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5. Classical Linear Theory Computational Aerodynamics 5.1 An Introduction Computational methods based on the linear potential flow theory described in Chapter 4 have been used to perform a great deal of good aerodynamic design. While some people believe that these methods are outdated, we believe they still have a valuable place in computational aerodynamics. This chapter describes two related linear theory approaches – panel methods and vortex lattice methods - that play important roles in aerodynamics; both approaches rely on the linear versions of the potential flow equation. For the potential flow assumption to be useful for aerodynamics calculations the primary requirement is that viscous effects are small, meaning that the flow is attached. Also, the flow must be either completely subsonic, or completely supersonic. If the flow contains regions of both subsonic and supersonic flow. then it is termed transonic, and requires a higher fidelity (nonlinear) flowfield model for a physically correct theoretical simulation. Note that supersonic velocities can occur locally at surprisingly low freestream Mach numbers, so great care must be taken to ensure that the flow is not locally supersonic. For airfoils at very high lift coefficients the peak 7/6/2022 5-1

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5. Classical Linear TheoryComputational Aerodynamics

5.1 An Introduction

Computational methods based on the linear potential flow theory described in Chapter 4 have

been used to perform a great deal of good aerodynamic design. While some people believe that

these methods are outdated, we believe they still have a valuable place in computational

aerodynamics. This chapter describes two related linear theory approaches – panel methods and

vortex lattice methods - that play important roles in aerodynamics; both approaches rely on the

linear versions of the potential flow equation. For the potential flow assumption to be useful for

aerodynamics calculations the primary requirement is that viscous effects are small, meaning that

the flow is attached. Also, the flow must be either completely subsonic, or completely

supersonic. If the flow contains regions of both subsonic and supersonic flow. then it is termed

transonic, and requires a higher fidelity (nonlinear) flowfield model for a physically correct

theoretical simulation. Note that supersonic velocities can occur locally at surprisingly low

freestream Mach numbers, so great care must be taken to ensure that the flow is not locally

supersonic. For airfoils at very high lift coefficients the peak velocities around the leading edge

can become supersonic at freestream Mach numbers as low as 0.20 ~ 0.25. However, if the local

flow is at a low speed everywhere it can be assumed incompressible (M ≤ 0.4, say), and

Laplace's Equation is essentially an exact representation of the inviscid flow. For higher subsonic

Mach numbers with small disturbances to the freestream flow, the Prandtl-Glauert Equation can

be used. The Prandtl-Glauert Equation can be converted intoto Laplace's Equation by a simple

transformation, which means that incompressible results can be transformed into subsonic

compressible results quite easily.1 This provides the basis for estimating the initial effects of

compressibility on the flowfield, i.e., “linearized” subsonic flow, and the flowfield can be found

by the solution of a single linear partial differential equation. Not only is the mathematical

problem much simpler than any of the other equations that can be used to model the flowfield,

but since the problem is linear, a large body of mathematical theory is available.

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The Prandtl-Glauert Equation can also be used to describe supersonic flows. In that case the

mathematical type of the equation is hyperbolic, as described in Chapter 3. Recall the important

distinction between the two cases:

subsonic flow: elliptic PDE, each point in the flowfield influences every other point,

supersonic flow: hyperbolic PDE, discontinuities can exist, “zone of influence” solution dependency.

Although there are supersonic as well as subsonic panel methods, vortex lattice methods are only

subsonic. We will discuss the similarities and differences between these methods in this chapter.

See Erickson2 for a good discussion of linear supersonic aerodynamic methods.

5.2 Panel Methods

Although we saw in the last chapter how simple shapes like circular cylinders can be

modeled with combinations of singularities that are solutions of Laplace’s Equation, completely

arbitrary shapes cannot be modeled exactly with singularities placed on the axis, and the

streamline of an arbitrary body determined by specifying the strengths of the singularities.

Instead, we need to use another approach to distributing singularities to model the flowfield.

In this chapter we consider incompressible flow only. One of the key features of Laplace’s

Equation is the property that allows the equation governing the flowfield to be converted from a

three-dimensional problem throughout the field (a PDE) to a two-dimensional problem for

finding the potential variation on the surface (an integral equation). The flowfield solution is then

found using this property by distributing “singularities” of unknown strength over discretized

portions of the surface: panels. Hence the flowfield solution is found by representing the surface

by a number of panels, and solving a linear set of algebraic equations to determine the unknown

strengths of the singularities;* Fig. 1 illustrates the idea. Figure 1a shows a panel representation

of an airplane, and Figure 1b shows how singularities may be distributed over the panels. The

flexibility and relative economy of the panel methods is so important in practice that the methods

continue to be widely used despite the availability of more exact methods. An entry into the

panel method literature is available through two reviews by Hess,3,4 the survey by

Erickson,Error: Reference source not found and the book by Katz and Plotkin.5

* The singularities are distributed across the panel. They are not specified at a point. However, the boundary conditions are usually satisfied at a specific location.

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a) a 7000 panel representation of a transport aircraft with flaps deflected.Error: Referencesource not found

arrows indicate constant distribution of the singularity across the panel

control point on each panel,satisfying the no-flow-through condition

smooth surface represented by straight line “panels”

b) local surface cut showing distribution of singularities on a panel.

Figure 5.1. Representation of an airplane by a panel model.

The derivation of the integral equation for the potential solution of Laplace’s equation is

given in Section 5.2.1. Details are outlined for one specific approach to solving the integral

equation in Section 5.2.2. For clarity and simplicity of the algebra, the analysis will use the two-

dimensional case to illustrate the methods. Details are available in Moran6 and Cebeci.7 Both

books contain FORTRAN programs that can be run on many computer systems. This results in

two ironic aspects of the presentation:

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• The algebraic forms of the singularities are different between 2D and 3D, due to 3D relief.

• The power of panel methods arises in three-dimensional applications.

Finally, examples of applications to aerodynamic analysis are presented.

5.2.1 The Integral Equation for the Potential

Potential theory is a well developed (old) and elegant mathematical theory, devoted to the

solution of Laplace’s Equation (as discussed in Chap. 4):

∇2φ = 0 . (5.1)

There are several ways to view the solution of this equation. The one most familiar to

aerodynamicists is the notion of “singularities”. These are algebraic functions that satisfy

Laplace’s equation, and can be combined to construct flowfields, as presented in Chapter 4.

Since the equation is linear, superposition of solutions can be used. The most familiar

singularities are the point source(sink), doublet and vortex. In classical examples the singularities

are located inside the body. Unfortunately, as noted above, an arbitrary body shape cannot be

created using singularities placed inside the body. A more sophisticated approach has to be used

to determine the potential flow over arbitrary shapes, and mathematicians have spent a great deal

of time developing this theory. We will draw on a few selected results to help understand the

development of panel methods. Initially, we are interested in the specification of the boundary

conditions. Consider the situation illustrated in Fig. 5.2.

The flow pattern is uniquely determined by giving either:

φ on Σ+κ {Dirichlet Problem: Design} (5.2)or

∂φ/∂n on Σ+κ {Neuman Problem: Analysis} . (5.3)

Potential flow theory states that you cannot specify both arbitrarily, but can have a mixed

boundary condition, aφ+b∂φ/∂n on Σ+κ . The Neumann Problem is identified as “analysis”

above because it naturally corresponds to the problem where the flow through the surface is

specified (usually zero). The Dirichlet Problem is identified as “design” because it tends to

correspond to the aerodynamic case where a surface pressure distribution is specified and the

body shape corresponding to the pressure distribution is sought. Because of the wide range of

problem formulations available in linear theory, some analysis procedures appear to be Dirichlet

problems, but Eq. (5-3) must still be used.

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Figure 5.2 also shows a wake behind the body, where the value of the potential can jump.

This is required to allow the flowfield to produce a value for the lift on the body, and will be

discussed further below.

Σ

Solid Body

κWake

Δφ

Figure 5.2. Boundaries for flowfield analysis.

Some other key properties of potential flow theory:

• If either or ∂φ/∂n is zero everywhere on Σ + κ then = 0 at all interior points.

• cannot have a maximum or minimum at any interior point. Its maximum value can only occur on the surface boundary, and therefore the minimum pressure (and maximum velocity) occurs on the surface.

We need to obtain the equation for the potential in a form suitable for use in panel method calculations. This section follows the presentation given by Karamcheti8 on pages 344-348 and Katz and PlotkinError: Reference source not found on pages 44-48. An equivalent analysis is given by MoranError: Reference source not found in his Section 8.1. The objective is to obtain an expression for the potential anywhere in the flowfield in terms of values on the surface bounding the flowfield. Starting with the Gauss Divergence Theorem, which relates a volume integral and a surface integral, (given previously in Chap. 3 as Eqn. 3.8)

A⋅ndΣ“∫∫ = ∇⋅AdV

v∫∫∫ (5.4)

we follow the classical derivation and consider the interior problem as shown in Fig. 5.3.

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x

y

z

R0

S0n

Figure 5.3. Nomenclature for integral equation derivation.

To start the derivation introduce the vector function of two scalars:

A =ωgradχ −χgradω . (5.5)

Substitute this function into the Gauss Divergence Theorem, Eq. (5.4), to obtain:

div ωgradχ −χgradω( )dV

R∫∫∫ = ωgradχ −χgradω( )⋅n dΣ

Σ“∫∫ . . (5.6)

Now use the vector identity: ∇⋅σ F= σ ∇⋅F + F ⋅∇σ to simplify the left hand side of Eq. (5.6). Recalling that ∇⋅A = divA , write the integrand of the left hand side of Eq. (5.6) as:

div ωgradχ −χgradω( )=∇⋅ω∇χ( )−∇⋅ χ∇ω( )=ω∇⋅∇χ +∇χ ⋅∇ω −χ∇⋅∇ω −∇ω ⋅∇χ

=ω∇2χ −χ∇2ω(5.7)

Substituting the result of Eq. (5.7) for the integrand in the left hand side of Eq. (5.6), we obtain:

ω∇2χ − χ∇2ω( )dV

R∫∫∫ = ωgradχ − χ gradω( ) ⋅n dS

S“∫∫ , (5.8)

or equivalently (recalling that gradχ ⋅n =∂χ / ∂ n ),

ω∇2χ − χ∇2ω( )dV

R∫∫∫ = ω

∂χ∂ n

− χ∂ω∂ n

⎛⎝⎜

⎞⎠⎟ dS

S“∫∫ . (5.9)

Either statement is known as Green’s theorem of the second form.

Now define ω = 1/r and χ = , where is a harmonic function (a function that satisfies

Laplace’s equation). The 1/r term is a source singularity in three dimensions. This makes our

analysis three-dimensional. In two dimensions the form of the source singularity is ln r, and a

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two-dimensional analysis starts by defining ω = ln r. Now rewrite Eq. (5.8) using the definitions

of ω and χ given at the first of this paragraph and switching sides,

1r∇φ−φ∇

1r

⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥Σ0

“∫∫ ⋅ndΣ=1r∇2φ−φ∇2 1

r⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥R0

∫∫∫ dV . (5.10)

R0 is the region enclosed by the surface S0. Recognize that on the right hand side the first term,

∇2φ , is equal to zero from Eq, (5.1) so that Eq. (5.10) becomes

1r∇φ−φ∇

1r

⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥Σ0

“∫∫ ⋅ndΣ=− φ∇2 1r

⎛⎝⎜

⎞⎠⎟

R0∫∫∫ dV . (5.11)

If a point P is external to S0, then ∇2 1

r⎛⎝⎜⎞⎠⎟ = 0 everywhere since 1/r is a source, and thus satisfies

Laplace’s Equation. This leaves the right hand side of Eq. (5.11) equal to zero, with the

following result:

1r∇φ−φ∇

1r

⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥Σ0

“∫∫ ⋅ndΣ=0 . (5.12)

However, we have included the origin in our region S0 as defined above. If P is inside S0, then

∇2 1r

⎛⎝⎜⎞⎠⎟→ ∞ at r = 0. Therefore, we exclude this point by defining a new region which excludes

the origin by drawing a sphere of radius around r = 0, and applying (5.12) to the region

between and S0:

1r∇φ−φ∇

1r

⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥⋅ndΣ

Σ0“∫∫

arbitrary rgion1 24 4 4 4 34 4 4 4

−1r∂φ∂r

+φr2

⎛⎝⎜

⎞⎠⎟

“∫∫ dΣ

σphr1 24 44 34 4 4

=0(5.13)

or:

1r∂φ∂r

+φr2

⎛⎝⎜

⎞⎠⎟

“∫∫ dΣ=

1r∇φ−φ∇

1r

⎛⎝⎜

⎞⎠⎟

⎡⎣⎢

⎤⎦⎥⋅ndΣ

Σ0“∫∫ . (5.14)

Consider the first integral on the left hand side of Eq. (5.14). Let 0, where (as 0)

we take constant (∂φ/∂ r == 0 ), assuming that is well-behaved and using the mean value

theorem. Then we need to evaluate

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dSr2

“∫∫

over the surface of the sphere where = r. Recall that for a sphere the elemental area is (see

Hildebrand,9 for an excellent review of spherical coordinates and vector analysis):

dS =r2σinθ dθdφ (5.15)

where we define the angles in Fig. 5.4. Do not confuse the classical notation for the spherical

coordinate angles with the potential function. The spherical coordinate will disappear as soon

as we evaluate the integral.

x

y

zP

φ

θ

Figure 5.4. Spherical coordinate system nomenclature.

