = c/2, freestream speed {V_{\infty}}, plunge displacement h(t), and pitch angle \theta(t), the effective angle of attack contains contributions from both pitch and vertical motion. In a small-disturbance approximation, the plunge contribution gives an effective angle of attack that contains a term of the form

(82)   \begin{equation*} \alpha_{\rm eff} \sim \theta + \frac{\overbigdot{h}}{V_{\infty}} \end{equation*}

with the sign depending on the convention used for positive plunge. Therefore, when the noncirculatory indicial response acts on the rate of change of the effective angle of attack, it naturally produces a term proportional to

(83)   \begin{equation*} \frac{d}{dt} \left( \frac{\overbigdot{h}}{V_{\infty}} \right) = \frac{\overbigddot{h}}{V_{\infty}} \end{equation*}

This is the time-domain mechanism by which the plunge-acceleration apparent-mass term appears. Physically, the airfoil must accelerate a surrounding mass of fluid as it plunges, so the resulting pressure field produces an instantaneous lift contribution proportional to \overbigddot{h}.

Pitch produces two related noncirculatory effects. First, pitch rate changes the local normal velocity distribution over the chord, giving an apparent-mass contribution proportional to V_{\infty}\overbigdot{\theta}. Second, pitch acceleration requires angular acceleration of the surrounding fluid, giving a contribution proportional to b\overbigddot{\theta} with a coefficient that depends on the location of the pitch axis. Therefore, the classical noncirculatory lift per unit span may be written as

(84)   \begin{equation*} L'_{\rm nc} = \pi \varrho_\infty b^2 \left( \overbigddot{h} + V_{\infty}\overbigdot{\theta} - a \, b \, \overbigddot{\theta} \right) \end{equation*}

where a locates the pitch axis relative to the mid-chord in semi-chord units. This form is written for a general pitch-axis location; simpler special cases follow by choosing the pitch-axis convention and sign definitions used in a particular example. The precise signs of the terms depend on the adopted sign convention for positive plunge, positive pitch, positive lift, and the definition of a. However, the structure of the result is the important point: the noncirculatory lift is local in time and contains apparent-mass terms proportional to plunge acceleration, pitch rate, and pitch acceleration.

These terms are the physical counterparts of the delta-function contribution in the indicial response. The term \pi \varrho_\infty b^2 \overbigddot{h} is the apparent-mass lift associated with accelerating the surrounding fluid in plunge. The term \pi \varrho_\infty b^2 V_{\infty}\overbigdot{\theta} is associated with the rotational velocity field produced by pitch rate in a forward stream, and the term -\pi \varrho_\infty b^3 a \overbigddot{\theta} is associated with angular acceleration about an axis displaced from the mid-chord. These contributions arise from the instantaneous pressure field needed to accelerate the surrounding fluid.

The connection with nondimensional indicial time follows by introducing

(85)   \begin{equation*} s=\frac{V_{\infty}t}{b} \end{equation*}

so that

(86)   \begin{equation*} \frac{d}{dt} = \frac{V_{\infty}}{b} \frac{d}{ds} \end{equation*}

and

(87)   \begin{equation*} \frac{d^2}{dt^2} = \left(\frac{V_{\infty}}{b}\right)^2 \frac{d^2}{ds^2} \end{equation*}

Therefore,

(88)   \begin{equation*} \overbigdot{\theta} = \frac{V_{\infty}}{b} \frac{d\theta}{ds} \qquad \text{and} \qquad \overbigddot{\theta} = \left(\frac{V_{\infty}}{b}\right)^2 \frac{d^2\theta}{ds^2} \end{equation*}

and

(89)   \begin{equation*} \overbigddot{h} = \left(\frac{V_{\infty}}{b}\right)^2 \frac{d^2 h}{ds^2} \end{equation*}

If the nondimensional plunge displacement is defined as \bar{h}=\dfrac{h}{b} then

(90)   \begin{equation*} \overbigddot{h} = \frac{V_{\infty}^2}{b} \frac{d^2\bar{h}}{ds^2} \end{equation*}

Therefore, the dimensional apparent-mass terms \overbigddot{h}, {\overbigdot{\theta}}, and \overbigddot{\theta} correspond in nondimensional indicial form to terms involving \dfrac{d^2\bar{h}}{ds^2}, \dfrac{d\theta}{ds}, and \dfrac{d^2\theta}{ds^2}. For harmonic forcing, for example, \theta(s)=\theta_0 \, e^{i \Omega s}, where \Omega is the nondimensional frequency based on s, then

(91)   \begin{equation*} \frac{d\theta}{ds} = i \, \Omega \theta_0 \, e^{i \Omega s} \end{equation*}

and

(92)   \begin{equation*} \frac{d^2\theta}{ds^2} = -\Omega^2 \, \theta_0 \, e^{i \Omega s} \end{equation*}

First-derivative apparent-mass terms therefore appear in the frequency domain as algebraic factors proportional to i\Omega, while second-derivative apparent-mass terms appear as factors proportional to -\Omega^2. The same reasoning applies to plunge. A harmonic plunge displacement produces \overbigddot{h} \sim -\Omega^2 \, h in nondimensional form, and so the plunge contribution appears as an algebraic acceleration term rather than as a wake-memory term.

Consequently, the delta-function part of the indicial response is the time-domain representation of the same apparent-mass physics that appears in the classical unsteady airfoil equations as local terms proportional to \overbigddot{h}, V_{\infty} \, \overbigdot{\theta}, and b\overbigddot{\theta}. The circulatory part has wake memory and is governed by Wagner’s function in the time domain or Theodorsen’s function in the frequency domain. The noncirculatory part has no wake memory and appears instead as instantaneous velocity- and acceleration-dependent terms.

Time- Vs. Frequency-Domain Functions

By now, it will be apparent that Theodorsen’s, Sears’s, Wagner’s, and Küssner’s functions are closely related, but they describe different forms of unsteady aerodynamic forcing. Theodorsen’s and Sears’s functions are frequency-domain transfer functions for harmonic forcing, whereas Wagner’s and Küssner’s functions are time-domain indicial response functions for step-type forcing.

For airfoil motions, Theodorsen’s function C(k) gives the circulatory lift response to harmonic pitching or plunging motion. In the time domain, the corresponding indicial response is Wagner’s function \phi(s), which describes the growth of circulatory lift after a sudden change in angle of attack. Therefore, Theodorsen’s and Wagner’s functions represent the same circulatory wake physics viewed from two different domains, i.e.,

(93)   \begin{equation*} \text{airfoil motion:} \qquad \phi(s) \;\longleftrightarrow\; C(k) \end{equation*}

where s=2V_{\infty}t/c is the nondimensional time and k=\omega c/(2V_{\infty}) is the reduced frequency.

For gust excitations, Sears’s function S(k_g) gives the circulatory lift response of a fixed airfoil to a sinusoidal vertical gust convected by the freestream. In the time domain, the corresponding indicial response is Küssner’s function \psi(s), which describes the growth of lift after the airfoil encounters a sharp-edged vertical gust. Therefore,

(94)   \begin{equation*} \text{gust forcing:} \qquad \psi(s) \;\longleftrightarrow\; S(k_g) \end{equation*}

The distinction between the two pairs is physical. Wagner’s and Theodorsen’s functions apply when the unsteadiness is generated by airfoil motion. Küssner’s and Sears’s functions apply when the flow field imposes the unsteadiness as a gust. In both cases, the time-domain and frequency-domain descriptions are complementary. The indicial response gives the lift history following a step input, while the frequency-domain transfer function gives the amplitude and phase response to harmonic forcing.

In practical calculations, arbitrary motions or gust histories may be treated in the time domain by convolution with the appropriate indicial response function. Harmonic motions or gusts may be treated in the frequency domain using the corresponding complex transfer function. Apparent-mass terms are added separately when the airfoil itself is accelerating, because those terms are noncirculatory and are not represented by the wake-response functions C(k), S(k_g), \phi(s), or \psi(s).

Numerical Solutions Using the Duhamel Integral

Unsteady aerodynamic problems are usually solved numerically because the aerodynamic loads depend not only on the instantaneous motion or gust input, but also on the prior wake history. In the time domain, this history dependence appears through convolution integrals such as Duhamel’s integral. Direct evaluation of the convolution at every time step is possible, but it can become inefficient because the entire previous input history must be retained and repeatedly integrated.

A more efficient approach is to approximate the indicial response function by a sum of exponentials. This converts the convolution integral into a set of first-order aerodynamic lag states that can be advanced recursively in time. The resulting method preserves the essential wake-history (hereditary) effects while avoiding repeated evaluation of the full convolution integral. It also provides a convenient way to include different types of inputs, such as airfoil motion through Wagner’s function and gust excitation through Küssner’s function, within the same time-marching framework.

Consider a general two-term indicial response function of the form

(95)   \begin{equation*} f(s) = 1 - A_1 e^{-b_1s} - A_2 e^{-b_2s} \end{equation*}

where f(s) may represent Wagner’s function \phi(s), Küssner’s function \psi(s), or another approximate indicial response function. For Wagner’s function, typical constants are

(96)   \begin{equation*} A_1=0.165, \quad b_1=0.0455, \qquad A_2=0.335, \quad b_2=0.3 \end{equation*}

whereas for the simple Küssner approximation used above, the constants are

(97)   \begin{equation*} A_1=0.5, \quad b_1=0.13, \qquad A_2=0.5, \quad b_2=1.0 \end{equation*}

For a generic input angle \alpha_i(s), the effective angle associated with the circulatory response may be written as

(98)   \begin{equation*} \alpha_{e,i}(s) = \alpha_i(s)-X_i(s)-Y_i(s) \end{equation*}

where X_i(s) and Y_i(s) are aerodynamic lag states associated with the two exponential terms in the chosen indicial response function. The corresponding circulatory lift coefficient is then

(99)   \begin{equation*} C_{l,i}^c(s) = 2\pi \, \alpha_{e,i}(s) \end{equation*}

For a piecewise-linear change in the input angle over the interval \Delta s, a practical recursive approximation is

(100)   \begin{equation*} X_i(s+\Delta s) = X_i(s)e^{-b_1\Delta s} + A_1\Delta\alpha_{i,s} \left[ \frac{1-e^{-b_1\Delta s}}{b_1\Delta s} \right] \end{equation*}

and

(101)   \begin{equation*} Y_i(s+\Delta s) = Y_i(s)e^{-b_2\Delta s} + A_2\Delta\alpha_{i,s} \left[ \frac{1-e^{-b_2\Delta s}}{b_2\Delta s} \right] \end{equation*}

where

(102)   \begin{equation*} \Delta\alpha_{i,s} = \alpha_i(s+\Delta s)-\alpha_i(s) \end{equation*}

so that the effective angle at the new time step is

(103)   \begin{equation*} \alpha_{e,i}(s+\Delta s) = \alpha_i(s+\Delta s)-X_i(s+\Delta s)-Y_i(s+\Delta s) \end{equation*}

The aerodynamic wake history is contained in the lag states X_i(s) and Y_i(s). For sufficiently small \Delta s, the bracketed factors approach unity, recovering the simpler first-order update.