Substituting for dS in the integral above, we get:

sinθ dθdφ

“∫∫ .

Integrating from θ = 0 to p, and from 0 to 2p, we get:

sinθ dθdφθ=0

θ=p

∫φ=0

φ=2p

∫ =4p . (5.16)

The final result for the first integral in Eq. (5.14) is:

1r∂φ∂r

+φr2

⎛⎝⎜

⎞⎠⎟

“∫∫ dΣ=4pφ . (5.17)

Replacing this integral by its value from Eq. (5.17) in Eq. (5.14), we can write the expression

for the potential at any point P as (where the origin can be placed anywhere inside S0):

φ p( ) =

14π

1r∇φ −φ∇ 1

r⎛⎝⎜⎞⎠⎟

⎡⎣⎢

⎤⎦⎥s0

“∫∫ ⋅ndS (5.18)

and the value of at any point p is now known as a function of and ∂φ/∂n on the boundary.

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We used the interior region to allow the origin to be written at point p. This equation can be

extended to the solution for for the region exterior to R0. Apply the results to the region

between the surface SB of the body and an arbitrary surface Σ enclosing SB and then let Σ go to

infinity. The integrals over Σ go to ∞ as Σ goes to infinity. Thus potential flow theory is used to

obtain the important result that the potential at any point p' in the flowfield outside the body can

be expressed as:

φ ′p( ) = φ∞ −

14π

1r∇φ −φ∇ 1

r⎛⎝⎜⎞⎠⎟

⎡⎣⎢

⎤⎦⎥SB

“∫∫ ⋅ndS . (5.19)

Here the unit normal n is now considered to be pointing outward and the area can include not

only solid surfaces but also wakes. Equation 5.19 can also be written using the dot product of the

normal and the gradient as:

φ ′p( ) = φ∞ −

14π

1r

∂φ∂n

−φ∂∂n

1r

⎛⎝⎜⎞⎠⎟

⎡⎣⎢

⎤⎦⎥SB

“∫∫ dS . (5.20)

The 1/r in Eq. (5.19) can be interpreted as a source of strength ∂φ / ∂n , and the ∇(1/r) term

in Eq. (5.19) as a doublet of strength . Both of these functions play the role of Green’s functions

in the mathematical theory. Therefore, we can find the potential as a function of a distribution of

sources and doublets over the surface. The integral in Eq. (5.20) is normally broken up into body

and wake pieces. The wake is generally considered to be infinitely thin. Therefore, only doublets

are used to represent the wakes.

Now consider the potential to be given by the superposition of two different known

functions, the first and second terms in the integral, Eq. (5-20). These can be taken to be the

distribution of the source and doublet strengths, σ and , respectively. Thus Eq (5.20) can be

written in the form usually seen in the literature,

φ ′p( ) = φ∞ − 1

4πσ

1r

− μ∂∂n

1r

⎛⎝⎜⎞⎠⎟

⎡⎣⎢

⎤⎦⎥SB

“∫∫ dS . (5.21)

The problem is to find the values of the unknown source and doublet strengths σ and for a

specific geometry and given freestream, .

What just happened? We replaced the requirement to find the solution over the entire

flowfield (a three-dimensional problem) with the problem of finding the solution for the

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singularity distribution over a surface (a two-dimensional problem). In addition, we now have an

integral equation to solve for the unknown surface singularity distributions instead of a partial

differential equation. The problem is linear, allowing us to use superposition to construct

solutions. We also have the freedom to pick whether to represent the solution as a distribution of

sources or doublets distributed over the surface. In practice it’s been found best to use a

combination of sources and doublets. The theory can also be extended to include other

singularities.

At one time the change from a three-dimensional to a two-dimensional problem was

considered significant. However, the total information content is the same computationally. This

shows up as a dense “2D” matrix compared to a large, but sparse “3D” matrix. As computational

methods for sparse matrix solutions evolved, the problems became nearly equivalent. The

advantage in using the panel methods arises because there is no need to define a grid throughout

the flowfield.

This is the theory that justifies panel methods, i.e. that we can represent the surface by panels

with distributions of singularities placed on them. Special precautions must be taken when

applying the theory described here. Care should be used to ensure that the region SB is in fact

completely closed. In addition, care must be taken to ensure that the outward normal is properly

defined.

Furthermore, in general, the interior problem cannot be ignored. Surface distributions of

sources and doublets affect the interior region as well as the exterior. In some methods the

interior problem is implicitly satisfied. In other methods the interior problem requires explicit

attention. The need to consider this subtlety arose when advanced panel methods were

developed. The problem is not well posed unless the interior problem is considered, and

numerical solutions failed when this aspect of the problem was not addressed. References Error:

Reference source not found and Error: Reference source not found provide further discussion.

When the exterior and interior problems are formulated properly the boundary value problem

is properly posed. Additional discussions are available in the books by Ashley and Landahl10 and

Curle and Davis.11

We implement the ideas give above by:

a) approximating the surface by a series of line segmentsb) placing distributions of sources and vortices or doublets on each panel.

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There are many ways to tackle the problem (and many codes). Possible differences in

approaches to the implementation include the use of:

- various singularities- various distributions of the singularity strength over each panel- panel geometry (panels don’t have to be flat).

Recall that superposition allows us to construct the solution by adding separate contributions

[Watch out! You have to get all of them. Sometimes this can be a problem]. Thus we write the

potential as the sum of several contributions. Figure 5.5 provides an example of a panel

representation of an airplane being used to develop the aerodynamic characteristics of a

morphing airplane for a flight simulation. The surface is colored to represent the pressure

distribution on the plane predicted by the panel model. The wakes are shown, and a more precise

illustration of a panel method representation is given in Section 5.2.4.

Figure 5.5. Panel model representation of an airplane.12 Wakes not shown.

An example of the implementation of a panel method is carried out in Section 5.2.2 in two

dimensions. To do this, we write down the two-dimensional version of Eq. 5.21. In addition, we

use a vortex singularity in place of the doublet singularity (Ref. Error: Reference source not

found and Error: Reference source not found provide details on this change). The resulting

expression for the potential is:

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φ = φ∞

uniform onset flow=V∞x cosα +V∞ysinα

{ +q(s)2π

ln r

q is the 2Dsource strength

1 24 34−

γ (s)2π

θ

this is a vortex singularityof strength γ (s)

1 2 3

⎢⎢⎢⎢

⎥⎥⎥⎥

S

⎮⎮⎮⎮⎮⎮⎮

ds (5.22)

and θ = tan-1(y/x). Equation (5.22) shows contributions from various components of the

flowfield, but the relation is still exact. No small disturbance assumption has been made.

5.2.2 An Example: The Classic Hess and Smith Method

A.M.O. Smith at Douglas Aircraft directed an incredibly productive aerodynamics development

group in the late ’50s through the early ’70s. In this section we describe the implementation of

the theory given above that originated in his group.* Our derivation follows Moran’s

descriptionError: Reference source not found of the Hess and Smith method quite closely. The

approach is to i) break up the surface into straight line segments, ii) assume the source strength

distribution is constant over each line segment (panel) but has a different value for each panel,

and iii) distribute a vortex singularity distribution over each panel, but with the vortex strength

constant and equal over each panel.

Think of the constant vortices as adding up to the circulation to satisfy the Kutta condition.

The sources are required to satisfy flow tangency on the surface (thickness).

Figure 5.6 illustrates the representation of a smooth surface by a series of line segments. The

numbering system starts at the lower surface trailing edge and proceeds forward, around the

leading surface and aft to the upper surface trailing edge. N+1 points define N panels. Note that

other implementations may use other numbering schemes.

Figure 5.6. Representation of a smooth airfoil with straight line segments.

* In the AIAA book, Applied Computational Aerodynamics, A.M.O. Smith contributed the first chapter, an account of the initial development of panel methods.

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The potential relation given above in Eq. (5.22) can then be evaluated by breaking the

integral up into segments along each panel:

φ=V∞ x cosα + ysinα( ) + q(s)2π

ln r − γ2π

θ⎡⎣⎢

⎤⎦⎥panel j

∫j=1

N

∑ dS (5.23)

with q(s) taken to be constant on each panel, allowing us to write q(s) = qi, i = 1, ... N. Here we

need to find N values of qi and one value of g.

Use Figure 5.7 to define the nomenclature on each panel. Let the ith panel be the one

between the ith and i+1th nodes, and let the ith panel’s inclination to the x axis be θ. Under these

assumptions the sin and cos of θ are given by:

sinθi =yi+1 −yi

li, χoσθi =

xi+1 −xili

(5.24)

and the normal and tangential unit vectors are:

ni =−σinθii+ χoσθiφti = χoσθii+σinθiφ

. (5.25)

li

i

i + 1

x

θi

a) baσiχ no nχlatur b) unitvχtororintation

i in ti + 1

θi

i x

φ

i

Figure 5.7. Nomenclature for local coordinate systems.

We will find the unknowns by satisfying the flow tangency condition on each panel at one

specific control point (also known as a collocation point) and requiring the solution to satisfy a

Kutta condition. The control point will be picked to be at the mid-point of each panel, as shown

in Fig. 5.8.

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•X

control point

panel

smooth shape

x

y

Figure 5.8. Local panel nomenclature.

Thus the coordinates of the midpoint of the control point are given by:

xi =xi + xi+1

2, yi =

yi + yi+12

(5.26)

and the velocity components at the control point xi , yi are ui =u(xi, yi), vi =v(xi, yi).

The flow tangency boundary condition is given by V⋅n =0 , and is written using the relations given here as (in the original coordinate system):

uii +viφ( )⋅−σinθii+ χoσθiφ( )=0

or−ui sinθ i + vi cosθ i = 0, for each i, i = 1, ..., N . (5.27)

The remaining relation is found from the Kutta condition. This condition states that the flow

must leave the trailing edge smoothly. Many different numerical approaches have been adopted

to satisfy this condition. In practice this implies that at the trailing edge the pressures on the

upper and lower surface are equal. Here the Kutta condition is satisfied approximately by

equating velocity components tangential to the panels adjacent to the trailing edge on the upper

and lower surface. Because of the importance of the Kutta condition in determining the flow, the

solution is extremely sensitive to the flow details at the trailing edge. Since the assumption is

made that the velocities are equal on the top and bottom panels at the trailing edge we need to

understand that we must make sure that the last panels on the top and bottom are small and of

equal length, otherwise we have an inconsistent approximation. Accuracy will deteriorate rapidly

if the trailing edge panels are not the same length. The specific numerical formula is developed

using the nomenclature for the trailing edge shown in Fig. 5.9. In two-dimensions, and especially

for a single airfoil, the Kutta condition is sufficient to handle the wake, and we don’t have to

address the wake explicitly in the formulation. This is not the case in three dimensions.

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••N+1

N

12

N

1

t

t

Figure 5.9. Trailing edge panel nomenclature.

Equating the magnitude of the tangential velocities on the upper and lower surface:

ut1=utN . (5.28)

and taking the difference in direction of the tangential unit vectors into account this is written as

V⋅t1 =−V ⋅t N . (5.29)

Carrying out the operation in the original coordinate system we get the relation:

u1i +v1φ( )⋅χoσθ1i+σinθ1φ( )=− uNi+vNφ( )⋅χoσθNi+σinθNφ( )

which is expanded to obtain the final relation:

u1 cosθ1 +v1σinθ1 =−uN χoσθN +vN σinθN (5.30)

The expression for the potential in terms of the singularities on each panel and the boundary

conditions derived above for the flow tangency and Kutta condition are used to construct a

system of linear algebraic equations for the strengths of the sources and the vortex. The steps

required are summarized below.

Steps to determine the solution:

1. Find the algebraic equations defining the “influence” coefficients. These are the relations connecting the velocities induced by the singularity distribution of unit strength over a panel at a control point. Each control point will have an influence coefficient for each of the panels on the surface, and are a function of the geometry.

2. Write down the velocities, ui, vi, in terms of contributions from all the singularities. This includes qi, g from each panel and the influence coefficients.

To generate the system of algebraic equations:

3. Write down flow tangency conditions in terms of the velocities (N eqn’s., N+1 unknowns).

4. Write down the Kutta condition equation to get the N+1 equation.

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5. Solve the resulting linear algebraic system of equations for the unknown qi and g.

6. Given qi and g, write down the equations for uti, the tangential velocity at each panel control point.

7. Determine the pressure distribution from Bernoulli’s equation using the tangential velocity on each panel.

The details are easily carried out, but the algebra gets tedious.

Program PANEL

In this section we illustrate the results of the procedure outlined above. Program PANEL is an

exact implementation of the analysis described above, and is essentially the program given by

Moran.Error: Reference source not found Other panel method programs are available in the

textbooks by Cebeci,Error: Reference source not found Houghton and Carpenter,13 and Kuethe

and Chow.14 Two other similar programs are available. A MATLAB program, Pablo, written at

KTH in Sweden is available on the web,15 as well as the program by Professor Drela at MIT,

XFOIL.16 Moran’s program includes a subroutine to generate the ordinates for the NACA 4-digit

and 5-digit airfoils (see Appendix A for a description of these airfoil sections). The main

drawback is the requirement for a trailing edge thickness that is exactly zero. To accommodate

this restriction, the ordinates generated internally have been altered slightly from the official

ordinates. The extension of the program to handle arbitrary airfoils is an exercise. The freestream

velocity in PANEL is assumed to be unity, since the inviscid solution in coefficient form is

independent of scale.

PANEL’s node points are distributed employing the widely used cosine spacing function.

The equation for this spacing is given by defining the points on the thickness distribution to be

placed at:

xi

c=12

1−χoσi−1( )pN−1( )

⎧⎨⎩

⎫⎬⎭

⎡⎣⎢

⎤⎦⎥ i =1,..., N . (5-31)

These locations are then altered when camber is added (see Eqns. A-1 and A-2 in App. A).

This approach is used to provide a smoothly varying distribution of panel node points that

concentrate points around the leading and trailing edges.

An example of the accuracy of program PANEL is illustrated in Fig. 5.10, where the results

from PANEL for the NACA 4412 airfoil are compared with results obtained from an exact

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conformal mapping of the airfoil (Conformal mapping methods were described in Chapter 4.

Conformal transformations can also be used to generate meshes of points for use in CFD

methods). The agreement is nearly perfect.

Numerical studies need to be conducted to determine how many panels are required to obtain

accurate results. Both forces and moments and pressure distributions should be examined. You

can select the number of panels used to represent the surface. How many should you use? Most

computational programs provide the user with freedom to decide how detailed (expensive - in

dollars or time) the calculations should be. One of the first things the user should do is evaluate

how detailed the calculation should be to obtain the level of accuracy desired. In the PANEL

code your control is through the number of panels used.

1.00

0.50

0.00

-0.50

-1.00

-1.50

-2.00

-2.50

-0.2 0.0 0.2 0.4 0.6 0.8 1.0 1.2

PANELExact Conformal Mapping

Cp

x/c

Figure 5.10. Comparison of results from program PANEL with an essentially exact mapping solution for the NACA 4412 airfoil at 6° angle-of-attack.

We check the sensitivity of the solution to the number of panels by comparing force and

moment results and pressure distributions with increasing numbers of panels. This is done using

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two different methods. Figures 5.11 and 5.12 present the change of drag and lift, respectively, by

varying the number of panels. For PANEL, which uses an inviscid incompressible flowfield

model, the drag should be exactly zero. The drag coefficient found by integrating the pressures

over the airfoil is an indication of the error in the numerical scheme. The drag obtained using a

surface (or “nearfield”) pressure integration is a numerically sensitive calculation, and is a strict

test of the method. The figures show the drag going to zero, and the lift becoming constant as the

number of panels increase. In this style of presentation it is hard to see exactly how quickly the

solution is converging to a fixed value.

The results given in Figs. 5.11 and 5.12 indicate that 60-80 panels (30 upper, 30 lower for

example) should be enough panels. Note that the lift coefficient is presented in an extremely

expanded scale, and the drag coefficient presented in Fig. 5.13 also uses an expanded scale.

Because drag is typically a small number, it is frequently described in drag counts, where 1 drag

count is a CD of 0.0001.

To estimate the limit for an infinitely large number of panels the results can be plotted as a

function of the reciprocal of the number of panels. Thus the limit result occurs as 1/n goes to

zero. Figures 5.13, 5.14, and 5.15 present the results in this manner for the case given above, and

with the pitching moment included for examination in the analysis.

0.000

0.002

0.004

0.006

0.008

0.010

0.012

0 20 40 60 80 100 120

CD

No. of Panels

NACA 0012 Airfoil, a = 8°

Figure 5.11. Change of drag with number of panels.

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0.950

0.955

0.960

0.965

0.970

0.975

0.980

0 20 40 60 80 100 120

CL

No. of Panels

NACA 0012 Airfoil, a = 8°

Figure 5.12. Change of lift with number of panels.

0.000

0.002

0.004

0.006

0.008

0.010

0.012

0 0.01 0.02 0.03 0.04 0.05 0.06

CD

1/n

NACA 0012 Airfoil, a = 8°

Figure 5.13. Change of drag with the inverse of the number of panels.

The results given in Figures 5.13 through 5.15 show that the program PANEL produces

results that are relatively insensitive to the number of panels once fifty or sixty panels are used,

and by extrapolating to 1/n = 0 an estimate of the limiting value can be obtained.

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0.950

0.955

0.960

0.965

0.970

0.975

0.980

0 0.01 0.02 0.03 0.04 0.05 0.06

CL

1/n

NACA 0012 Airfoil, a = 8°

Figure 5.14. Change of lift with the inverse of the number of panels.

-0.250

-0.248

-0.246

-0.244

-0.242

-0.240

0 0.01 0.02 0.03 0.04 0.05 0.06

Cm

1/n

NACA 0012 Airfoil, a = 8°

Figure 5.15. Change of pitching moment with the inverse of the number of panels.

In addition to forces and moments, the sensitivity of the pressure distributions to changes in

panel density must also be investigated: pressure distributions are shown in Figs. 5.16 and 5.17.

The 20 and 60 panel results are given in Fig. 5.16. In this case it appears that the pressure

distribution is well defined with 60 panels. This is confirmed in Figure 5-17, which demonstrates

that it is almost impossible to identify the differences between the 60 and 100 panel cases. This

type of study should (in fact must) be conducted when using computational aerodynamics

methods.

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-5.00

-4.00

-3.00

-2.00

-1.00

0.00

1.000.0 0.2 0.4 0.6 0.8 1.0

20 panels60 panels

CP

x/c

NACA 0012 airfoil, a = 8°

Figure 5.16. Pressure distribution from progrm PANEL, comparing results using 20 and 60 panels.

-5.00

-4.00

-3.00

-2.00

-1.00

0.00

1.000.0 0.2 0.4 0.6 0.8 1.0

60 panels100 panels

CP

x/c

NACA 0012 airfoil, a = 8°

Figure 5.17. Pressure distribution from program PANEL, comparing results using 60 and 100 panels.

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Having examined the convergence of the mathematical solution, we investigate the

agreement with experimental data. Figure 5.18 compares the lift coefficients from the inviscid

solutions obtained from PANEL with experimental data from Abbott and von Doenhof.17

Agreement is good at low angles of attack, where the flow is fully attached. The agreement

deteriorates as the angle of attack increases, and viscous effects start to show up as a reduction in

lift with increasing angle of attack, until, finally, the airfoil stalls. The inviscid solutions from

PANEL cannot capture this part of the flow physics. The different stall character between the

two airfoils arises due to different flow separation locations on the different airfoils. The

cambered airfoil separates at the trailing edge first. Stall occurs gradually as the separation point

moves forward on the airfoil with increasing incidence. The uncambered airfoil stalls due to a

sudden separation at the leading edge. An examination of the difference in pressure distributions

can be made to see why this might be the case.

-0.50

0.00

0.50

1.00

1.50

2.00

2.50

-5.0° 0.0° 5.0° 10.0° 15.0° 20.0° 25.0°

CL, NACA 0012 - PANEL

CL, NACA 0012 - exp. data

CL, NACA 4412 - PANEL

CL, NACA 4412 - exp. data

CL

a

Figure 5.18. Comparison of PANEL lift predictions with experimental data (Ref.

Error: Reference source not found).

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The pitching moment characteristics are also important. Figure 5.19 provides a comparison

of the PANEL pitching moment predictions (taken about the quarter chord point) with

experimental data. In this case the calculations indicate that the computed location of the

aerodynamic center, dCm / dCL =0 , is not exactly at the quarter chord, although the

experimental data is very close to this value. The uncambered NACA 0012 data shows nearly

zero pitching moment until flow separation starts to occur. The cambered airfoil shows a

significant nose down pitching moment, Cm0, and a trend with angle of attack due to viscous

effects that is exactly opposite the inviscid prediction. This occurs because the separation is

moving forward from the trailing edge of the airfoil and the load over the aft portion of the airfoil

does not increase as fast as the forward loading. This leads to a nose up pitching moment until

eventually the separation causes the airfoil to stall, resulting in a nose down pitching moment.

-0.30

-0.25

-0.20

-0.15

-0.10

-0.05

-0.00

0.05

0.10

-5.0 0.0 5.0 10.0 15.0 20.0 25.0

Cm, NACA 0012 - PANELCm, NACA 4412 - PANELCm, NACA 0012 - exp. dataCm, NACA 4412 - exp. data

Cm

a

χ/4

Figure 5.19 Comparison of PANEL moment predictions with experimental data, (Ref.

Error: Reference source not found).

We do not compare the drag prediction from PANEL with experimental data. For two-

dimensional incompressible inviscid flow the drag is theoretically zero. In the actual case, drag

arises from skin friction effects, further additional form drag due to the small change of pressure

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on the body due to the boundary layer (which primarily prevents full pressure recovery at the

trailing edge), and drag due to increasing viscous effects with increasing angle of attack. A well

designed airfoil will have a drag value very nearly equal to the skin friction and nearly invariant

with incidence until the maximum lift coefficient is approached.

In addition to the force and moment comparisons, we need to compare the pressure

distributions predicted with PANEL to experimental data. Figure 5.20 provides one example.

The NACA 4412 experimental pressure distribution is compared with PANEL predictions. In

general the agreement is very good. The primary area of disagreement is at the trailing edge.

Here viscous effects act to prevent the recovery of the experimental pressure to the levels

predicted by the inviscid solution. The disagreement on the lower surface is a little surprising,

and suggests that the angle of attack from the experiment may not be precise.

-1.2

-0.8

-0.4

-0.0

0.4

0.8

1.20.0 0.2 0.4 0.6 0.8 1.0 1.2

a = 1.875°M = 0.191Re = 720,000transition free

Cp

x/c

NACA 4412 airfoil

Predictions from PANEL

data from NACA R-646

Figure 5.20. Comparison of pressure distribution from PANEL with data,18

Panel methods often have trouble with accuracy at the trailing edge of airfoils with cusped

trailing edges, when the included angle at the trailing edge is zero. Figure 5.21 shows the

predictions of program PANEL compared with an exact mapping solution (a FLO3619 run at low

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Mach number) for two cases. Figure 5.21a is for a case with a small trailing edge angle: the

NACA 651-012, while Fig. 5.21b is for the more standard 6A version of the airfoil. The

corresponding airfoil shapes are shown Fig. 5.22. The “loop” in the pressure distribution in Fig.

5.21a is an indication of a problem with the method.

-0.60

-0.40

-0.20

0.00

0.20

0.40

0.600.6 0.7 0.8 0.9 1.0 1.1

Cp

X/C

NACA 651-012

PANELFLO36

a = 8.8°

a. 6-σriσ, χuσpd TE

-0.60

-0.40

-0.20

0.00

0.20

0.40

0.600.6 0.7 0.8 0.9 1.0 1.1

Cp

X/C

NACA 651A012

FLO36PANEL

a = 8.8°

b. 6A-σriσ, init TE angl

Figure 5.21. PANEL Performance near the airfoil trailing edge

-0.05

0.00

0.05

0.70 0.80 0.90 1.00

y/c

x/c

NACA 65(1)-012

NACA 65A012

Figure 5.22. Comparison at the trailing edge of 6- and 6A-series airfoil geometries.

This case demonstrates a situation where this particular panel method is not accurate. Is this

a practical consideration? Yes and no. The 6-series airfoils were theoretically derived by

specifying a pressure distribution and determining the required shape. The small trailing edge

angles (less than half those of the 4-digit series), cusped shape, and the unobtainable zero

thickness specified at the trailing edge resulted in objections from the aircraft industry. These

airfoils were very difficult to manufacture and use on operational aircraft. Subsequently, the 6A-

series airfoils were introduced to remedy the problem. These airfoils had larger trailing edge

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angles (approximately the same as the 4-digit series), and were made up of nearly straight (or

flat) surfaces over the last 20% of the airfoil. Most applications of 6-series airfoils today actually

use the modified 6A-series thickness distribution. This is an area where the user should check the

performance of a particular panel method.

5.2.3 Geometry and Design

Effects of Shape Changes on Pressure Distributions: So far we have been discussing

aerodynamics from an analysis point of view. To develop an understanding of the typical effects

of adding local modifications to the airfoil surface, Exercise 5 provides a framework for the

reader to carry out an investigation to help understand what happens when changes are made to

the airfoil shape. It is also worthwhile to investigate the very powerful effects that small

deflections of the trailing edge can produce. This reveals the power of the Kutta condition, and

alerts the aerodynamicist to the basis for the importance of viscous effects at the trailing edge.

Making ad hoc changes to an airfoil shape is extremely educational when implemented in an

interactive computer program, where the aerodynamicist can easily make shape changes and see

the effect on the pressure distribution immediately. An outstanding code that does this has been

created by Ilan Kroo and is known as PANDA. 20 Strictly speaking, PANDA is not a panel

method, but it is an accurate subsonic airfoil prediction method.

Shape for a specified pressure distribution: There is another way that aerodynamicists view

the design problem. Although the local modification approach described above is useful to make

minor changes in airfoil pressure distributions, often the aerodynamic designer wants to find the

geometric shape corresponding to a prescribed pressure distribution from scratch. This problem

is known as the inverse problem. This problem is more difficult than the analysis problem. It is

possible to prescribe a pressure distribution for which no geometry exists. Even if the geometry

exists, it may not be acceptable from a structural standpoint. For two-dimensional incompressible

flow it is possible to obtain conditions on the surface velocity distribution that ensure that a

closed airfoil shape exists. Excellent discussions of this problem have been given by Volpe21 and

Sloof.22 A two-dimensional inverse panel method has been developed by Bristow.23 XFOIL also

has an inverse design option.Error: Reference source not found Numerical optimization can also

be used to find the shape corresponding to a prescribed pressure distribution.24

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5.2.4 Issues in the Problem formulation for 3D potential flow over aircraft

The extension of panel methods to three dimensions leads to fundamental questions

regarding the proper specification of the potential flow problem for flow over an aircraft. The

main problem is how to model the wake coming from the fuselage aft of the wing and wing tips.