For airfoil-motion forcing, the input angle may be denoted by \alpha_m(s), and the Wagner-function constants are used. The corresponding circulatory lift contribution is

(104)   \begin{equation*} C_{l,\mathrm{motion}}^c(s_n) = 2\pi \, \alpha_{e,m}(s_n) \end{equation*}

where

(105)   \begin{equation*} \alpha_{e,m}(s_n) = \alpha_m(s_n)-X_m(s_n)-Y_m(s_n) \end{equation*}

For gust forcing, the input angle may be written as

(106)   \begin{equation*} \alpha_g(s)=\frac{w_g(s)}{V_{\infty}} \end{equation*}

and the Küssner-function constants are used. The corresponding gust-induced circulatory lift contribution is

(107)   \begin{equation*} C_{l,\mathrm{gust}}^c(s_n) = 2\pi \, \alpha_{e,g}(s_n) \end{equation*}

where

(108)   \begin{equation*} \alpha_{e,g}(s_n) = \alpha_g(s_n)-X_g(s_n)-Y_g(s_n) \end{equation*}

For a general unsteady problem, both airfoil motion and gust excitation may be present simultaneously. Under the assumptions of linear thin-airfoil theory, their circulatory contributions may be superposed, so that

(109)   \begin{equation*} C_l^c(s_n) = C_{l,\mathrm{motion}}^c(s_n) + C_{l,\mathrm{gust}}^c(s_n) \end{equation*}

or

(110)   \begin{equation*} C_l^c(s_n) = 2\pi \, \alpha_{e,m}(s_n) + 2\pi \, \alpha_{e,g}(s_n) \end{equation*}

The apparent-mass terms are not included in the lag states because they have no wake history effects. They are evaluated directly from the instantaneous velocity or acceleration of the airfoil motion at the current time step. Therefore, the total lift coefficient is assembled as

(111)   \begin{equation*} C_l(s_n) = C_l^c(s_n) + C_{l_{\rm nc}}(s_n) \end{equation*}

or, equivalently,

(112)   \begin{equation*} C_l(s_n) = C_{l,\mathrm{motion}}^c(s_n) + C_{l,\mathrm{gust}}^c(s_n) + C_{l_{\rm nc}}(s_n) \end{equation*}

For example, for small-amplitude plunge and pitch motions of a thin airfoil, the noncirculatory lift contribution may be written in coefficient form as

(113)   \begin{equation*} C_{l_{\rm nc}}(s_n) = \left( \frac{\pi \, c}{2V_{\infty}^2} \right) \overbigddot{h}(t_n) + \left( \frac{\pi \, c^2}{4V_{\infty}^2} \right) \overbigddot{\theta}(t_n) \end{equation*}

with signs interpreted according to the chosen definitions of positive h, positive \theta, and positive lift. These acceleration terms are evaluated locally from the imposed motion or from the structural equations of motion. If the motion history is prescribed or has already been computed, then finite-difference approximations may be used, such as

(114)   \begin{equation*} \overbigddot{h}(t_n) \approx \frac{h_{n+1}-2h_n+h_{n-1}}{\Delta t^2} \end{equation*}

and

(115)   \begin{equation*} \overbigddot{\theta}(t_n) \approx \frac{\theta_{n+1}-2\theta_n+\theta_{n-1}}{\Delta t^2} \end{equation*}

For a coupled aeroelastic time-marching solution, the apparent-mass terms are usually assembled consistently with the structural equations at the current time step. Therefore, the numerical procedure is to compute the circulatory lift from the appropriate Wagner or Küssner lag-state recursion and then add the local apparent-mass correction without passing it through the wake lag states.

Check Your Understanding #4 – Combining motion and gust inputs in the time domain

A thin airfoil in incompressible flow undergoes a prescribed plunge motion h(t) while also encountering a time-varying vertical gust w_g(t). The freestream speed is constant and equal to {V_{\infty}}. Let the nondimensional time be s=\dfrac{2V_{\infty}t}{c} and define the motion-induced and gust-induced effective angles of attack as

    \[ \alpha_m(s)=\frac{\overbigdot{h}(s)}{V_{\infty}} \qquad \text{and} \qquad \alpha_g(s)=\frac{w_g(s)}{V_{\infty}} \]

where the sign convention is such that positive \alpha_m and positive \alpha_g both increase lift. Using unsteady thin-airfoil theory, write the total lift coefficient as the sum of: (i) the circulatory response to the airfoil motion, (ii) the circulatory response to the gust input, and (iii) the noncirculatory apparent-mass contribution from the plunge acceleration. Identify which indicial function is used for each circulatory part.

Show solution/hide solution.

For a general linear unsteady aerodynamic problem, the total lift coefficient may be written as

    \[ C_l(s) = C_{l,\mathrm{motion}}^c(s) + C_{l,\mathrm{gust}}^c(s) + C_{l_{\rm nc}}(s) \]

The motion-induced circulatory response is obtained using Wagner’s function, \phi(s), because the forcing is generated by airfoil motion. Therefore,

    \[ C_{l,\mathrm{motion}}^c(s) = 2\pi \left[ \alpha_m(0)\phi(s) + \int_0^s \frac{d\alpha_m(\sigma)}{d\sigma} \,\phi(s-\sigma)\,d\sigma \right] \]

The gust-induced circulatory response is obtained using Küssner’s function, \psi(s), because the forcing is imposed by the flow field. Therefore,

    \[ C_{l,\mathrm{gust}}^c(s) = 2\pi \left[ \alpha_g(0)\psi(s) + \int_0^s \frac{d\alpha_g(\sigma)}{d\sigma} \,\psi(s-\sigma)\,d\sigma \right] \]

The noncirculatory apparent-mass contribution is not included in either indicial convolution because it has no wake history effects. For the plunge motion, it is evaluated locally from the instantaneous plunge acceleration:

    \[ C_{l_{\rm nc}}(s) = \left( \frac{\pi \, c}{2V_{\infty}^2} \right) \overbigddot{h}(t) \]

with the sign interpreted consistently with the definitions of positive h, positive \alpha_m, and positive lift. Therefore, the total lift coefficient may be assembled from

    \[ C_l(s) = C_{l,\mathrm{motion}}^c(s) + C_{l,\mathrm{gust}}^c(s) + C_{l_{\rm nc}}(s) \]

where

    \[ C_{l,\mathrm{motion}}^c(s) = 2\pi \left[ \alpha_m(0)\phi(s) + \int_0^s \frac{d\alpha_m(\sigma)}{d\sigma} \,\phi(s-\sigma)\,d\sigma \right] \]

    \[ C_{l,\mathrm{gust}}^c(s) = 2\pi \left[ \alpha_g(0)\psi(s) + \int_0^s \frac{d\alpha_g(\sigma)}{d\sigma} \,\psi(s-\sigma)\,d\sigma \right] \]

and, for plunge only,

    \[ C_{l_{\rm nc}}(s) = \left( \frac{\pi \, c}{2V_{\infty}^2} \right) \overbigddot{h}(t) \]

This result shows the essential structure of the time-domain solution: Wagner’s function accounts for the wake response to airfoil motion, Küssner’s function accounts for the wake response to gust input, and the apparent-mass term is added separately as a local acceleration-dependent contribution.

State-Space Form of the Indicial Response

For aeroelastic applications, the indicial-response approximation is often recast into state-space form. In this form, the aerodynamic lag states represent the wake history associated with the exponential terms in the indicial response. The convolution integral is then replaced by a set of first-order differential equations that can be advanced in time or appended directly to the structural equations of motion. This formulation is especially useful because the coupled aeroelastic system can be analyzed using eigenvalue methods or integrated forward in time with standard numerical algorithms.

In general, a linear state-space system may be written as

(116)   \begin{equation*} \overbigdot{\mathbf{x}} = \mathbf{A}\mathbf{x} + \mathbf{B}u \end{equation*}

with the output equation

(117)   \begin{equation*} y = \mathbf{C}\mathbf{x} + \mathbf{D}u \end{equation*}

where \mathbf{x} is the state vector, u is the input, and y is the output. In the present application, the input is an effective angle of attack, such as a motion-induced angle \alpha_m(s) or gust-induced angle \alpha_g(s), and the output is the corresponding circulatory lift coefficient.

Consider the two-term indicial response approximation

(118)   \begin{equation*} f(s) = 1 - A_1e^{-b_1s} - A_2e^{-b_2s} \end{equation*}

where f(s) may represent Wagner’s function, Küssner’s function, or another approximate indicial response. The lag-state form introduced above is already a state-space realization of this response. In nondimensional time s, define two aerodynamic states X(s) and Y(s) such that

(119)   \begin{equation*} \alpha_e(s) = \alpha(s)-X(s)-Y(s) \end{equation*}

The corresponding first-order state equations are

(120)   \begin{equation*} \frac{dX}{ds} = -b_1 X + A_1 b_1 \alpha(s) \end{equation*}

and

(121)   \begin{equation*} \frac{dY}{ds} = -b_2 Y + A_2 b_2 \alpha(s) \end{equation*}

These equations show that each exponential term in the indicial response becomes one aerodynamic lag state. The circulatory lift coefficient is then

(122)   \begin{equation*} C_l^c(s) = C_{l_{\alpha}} \left[ \alpha(s)-X(s)-Y(s) \right] \end{equation*}

or, for a thin airfoil in incompressible flow,

(123)   \begin{equation*} C_l^c(s) = 2\pi \left[ \alpha(s)-X(s)-Y(s) \right] \end{equation*}

In matrix form, this state-space model may be written as

(124)   \begin{equation*} \frac{d}{ds} \begin{bmatrix} X \\[4pt] Y \end{bmatrix} = \begin{bmatrix} -b_1 & 0 \\[4pt] 0 & -b_2 \end{bmatrix} \begin{bmatrix} X \\[4pt] Y \end{bmatrix} + \begin{bmatrix} A_1b_1 \\[4pt] A_2b_2 \end{bmatrix} \alpha(s) \end{equation*}

with the output equation

(125)   \begin{equation*} C_l^c(s) = C_{l_{\alpha}} \left\{ \alpha(s) - \begin{bmatrix} 1 & 1 \end{bmatrix} \begin{bmatrix} X \\[4pt] Y \end{bmatrix} \right\} \end{equation*}

This form is equivalent to the Duhamel convolution when the same exponential approximation is used for the indicial response function.