The issue is how to specify the wake behind surfaces without sharp edges. The Kutta condition

applies to distinct edges, and is not available if there are not well defined trailing edges.

In some methods wakes are handled automatically. In other methods the wakes must be

specified by the user. This provides complete control over the simulation, but means that the user

must understand precisely what the problem statement should be. The details of the wake

specification often cause users difficulties in making panel models. Figure 5.23, from

Erickson,Error: Reference source not found shows an example of a panel model including the

details of the wakes. For high lift cases and for cases where wakes from one surface pass near

another, wake deflection must be computed as part of the solution. Figure 5.24 comes from a one

week “short” course that was given to prospective users of an advanced panel method, PAN

AIR.25 Each surface has to have a wake, and the wakes need to be connected, as illustrated in

Fig.5.24. The modeling can be complicated. Special attention to wake layout must be made by

the user. To ensure that the problem is properly specified and to examine the entire flowfield in

detail a complete graphics capability is required.

Hess26 provides an excellent discussion of these problems. Many different approaches have

been used. Carmichael and Erickson27 also provide good insight into the requirements for a

proper panel method formulation. Similarly, references Error: Reference source not found and

Error: Reference source not found provide good overviews.

As illustrated above, a practical aspect of using panel methods is the need to pay attention to

details (actually true for all engineering work). This includes making sure that the outward

surface normal is oriented in the proper direction and that all surfaces are properly enclosed.

Aerodynamics panel methods generally use quadrilateral panels to define the surface. Since three

points determine a plane, the quadrilateral may not necessarily define a consistent flat surface. In

practice, the methods actually divide panels into triangular elements to determine an estimate of

the outward normal. It is also important that edges fit so that there is no leakage in the panel

model representation of the surface. Nathman has recently extended a panel method to have

panels include “warp”.28

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Figure 5.23. Illustration of the panel model of an F-16XL,Error: Referencesource not found including the wakes usually not shown in figures of panel

models, but critical to the model.

Figure 5.24. Details of a panel model showing the wake model details and that the wakes are connected. (from a viewgraph presented at a PAN AIR user’s short course, Ref. Error:

Reference source not found)

There is one other significant difference between two-dimensional and three-dimensional

panel methods. Induced drag occurs even in inviscid, irrotational flow, and this component of

drag can be computed by a panel model. However, its calculation by integration of pressures

over the surface requires extreme accuracy, as we saw above for the two-dimensional example.

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The use of a farfield momentum approach is much more accurate. For drag this is known as a

Trefftz plane analysis, see Katz and Plotkin.Error: Reference source not found

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5.2.5 Example applications of panel methods

Many examples of panel methods have been presented in the literature. Figure 5.25 shows an example of the use of a panel model to evaluate the effect of the space shuttle on the Boeing 747. This is a classic example. Other uses include the simulation of wind tunnel walls, support interference, and ground effects. Panel methods are also used in ocean engineering. Recent America’s Cup designs have been dependent on panel methods for hull and keel design. The effects of the free surface can be treated using panel methods.

Figure 5.25. The space shuttle mounted on a Boeing 747.(from the cover of an AIAA Short Course with the title Applied Computational Aerodynamics)

One example has been selected to present in some detail. It is an excellent illustration of

how a panel method is used in design, and provides a realistic example of the typical agreement

that can be expected between a panel method and experimental data in a demanding real world

application. The work was done by Ed Tinoco and co-workers at Boeing.29 Figure 5.26 shows the

modifications required to modify a Boeing 737-200 to the 737-300 configuration. The panel

method was used to investigate the design of a new high lift system. They used PAN AIR, which

is a Boeing developed advanced panel method.30 Figure 5.27 shows the panel method

representation of the airplane.

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Figure 5.26. The Boeing 737-300 relative to the model 737-200 (Ref. Error: Reference

source not found.).

Figure 5.27. The panel representation of the 737-300 with 15° flap deflection (Ref. Error: Reference source not found).

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An understanding of the wing flowfield for two different takeoff flap settings was desired. The cases are “flaps 15”, the normal takeoff setting, and “flaps 1”, the high altitude, hot day setting. The work was conducted in concert with the flight test program to provide insight into the flight test results by providing complete flowfield details not available from the flight test. The computational models used 1750 panels for “flaps 1” and 2900 panels for “flaps 15.” The modeling used to simulate this flowfield illustrates typical idealizations employed when applying panels methods to actual aircraft. Although typical, it is one of the most geometrically complicated examples ever published.

Figure 5-28 shows the wing leading edge and nacelle. The inboard Krueger flap was actually modeled as a doublet of zero thickness. The position was adjusted slightly to allow the doublet sheet to provide a simple matching of the trailing edge of the Krueger and the leading edge of the wing. These types of slight adjustments to keep panel schemes relatively simple are commonly used. The outboard leading and trailing edge flap geometries were also modified for use in this inviscid simulation. Figure 5-29a) shows the actual and computational “flaps 1” geometry. In this case the airfoil was modeled as a single element airfoil. The “flaps 15” trailing edge comparison between the actual and computational geometry is shown in Fig. 5-29b). The triple slotted flap was modeled as a single element flap. At this setting the gap between the forward vane and main flap is closed, and the gap between the main and aft flap is very small.

Figure 5.28. Inboard wing leading edge and nacelle details (Ref. Error: Reference source

not found).

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a) Comparison of actual and computational wing geometry for the flaps 1 case (Ref. Error:

Reference source not found).

b) Actual and computational trailing edge geometry for the flaps 15 case (Ref. Error: Reference

source not found).

Figure 5.29. Examples of computational modeling for a real application.

Several three-dimensional modeling considerations also required attention. In the “flaps 1”

case shown in Fig. 5.30, spanwise discontinuities included the end of the outboard leading edge

slat and trailing edge discontinuities at the back of the nacelle installation (called the thrust gate)

between the inboard and outboard flaps. At the outboard leading edge the edges of the slat and

wing were paneled to prevent leakage. A 0.1 inch gap was left between these surfaces. At the

trailing edge discontinuity a wake was included to model a continuous trailing edge from which

a trailing vortex sheet could be shed.

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Figure 5.30. Spanwise discontinuity details requiring modeling for flaps 1 case (Ref. Error:

Reference source not found).

Similar considerations are required for the “flaps 15.” Here, special care was taken to make sure that the configuration was closed, and contained no holes in the surface at the ends of the flap segments.

Another consideration is the nacelle model. This requires the specification of the inlet flow at the engine face, a model of the strut wake, and both the outer bypass air plume and the primary wake from the inner hot gas jet. Figure 5.31 shows the details.

Figure 5.31 Nacelle model illustrating the application of boundary conditions (Ref. Error:

Reference source not found).

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Complete details of the model are contained in Ref. Error: Reference source not found. With the model complete, the solution was obtained. The spanwise distribution of airfoil section lift coefficients is presented in Figure 5-32. The first part of the figure shows the results for the “flaps 1” case, and the second part of the figure presents the “flaps 15” case. In both cases the jig shape and flight shape including aeroelastic deformation are included. This is another consideration in making a proper aerodynamic simulation. In both cases the shape including the deformation under load shows much better agreement with flight and wind tunnel data. Notice the loss of lift on the wing at the nacelle station, and the decrease in lift outboard of the trailing edge flap location.

a) flaps 1 case

b) flaps 15 case

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Figure 5.32. Spanwise distribution of lift coefficient on the Boeing 737-300 (Ref. Error:

Reference source not found).

Figure 5-33 presents the change in section lift coefficient with angle of attack at several span stations. The agreement between PAN AIR and flight test is better for the “flaps 1” case. Viscous effects are becoming important for the “flaps 15” case.

a) flaps 1 case

1 Bertin, J.J., and Cummings, R.M., Aerodynamics for Engineers, 5th Edition, Prentice-Hall, Inc., Upper Saddle River, 2008.

2 Erickson, L.L., “Panel Methods—An Introduction,” NASA TP-2995, Dec. 1990.9 Hildebrand, F.B., Advanced Calculus for Applications, Prentice-Hall, Englewood Cliffs, 196210 Ashley, H, and Landahl, M., Aerodynamics of Wings and Bodies, Addison-Wesley, Reading,

1965 (republished in paperback by Dover Publishing).11 Curle, N., and Davis, H.J., Modern Fluid Dynamics, Volume 1: Incompressible Flow, Van

Nostrand, London, 1968.12 Neal, David, PhD Student, Virginia Tech, 2007, private communication17 Abbott, I.H., and von Doenhoff, A.E., Theory of Wing Sections, Dover, New York, 1959.

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b) flaps 15 case

Figure 5.33. Comparison of section lift coefficient change with angle of attack (Ref. Error:

Reference source not found)

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Figure 5-34 completes this example by presenting the comparison of pressure distributions for the two cases at four spanwise stations. The “flaps 1” case agreement is generally good. Calculations are presented for both the actual angle of attack, and the angle of attack that matches the lift coefficient. Matching lift coefficient instead of angle of attack is a common practice in computational aerodynamics. Considering the simplifications made to the geometry and the absence of the simulation of viscous effects the agreement is very good. The “flaps 15” case starts to show the problems that arise from these simplifications. This is a good example of the use of a panel method. It illustrates almost all of the considerations that must be addressed in actual applications.

a) flaps 1 case b) flaps 15 case

Figure 5.34. Comparison of pressure distributions between flight and computations for the 737-300, solid line is PAN AIR at flight lift, dashed line is PAN AIR at flight angle of attack (Ref. Error: Reference source not found).

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5.2.6 Using Panel MethodsCommon sense rules for panels

• Vary the size of panels smoothly• Concentrate panels where the flowfield and/or geometry is changing rapidly• Don’t spend more money and time (i.e., numbers of panels) than required

Panel placement and variation of panel size affect the quality of the solution. However, extreme sensitivity of the solution to the panel layout is an indication of an improperly posed problem. If this happens, the user should investigate the problem thoroughly.

Panel methods are an aid to the aerodynamicist. You must use the results as a guide to help you develop your own judgment. Remember that the panel method solution is an approximation of the real life problem; an idealized representation of the flowfield. An understanding of aerodynamics that provides an intuitive expectation of the types of results that may be obtained, and an appreciation of how to relate your idealization to the real flow, is required to get the most from the methods. This insight requires experience and study.

What a Panel Method Can and Can't Do

1. Panel methods are inviscid solutions. You will not capture viscous effects except via user “modeling” by changing the geometry.

2. Solutions are invalid as soon as the flow develops local supersonic zones

[i.e., Cp < Cpcrit]. For two-dimensional isentropic flow, the exact value of Cp for critical flow is:

Cpcrit=−

2gM∞

2 1−1+

g −12

M∞2

g +12

⎛⎝⎜

⎞⎠⎟

⎧⎨⎪⎪

⎩⎪⎪

⎫⎬⎪⎪

⎭⎪⎪

gg−1

⎢⎢⎢⎢⎢

⎥⎥⎥⎥⎥

(5.32)

5.2.7 Advanced panel methods: What is a “Higher Order” Panel Method?

So-called “higher-order” panel methods use singularity distributions that are not constant

over the panel, and may also use panels that are non-planar. Higher-order methods were actually

found to be crucial in obtaining accurate solutions for the Prandtl-Glauert Equation at supersonic

speeds. At supersonic speeds, the Prandtl-Glauert equation is actually a wave equation

(hyperbolic), and requires much more accurate numerical solution than the subsonic case to

avoid “noisy” pressure distributions as the solution (Magnus and EptonError: Reference source

not found). However, subsonic higher-order panel methods, although not as important as the

supersonic flow case, have been studied in some detail. In theory, good results can be obtained

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using far fewer panels with higher-order methods. In practice the need to resolve geometric

details often leads to the need to use small panels anyway, and all the advantages of higher-order

panelling methods are not necessarily obtained. Nevertheless, since a higher-order panel method

may also be a relatively new program taking advantage of many years of experience, the higher-

order code may still be a good candidate for use.

5.2.8 Today’s standard programs: a brief survey

Panel methods are widely used in the aircraft industry, and have been for a long time. Comparisons between various panel codes have been made (e.g., Margason, et al.31), and in general, all the new professionally-developed codes can be made to work well (recall the attention to detail required illustrated above). The selection of a specific code will likely be based on non-technical considerations, such as cost or availability. One of the newest panel codes is known as PMARC,32 for Panel Method Ames Research Center, and has received a great deal of development effort. We provide a brief description of the codes a new aerodynamicist will most likely encounter, either at work or reading the literature. Tables 5-1 through 5-3 are based on the summary by Magnus and Epton,Error: Reference source not found with slight updating, and provide specific references.

PAN AIR - Boeing-developed code, funded by a variety of government agencies.This code provides total flexibility, i.e. it is really an integral equation solver and not an

aerodynamicist’s tool per se. It is a higher-order panel method, and can handle both subsonic and supersonic flow. It is relatively expensive and difficult to run (a PAN AIR user would take months to train, and it would probably become his primary job).

To effectively use the code good pre- and post- processing systems must be available. Although Boeing has these systems in place, they were internally developed and are not available outside the company.

VSAERO - AMI developed (Analytical Mechanics Inc., Frank Dvorak and Brian Maskew).

This code was originally a low-order method, but has been extended to include variations of the singularity strength over a panel, and has now been described as “multi-order.”Error:Reference source not found It is for subsonic flow only. It handles general geometries, and includes options to treat viscous effects and vortex flows. Originally developed for NASA, the code has been much further developed by AMI as a commercial product (they also have a plotting package and other supporting software available for purchase) This code requires considerable user training. Support from AMI is available, but none of the codes are priced for student use. Typical development enhancements of the code are described by Nathman.33

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The public domain version of this code was obtained by several groups that worked on the design of the America’s Cup Yacht competitors in the mid-1980s. The code was used for hull and keel design. One of the modifications that was made for this application was the addition of the free surface representing the air-water interface (recall that the free surface problem means that the surface displacement is unknown, and the boundary condition is that a constant pressure exists at the interface).

Versions of the “Hess Code” - further developments of the research team at Douglas, now Boeing, McDonnell Douglas developed numerous versions under various government contracts, and it seems to be available mainly at Navy facilities.

Woodward: An old panel method that is sometimes encountered is the code known as the “Woodward” or “Woodward-Carmichael” code. Woodward's first methods were developed while he was at Boeing, and were supported by NASA Ames, primarily for the US Supersonic Transport program (which was an important national effort in the 1960s). Subsequently, Woodward went into business and continued to develop codes. USSAERO treats both supersonic and subsonic flow, and a version that combines a number of features of each code, as well as additional design options is also available, and known as “Woodward 12” or W12SC3.

PMARC -This is the newest panel method code, and was developed at NASA Ames to provide an extremely flexible method to simulate a wide range of very general geometries. An example is the simulation of high lift systems and jet exhausts for VSTOL aircraft. The code is a lower-order panel method, and can simulate unsteady as well as steady flow. The wake position can be obtained as part of the solution. It has been used for underwater applications as well as for aircraft.

The history of panel methods is illustrated in the following tables. Table 5.1 summarizes some of the key early methods that were developed. (W12SC3 is included because it was a valuable combination of two early codes,34 providing significant new design capability, particularly at supersonic speeds; despite the title of the report, W12SC3 can be run at subsonic speeds.) Table 5.2 reviews the extremely active era of the development of advanced panel methods. Finally, Table 5.3 provides details on the current production codes likely to be used on current aerodynamic design and analysis projects. Panels methods can also treat unsteady flows, with a recent example being the developments made by van Zyl.35

Source code and PC executable versions of the PAN AIR and Woodward codes are available for a low price, together with a collection of other programs aerodynamic analysis and design programs, from Public Domain Aeronautical Software.36

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Table 5.1 Comparison of Some Major Panel Method Programs: Early CodesOriginator and Method Name

Year PanelGeometry

SourceType

Doublet Type

BoundaryConditions

Restrictions Comments

Hess and Smith37

(Douglas)

1962 flat constant none Specificaton of normal flow

non-lifting wings and bodies only

Rubbert38

(vortex lattice)1964 flat none constant normal flow planar wings

onlyWoodward39

(Woodward I)1967 flat constant linear normal flow wings must be

planarRubbert and

Saaris40

(Boeing A-230)

1968 flat constant constant normal flow nearly constant panel density

Hess I41 1972 flat constant linear normal flow wings and bodies only

USSAERO42

(Woodward II)1973 flat subsonic

and supersonic, analysis only

W12SC3Error:Referencesource not

found(Grumman)

1983 flat mixed design and analysis

combines Woodward I & II features

Table 5.2 Comparison of Some Major Panel Method Programs: Advanced MethodsOriginator

and Method Name

Year PanelGeometry

SourceType

Doublet Type

BoundaryConditions

Restrictions Comments

Roberts and Rundle43

1973 paraboloidal quadratic quadratic normal flow

Numerical integrations, very expensive

Mercer, Weber and Lesford44

1973 flat none Smooth, cubic,

quadratic

Normal flow in

least squares sense

planar wings Subsonic/supersonic, cubic spanwise, quadratic chordwise

Morino and Kuo45

(SOUSSA)

1974 continuous, hyperboloidal

constant constant potential no thin configurations

unsteady

Johnson and Rubbert46

1975 paraboloidal linear quadratic normal flow

Ehlers and Rubbert47 (Mach line paneling)

1976 flat linear continuous quadratic

normal flow

Planar wings, special

paneling

supersonic flow

Ehlers et al.48

(PAN AIR

1977 continuous piecewise flat

linear continuous quadratic

arbitrary in , D

subsonic and supersonic

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pilot code)

Table 5.3 Comparison of Major Panel Method Programs: Production Codes

Originator and Method Name

Year PanelGeometry

SourceType

Doublet Type

BoundaryConditions

Restrictions Comments

MCAIR49

(MacDonnell)1980 flat constant quadratic Design option

PAN AIRError:Referencesource not

found(Boeing)

1980 continuous piecewise flat

continuous linear

continuous quadratic

arbitrary in , D

Subsonic and supersonic

Hess II50

(Douglas)1981 parabolic linear quadratic normal

flowVSAERO51

(AMI)1981 flat constant constant Exterior

and interior normal flow

subsonic

QUADPAN52

(Lockheed)1981 flat constant constant

PMARCError: Referencesource not

found(NASA Ames)

1988 flat constant constant Unsteady,wake rollup

5.3 Vortex Lattice Methods

Vortex Lattice Methods (vlm) are similar to panel methods but easier to use and capable of

providing remarkable insight into wing aerodynamics and component interaction. They were

among the earliest methods utilizing computers to actually assist aerodynamicists in estimating

aircraft aerodynamics. Vortex lattice methods are based on solutions to Laplace’s Equation, and

are subject to the same basic theoretical restrictions that apply to panel methods.

As a comparison, most vortex lattice methods are:

Similar to Panel methods:• singularities are placed on a surface• the no flow-through condition is satisfied at a number of control points• a system of linear algebraic equations is solved to determine singularity strengths

Different from Panel methods:• Oriented toward lifting effects, and classical formulations ignore thickness• Boundary conditions (BCs) are applied on a mean surface, not the actual surface

(not an exact solution of Laplace’s equation over a body, but embodies some additional approximations, i.e., together with the first item, we find DCp, not Cpupper and Cplower)

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• Singularities are not distributed over the entire surface• Oriented toward combinations of thin lifting surfaces (recall panel methods had no limitations on thickness).

Vortex lattice methods were first formulated in the late 1930s, and the method includes wing-

tip vortex effects through the use of a trailing vortex filament system. It was first called a

“Vortex Lattice” in 1943 by Faulkner. The concept is extremely simple, but because of its purely

numerical approach (i.e., no answers are available at all without finding the numerical solution of

a matrix too large for routine hand calculation) practical applications awaited sufficient

development of computers—the early 1960s saw widespread adoption of the method. A

workshop was devoted to these methods at NASA in the mid 1970s.53 A nearly universal

standard for vortex lattice predictions was established by a code developed at NASA Langley,

whose authors include Margason and Lamar54, Lamar and Gloss,55 and Lamar and Herbert.56,57 It

is generally known as the “Lamar Vortex Lattice Method”. Each new version had considerably

more capability than the previous version. The “final” development in this series is designated

VLM4.997. The original codes could handle two lifting surfaces, while VLM4.997 can handle

four. Many other people have written vortex lattice method codes. The current methods that are

widely used are the code by Drela and Youngren, AVL,58 and Tornado, a MATLAB code

developed by Tomas Melin at KTH in Sweden.59 VORLAX,60 as part of the HASC code61 is also

widely used. AMI, the authors of the VSAERO panel method described above have also

released a vortex lattice code, VLAERO.62 The vlm method is simple enough that many students

have written their own codes, which are easily executed on current personal computers.

Noteworthy variations on the basic method have been developed by Lan63 (Quasi-Vortex

Lattice Method), and Mook64 and co-workers. Mook developed vortex lattice class methods that

treat flowfields that contain leading edge vortex-type separation and also handle general

unsteady motions. The book by Katz and PlotkinError: Reference source not found contains

another variation, using vortex rings, and includes a FORTRAN code. Kay wrote a code65

(JKayVLM) using the method of Katz and Plotkin to estimate stability derivatives and that code

is also readily available.

To understand the method, a number of basic concepts must be reviewed. Then we describe

one implementation of the vlm method, and use it to obtain insights into wing and wing-canard

aerodynamics. Naturally, the method is based on the idea of a vortex singularity as the solution

of Laplace’s equation. A good description of the basic theory for vortices in inviscid flow and

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thin wing analysis is contained in Karamcheti,Error: Reference source not found pp. 494-496,

499-500, and 518-534 and has been reviewed in Chapter 4. A good general description of the

vortex lattice method is given by Bertin and Cummings.Error: Reference source not found After

some illustrations of the results from vlm methods, an example of a vortex lattice method used in

a design mode is presented, where the camber line required to produce a specified loading is

found.

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5.3.1 Boundary conditions on the mean surface and the pressure relation

An important difference between vortex lattice methods and panel methods is the way in

which the boundary conditions are handled. Typically, the vortex lattice method uses an

approximate boundary condition treatment; this boundary condition can also be used in other

circumstances to good advantage. This is a good “trick” applied aerodynamicists should know

and understand, and that is why it is covered in detail here. In general, this approach results in

the so-called “thin airfoil boundary condition,” and arises by linearizing and transferring the

boundary condition from the actual surface to a flat mean “reference” surface, that is typically a

constant coordinate surface. Consistent with the boundary condition simplification, a simplified

relation between the pressure and velocity is also possible. The simplification in the boundary

condition and pressure-velocity relation provides a basis for treating the problem as a

superposition of the lift and thickness contributions to the aerodynamic results. KaramchetiError:

Reference source not found provides an excellent discussion of this approach.

To understand the thin airfoil theory boundary condition treatment, we provide an example in

two dimensions. Recall (from Eqn. 2-54) that the exact surface boundary condition for steady

inviscid flow is:

V⋅n =0 (5.33)

on F(x, y)=0 =y−(x). The unit normal vector is n =∇F(x,y) / ∇F(x,y) and the velocity

field is defined using the notation defined in Fig. 5.35.

V

V cosV sin

α

αα

∞∞

y

x

Figure 5.35. Basic coordinate system for boundary condition analysis.

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Define the velocity components of V as:

V =V ∞ + θ(x,y)

a diσturbanχ vloχity1 2 3 (5.34)

where q is a disturbance velocity with components u and v. If we assume irrotational flow, then these components are described in terms of a scalar potential function, u = x and v = y. The total velocity V then becomes (in terms of velocity components):

uTOT =V∞ χoσa +u(x,y)vTOT =V∞σina +v(x,y)

(5.35)

and we can write out the boundary condition as:

V⋅n =(uTOTi+vTOTφ)⋅∂F∂ x

i+∂F∂ y

φ⎛⎝⎜

⎞⎠⎟=0 (5.36)

or

V∞ χoσa +u(x,y)[ ]∂F∂ x

+ V∞σina +v(x,y)[ ]∂F∂ y

=0 (5.37)

on F(x,y) = 0, and recalling the relationship between F and f given below Eqn. (5.33):

∂F∂ x

=∂∂ x

y − f (x){ } = −df (x)

dx∂F∂ y

=∂∂ y

y − f (x){ } = 1. (5.38)

Substituting for F in Eq.(5.37) we have:

V∞ χoσa +u( ) −ddx

⎛⎝⎜

⎞⎠⎟+ V∞σina +v( )=0 (5.39)

which, solving for v, is:

v = V∞ χoσa +u( )ddx

−V∞σina (5.40)

on y = f(x). Note that v is defined in terms of the unknown u. Thus Eq. (5.40) is a nonlinear boundary condition and further analysis is needed to obtain a useful relation.*

Linearized form of the boundary conditionThe relation given above by Eq.(5.40) is exact. It has been derived as the starting point for

the derivation of useful relations when the body (which is assumed to be a thin surface at a small

angle of attack) induces disturbances to the freestream velocity that are small in comparison to

the freestream velocity. Thus we assume: u << V∞, v << V∞, and ∂F/∂x < ∂F/∂y. Note that this

* Observe that even when the flowfield model is defined by a linear partial differential equation, an assumption which we have not yet made, the boundary condition can make the problem nonlinear.

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introduces a bias in the coordinate system to simplify the analysis, a typical consequence of

introducing simplifying assumptions. Consistent with this assumption, the components of the

freestream velocity are (remembering that a is in radians and small):

V∞ χoσa ≈V∞

V∞σina ≈V∞a(5.41)

and the expression for v in Eq.(5.40) becomes:

v = V∞ +u( )ddx

−V∞a . (5.42)

Dividing by V∞,

vV∞

= 1+uV∞

⎛⎝⎜

⎞⎠⎟ddx

−a (5.43)

the linearized boundary condition is obtained by neglecting u/V∞ compared with unity

(consistent with the previous approximations). With this assumption, the linearized boundary

condition becomes:

vV∞

=ddx

−a on y=(x) . (5.44)

This form of the boundary condition is not valid if the flow disturbance is large compared to

the freestream velocity {for aerodynamically streamlined shapes this is usually valid everywhere

except at the leading edge of the airfoil, where a stagnation point exists (u = -V∞) and the slope

is infinite (df/dx = ∞)}. In practice, a local violation of this assumption leads to a local error. So,

if the details of the flow at the leading edge are not important to the analysis, which surprisingly

is often the case at low angles of attack, the linearized boundary condition can be used.