If dimensional time t is used instead of nondimensional time s, then

(126)   \begin{equation*} s=\frac{2V_{\infty}t}{c} \end{equation*}

for constant {V_{\infty}}, and so

(127)   \begin{equation*} \frac{d}{dt} = \frac{2V_{\infty}}{c} \frac{d}{ds} \end{equation*}

Therefore, the dimensional-time state equations become

(128)   \begin{equation*} \frac{dX}{dt} = -\left(\frac{2V_{\infty}}{c}\right)b_1 X + \left(\frac{2V_{\infty}}{c}\right)A_1b_1 \, \alpha(t) \end{equation*}

and

(129)   \begin{equation*} \frac{dY}{dt} = -\left(\frac{2V_{\infty}}{c}\right)b_2 Y + \left(\frac{2V_{\infty}}{c}\right)A_2b_2 \, \alpha(t) \end{equation*}

The same state-space structure may be used separately for airfoil-motion and gust inputs. For example, motion-induced states X_m, Y_m may be used with Wagner-function constants, while gust-induced states X_g, Y_g may be used with Küssner-function constants. The total circulatory lift is then obtained by superposition, i.e.,

(130)   \begin{equation*} C_l^c = C_{l,\mathrm{motion}}^c + C_{l,\mathrm{gust}}^c \end{equation*}

and the noncirculatory apparent-mass terms are added separately.

The important practical point is that the state-space form converts the wake-hereditary problem into a system of ordinary differential equations. These aerodynamic equations can then be combined directly with the structural equations of motion to form a coupled aeroelastic state-space model. Flutter can then be studied by computing the eigenvalues of the complete aeroelastic system or by integrating the coupled equations forward in time.

Compressibility Effects on Unsteady Airfoil Theory

The classical Theodorsen, Sears, Wagner, and Küssner functions discussed above are incompressible-flow results. They are valuable because they reveal the basic physics of unsteady aerodynamic response, including wake history, amplitude attenuation, phase lag, and the distinction between circulatory and noncirculatory loading. However, they should be regarded as low-Mach-number baseline models.

Compressibility affects both the circulatory and noncirculatory parts of the unsteady airloads. The circulatory response changes because pressure disturbances and wake-induced effects no longer propagate as they do in incompressible flow. The noncirculatory, or apparent-mass, response also changes because the local pressure field required to accelerate the surrounding fluid is no longer incompressible. Therefore, compressibility should not be introduced by simply multiplying the incompressible Theodorsen, Sears, Wagner, or Küssner functions, or the incompressible apparent-mass terms, by a Prandtl-Glauert factor.

For subsonic compressible flow, the incompressible response functions are not replaced by simple exact closed-form analogs. Instead, practical engineering methods use approximate or semi-empirical compressible indicial functions and aerodynamic response models. To avoid implying that these are merely the incompressible functions with an added Mach-number argument, they may be denoted generically as

(131)   \begin{equation*} \mathcal{C}(k,M_{\infty}) \qquad \mbox{and} \qquad \mathcal{S}(k_g,M_{\infty}) \end{equation*}

in the frequency domain, and

(132)   \begin{equation*} \Phi(s,M_{\infty}) \qquad \mbox{and} \qquad \Psi(s,M_{\infty}) \end{equation*}

in the time domain. These symbols denote approximate compressible aerodynamic response functions, not exact extensions of Theodorsen’s, Sears’s, Wagner’s, or Küssner’s incompressible functions.

Approximate compressible indicial functions for two-dimensional subsonic flow have been developed and validated by Leishman.[11] In this approach, the unsteady aerodynamic response is obtained from oscillatory lift data over a range of reduced frequencies and Mach numbers. The frequency-domain response is then related back to an equivalent time-domain indicial response using Fourier-transform relationships. The resulting indicial functions are approximate or semi-empirical engineering representations that reproduce the principal Mach-number effects on the unsteady aerodynamic response, rather than exact closed-form counterparts to the incompressible Wagner or Küssner functions.

The incompressible apparent-mass terms must be interpreted with the same caution. For example,

(133)   \begin{equation*} C_{l_{\rm nc}} = \left( \frac{\pi \, c}{2V_{\infty}^2} \right)\overbigddot{h} + \left( \frac{\pi \, c^2}{4V_{\infty}^2} \right)\overbigddot{\theta} \end{equation*}

is an incompressible result. At appreciable Mach numbers, the corresponding noncirculatory response must be obtained from the compressible unsteady aerodynamic model being used. A useful limiting viewpoint is that the very early-time response, or equivalently the large-reduced-frequency limit, is increasingly dominated by local pressure effects rather than by long-time wake-history effects. Piston theory provides one local compressible-pressure approximation for this limiting behavior,[12] but it should not be viewed as a replacement for the full unsteady response functions over the complete range of reduced frequency.

The main practical point is that incompressible unsteady aerodynamic functions and apparent-mass terms are useful reference results, but they should not be used blindly at appreciable Mach numbers. For low-subsonic preliminary calculations, the incompressible functions may still provide useful trends. For subsonic compressible calculations, approximate compressible indicial functions or equivalent compressible aerodynamic response models should be used. For higher-fidelity aeroelastic analysis, the aerodynamic model may instead be based on experimentally identified aerodynamic influence coefficients, linearized compressible-flow methods, Euler calculations, or Reynolds-averaged Navier-Stokes CFD coupled to the structural model. The required model depends on the Mach number, reduced frequency, geometry, and whether the flow remains attached and linear or becomes nonlinear because of shocks, flow separation, or other effects.

Aeroelastic Analysis

The field of aeroelasticity is not easy to master, but understanding the basics, especially the underlying physics in a qualitative context, is a good place to start. Flutter is a self-excited oscillation caused by the interaction of aerodynamic, elastic, and inertial forces. In a fairly general way, the structural dynamics of an aeroelastic system can be described by

(134)   \begin{equation*} { M  \,\overbigddot{q} + C \, \overbigdot{q} + K \, q = F_a } \end{equation*}

where M is the mass matrix, C is the damping matrix, K is the stiffness matrix, q is the displacement vector, and F_a is the aerodynamic force vector. Aerodynamic forces can be computed using computational fluid dynamics (CFD), but panel methods or unsteady airfoil theory may also be used, with their limitations acknowledged. The aerodynamic force F_a on the structure using CFD or panel methods is usually extracted from the pressure distribution, p(x, y, z, t), that acts over the surface, i.e.,

(135)   \begin{equation*} \vec{F}_a(t) = -\int_S p(x,y,z,t) \, \vec{n} \, dS = -\int_S p(x,y,z,t) \, d\vec{S} \end{equation*}

where d\vec{S} = \vec{n}\,dS is the differential vector area and \vec{n} is the outward unit normal. Other methods, however, may be used to approximate aerodynamics, including unsteady airfoil theory (utilizing the Wagner function with the Duhamel integral), panel methods, and others. It is not unusual for flutter calculations to be performed using various aerodynamic methods (with different assumptions) and for the results to be compared.

Combining the aerodynamic and structural models then gives

(136)   \begin{equation*} M \, \overbigddot{q} + (C + B) \, \overbigdot{q} + (K + A) \, q = 0 \end{equation*}

where A and B are called aerodynamic influence matrices. Flutter is a dynamic instability, and its condition is determined by solving the complex eigenvalue problem

(137)   \begin{equation*} \left[ K + A - \omega^2 M + i \, \omega (C + B) \right]\Phi = 0 \end{equation*}

where \omega is the complex circular frequency and \Phi is the corresponding eigenvector (mode shape). Each eigenvalue has an associated eigenvector that describes the deformation pattern of the structure during oscillation. This frequency-domain form shows the stiffness, inertia, and damping contributions to the aeroelastic eigenvalue problem, i.e.,

(138)   \begin{equation*} \left( K + A - \omega^2 M \right)\Phi \;+\; i\,\omega (C + B)\Phi = 0 \end{equation*}

When the eigenvalue is written as a complex circular frequency, the real part of \omega, i.e., \Re(\omega), represents the oscillation frequency of the system. The imaginary part, \Im(\omega), determines the temporal growth or decay of the motion. For the assumed convention e^{i\omega t}, then

(139)   \begin{equation*} e^{i\omega t} = e^{i\Re(\omega)t-\Im(\omega)t} \end{equation*}

so that if \Im(\omega) > 0, the motion is damped and stable, whereas if \Im(\omega) < 0, the motion grows with time, indicating an instability. Equivalently, the modal growth rate may be defined as

(140)   \begin{equation*} \sigma = -\Im(\omega) \end{equation*}

so that \sigma < 0 is stable, \sigma = 0 is neutrally stable, and \sigma > 0 is unstable. Flutter occurs when \sigma = 0, which corresponds to the transition from a stable damped response to an unstable oscillatory response.

The balance between stiffness (including aerodynamic stiffness) and inertial forces is contained within the term (K + A - \omega^2 M), which governs the oscillatory behavior of the system. The damping effects, including aerodynamic damping, are contained within the term \omega (C + B). If the dynamic terms are neglected, the governing equation reduces to

(141)   \begin{equation*} (K + A)\,q = 0 \end{equation*}

which corresponds to a static aeroelastic problem. A non-trivial solution exists when

(142)   \begin{equation*} \det(K + A) = 0 \end{equation*}

which defines the condition for static divergence. At this point, the structure loses stiffness and can undergo unbounded deformation under aerodynamic loading.

A typical flutter boundary is shown in Figure 15, which plots the modal growth or decay rate as a function of airspeed. Flutter speed is the point at which damping equals zero, indicating the onset of unstable oscillation. Notice that negative values indicate a stable system with decaying motion, the zero crossing marks the critical flutter speed, and positive values indicate an unstable system with growing oscillations.

A typical flutter boundary, plotted as a function of airspeed, in terms of the modal growth or decay rate.

The field of aeroelasticity also considers limit-cycle oscillations (LCOs), in which periodic, self-sustaining oscillations arise from nonlinearities in the aerodynamic or structural response. Engineers use sophisticated computational methods and experimental testing to predict and mitigate these aeroelastic phenomena, ensuring that aircraft and spacecraft designs meet stringent safety, performance, and certification standards in diverse flight conditions.

Torsional Divergence and Flutter of a Cantilevered Wing

Understanding aeroelastic instability is often obscured by complex mathematics or code used as a “black box.” However, a classic example for those being introduced to the field of aeroelasticity is a cantilever wing encastré at its root with a single degree of freedom in pitch (torsional motion), as shown in Figure 16. This simple model can illustrate static torsional divergence, in which the effective torsional stiffness becomes zero. Classical flutter, however, is a dynamic instability involving oscillatory motion and aerodynamic damping, and it generally requires at least two coupled degrees of freedom or an equivalent unsteady aerodynamic coupling. Therefore, the maximum airspeed of many aircraft may be limited by aeroelastic effects, which involve compromises among wing strength, torsional rigidity, damping, weight, and cost.