Transfer of the boundary condition Although Eqn. (5.44) is linear, it is hard to apply because it is not applied on a coordinate

line.* We now use a further approximation of this relation to get the useful form of the linearized

boundary condition. Using a Taylor series expansion of the v component of velocity about the

coordinate axis we obtain the v velocity on the surface:

v{x, y =(x)} =v(x,0)+ (x)∂v∂ yy=0

+... . (5.45)

* The simplification introduced by applying boundary conditions on constant coordinate surfaces justifies the use of rather elaborate transformations, which will be discussed in more detail in Chap. 7, Geometry and Grids: Major Considerations in Using Computational Aerodynamics.

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For the thin surfaces under consideration, f(x) is small, and because the disturbances are assumed

small, ∂v/∂y is also small. For example, assume that v and ∂v/∂y are the same size, equal to 0.1,

and df/dy is also about 0.1. The relation between v on the airfoil surface and the axis is:

v{x, y =(x)} =(0.1)+ (0.1)(0.1)=0.1 +0.01

nglχt{ . (5.46)

Neglecting the second term, we assume:v{x, f (x)} ≈v(x,0). (5.47)

We now apply both the upper and lower surface boundary conditions on the axis y = 0, and

distinguish between the upper and lower surface shapes by using:

f =u on th uppr σuraχ=l on th loωr σuraχ

. (5.48)

Using Eq. (5.48), we write the upper and lower surface boundary conditions as:

v x,0+( )V∞ up

=dudx

−a,v x,0−( )V∞ loω

=dldx

−a . (5.49)

These are the linearized and transferred boundary conditions. Frequently, these boundary

conditions result in a surprisingly good approximation to the flowfield, even in transonic and

supersonic flow.

Decomposition of boundary conditions to camber/thickness/alpha

Further simplification and insight can be gained by considering the airfoils in terms of the

combination of thickness and camber, a natural point of view. We thus write the upper and lower

surface shapes in terms of camber, fc, and thickness, ft, as:

fu =χ + tl=χ −t

(5.50)

and the general problem is then divided into the sum of three parts as shown in Fig. 5.36.

Generalairfoilat a

Thiχκnσσat a = 0°

Cabrat a = 0°

Flat platat a

= + +

Figure 5.36. Decomposition of a general shape at incidence.

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The decomposition of the problem is somewhat arbitrary, since linearity allows for any decomposition to be used. Camber could also be considered to include angle of attack effects using the boundary condition relations given above. The aerodynamicist must keep track of details for a particular problem. To proceed further, we make use of the basic vortex lattice method assumption: the flowfield is governed by a linear partial differential equation (Laplace’s equation, allowing for superposition of solutions). Superposition allows us to solve the problem in pieces and add up the contributions from the various parts of the problem. This results in the final form of the thin airfoil theory boundary conditions, substituting Eq. (5.50) into Eq. (5.49):

v x,0+( )V∞ up

=dχdx

+dtdx

−a

v x,0−( )V∞ loω

=dχdx

−dtdx

−a

. (5.51)

The problem can be solved for the various contributions and the contributions are added together

to obtain the complete solution. If thickness is neglected the boundary conditions are the same

for the upper and lower surface. Thin airfoil theory pressure relation

Consistent with the linearization of the boundary conditions, a useful relation between the

pressure and velocity can also be obtained. For incompressible flows, the exact relation between

the pressure coefficient and velocity is:

Cp =1−VV∞

⎛⎝⎜

⎞⎠⎟2

(5.52)

Assuming two-dimensional flow for this example, we express the velocity considering

disturbances to the freestream velocity using the approximations discussed above:

V 2 = V∞ χoσa +u( )2+ V∞σina +v( )

2≈ V∞ +u( )

2+ V∞a +v( )

2 (5.53)

Expanding and dividing by V∞2 we get:

V 2

V∞2 =1+ 2

uV∞

+u2

V∞2 +a

2 + 2avV∞

+v2

V∞2 . (5.54)

Substituting into the Cp relation, Eqn. (5-52), we get:

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CP =1− 1+2uV∞

+u2

V∞2 +a

2 + 2avV∞

+v2

V∞2

⎛⎝⎜

⎞⎠⎟

=1−1−2uV∞

−u2

V∞2 −a

2 −2avV∞

−v2

V∞2

(5.55)

and if a, u/V∞ and v/V∞ are << 1, then the last four terms can be neglected in comparison with

the third term. The final result is:

Cp =−2uV∞

. (5.56)

This is the linearized or “thin airfoil theory pressure formula”. From experience gained

comparing various computational results, we have found that this formula is a slightly more

severe restriction on the accuracy of the solution than the linearized boundary condition.

Equation (5.56) shows that under the small disturbance approximation, the pressure is a linear

function of u, and we can add the Cp contribution from thickness, camber, and angle of attack by

superposition. A similar derivation can be used to show that Eq. (5.56) is also valid for

compressible flow up to moderate supersonic speeds.

DCp due to camber/alpha (thickness effects cancel!)

Next, we make use of the result in Eq. (5.56) to obtain a formula for the load distribution on

the wing, which is the difference between the pressure on the top and bottom surfaces:

DCp = Cpl− Cpu . (5.57)

Using superposition, the pressures can be obtained as the contributions from wing thickness,

camber, and angle of attack effects:

Cpl=CpThiχκnσσ

+CpCa br+CpAngl o attaχκ

Cpu=CpThiχκnσσ

−CpCa br−CpAngl o attaχκ

(5.58)

so that:DCp = CpThickness

+ CpCamber+ CpAngle of attack( )

− CpThickness− CpCamber

− CpAngle of attack( )

= 2 CpCamber+ CpAngle of attack( )

. (5.59)

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Equation (5.59) demonstrates that for cases where the linearized pressure coefficient relation is

valid, thickness does not contribute to lift to first order in the velocity disturbance.

The importance of this analysis is that we have shown:

1. how the lifting effects can be obtained without considering thickness, and

2. that the cambered surface boundary conditions can be applied on a flat coordinate surface, resulting in an easy to apply boundary condition.

The principles demonstrated here for transfer and linearization of boundary conditions can be

applied in a variety of situations other than the application to vortex lattice methods. Often this

idea can be used to handle complicated geometries that cannot easily be treated exactly.

The analysis shown here produces an entirely consistent problem formulation. This includes

the linearization of the boundary condition, the transfer of the boundary condition, and the

approximation between velocity and pressure. All of the approximations are consistent with each

other, and improving one of these approximations without improving them all in a consistent

manner may actually lead to worse results. Sometimes you can make agreement with data better,

sometimes it may get worse. You have to be careful when trying to improve theory on an ad hoc

basis.

To examine the use of these ideas we present a two-dimensional example. For the numerical

calculation the airfoil is divided into a number of equal length panels. A vortex is placed at the

quarter-chord point of each panel and the no-flow-through boundary condition is satisfied at the

three-quarter chord point of the individual panel. This can be shown to produce exact thin airfoil

theory for a small number of panels, and is known as the “1/4 – 3/4 rule”. The example illustrates

the accuracy of the methods described above. In Fig. 5.37, we compare the results obtained for a

5% circular arc camber.* Three solutions are presented. The curve labeled linear theory uses

classical analytical thin airfoil theory with results obtained satisfying the boundary condition on

the mean surface. This is compared with numerical results for the case where the boundary

condition is applied exactly on the camber line, and the result obtained applying the boundary

condition on the mean surface using the approximate method described above. The difference

between placing the vortex on the actual camber surface and satisfying the boundary condition

* A relatively large camber for a practical airfoil, the NACA 4412 example we used above illustrating panels methods was an extreme case with 4% camber.

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on the actual surface, and the more approximate traditional approach of locating the vortex and

control point on the mean surface is extremely small.

0.10

0.20

0.30

0.40

0.50

0.60

0.70

0.80

0.90

0.0 0.2 0.4 0.6 0.8 1.0

5% Circular arc camber linea = 0 °40 panlσ

DCp bχ'σ on χabr linDCp bχ'σ on axiσDCp linar thory

DCp

x/χ

DCp bχ'σ on χabr linDCp bχ'σ on axiσ DCp linar thory

Figure 5.37. Comparison in 2D of the 1/4-3/4 rule for vortex-control point locations with linear theory, and including a comparison between placing the vortex and control point on the camber line or on the axis.

5.3.2 The Classical Vortex Lattice Method

There are many different vortex lattice schemes. In this section we describe the “classical”

implementation, in which a horseshoe vortex is placed on each panel.* Knowing that vortices can

represent lift from our airfoil analysis, this approach places a vortex filament at the 1/4 chord

location of a “panel” and then the boundary condition is satisfied at the 3/4 chord point on the

panel, the so-called “1/4 - 3/4 rule.” This was the approach used above to obtain the results

shown in Fig. 5.37. This is illustrated in Fig. 5.38, where the “horseshoe vortex” is shown on

each panel. Each horseshoe vortex consists of the “bound vortex” attached to the panel, and two

* Alternately, methods have been developed that employ vortex rings around each panel. The panel at the trailing edge still has to use a vortex that extends to downstream infinity to model the wake. A curious property of vortex rings is that they are equivalent to a constant strength doublet panel, as pointed out by Paul Rubbert in a 1978 AIAA short course on Applied Computational Aerodynamics.

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trailing vortex legs that attach to the end of the bound vortex and extend to downstream infinity

(since a vortex cannot end in a fluid). Using this approach, we proceed as follows:

1. Divide the planform up into a lattice of quadrilateral panels, and put a horseshoe vortex on each panel.

2. Place the bound vortex of the horseshoe vortex on the 1/4 chord element line of each panel.

3. Place the control point on the 3/4 chord point of each panel at the midpoint in the spanwise direction (sometimes the lateral panel centroid location is used).

4. Assume a flat wake in the usual classical method.

5. Determine the strengths of each n required to satisfy the boundary conditions by solving a system of linear equations. This system comes from writing down the sum of all the horseshoe vortex induced velocity contributions at each control point, and then using that velocity in the equation required to satisfy the no flow-through condition. This results in a system for the unknown values of the n’s.

y

x

X

X

X

X

XX

XX

X

Trailing vortices extend to infinity

bound vortices

control points1

2

3n

n−1

Figure 5.38. The horseshoe vortex layout for the classical vortex lattice method.

Note that the lift is on the bound vortices. To understand why, consider the vector statement

of the Kutta-Joukowski Theorem, F =rV × . Assuming the freestream velocity is the primary

contributor to the velocity, the trailing vortices are parallel to the velocity vector and hence the

force on the trailing vortices are zero (recall that if vectors are parallel, the cross product is zero).

More accurate methods find the wake deformation required to eliminate the force in the presence

of the complete induced flowfield.

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As in the case of panels methods, the algebra required to obtain the influence coefficients

connecting the velocities induced at a specific location by each horseshoe vortex is lengthy. The

velocity induced by a vortex filament is given by the Biot-Savart Law, see Section 4.8.3 above.

Each horseshoe vortex makes a contribution with a single value of . Bertin and

CummingsError: Reference source not found contains a detailed derivation. To illustrate the

essence of the method, we consider the simple planar surface case, without dihedral. Using the

basic boundary condition relation given in Eq. (5.51) and realizing that in 3D the downwash

velocity is w, the boundary condition is:

wV∞

=dχdx

−a (5.60)

Now, the downwash w at a point m, due to a horseshoe vortex, n, can be written as:

wm =C ,nn . (5.61)

where Cm,n is an influence coefficient that is based on the Biot-Savart Law and the geometric

distance between point m and the horseshoe vortex n. The next step is to sum the induced

velocities from all the horseshoe vortices at a point m, and use that velocity in the boundary

condition, Eq. (5.60),

wm = C ,nκn

n=1

2N

∑ =V∞

dχdx

−a⎛⎝⎜

⎞⎠⎟

. (5.62)

where there are N horseshoe vortices on each side of the wing, resulting in a total of 2N

horseshoe vortices representing the wing. Thus we have the following equation that satisfies the

boundary conditions and can be used to relate the circulation distribution and the wing camber

and angle of attack:

Cm,nk

n

V∞

⎛⎝⎜

⎞⎠⎟n=1

2N

∑ =dχdx

−a⎛⎝⎜

⎞⎠⎟

=1,...,2N . (5.63)

Equation (5.63) contains two cases:

1. The Analysis Problem. Given camber slopes and a, solve for the circulation strengths, (/V∞) [ a system of 2N simultaneous linear equations].

or2. The Design Problem. Given (n/V∞), which corresponds to a specified surface

loading, we want to find the camber and a required to generate this loading (only requires simple algebra, no system of equations must be solved).

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Notice that the way dfc/dx and a are combined illustrates that the division between camber,

angle of attack and wing twist is arbitrary (twist can be considered a separate part of the camber

distribution, and is useful for wing design). However, care must be taken in keeping the

bookkeeping straight.