A cantilever wing encastré at its root with a single degree of freedom in pitch (torsional motion).

In this simplified sectional idealization, the generalized coordinate q is equivalent to \theta, the pitch angle of the section about its elastic axis, so the equation of motion per unit span is

(143)   \begin{equation*} I' \, \overbigddot{\theta} + C' \, \overbigdot{\theta} + K' \, \theta = M'_{\rm ac} \end{equation*}

where I' is the mass moment of inertia per unit span about the elastic axis, C' is the structural damping coefficient per unit span, K' is the torsional stiffness per unit span, and {M'_{\rm ac}} is the aerodynamic moment per unit span. A simple linearized aerodynamic model for this moment may be written as

(144)   \begin{equation*} M'_{\rm ac} = \frac{1}{2} \varrho \, V_{\infty}^2 \, \bar{c}^2 \, C_{m_\theta} \, \theta + \frac{1}{2} \varrho \, V_{\infty} \, \bar{c}^3 \, C_{m_{\dot{\theta}}} \, \overbigdot{\theta} \end{equation*}

where C_{m_\theta} is the aerodynamic moment slope about the elastic axis with respect to torsional displacement, C_{m_{\dot{\theta}}} is the aerodynamic moment slope with respect to pitch rate, and \bar{c} is the mean chord of the section. The first aerodynamic term represents an aerodynamic stiffness effect. The second aerodynamic term represents an aerodynamic damping or phase-lag effect. If the change in aerodynamic angle of attack, {\alpha}, is proportional to the change in \theta, then C_{m_\theta} may also be written as C_{m_\alpha} under this convention.

Therefore, the equation of motion becomes

(145)   \begin{equation*} I' \, \overbigddot{\theta} + \left( C' - \frac{1}{2} \varrho \, V_{\infty} \, \bar{c}^3 \, C_{m_{\dot{\theta}}} \right) \overbigdot{\theta} + \left( K' - \frac{1}{2} \varrho \, V_{\infty}^2 \, \bar{c}^2 \, C_{m_\theta} \right) \theta = 0 \end{equation*}

This equation shows that the aerodynamic terms modify both the effective damping and the effective torsional stiffness of the system.

Analytical Approach

Assume a trial solution of the form

(146)   \begin{equation*} \theta(t) = \theta_0 \, e^{i \omega \, t} \end{equation*}

Differentiating once and twice gives

(147)   \begin{equation*} \overbigdot{\theta}(t) = i \, \omega \, \theta_0 \, e^{i \omega \, t} \quad \mbox{and} \quad \overbigddot{\theta}(t) = -\omega^2 \, \theta_0 \, e^{i \omega \, t} \end{equation*}

Substituting these results into the equation of motion gives the characteristic equation

(148)   \begin{equation*} -I' \, \omega^2 + i \, \omega \left( C' - \frac{1}{2} \varrho \, V_{\infty} \, \bar{c}^3 \, C_{m_{\dot{\theta}}} \right) + \left( K' - \frac{1}{2} \varrho \, V_{\infty}^2 \, \bar{c}^2 \, C_{m_\theta} \right) =0 \end{equation*}

The real and imaginary parts of this equation identify two different aeroelastic instability mechanisms.

Static Torsional Divergence

Static torsional divergence occurs when the effective torsional stiffness becomes zero. In this case, the instability is non-oscillatory, so

(149)   \begin{equation*} \omega = 0 \end{equation*}

The characteristic equation then reduces to

(150)   \begin{equation*} K' - \frac{1}{2} \varrho \, V_D^2 \, \bar{c}^2 \, C_{m_\theta} = 0 \end{equation*}

or

(151)   \begin{equation*} K' = \frac{1}{2} \varrho \, V_D^2 \, \bar{c}^2 \, C_{m_\theta} \end{equation*}

where V_D is the divergence speed. Rearranging gives

(152)   \begin{equation*} V_D = \sqrt{ \frac{2 \, K'} {\varrho \, \bar{c}^2 \, C_{m_\theta}} } \end{equation*}

This result applies when the aerodynamic moment slope is destabilizing, i.e., when it reduces the effective torsional stiffness. If the aerodynamic moment is stabilizing, then this simple divergence condition is not obtained.

Torsional Flutter

Flutter is an oscillatory instability, so the flutter condition must be obtained for

(153)   \begin{equation*} \omega \ne 0 \end{equation*}

The imaginary part of the characteristic equation gives

(154)   \begin{equation*} \omega \left( C' - \frac{1}{2} \varrho \, V_{\infty} \, \bar{c}^3 \, C_{m_{\dot{\theta}}} \right) =0 \end{equation*}

Because \omega \ne 0 for flutter, the term in parentheses must vanish. Therefore,

(155)   \begin{equation*} C' - \frac{1}{2} \varrho \, V_f \, \bar{c}^3 \, C_{m_{\dot{\theta}}} = 0 \end{equation*}

where V_f is the critical airspeed at which torsional flutter will occur. Rearranging gives

(156)   \begin{equation*} V_f = \frac{2 \, C'} {\varrho \, \bar{c}^3 \, C_{m_{\dot{\theta}}}} \end{equation*}

with the understanding that C_{m_{\dot{\theta}}} must have the sign that makes the aerodynamic damping destabilizing.

The corresponding flutter frequency is obtained from the real part of the characteristic equation, i.e.,

(157)   \begin{equation*} -I' \, \omega_f^2 + K' - \frac{1}{2} \varrho \, V_f^2 \, \bar{c}^2 \, C_{m_\theta} =0 \end{equation*}

so

(158)   \begin{equation*} \omega_f^2 = \frac{1}{I'} \left( K' - \frac{1}{2} \varrho \, V_f^2 \, \bar{c}^2 \, C_{m_\theta} \right) \end{equation*}

This exemplar illustrates the difference between two aeroelastic instabilities. Divergence is a static instability associated with loss of effective stiffness, whereas flutter is a dynamic instability associated with loss of effective damping at a nonzero oscillation frequency. Notice from Eq. 152 that increasing torsional stiffness raises the divergence speed. Notice also from Eq. 156 that, in this simplified model, the flutter speed depends on the balance between structural damping and aerodynamic damping. In more complete wing models, bending, torsion, structural mode shapes, and unsteady aerodynamic phase lags are coupled, so the flutter speed is normally obtained from a full eigenvalue analysis.

Time-Marching Solution

Another approach to determining flutter onset is a numerical integration method that marches the equations of motion forward in time. First, a time step \Delta t must be chosen that is small enough to capture the response accurately. Second, initial values for {\theta(0)} and \overbigdot{\theta}(0) must be specified; these values represent disturbances used to excite the aeroelastic system. Physically, such a disturbance could be a gust or a sudden flight control input. During flight testing, mechanical shakers may also be used to excite the structure at selected frequencies to examine potential aeroelastic problems, such as flutter.

For a single torsional degree of freedom, the governing equation per unit span can be written as

(159)   \begin{equation*} I' \, \overbigddot{\theta} + C'_{\rm eff}(V_{\infty}) \, \overbigdot{\theta} + K'_{\rm eff}(V_{\infty}) \, \theta = 0 \end{equation*}

where C'_{\rm eff} and K'_{\rm eff} include both structural and aerodynamic contributions per unit span. Rearranging gives the angular acceleration at the current time step, i.e.,

(160)   \begin{equation*} \overbigddot{\theta}_n = -\frac{C'_{\rm eff}(V_{\infty})}{I'} \, \overbigdot{\theta}_n -\frac{K'_{\rm eff}(V_{\infty})}{I'} \, \theta_n \end{equation*}

Then, a numerical integration method, such as the Euler method, which is only first-order accurate, or a Runge-Kutta method, which is much more accurate but more computationally expensive, can be used to update the solution at each step, e.g.,

(161)   \begin{equation*} \overbigdot{\theta}_{n+1} = \overbigdot{\theta}_n + \overbigddot{\theta}_n \, \Delta t \qquad \mbox{and} \qquad \theta_{n+1} = \theta_n + \overbigdot{\theta}_n \, \Delta t \end{equation*}

The aerodynamic moment at each time step may be computed from the current values of \theta_n, \overbigdot{\theta}_n, and {V_{\infty}}. Unsteady aerodynamic effects can also be incorporated using the indicial method with superposition, as described previously for the numerical solution of the Duhamel integral. The process continues by analyzing the aerodynamic and structural responses until the desired end time or a specified condition, such as flutter onset, is reached.

When the aerodynamic lag states are included, the time-marching problem can also be written in augmented state-space form. For example, for a single torsional structural degree of freedom with indicial aerodynamic states, define the structural state vector as

(162)   \begin{equation*} \mathbf{x}_s = \begin{bmatrix} \theta \\[4pt] \overbigdot{\theta} \end{bmatrix} \end{equation*}

and let the aerodynamic lag states be collected into

(163)   \begin{equation*} \mathbf{x}_a = \begin{bmatrix} X \\[4pt] Y \end{bmatrix} \end{equation*}

where {X} and {Y} represent the wake-memory states associated with the exponential approximation to the indicial response. The complete aeroelastic state vector may then be written as

(164)   \begin{equation*} \mathbf{x} = \begin{bmatrix} \mathbf{x}_s \\[4pt] \mathbf{x}_a \end{bmatrix} = \begin{bmatrix} \theta \\[4pt] \overbigdot{\theta} \\[4pt] X \\[4pt] Y \end{bmatrix} \end{equation*}

The coupled equations can then be written as

(165)   \begin{equation*} \overbigdot{\mathbf{x}} = \mathbf{A}_{\rm ae}(V_{\infty})\,\mathbf{x} \end{equation*}

where \mathbf{A}_{\rm ae} is the aeroelastic state matrix. This matrix contains the structural inertia, stiffness, and damping terms, as well as the aerodynamic lag-state equations and their coupling to the structural motion. For a forced response problem, gusts or control inputs may be added through an input matrix, giving

(166)   \begin{equation*} \overbigdot{\mathbf{x}} = \mathbf{A}_{\rm ae}(V_{\infty})\,\mathbf{x} + \mathbf{B}_{\rm ae}\mathbf{u} \end{equation*}

where \mathbf{u} represents prescribed inputs such as gust velocity or control-surface motion.

This state-space form is useful because the same equations can be used for both time integration and stability analysis. In a time-marching calculation, the augmented state vector is advanced using a numerical integration method. For stability analysis, the eigenvalues of \mathbf{A}_{\rm ae} are computed at each airspeed. Flutter occurs when a complex-conjugate pair of eigenvalues crosses into the right-half plane, i.e., when its real part changes from negative to positive.

Figure 17 shows typical results obtained from an aeroelastic stability calculation. If the response decays sufficiently long after the disturbance, the system is stable at that airspeed. The process can then be repeated for other airspeeds or for variations in other parameters, such as the center-of-gravity location, which affects the torsional inertia about the elastic axis. Depending on the wing design, its aeroelastic response may be well damped, lightly damped, exhibit limit-cycle oscillations, or become dynamically unstable. The process would be repeated at different airspeeds and air-density values to estimate the stability boundaries for the structure or the entire aircraft.

The frequency and damping of two structural modes as a function of airspeed indicate that the likelihood of flutter increases as the structural frequencies coalesce.

Flutter of a Two-Dimensional Airfoil Section

The flutter of a two-dimensional (2D) airfoil section is a more tangible case to study. Consider a two-degree-of-freedom model for a typical 2D airfoil section, as shown in Figure 18. The section can undergo plunge motion, h(t), which represents vertical displacement of the elastic axis, and pitch motion, \theta(t), which represents rotation about the elastic axis.

Two-dimensional section used for flutter analysis.

Let b=c/2 be the semi-chord. The parameter a represents the non-dimensional location of the elastic axis relative to the aerodynamic center, i.e.,

(167)   \begin{equation*} a = \frac{x_{\text{ea}} - x_{\text{ac}}}{b} \end{equation*}

If a = 0, then the elastic axis coincides with the aerodynamic center, which is usually near the 1/4-chord for a thin airfoil in incompressible subsonic flow. If a > 0, then the elastic axis is located aft of the aerodynamic center. If a < 0, then the elastic axis is located forward of the aerodynamic center. The value of a affects the aerodynamic moment arm and the coupling between plunge and pitch motions in the flutter analysis.

The governing equations for the plunge and pitch degrees of freedom may be written as

(168)   \begin{equation*} m \, \overbigddot{h} + S_{\alpha} \, \overbigddot{\theta} + K_h \, h = L' \qquad \mbox{and} \qquad S_{\alpha} \, \overbigddot{h} + I_{\alpha} \, \overbigddot{\theta} + K_{\alpha} \, \theta = M' \end{equation*}

where m is the mass per unit span, S_{\alpha} = m x_{\alpha} is the static moment about the elastic axis, and I_{\alpha} = m r_{\alpha}^2 is the mass moment of inertia about the elastic axis, where r_{\alpha} is the radius of gyration. The quantities K_h and {K_{\alpha}} denote the plunge stiffness and torsional stiffness, respectively. The aerodynamic lift force and pitching moment per unit span are denoted by L' and M'.

Using a quasi-steady thin-airfoil approximation, the aerodynamic lift and pitching moment may be written as

(169)   \begin{equation*} L' = \frac{1}{2} \varrho \, V_{\infty}^2 \, (2b) \, C_l \qquad \mbox{and} \qquad M' = \frac{1}{2} \varrho \, V_{\infty}^2 \, (2b)^2 \, C_m \end{equation*}

where

(170)   \begin{equation*} C_l = 2\pi \left[ \left(a+\frac{1}{2}\right)\theta + \frac{\overbigdot{h}}{V_{\infty}} + \left(a+\frac{1}{2}\right)\frac{b\overbigdot{\theta}}{V_{\infty}} \right] \end{equation*}

and

(171)   \begin{equation*} C_m = -\pi \left[ \left(a^2+\frac{1}{8}\right)\theta + \left(a+\frac{1}{2}\right)\frac{\overbigdot{h}}{V_{\infty}} + \left(a^2+\frac{1}{8}\right)\frac{b\overbigdot{\theta}}{V_{\infty}} \right] \end{equation*}

These expressions include both displacement-dependent and velocity-dependent aerodynamic terms. The displacement-dependent terms modify the effective stiffness of the airfoil section, while the velocity-dependent terms modify the effective damping.

It is useful to write the equations in matrix form. Define

(172)   \begin{equation*} \mathbf{x} = \begin{bmatrix} h \\[4pt] \theta \end{bmatrix} \end{equation*}

The structural mass and stiffness matrices are

(173)   \begin{equation*} \mathbf{M}_s = \begin{bmatrix} m & S_{\alpha} \\[6pt] S_{\alpha} & I_{\alpha} \end{bmatrix} \qquad \mbox{and} \qquad \mathbf{K}_s = \begin{bmatrix} K_h & 0 \\[6pt] 0 & K_{\alpha} \end{bmatrix} \end{equation*}

The aerodynamic forces can then be written as

(174)   \begin{equation*} \begin{bmatrix} L' \\[4pt] M' \end{bmatrix} = q_{\infty} \left( \mathbf{A}_0 \, \mathbf{x} + \frac{1}{V_{\infty}} \mathbf{A}_1 \, \overbigdot{\mathbf{x}} \right) \end{equation*}

where

(175)   \begin{equation*} q_{\infty} = \frac{1}{2}\varrho V_{\infty}^2 \end{equation*}

and

(176)   \begin{equation*} \mathbf{A}_0 = \begin{bmatrix} 0 & 4\pi \, b\left(a+\dfrac{1}{2}\right) \\[10pt] 0 & -4\pi \, b^2\left(a^2+\dfrac{1}{8}\right) \end{bmatrix} \end{equation*}

with

(177)   \begin{equation*} \mathbf{A}_1 = \begin{bmatrix} 4\pi \, b & 4\pi \, b^2\left(a+\dfrac{1}{2}\right) \\[10pt] -4\pi \, b^2\left(a+\dfrac{1}{2}\right) & -4\pi \, b^3\left(a^2+\dfrac{1}{8}\right) \end{bmatrix} \end{equation*}

Therefore, the aeroelastic equations of motion become

(178)   \begin{equation*} \mathbf{M}_s \, \overbigddot{\mathbf{x}} - \frac{q_{\infty}}{V_{\infty}} \mathbf{A}_1 \, \overbigdot{\mathbf{x}} + \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right)\mathbf{x} = \mathbf{0} \end{equation*}

This form explicitly shows how the aerodynamic terms alter both the damping and stiffness of the system.

For flutter, assume a harmonic motion of the form

(179)   \begin{equation*} \mathbf{x}(t)=\mathbf{x}_0 \, e^{i\omega t} \end{equation*}

so that

(180)   \begin{equation*} \overbigdot{\mathbf{x}}= i\omega \mathbf{x} \qquad \mbox{and} \qquad \overbigddot{\mathbf{x}}=-\omega^2 \mathbf{x} \end{equation*}

Substituting into the equations of motion gives

(181)   \begin{equation*} \left[ -\omega^2 \mathbf{M}_s - i\omega \frac{q_{\infty}}{V_{\infty}} \mathbf{A}_1 + \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right) \right]\mathbf{x}_0 = \mathbf{0} \end{equation*}

A non-trivial solution requires that

(182)   \begin{equation*} \det \left[ -\omega^2 \mathbf{M}_s - i\omega \frac{q_{\infty}}{V_{\infty}} \mathbf{A}_1 + \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right) \right] = 0 \end{equation*}

This determinant is the flutter equation for the simplified two-degree-of-freedom airfoil section. It must generally be solved numerically for each value of airspeed. As {V_{\infty}} is increased, the roots of this equation change. Flutter occurs when one of the roots reaches zero damping, so that the corresponding oscillatory motion no longer decays with time. The associated airspeed is the flutter speed, V_f, and the corresponding oscillation frequency is the flutter frequency, \omega_f.

This formulation is still quasi-steady, so it is best interpreted as an introductory model. More complete flutter calculations replace the quasi-steady aerodynamic matrices with unsteady aerodynamic influence matrices, often involving Theodorsen’s function, indicial-response approximations, panel methods, or CFD-based aerodynamic models. Nevertheless, this two-degree-of-freedom airfoil section illustrates the essential mechanism of flutter: the coupling of plunge, pitch, inertia, stiffness, and aerodynamic phase effects.

Check Your Understanding #5 – Estimating divergence and flutter speeds

Consider a two-degree-of-freedom airfoil section with plunge displacement h(t) and pitch angle \theta(t) about the elastic axis. The section has the following structural matrices:

    \[ \mathbf{M}_s = \begin{bmatrix} 10 & -0.5 \\[4pt] -0.5 & 1.0 \end{bmatrix}, \qquad \mathbf{K}_s = \begin{bmatrix} 10{,}000 & 0 \\[4pt] 0 & 500 \end{bmatrix} \]

and structural damping matrix

    \[ \mathbf{C}_s = \begin{bmatrix} 300 & 0 \\[4pt] 0 & 20 \end{bmatrix} \]

The aerodynamic stiffness and damping-influence matrices for this simplified quasi-steady model are

    \[ \mathbf{A}_0 = \begin{bmatrix} 0 & 0.70 \\[4pt] 0 & 0.35 \end{bmatrix}, \qquad \mathbf{A}_1 = \begin{bmatrix} 10 & 0 \\[4pt] 0 & 1 \end{bmatrix} \]

Assume air density \varrho = 1.225~\text{kg m}^{-3}. Determine the static divergence speed and the flutter speed predicted by this simplified model.

Show solution/hide solution.

The equations of motion are written in the form

    \[ \mathbf{M}_s \, \overbigddot{\mathbf{x}} + \left( \mathbf{C}_s - \frac{q_{\infty}}{V_{\infty}}\mathbf{A}_1 \right) \overbigdot{\mathbf{x}} + \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right) \mathbf{x} = \mathbf{0} \]

where

    \[ \mathbf{x} = \begin{bmatrix} h \\[4pt] \theta \end{bmatrix} \qquad \mbox{and} \qquad q_{\infty} = \frac{1}{2}\varrho V_{\infty}^2 \]

Static divergence is obtained by neglecting the inertia and damping terms, which gives

    \[ \det \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right) = 0 \]

Therefore,

    \[ \mathbf{K}_s - q_{\infty}\mathbf{A}_0 = \begin{bmatrix} 10{,}000 & -0.70q_{\infty} \\[4pt] 0 & 500-0.35q_{\infty} \end{bmatrix} \]

and the determinant is

    \[ 10{,}000\left(500-0.35q_{\infty}\right)=0 \]

Hence,

    \[ q_D = \frac{500}{0.35} = 1{,}428.6~\text{N m}^{-2} \]

and the corresponding divergence speed is

    \[ V_D = \sqrt{\frac{2q_D}{\varrho}} = \sqrt{\frac{2(1{,}428.6)}{1.225}} = 48.3~\text{m s}^{-1} \]

For flutter, assume a solution of the form

    \[ \mathbf{x}(t)=\mathbf{x}_0 e^{\lambda t} \]

so that

    \[ \overbigdot{\mathbf{x}}=\lambda \mathbf{x} \qquad \mbox{and} \qquad \overbigddot{\mathbf{x}}=\lambda^2 \mathbf{x} \]

Substitution gives the flutter determinant

    \[ \det \left[ \lambda^2\mathbf{M}_s + \lambda \left( \mathbf{C}_s - \frac{q_{\infty}}{V_{\infty}}\mathbf{A}_1 \right) + \left( \mathbf{K}_s - q_{\infty}\mathbf{A}_0 \right) \right] = 0 \]

For each value of {V_{\infty}}, this equation gives four roots for \lambda. The system is stable when all roots have negative real parts. Flutter occurs when one complex-conjugate pair reaches

    \[ \Re(\lambda)=0 \]

at a nonzero oscillation frequency.