A reduction in the size of the problem is available in many cases. If the geometry is

symmetrical and the camber and twist are also symmetrical, then n is the same on each side of

the planform (but not the influence coefficient). Therefore, we only need to solve for N ’s, not

2N. This is also true if ground effects are desired, where the image of a vortex placed

symmetrically below the ground plane can be included in the influence coefficient matrix

without adding additional unknowns, as shown in Katz and PlotkinError: Reference source not

found. The system of equations for the case of planform symmetry becomes:

Cm,nkleft+C ,nκright

⎡⎣ ⎤⎦n=1

N

∑ n

V∞

⎛⎝⎜

⎞⎠⎟ =

dχdx

−a⎛⎝⎜

⎞⎠⎟

=1,..., N . (5.64)

Doing this seems easy—why not just program it up ourselves? You can, but most of the work is

taken up by:

A. Automatic layout of panels for arbitrary geometry. As an example, when considering multiple lifting surfaces, the horseshoe vortices on each surface must “line up”. The downstream leg of a horseshoe vortex cannot pass through the control point of another panel.

and B. Converting n to the aerodynamics values of interest, CL, Cm, etc., and the

spanload, is tedious for arbitrary configurations.

Nevertheless, many people, including lots of students have written vlm codes. The method is

widely used in industry and government for aerodynamic estimates for conceptual and

preliminary design predictions. It provides good insight into the aerodynamics of wings,

including interactions between lifting surfaces.

Typical analysis uses (in a design environment) include• Predicting the configuration neutral point during initial configuration layout, and

studying the effects of wing placement and canard and/or tail size and location.• Finding the induced drag, CDi, from the spanload in conjunction with farfield methods.

• With care, estimating control and device deflection effectiveness (estimates where viscous effects may be important require calibration. Some examples are shown in the next section. For example, take 60% of the inviscid value to account for viscous losses,

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and also realize that a deflection of df = 20 - 25° is about the maximum useful device deflection in practice).

• Investigating the aerodynamics of interacting surfaces.• Finding the lift curve slope, CLa, approach angle of attack, etc.

Typical design applications include:• Initial estimates of twist to obtain a desired spanload, or root bending moment.• Starting point for finding a camber distribution in purely subsonic cases.

Before examining how well the method works, two special cases require comments. The

first case arises when a control point is in line with the projection of one of the finite length

vortex segments. This problem occurs when the projection of a swept bound vortex segment

from one side of the wing intersects a control point on the other side. This happens surprisingly

frequently. The velocity induced by this vortex is zero, but the equation as usually written

degenerates into a singular form, with the denominator going to zero. Thus a special form of the

equation should be used. In practice, when this happens the contribution can be set to zero

without invoking the special form. Figure 5.39 shows how this happens. Using the so-called

Warren 12 planform and 36 vortices on each side of the wing, we see that the projection of the

line of bound vortices on the last row of the left hand side of the planform intersects one of the

control points on the right hand side.

A model problem illustrating this can be constructed for a simple finite length vortex

segment. The velocity induced by this vortex is shown in Fig. 5.40. When the vortex is

approached directly, x/l = 0.5, the velocity is singular for h = 0. However, as soon as you

approach the axis (h = 0) off the end of the segment (x/l > 1.0) the induced velocity is zero. This

illustrates why you can set the induced velocity to zero when this happens.

The second special case that needs to be discussed arises when two or more planforms are

used with this method, which is one of the most powerful applications of the vortex lattice

method. However, care must be taken to make sure that the trailing vortices from the first surface

do not intersect the control points on the second surface. In this case the induced velocity is in

fact infinite, and the method breaks down. Usually this problem is solved by using the same

spanwise distribution of horseshoe vortices on each surface. This aligns the vortex legs, and the

control points are well removed from the trailing vortices of the forward surfaces.

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-0.50

0.00

0.50

1.00

1.50

2.00

2.50

3.00-2.0 -1.5 -1.0 -0.5 0.0 0.5 1.0 1.5 2.0

trailing legs extend to infinity

Warren 12 planform

example is for 36 horseshoevortices on each side, all

vortices not shown forclarity

projection of boundvortices on this rowintersect control pointon other sideof planform horseshoe vortex

control point

Figure 5.39. Example of case requiring special treatment, the intersection of the projection of a vortex with a control point.

0.00

0.20

0.40

0.60

0.80

1.00

0.0 0.5 1.0 1.5 2.0

Vp

h/l

0.5

1.5

2.0

3.0

x/l

hx

p

l

x=0

Figure 5.40. Velocity induced by finite straight line section of a vortex.

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5.3.3 Examples of the Use and Accuracy of the vlm Method

How well does the vortex lattice method work? In this section we describe how the method is

normally applied and present several example results obtained using the method. The vortex

lattice layout is clear for most wings and wing-tail or wing-canard configurations. The method

can be used for wing-body cases by simply specifying the projected planform of the entire

configuration as a flat lifting surface made up of a number of straight line segments. The exact

origin of this somewhat surprising approach is unknown, but its success is illustrated in examples

given below.

To get good, consistent, and reliable results using Lamar’s program discussed above some

simple rules for panel layout should be followed (likely equally valid for any vlm method). This

requires that a few common rules of thumb be used in selecting the planform break points: i) the

number of line segments should be minimized, ii) breakpoints should line up streamwise on front

and rear portions of each planform, and should line up between planforms, iii) streamwise tips

should be used, iv) small spanwise distances should be avoided by making edges streamwise if

they are actually highly swept, and v) trailing vortices from forward surfaces cannot hit the

control point of an aft surface. Figure 5-41 illustrates these requirements.

The Warren 12 Test Case

One reference wing case that is a standard used to check the accuracy of vortex lattice codes

is the Warren 12 planform. It provides a check case for the evaluation of any new or modified

vlm code, as well as a check on the panel scheme layout, and is defined, together with the

“official” characteristics from previous calculations, in Fig. 5.42 below. For the Warren 12

results, the reference chord used in the moment calculation is the average chord (slightly

nonstandard, normally the reference chord used is the mean aerodynamic chord) and the moment

reference point is located at the wing apex (which is also nonstandard).

As with all computational aerodynamics methods, vlm should be checked to assess the

convergence characteristics. Figure 5.43 is taken from the original NASA report describing the

Lamar program,Error: Reference source not found and shows that the basic force results can be

obtained with a relatively small number of chordwise panels, but requires a farily large number

of spanwise rows of panels. The original program distributed by NASA allowed for a maximum

of 200 horseshoe vortices, which is about what is needed to obtain results that are converged in

the number of vortices.

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Make edgesstreamwise

first planform

second planform

y

x

line up spanwisebreaks on a commonbreak, and make theedge streamwise

Model Tips• start simple• crude representation of the planform is all right• keep centroids of areas the same: actual planform to vlm model

Figure 5.41. Example of a vlm model of an aircraft configuration. Note that one side of a symmetrical planform is shown.

Figure 5.42. Definition and reference results for the Warren-12 wing.

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Figure 5.43 Convergence of the lift curve slope and stability with increasing numbers of panels, N s is the number of spanwise panels, Nc is the number of chordwise panels. (from Ref. Error: Reference source not found).

Isolated swept wing example

Next, we show how a vlm calculation compares with experimental data for an isolated wing

case.Error: Reference source not found Here we selected an aspect ratio 10 wing with a quarter

chord sweep of 35° and a taper ratio of 0.5. The airfoil was a 12% thick NACA 65A012 section.

The Mach number is low, 0.14, and the Reynolds number is 6 million for the lift comparison,

and 10 million for the pitching moment comparison. The test was conducted at the NACA Ames

Research Center. The results are given in Fig. 5.44. The agreement for the prediction of lift is

given in Fig. 5.44a. We see very good agreement at low alpha, where the flow is attached. Figure

5.44b compares the pitching moment variation with the lift coefficient. This is one of the most

important considerations in airplane aerodynamics, and the agreement is excellent until the flow

starts to separate at the wingtip and the wing “pitches up”, a problem with swept wings.

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-0.50

0.00

0.50

1.00

1.50

-10.0 -5.0 0.0 5.0 10.0 15.0 20.0

CL

Angle of attack, a, dg.

AR = 10, Λχ/4 = 35°, l = 0.5data ro NACA RM A50K27

M = 0.14, R = 6 illion

VΛMpχ χalχulation

a) lift coefficient

-0.06

-0.04

-0.02

0.00

0.02

0.04

0.06

0.08

-0.4 -0.2 0.0 0.2 0.4 0.6 0.8 1.0 1.2

Cm

CL

AR = 10, Λχ/4 = 35°, l = 0.5data ro NACA RM A50K27

R = 10 illion

x r = χ/4

VΛMpχ χalχulation

b) pitching moment

Figure 5.44 Comparison of VLMpc with wind tunnel data for an isolated wing.66

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Wing-Body-Tail ExampleThe comparison of vlm results with wind tunnel data for a wing-body-tail configuration67 is given in Fig. 5.45. Figure 5.45a shows the configuration, and Figs. 5.45b and c compare the results with the wind tunnel data for the lift and pitching moment coefficients. The effect of the horizontal tail is included in each figure.

a) the model

-0.20

0.00

0.20

0.40

0.60

0.80

1.00

-2.0° 0.0° 2.0° 4.0° 6.0° 8.0° 10.0° 12.0° 14.0°

CL

a

M = 0.60data ro NAΣA TN D-13

Σybolσ: Wind Tunnl DataΛinσ: VΛMpχ prdiχtionσ

Tail on

Tail o

b) liftFigure 5.45 Wing Body Tail case

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-0.40

-0.20

0.00

0.20

0.40

0.60

0.80

1.00

-0.25-0.20-0.15-0.10-0.050.000.05

CL

Cm

M = 0.60

Tail off

Tail on

VLMpc

Wind Tunnel Data

data from NASA TN D-13

c) comparison of pitching moment estimate from VLMpc with wind tunnel data

Figure 5.45 Wing Body Tail case Concluded (NASA TN D-13)

Control Surface Deflection ExampleThe vlm method can also be used to estimate control surface deflection effects. An example is

shown in Fig. 5.46. Because the method is inviscid, and the control device is at the back end of

the surface and subjected to significant viscous effects, the method generally overpredicts the

effectiveness. The case shown is for an NACA 23012 airfoil with a 20% chord plane flap at a

Reynolds number of 8 million.68

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0.0

0.2

0.4

0.6

0.8

1.0

1.2

1.4

0° 10° 20° 30° 40° 50°

VLM and Thin Airfoil Theory CLExperimental Delta CL

DCΛ

lap dlχtion

Flap χhord to airoil χhord ratio = 0.20Rynoldσ nubr = 8 illionWT data ro NACA R 661

Figure 5.46 Control surface deflection effectiveness comparison betweena vlm calculation and wind tunnel data.

Pitch and Roll Damping Estimation ExampleThe vlm method can also be used to predict the value of the pitch and roll damping coefficients,

Cmq and Clp . These characteristics are important in establishing the stability characteristics of

airplanes, and the method described in Etkin69 is easily implemented. Figure 5.47 shows a

comparison of the vlm pitch and roll damping results using another vlm method, JKayVLM, for

an F-18-type airplane compared to estimates from DATCOM,Error: Reference source not found

which we described previously in Chap. 2. The case shows reasonably good, but not perfect

agreement. More details can be found in the report by Kay, et al.Error: Reference source not

found

-7.00-6.00-5.00-4.00-3.00-2.00-1.000.001.00

Mach .2 Mach .6

Data VLM DATCOM

Cm q

a) pitch damping

-0.50

-0.40

-0.30

-0.20

-0.10

0.00

0.10

Mach .2 Mach .6

Data VLM DATCOM

Cl p

b) roll damping

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Figure 5.47 VLM Pitch and roll damping result comparison with data and

DATCOM.Error: Reference source not found

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Classical Linear Theory Computational Aerodynamics 5-67

Slender lifting body results from Jim Pittman70

To illustrate the capability of the vortex lattice method for bodies that are more fuselage-like than wing-like, we present the lifting body comparison of the experimental and vlm results published by Jim Pittman of NASA Langley. Figure 5.48 shows the configuration used. Figure 5.49 provides the results of the vortex lattice method compared with the experimental data. In this case the camber shape was modeled by specifying camber slopes on the mean surface. The model used 138 vortex panels. The bars at several angles of attack illustrate the range of predictions obtained with different panel arrangements. For highly swept wings, leading edge vortex flow effects are included, as described in Chapter 4. Lamar’s program contains the option of using the leading edge suction analogy71 to model these effects.* Remarkably good agreement with the force and moment data is demonstrated in Fig. 5-49. The nonlinear variation of lift and moment with angle of attack arises due to the inclusion of the vortex lift effects. The agreement between data and computation breaks down at higher angles of attack because the details of the distribution of vortex flow separation are not provided by the leading edge suction analogy. The drag prediction is also very good. The experimental drag is adjusted by removing the zero lift drag, which contains the drag due to friction and separation. The resulting drag due to lift is compared with the vlm estimates. The comparisons are good primarily because this planform is achieving, essentially, no leading edge suction (see Katz and Plotkin, Ref. Error: Referencesource not found, pp. 107 and 131-133 to review the leading edge suction concept) and hence the drag is simply CD = CLtana, which is easy to predict, but aerodynamically inefficient.

Figure 5.48. Highly swept lifting body type hypersonic concept (Ref. Error: Referencesource not found).

* The leading edge suction analogy is the empirical observation by Eddie Polhamus, after examining experimental data, that the magnitude of the vortex lift is approximately equal to the value of the leading edge suction for attached flow, but rotated 90°.

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Figure 5.49. Comparison of CL, Cm, and CD predictions with data (Ref. Error: Referencesource not found).

Non-planar results from Kalman, Rodden, and Giesing72

All of the examples presented above considered essentially planar lifting surface cases. The

vortex lattice method can also be used for highly non-planar analysis, and the example cases

used at Douglas Aircraft Company in a classic paperError: Reference source not found have been

selected to illustrate the capability. Several of the cases were re-computed using the JKayVLM

code,Error: Reference source not found and provide an interesting comparison with the original

results from Douglas.