Solving the determinant as {V_{\infty}} is varied gives the first zero-damping crossing at

    \[ V_f = 32.5~\text{m s}^{-1} \]

At this speed,

    \[ q_f = \frac{1}{2}(1.225)(32.5)^2 = 647.8~\text{N m}^{-2} \]

and the critical roots are approximately

    \[ \lambda = \pm i\,16.7~\text{rad s}^{-1} \]

Therefore, the flutter speed and flutter frequency are

    \[ V_f = 32.5~\text{m s}^{-1} \qquad \mbox{and} \qquad \omega_f = 16.7~\text{rad s}^{-1} \]

or

    \[ f_f = \frac{\omega_f}{2\pi} = 2.66~\text{Hz} \]

This example shows that flutter and divergence are different aeroelastic instabilities. The divergence speed is obtained from the static stiffness determinant, whereas the flutter speed is obtained from the dynamic eigenvalue problem. For this set of numerical values, flutter occurs first because

    \[ V_f = 32.5~\text{m s}^{-1} < V_D = 48.3~\text{m s}^{-1} \]

so the section would encounter flutter before reaching its static divergence speed.

Why use quasi-steady aerodynamics in initial flutter analysis?

Quasi-steady aerodynamics is useful in initial flutter analysis because it yields a relatively simple aeroelastic model and can provide rapid analytical insight into the roles of stiffness, inertia, and aerodynamic damping. It is most appropriate when the reduced frequency is small, so that wake-history effects and phase lags in the aerodynamic response are weak. It should be regarded as a first-cut or screening approximation, not as a general flutter-prediction method. More complete analyses use unsteady aerodynamic models, such as Theodorsen’s theory for two-dimensional incompressible airfoil sections, doublet-lattice methods for lifting surfaces, or CFD-based methods when compressibility, transonic effects, separation, or complex geometry must be represented.

Flutter Speeds Using Theodorsen’s Function

The quasi-steady two-degree-of-freedom airfoil-section model developed above is useful for illustrating the basic flutter mechanism, but it does not fully represent the wake history and frequency-dependent phase lag of the aerodynamic loads. A more complete two-dimensional incompressible analysis uses Theodorsen’s function to represent the circulatory part of the unsteady aerodynamic response.

The key difference from the quasi-steady model is that the circulatory aerodynamic terms are no longer real constants. They depend on the complex Theodorsen function C(k), where

(183)   \begin{equation*} k=\frac{\omega b}{V_{\infty}} \end{equation*}

and b=c/2. Therefore, the aerodynamic stiffness and damping contributions depend on the oscillation frequency as well as on the airspeed. The noncirculatory apparent-mass terms must also be retained separately because they are not multiplied by C(k).

The resulting flutter problem is a coupled eigenvalue problem. In symbolic form, it may be written as

(184)   \begin{equation*} \left[ -\omega^2\mathbf{M} + i\omega\mathbf{C}_{\rm eff}(V_{\infty},k) + \mathbf{K}_{\rm eff}(V_{\infty},k) \right]\mathbf{x}_0 = \mathbf{0} \end{equation*}

where \mathbf{M} is the structural mass matrix, while \mathbf{C}_{\rm eff} and \mathbf{K}_{\rm eff} contain both structural and unsteady aerodynamic contributions. The aerodynamic contributions depend on C(k), and hence on the reduced frequency.

A non-trivial solution requires

(185)   \begin{equation*} \det \left[ -\omega^2\mathbf{M} + i\omega\mathbf{C}_{\rm eff}(V_{\infty},k) + \mathbf{K}_{\rm eff}(V_{\infty},k) \right] = 0 \end{equation*}

with

(186)   \begin{equation*} k=\frac{\omega b}{V_{\infty}} \end{equation*}

No general closed-form flutter speed follows from this formulation because V_f, \omega_f, and k_f are coupled through

(187)   \begin{equation*} k_f=\frac{\omega_f b}{V_f} \end{equation*}

In practice, the airspeed is varied, the corresponding complex eigenvalues are computed, and the flutter speed is identified as the speed at which one oscillatory mode first reaches zero damping.

For low-speed, two-dimensional incompressible problems, Theodorsen’s function provides an instructive analytical aerodynamic model. For finite wings, compressible flow, transonic flow, separated flow, or complex aircraft geometry, higher-fidelity aerodynamic models such as doublet-lattice methods, experimentally identified aerodynamic influence coefficients, Euler methods, or CFD-based methods are normally required.

Flutter Using FEM/CFD Coupling

Aeroelastic analyses may be conducted using time-marching methods, frequency-domain eigenvalue methods, or iterative coupling between aerodynamic and structural models. An iterative coupling process will typically proceed along these lines:

  1. Define the geometry and grids for FEM and CFD. They will differ because the grids required to address aerodynamics have different requirements from those for the structural shape.
  2. Apply the material properties and boundary conditions in the FEM. Using isotropic materials, such as aluminum, will yield different properties than composites.
  3. Set up the CFD with the specified flow conditions, or use an alternative aerodynamic model, e.g., a panel method.
  4. Compute the aerodynamic forces, F_a, from the selected aerodynamic model.
  5. Update the FEM model with the aerodynamic forces F_a.
  6. Iterate between CFD and FEM to capture aeroelastic interactions, i.e., couple the aerodynamics and structural dynamics in the form

    (188)   \begin{equation*} M \, \overbigddot{q} + (C + B) \, \overbigdot{q} + (K + A) \, q = 0 \end{equation*}

  7. Repeat the FEM analysis to obtain the structural response of the deformed structure.
  8. Conduct CFD simulations of the deformed structure to obtain new aerodynamic loads.
  9. Exchange data between FEM and CFD to formalize the coupled analysis.
  10. Analyze displacements, stresses, and aerodynamic forces.
  11. Evaluate the results against the stability criteria for flutter or divergence.

By integrating CFD and FEM, engineers can accurately predict and analyze aeroelastic phenomena, thereby ensuring the safety and performance of aerospace structures. For example, this process has been applied to large aircraft such as the Boeing 747, as shown in Figure 19. These results provide valuable information on the stiffness of airframe components, helping to prevent aeroelastic and flutter issues before the first flight. However, flight testing is essential to validate these calculations and ensure the aircraft is flutter-free across its operational flight envelope.

A model created by ZONA Technology shows aircraft deformations because of flutter.
A finite-element flutter model of a Boeing 747 depicts the aircraft’s deformations induced by flutter. (Credit: ZONA Technology)

Flutter Occurrences in Practice

In practice, aircraft structures can exhibit coupled responses between different “modes,” e.g., between wing torsion and bending, between the engine mount and the wing, or between the wing and a control surface. Two fatal crashes of the Lockheed Electra were attributed to a phenomenon known as “pylon whirl flutter,” in which propeller aerodynamic forces, gyroscopic moments, nacelle motion, engine-mount flexibility, and wing structural dynamics coupled to produce an unstable oscillation. Extensive structural modifications were made to the Electra’s design, including changes to the wings and the engine mounts to increase their stiffness.

During its first flight tests, the Boeing Dash 80 (predecessor to the Boeing 707) experienced aileron flutter, after which modifications were made to the control system. This incident underscored the importance of flutter testing for jet airliners and led to improvements in control-surface design and testing protocols. The Boeing 747 experienced unexpected flutter in its horizontal stabilizers during flight testing, and the Boeing 747-8 experienced wingtip flutter before it was resolved.[13]

The interaction among the relevant structural modes must be accounted for in an aircraft to capture the overall coupled dynamic behavior of the structure. This requires a structural dynamics model coupled to an appropriate aerodynamic model, which may range from linear unsteady aerodynamic methods, such as panel or doublet-lattice methods, to higher-fidelity CFD when nonlinear, transonic, or separated-flow effects are important. The process involves solving the coupled structural and aerodynamic equations and determining the eigenvalues that represent the system’s natural frequencies and damping ratios, as previously outlined. Figure 20 illustrates the information that can be extracted from this type of aeroelastic analysis: frequency and damping as functions of airspeed or dynamic pressure.

The frequency and damping of two structural modes as a function of airspeed, showing that flutter is likely to occur near frequency coalescence.
The frequency and damping of two structural modes as functions of airspeed indicate that flutter is likely to occur near frequency coalescence.

The frequency and damping of two structural modes as a function of airspeed can indicate that the likelihood of flutter increases as modal frequencies approach one another. The undamped zero airspeed frequencies are distinct at low speeds, and the system remains stable. As the airspeed increases, the aerodynamic forces acting on the structure also increase in magnitude. These forces alter the structure’s frequencies by introducing effective aerodynamic stiffness and damping, which, in some cases, may cause the modal frequencies to converge, a phenomenon known as frequency coalescence. Frequency coalescence is often associated with classical flutter, although it is not a universal flutter criterion.

Flutter arises when the net structural-aerodynamic damping of an aeroelastic mode becomes negative. In this condition, the unsteady aerodynamic forces transfer energy into the coupled structural motion at a rate exceeding the energy dissipated by structural and aerodynamic damping. The resulting flutter frequency is an eigenfrequency of the coupled aeroelastic system, not necessarily one of the zero-airspeed structural natural frequencies. If the net energy input over an oscillation cycle is positive, the oscillations grow exponentially, leading to flutter.

Flight Control Reversal

Control reversal occurs when the deflection of a control surface, such as an aileron, rudder, or elevator, produces an aircraft response opposite to the pilot’s intended input as a result of adverse aerodynamic or structural interactions. This behavior typically occurs at higher airspeeds, when aerodynamic forces on the control surface may induce excessive structural deformation, particularly in the wing or tail section. Suppose a pilot applies aileron inputs to roll the aircraft. For example, aerodynamic forces on the wing may cause it to twist, thereby increasing the effective angle of attack rather than decreasing it. This leads to an unintended rolling motion in the opposite direction, as shown in Figure 21.

A wing section without sufficient torsional stiffness can exhibit control reversal, where the opposite effect is obtained from control inputs.

This undesirable effect is particularly pronounced in aircraft with long, slender wings, such as sailplanes, or those with wings that have insufficient torsional stiffness. In an attempt to minimize structural weight, wing skins are sometimes too thin to provide the necessary torsional stiffness. Historically, roll or aileron reversal was a significant issue in high-performance fighter airplanes during WWII and in early jet airplanes. Some aircraft, such as the Supermarine Spitfire, exhibited aileron reversal at high speeds, thereby limiting maneuverability in combat. Another contributing factor is the shifting of the aerodynamic center as speed and Mach number increase. If the aircraft is not adequately designed to counteract these forces, control effectiveness can degrade as speed increases, eventually leading to reversal. This issue was common in early high-speed aircraft before engineers developed techniques to counteract it.

To mitigate control reversal, engineers may employ several strategies. Increasing the torsional stiffness of the aircraft’s structure, particularly in the wing and empennage, is usually the most direct way to resist excessive structural twisting. Other approaches include changing the size or spanwise placement of the control surface, using aerodynamic balance or geared tabs to reduce hinge moments, limiting control deflection at high dynamic pressure, or using spoilers for roll control. Mass balancing is important for suppressing control-surface flutter and buzzing, but it does not by itself prevent static control reversal. On modern high-speed aircraft, powered control systems, such as hydraulic or fly-by-wire actuators, can mitigate aeroelastic problems by ensuring that pilot inputs are consistently applied to minimize structural flexing.

Dynamic Stall & Stall Flutter

Stall flutter is an aeroelastic phenomenon that occurs when flow separation induces unsteady aerodynamic forces that couple with structural dynamics, leading to oscillatory instability. It is relevant in various aerospace and engineering applications, where predicting and mitigating its effects are essential for ensuring structural integrity and aerodynamic performance. Understanding stall flutter requires nonlinear aerodynamic modeling and experimental validation to develop practical mitigation steps and design improvements.

Physics of Dynamic Stall

Under unsteady conditions, airfoils and wings behave differently from those in steady flow. In particular, their stall characteristics differ significantly, a phenomenon known as dynamic stall. This phenomenon has attracted considerable research interest because of its unsteady aerodynamic effects, including the shedding of a leading-edge vortex, as illustrated in the simulation in Figure 22. The onset of a dynamic stall can lead to another type of aeroelastic behavior called stall flutter, which can occur on helicopter blades.

A CFD animation of a dynamic stall on an oscillating airfoil. (With permission of Dr. George Barakos.)

Vortex shedding increases lift and drag, resulting in powerful nose-down (negative) pitching moments induced by the aft-moving center of pressure, as illustrated in Figure 23, based on measurements and flow visualization. Dynamic stall is characterized by higher values of maximum lift, drag, and pitching moment, as well as hysteresis effects that can lead to flutter. It is particularly relevant in the design and analysis of helicopter rotors, wind turbine blades, and specific aircraft configurations.

Dynamic stall characteristics differ significantly from those under steady conditions.

A defining feature of dynamic stall is the presence of strong hysteresis and phase lag between the airfoil motion and the resulting aerodynamic loads. Unlike steady aerodynamics, in which lift and moment depend only on the instantaneous angle of attack, unsteady forces during dynamic stall depend on the prior history of flow separation and reattachment. Consequently, the lift and pitching moment do not remain in phase with the airfoil motion and generally lag behind it because of delayed separation, vortex formation, and reattachment.

This phase lag is especially pronounced in the pitching moment because of the formation and downstream convection of a leading-edge vortex and the associated aft movement of the center of pressure. During portions of an oscillation cycle, the aerodynamic moment can act in the same sense as the airfoil’s angular velocity rather than opposing it. In energy terms, unsteady aerodynamics can perform positive net work on the airfoil over part of a cycle rather than dissipating energy.

This history-dependent behavior provides the essential aerodynamic mechanism by which dynamic stall can reduce or even reverse aerodynamic damping. When such unsteady separated-flow forces act on a flexible lifting surface, they can couple with the structural dynamics, triggering an aeroelastic instability known as stall flutter.

Engineers and researchers study dynamic stall to understand its effects better and develop strategies to mitigate its adverse impacts on the performance of aerospace systems. In particular, helicopter rotor blades often experience dynamic stall during higher-speed forward flight or during maneuvers, and its onset effectively limits the helicopter’s operational flight envelope. Wind turbine blades may also experience dynamic stall during sudden changes in wind conditions, leading to fluctuations in power output and high blade loads that can result in alarmingly high vibration levels. Aircraft wings can also experience dynamic stall during aggressive maneuvers, a phenomenon that must be accounted for when establishing the maneuvering flight envelope for military combat airplanes.

Leishman-Beddoes Dynamic-Stall Model

A widely used engineering model for dynamic stall is the Leishman-Beddoes model.[14] It is a semi-empirical model that represents the main unsteady aerodynamic processes observed during dynamic stall, including attached-flow unsteady response, trailing-edge separation, leading-edge vortex formation, vortex convection, and reattachment. The model was originally developed for practical rotorcraft and airfoil applications, where fully resolved unsteady separated-flow calculations were too expensive for routine aeroelastic analysis.

The Leishman-Beddoes model may be implemented either as time-marching recurrence relations or in state-space form. The state-space formulation is especially useful for aeroelastic stability analysis because the aerodynamic states can be appended directly to the structural equations of motion.[15]

The important point is that the Leishman-Beddoes model is not simply a corrected lift curve. It is a dynamic model with internal aerodynamic states. These states represent the lagged response of the attached flow, the delay in the onset of flow separation, the growth and convection of the dynamic-stall vortex, and the flow recovery after vortex shedding. In this sense, it extends the same general idea used in indicial-response modeling, i.e., the aerodynamic loads depend not only on the instantaneous angle of attack but also on the airfoil’s previous motion history.

In time-marching calculations, the model is often implemented using recurrence relations. At each time step, the effective angle of attack and the attached-flow response are updated, separation-point delays are computed, vortex-induced lift and pitching moment increments are added when appropriate, and the normal-force, chord-force, and pitching-moment coefficients are assembled from these components, which can be written as

(189)   \begin{equation*} \mathbf{z}_{n+1} = \mathcal{F} \left( \mathbf{z}_n,\alpha_n,\overbigdot{\alpha}_n,M_{\infty},\Delta t \right) \end{equation*}

and

(190)   \begin{equation*} \mathbf{C}_{a,n} = \mathcal{G} \left( \mathbf{z}_n,\alpha_n,\overbigdot{\alpha}_n,M_{\infty} \right) \end{equation*}

where \mathbf{z}_n denotes the aerodynamic memory variables at the current time step and \mathbf{C}_{a,n} represents the resulting aerodynamic coefficients, such as normal force, chord force, and pitching moment. This recurrence form is convenient for time-domain simulations of rotor blades, wind-turbine blades, or airfoils undergoing large-amplitude motion.

The same model can also be cast in state-space form. In that case, the aerodynamic memory variables are collected into a state vector and advanced through first-order evolution equations, e.g.,

(191)   \begin{equation*} \overbigdot{\mathbf{z}} = \mathbf{f} \left( \mathbf{z},\alpha,\overbigdot{\alpha},M_{\infty} \right) \end{equation*}

with output equations of the form

(192)   \begin{equation*} \mathbf{C}_a = \mathbf{g} \left( \mathbf{z},\alpha,\overbigdot{\alpha},M_{\infty} \right) \end{equation*}

This form is especially useful in aeroelastic analysis because the aerodynamic states can be appended to the structural states, just as with the linear indicial-response states described earlier. The resulting coupled system can then be integrated forward in time, linearized locally for stability analysis, or used to predict the onset of stall flutter and limit-cycle oscillations

The Leishman-Beddoes model reproduces the hysteresis in lift, and pitching moment that occurs during dynamic stall. Figure 24 compares measured data with model predictions and static airfoil data for two oscillatory pitching cases. The loops in the pitching-moment coefficient are particularly important for aeroelasticity because their orientation indicates whether the unsteady aerodynamic moment extracts energy from the motion or feeds energy into it. Portions of the loop may correspond to positive aerodynamic damping, while others may correspond to negative aerodynamic damping. If the net aerodynamic work over a cycle becomes destabilizing and exceeds the available structural damping, stall flutter or a limit-cycle oscillation may occur.

Predictions of the dynamic stall airloads using the Leishman-Beddoes model.

Therefore, the Leishman-Beddoes model bridges the linear unsteady aerodynamic models discussed earlier and the nonlinear separated-flow behavior associated with dynamic stall. Theodorsen’s theory, Wagner’s function, and related indicial models describe attached-flow unsteady aerodynamics, whereas the Leishman-Beddoes model adds semi-empirical state variables for flow separation, vortex shedding, and reattachment. This capability is why it has been widely used in rotorcraft, wind-turbine, and other aeroelastic calculations involving dynamic stall.

Stall Flutter

Stall flutter is a nonlinear aeroelastic phenomenon that occurs when an airfoil or structure experiences flow separation, such as dynamic stall, leading to oscillatory instability. This separation produces unsteady aerodynamic forces that can destabilize the structural response. Unlike classical flutter, which occurs in a linear aerodynamic regime before stall, stall flutter happens post-stall, when the flow has already separated from the surface. Because it depends on unsteady, nonlinear aerodynamics, stall flutter is more complex to analyze and predict.

The primary cause of stall flutter is flow separation, which occurs when the angle of attack exceeds the critical stall limit. Dynamic stall further intensifies this phenomenon, as lags in periodic flow separation and reattachment reduce or even reverse aerodynamic damping, as shown in Figure 25 for the pitching moment. If a structure has limited structural stiffness and/or damping, it can lead to stall flutter.

Reduced aerodynamic damping near stall can lead to stall flutter.

From a dynamical standpoint, stall flutter can be interpreted as a loss of net structural damping. Consider, for simplicity, a single generalized structural degree of freedom q(t) governed by

(193)   \begin{equation*} m \, \overbigddot{q} + c_s \, \overbigdot{q} + k \, q = Q_a(q,\overbigdot{q},\ldots) \end{equation*}

where m is the generalized mass, c_s is the structural damping coefficient, k is the structural stiffness, and Q_a represents the unsteady aerodynamic generalized force. Although Q_a is inherently nonlinear in stalled flow, it may be locally linearized about a mean post-stall condition or a small oscillatory motion as

(194)   \begin{equation*} Q_a \approx -\, c_a \,  \overbigdot{q} - k_a \,  q + \cdots \end{equation*}

where c_a and k_a are effective aerodynamic damping and stiffness coefficients, respectively. The resulting equation of motion becomes

(195)   \begin{equation*} m \,  \ddot{q} + \underbrace{\left(c_s + c_a\right)}_{c_{\mathrm{eff}}}\overbigdot{q} \;+\; \underbrace{\left(k + k_a\right)}_{k_{\mathrm{eff}}} q \;=\; 0 \end{equation*}

In attached flow, c_a is typically stabilizing, so that the effective damping c_{\mathrm{eff}} remains positive. Near and beyond stall, however, phase lags associated with flow separation and reattachment can cause the aerodynamic contribution c_a to become destabilizing, reducing or even reversing the net damping. Stall flutter corresponds to the condition

(196)   \begin{equation*} c_{\mathrm{eff}} = c_s + c_a < 0 \end{equation*}

at which point small perturbations grow rapidly until nonlinear aerodynamic effects limit the motion, establishing a finite-amplitude oscillation (a limit cycle).

Stall flutter can be an issue for wings and control surfaces, such as flaps and ailerons, at high angles of attack. Helicopter rotor blades have been known to encounter stall flutter in the retreating blade region, where local angles of attack can become high during forward flight. Stall flutter can also affect compressor and turbine blades in jet engines, where unsteady flow interactions are crucial in their performance. Civil engineering structures, such as bridges and tall buildings, may exhibit vortex-induced oscillations that resemble stall flutter.

Mathematically, stall flutter is challenging to model because of its nonlinearity. Traditional linear aeroelastic models, such as Theodorsen’s theory or the linear indicial response method, are insufficient because they assume attached flow. Instead, nonlinear aerodynamic models are required to capture the complex flow physics. Semi-empirical models, such as the Leishman-Beddoes dynamic-stall model, provide approximations of the unsteady aerodynamic forces encountered in stall flutter. Coupled fluid-structure interaction simulations are employed to investigate the impact of separated flow on structural vibrations. Mitigating stall flutter involves several approaches, including modifying the airfoil’s geometry to delay flow separation and reduce vortex shedding. Increasing structural stiffness and damping can also help dissipate energy and suppress the structural response.

Buffeting & Buzzing

While buffeting, buzzing, and stall flutter all involve unsteady aerodynamic forces acting on flexible structures, they differ fundamentally in their underlying mechanisms. Buffeting is a forced structural response to aerodynamic disturbances, whereas buzzing and stall flutter are self-excited aeroelastic instabilities. Buzzing is a self-excited, high-frequency oscillation of control surfaces, often because of aeroelastic feedback and insufficient damping.

Buffeting

Buffeting is a random, low-frequency, forced vibration caused by unsteady aerodynamic forces acting on a structure. It typically occurs when a lifting surface, such as an aircraft wing or tailplane, is subjected to turbulence or wake disturbances originating from another part of the airplane. One of the most common causes of buffeting is flow separation and vortex shedding behind a stalled airfoil. When a surface encounters separated flow, turbulent eddies form and impinge on downstream airframe structures, generating fluctuating forces, as shown in the schematic in Figure 26.

Under some conditions, an aircraft’s horizontal stabilizer may experience buffeting when operating within the wing’s wake.

For example, an aircraft’s horizontal stabilizer may experience buffeting when positioned in the wake of the wing or fuselage, as shown in this video of MD-11 airliner stall tests. This behavior may occur at higher angles of attack, such as during takeoff or landing, especially when flaps are deployed. Similarly, shock waves interacting with boundary layers in transonic or supersonic flight can induce separated flow regions that produce turbulence and cause severe buffeting on downstream airframe structures.

Buffeting is a crucial consideration in airplane design because it can increase aerodynamic drag, lead to control difficulties, and cause structural fatigue. Engineers analyze buffeting using wind tunnel testing, CFD simulations, and flight testing, and develop mitigation strategies based on these results. Techniques to reduce buffeting include optimizing the shape and size of aerodynamic surfaces, adding vortex generators to reduce or control flow separation, and designing control systems to minimize buffeting response.

Buzzing

Buzzing is a high-frequency, self-excited aeroelastic behavior that occurs primarily in control surfaces such as ailerons, rudders, and elevators. It is caused by the interaction between the aerodynamic forces acting on a control surface and the structural dynamics of the hinge mechanism. Unlike buffeting, which is an externally forced vibration, buzzing is a self-excited oscillation resulting from unsteady aerodynamic loading on a lightly damped control surface. A common cause of buzzing is aeroelastic feedback from hinged surfaces, as shown in Figure 27.

Buzzing can result from shock-induced separation and reattachment over a control surface in transonic or supersonic flight.

If a control surface is not sufficiently stiff or damped, minor disturbances in the airflow can cause rapid surface oscillations that are then amplified by aerodynamic forces. In transonic or supersonic flight, buzzing can also result from shock-induced separation and reattachment over a control surface. This creates fluctuating pressure loads that drive oscillations in the strength and location of high-frequency shock waves. Engineers can mitigate buzzing by adding stiffness, mass-balancing weights, or dampers to suppress rapid, undesirable control-surface movements.

For further clarity, the table below compares buffeting, buzzing, dynamic stall, stall flutter, and classical flutter with respect to excitation mechanism, flow regime, and aeroelastic coupling.

Phenomenon Forced or Self-Excited Flow Regime Physical Mechanism Typical Examples
Buffeting Externally forced. Separated or turbulent flow. Turbulent eddies and wake fluctuations impose random pressure loads. Horizontal tail in wing wake; transonic buffet.
Buzzing Self-excited. Often transonic or supersonic. Shock-induced separation and hinge-moment feedback drive control-surface oscillations. Ailerons or elevators in transonic flight.
Dynamic Stall Motion-driven (aerodynamic). Separated, unsteady flow. Leading-edge vortex formation, hysteresis, and phase lag in loads. Helicopter retreating blades; wind-turbine blades.
Stall Flutter Self-excited. Post-stall, separated flow. Negative aerodynamic damping from separated-flow phase lag. Retreating helicopter blades; stalled control surfaces.
Classical Flutter Self-excited. Attached flow. Phase lag between motion and lift produces negative damping. Wings and control surfaces at high speed.

Summary & Closure

Aeroelasticity concerns the coupling between aerodynamic forces, elastic deformation, and structural dynamics. These interactions can produce static instabilities, such as divergence and control reversal, as well as dynamic instabilities, such as classical flutter, whirl flutter, buzzing, and stall flutter. The common thread is that aerodynamic loading and structural motion cannot always be treated separately; under some conditions, they couple in ways that reduce stiffness, reduce damping, or feed energy into the motion of the structure.

A central theme in aeroelastic analysis is the role of unsteady aerodynamics. Theodorsen’s and Sears’s functions describe harmonic unsteady responses in the frequency domain, while Wagner’s and Küssner’s functions describe corresponding indicial responses in the time domain. These classical incompressible theories clarify wake memory, phase lag, amplitude attenuation, and the distinction between circulatory and noncirculatory loading. However, they are baseline models; compressibility, separated flow, dynamic stall, and nonlinear structural effects may require semi-empirical models, state-space formulations, or higher-fidelity aerodynamic methods.

Modern aeroelastic analysis uses a hierarchy of models, from simple quasi-steady and two-degree-of-freedom section models to finite-element structural models coupled with panel methods, doublet-lattice methods, Euler methods, or Reynolds-averaged Navier-Stokes CFD. Wind-tunnel testing, ground vibration testing, and flight flutter testing remain essential for validation. The practical goal is to ensure that aircraft, rotor systems, and other aerospace vehicles remain free from destructive aeroelastic behavior throughout their operating envelopes while meeting structural, aerodynamic, performance, and certification requirements.

5-Question Self-Assessment Quickquiz

For Further Thought or Discussion

  • What are the key differences between static and dynamic aeroelasticity? Can you provide examples of each?
  • Why is divergence considered a catastrophic failure mode, and how can it be prevented in modern aircraft design?
  • What role might composite materials play in controlling aeroelastic effects in modern aircraft design?
  • Identify a historical aircraft accident attributable to aeroelastic effects. What lessons were learned?
  • How did the introduction of swept-wing designs impact the aeroelasticity of jet aircraft?
  • How might controlled aeroelastic effects be intentionally used to enhance aircraft performance rather than being just a constraint?
  • How might aeroelasticity impact the design of wind turbines? Hint: Do not limit your discussion to the turbine blades alone.

Other Useful Online Resources

Visit the following websites to learn more about the phenomenon of flutter:


  1. Named after Arthur Roderick Collar, who worked extensively on aeroelasticity.
  2. At least initially, but this issue was soon rectified as flutter became better understood.
  3. The inclusion of the zero "0" in F0VMS is deliberate.
  4. And under all the same assumptions as the classic thin airfoil theory.
  5. . The terms "noncirculatory," "apparent mass," or "added mass" are often used synonymously.
  6. Theodorsen, T., "General Theory for Aerodynamic Instability and the Mechanism of Flutter," NACA TR 496, 1935.
  7. Notice that this case does not represent an oscillating airfoil because the pitch-rate terms are not included.
  8. von Kármán, T., & Sears, W. R., "Airfoil Theory for Non-Uniform Motion," Journal of the Aeronautical Sciences, 5(5), 379–390.
  9. Wagner, H., “Über die Entstehung des dynamischen Auftriebes von Tragflügeln,” Zeitschrift für Angewandte Mathematik und Mechanik, Vol. 5, No. 1, 1925, pp. 17–35.
  10. Küssner, H. G., “Zusammenfassender Bericht über den instationären Auftrieb von Flügeln,” Luftfahrtforschung, Vol. 13, No. 12, 1936, pp. 410–424.
  11. Leishman, J. G., “Validation of Approximate Indicial Aerodynamic Functions for Two-Dimensional Subsonic Flow,” Journal of Aircraft, Vol. 25, No. 10, 1988, pp. 914–922. https://doi.org/10.2514/3.45680
  12. Ashley, H., and Zartarian, G., “Piston Theory: A New Aerodynamic Tool for the Aeroelastician,” Journal of the Aeronautical Sciences, Vol. 23, No. 12, 1956, pp. 1109–1118. https://doi.org/10.2514/8.3740
  13. The design was modified by adding additional structural reinforcements to ensure flutter-free operation.
  14. Leishman, J. G., and Beddoes, T. S., “A Semi-Empirical Model for Dynamic Stall,” Journal of the American Helicopter Society, Vol. 34, No. 3, 1989, pp. 3–17. https://doi.org/10.4050/JAHS.34.3.3
  15. Leishman, J. G., and Crouse, G. L., Jr., “State-Space Model for Unsteady Airfoil Behavior and Dynamic Stall,” AIAA Paper 89-0022, 1989. https://doi.org/10.2514/6.1989-22

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