Figure 5.50 provides an example of the results obtained for an extreme non-planar case: the

ring, or annular, wing. In this case the estimates are compared with other theories, and seen to be

very good. The figure also includes the estimate of Cmq. As illustrated above, Cmq and Clp can

be computed using vlm methods, and this capability is included in the John Lamar’s vortex

lattice method, VLMpc.*

* JKayVLM and VLMpc are available on the web at http://www.aoe.vt.edu/~mason/Mason_f/MRsoft.html, together with links to a few other vlm codes.

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Classical Linear Theory Computational Aerodynamics 5-69

Figure 5.50. Predictions by Kalman, Rodden, and GiesingError: Reference source not found using vlm (symbols) of the aerodynamic characteristics of a ring wing, compared with theory (solid lines) and slender wing theory (dashed lines), both from Belotserkovskii. 73

Ground Effects and Dihedral Effects Examples

Figure 5.51 provides an example of the effects of the presence of the ground on the

aerodynamics of simple unswept rectangular wings. The lift and pitching moment slopes are

presented for calculations made using JKayVLM and compared with the results published by

Kalman, Rodden and Giesing,Error: Reference source not found and experimental data. An

image is used below the ground plane to represent grount effect, as described above. The

6 Moran, J. An Introduction to Theoretical and Computational Aerodynamics, John Wiley & Sons, New York, 1984. pp. 103-112, 118-123, 260-287 republished by Dover, 2003.

7 Cebeci, T., An Engineering Approach to the Calculation of Aerodynamic Flows, Horizon Publishing, Long Beach, 1999.

18 Stack, J., Lindsey, W.F., and Littell, R.E., “The Compressibility Burble and the Effect of Compressibility on Pressures and Forces Acting on an Airfoil,” NACA R-646, 1938.

19 Jameson, A., “Acceleration of Transonic Potential Flow Calculations on Arbitrary Meshes by the Multiple Grid Method,” AIAA Paper 79-1458, Proceedings of the AIAA 4th Computational Fluid Dynamics Conference, AIAA, New York, 1979, pp. 122-146.

20 Kroo, Ilan, “Aerodynamic Analyses for Design and Education,” AIAA Paper 92-2664, June 1992.

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agreement between the data and calculations is excellent for the lift curve slope. The AR = 1

wing shows the smallest effects of ground proximity because of the three-dimensional relief

provided around the wing tips. As the aspect ratio increases, the magnitude of the ground effects

increases. The lift curve slope starts to increase rapidly as the ground is approached.

The wings also experience a significant change in the pitching moment slope (aerodynamic

center shift),* and this is also shown. Note that the predictions start to differ as the ground is

approached. JKayVLM actually rotates the entire surface to obtain another solution to use in

estimating the lift curve slope. The standard procedure used by most methods is to simply change

the slope condition at the mean line, as discussed previously in this chapter. Because of the

proximity to the ground, this might be a case where the transfer of the boundary condition may

not be accurate.

* This shift is the reason that ground effects machines cannot just “takeoff” and why WIG vehicles cannot fly out of ground effect.28 Nathman, James K., “Improvement of a Panel Method by Including Panel Warp,” AIAA

Paper 2004-721, Jan. 2004.29 Tinoco, E.N., Ball, D.N., and Rice, F.A. II, “PAN AIR Analysis of a Transport High-Lift

Configuration,” Journal of Aircraft, Vol. 24, No. 3, 1987, pp. 181-188.30 Magnus, A.E., and Epton, M.A., “PAN AIR - A Computer Program for Predicting Subsonic or

Supersonic Linear Potential Flows About Arbitrary Configurations Using a Higher Order Panel Method,” Volume I - Theory Document (Version 1.0), NASA CR 3251, April 1980.

34 Mason, W.H., and Rosen, B.S., “The COREL and W12SC3 Computer Programs for Supersonic Wing Design and Analysis,” NASA CR-3676, Dec. 1983.

35 Van Zyl, L.H., “Unsteady Panel Method for Complex Configurations Including Wake Modeling,” Journal of Aircraft, Vol. 45, No. 1, Jan-Feb. 2008, pp. 276-285.

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1.0

2.0

3.0

4.0

5.0

6.0

7.0

8.0

0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4

CLa

h/χ

AR4

2

1

hU∞

χ

χ/4

36 Public Domain Aeronautical Software, http://www.pdas.com37 Hess, J.L., and Smith A.M.O., “Calculation of Nonlifting Potential Flow About Arbitrary

Three-Dimensional Bodies,” Douglas Report ES40622, Douglas Aircraft Company, 196238 Rubbert, P.E., “Theoretical Characteristics of Arbitrary Wings by a Nonplanar Vortex Lattice

Method,” Boeing Report D6-9244, The Boeing Company, 1964.39 Woodward, F.A., Tinoco, E.N., and Larsen, J.W., “Analysis and Design of Supersonic Wing-

Body Combinations, Including Flow Propertis in the Near Field,” Part I – Theory and Application, NASA CR-73106, 1967.

40 Rubbert, P.E., and Saaris, G.R., “A General Three-Dimensional Potential Flow Method Applied to V/STOL Aerodynamics,” SAE Paper No. 680304, 1968.

41 Hess, J.L., “Calculation of Potential Flow About Arbitrary 3-D Lifting Bodies,” Douglas Report MDC-J5679-01, Oct. 1972.

42 Wooward, F.A., “An Improved Method for the Aerodynamic Analysis of Wing-Body-Tail Configurations in Subsonic and Supersonic Flow,” NASA CR-2228, Parts I and II, 1973.

43 Roberts, A., and Rundle, K., “Computation of First Order Compressible Flow About Wing-Body Configurations,” AERO MA No. 20, British Aircraft Corporaion, Feb. 1973

44 Mercer, J.E., Weber, J.A., and Lesfor, E.P., “Aerodynamic Influence Coeficient Method Using Singularity Splines,” NASA CR-2423, May 1974.

45 Morino, L., and Kuo, C-C, “Subsonic Potential Aerodynamics for Complex Configurations: A General Theory,” AIAA J., Vol. 12, No. 2, pp 191-197, Feb. 1974.

46 Johnson, F.T., and Rubbert, P.E., “Advanced Panel-Type Influence Coefficient Methods Applied to Subsonic Flow,” AIAA Paper no. 75-50, Jan. 1975.

47 Ehlers, F.E., and Rubbert, P.E., “A MAch Line Panel Method for Computingthe Linearized Supersonic Flow,” NASA CR-152126, 1979.

48 Ehlers, F.E., Epton, M.A., Johnson, F.T., Magnus, A.E., and Rubbert, P.E., “A Higher Order Panel Method for Linearized Flow,” NASA CR-3062, 1979.

49 Bristow, D.R., “Development of Panel Methods for Subsonic Analysis and Design,” NASA CR 3234, 1980.

50 Hess, J.L., and Friedman, D.M., “An Improved Higher Order Panel Method for Three-Dimensional Lifting flow,” Douglas Aircraft Co. Report No. NADC-79277-60, 1981.

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-0.40

-0.30

-0.20

-0.10

0.00

0.10

0.20

0.0 0.2 0.4 0.6 0.8 1.0 1.2 1.4

CMa

h/χ

AR = 1

AR = 2

AR = 4

Figure 5.51. Example of ground effects for a simple rectangular wing. Dashed lines from Kalman, Rodden, and Giesing,Error: Reference source not found, solid lines are predictions by JKayVLM.Error: Reference source not found Symbols are experimental results by Sanders.74 Pitching moment reference taken about the quarter chord.

51 Maskew, B., “Prediction of Subsonic Aerodynamic Characteristics: A Case for Lower Order Panel Methods,” Journal of Aircraft, Vol. 19, no. 2, 1982 pp. 157-163..

52 Coopersmith, R.M., Youngren, H.H., and Bouchard, E.E., “Quadrilateral Element Panel Method (QUADPAN),” Lockheed-California Rpt. LR 29671, 1981.

53 Vortex Lattice Utilization, NASA SP-405, May 197654 Margason, R.J., and Lamar, J.E., “Vortex-Lattice FORTRAN Program for Estimating

Subsonic Aerodynamic Characteristics of Complex Planforms,” NASA TN D-6142, Feb. 197155 Lamar, J.E., and Gloss, B.B., “Subsonic Aerodynamic Characteristics of Interacting Lifting

Surfaces With Separated Flow Around Sharp Edges Predicted by a Vortex-Lattice Method,” NASA TN D-7921, 1975

56 Lamar, J.E., and Herbert, H.E., “Production Version of the Extended NASA-Langley Vortex Lattice FORTRAN Computer Program,” Vol. I, User’s Guide, NASA TM 83303, 1982 (requires update packet, July, 1984)

57 Herbert, H.E, and Lamar, J.E., “Production Version of the Extended NASA-Langley Vortex Lattice FORTRAN Computer Program,” Vol. II, Source Code, NASA TM 83304, 1982

58 Drela, M., and Youngren, H., AVL, An extended Vortex Lattice Method, http://web.mit.edu/drela/Public/web/avl.

59 Melin, T., Tornado, http://www.redhammer.se/tornado/60 Miranda, L.R., Eliott, R.D., and Baker, W.M., “A Generalized Vortex Lattice Method for

Subsonic and Supersonic Flow Applications,” NASA CR-2865, Dec. 1977.61 Albright, A.E., Dixon, C.J., and Hegedus, M.C., “Modification and Validation of Conceptual

Design Aerodynamic Prediction Method HASC95 With VTXCHN,” NASA CR 4712, March 1996.

62 Nathman, J.K., and McComas, A., “Comparison of Stability and Control Calculations from Vortex Lattice and Panel Methods,” AIAA Paper 2008-314, Jan., 2008.

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Figure 5.52 presents similar information for the effect of dihedral angle on a wing. In this

case the effects of anhedral, where the wing tip approach the ground, are extremely large. The

results of dihedral changes for a wing out of ground effect are shown for comparison. Both

methods agree well with each other, with differences appearing only as the wingtips approach

the ground. Here again, JKayVLM actually rotates the entire geometry, apparently resulting in

an increase in the effects as the tips nearly contact the ground. It also prevents calculations from

being obtained as close to the ground as the published results. In making these calculations it was

discovered that the wing panel was rotated and not sheared, so that the projected span decreases

as the dihedral increases, and this produces much more pronounced changes in the lift curve

slope due to the reduction in projected span.

66 Tinling, B.E., and Kolk, W.R., “The Effects of Mach Number and Reynolds Number on the Aerodynamic Characteristics of Several 12-Percent-Thick Wings Having 35° of Sweepback and Various Amounts of Camber,” NACA RM A50K27, Feb. 1951.

67 Stivers, Louis S., Jr., “Effectiveness of an All-Movable Horizontal Tail on an Unswept-Wing and Body Combination for Mach Numbers from 0.60 to 1.40,” NASA TN D-13, Aug. 1959.

68 Abbott, Ira H., and Greenberg, Harry, “Test in the Variable-Density Wind Tunnel of the NACA 23012 Airfoil with Plain and Split Flaps,” NACA R No. 661, 1938.

70 Pittman, J.L., and Dillon, J.L., “Vortex Lattice Prediction of Subsonic Aerodynamics of Hypersonic Vehicle Concepts,” Journal of Aircraft, Vol. 14, No. 10, 1977, pg 1017-1018.

72 Kalman, T.P., Rodden, W.P., and Giesing, J., “Application of the Doublet-Lattice Method to Nonplanar Configurations in Subsonic Flow,” Journal of Aircraft, Vol. 8, No. 6, 1971, pp. 406-415.

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0

2

4

6

8

10

12

-40° -30° -20° -10° 0° 10° 20° 30° 40°

CLa

Dihdral angl,

h/χ = 0.5

h/χ = 1

h/χ = ∞

Σolid linσ: χoputd uσing JKayVΛMDaσhd linσ: ro Kalan, Roddn, and iσingARr = 4, Planor rotatd by th dihdral angl, .

Not: Moσt o th dχraσ in lit χurv σlop or th ωing out o groundχt iσ du to th χt o rduχd σpan aσ th ωing rotatσ roth zro dihdral χondition

h

Figure 5.52. Example of ground effects for a wing with dihedral (a case from Kalman, Rodden and Giesing, Ref. Error: Reference source not found), including a comparison with results from JKayVLM (Ref. Error: Reference source not found)

5.3.4 Inverse Design Methods and Program DesCam

Although most of the analysis discussed above corresponds to the analysis problem, the

design problem can also be treated. In this section we provide one example: the determination of

the camber line shape required to obtain a specific chord load in the two dimensional case. We

take the opportunity to illustrate a method due to LanError: Reference source not found that uses

a mathematically based selection of vortex and and control point placements instead of the 1/4 -

3/4 rule used above.

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Recall that a line of vortex singularities induces a vertical velocity on the singularity line

given by (see Chapter 4 and Karamcheti.Error: Reference source not found)

w(x) =−12p

g( ′x )x− ′x

0

χ⌠

⌡⎮⎮ d ′x . (5.65)

In thin wing theory the vertical velocity, w, can be related to the camber line slope as shown in

Eq. 5.51. Vortex strength can be related to the streamwise velocity by g =ul V∞ − uu V∞ , where

the induced velocities are anti-symmetric above and below the camber line. This in turn can be

used to relate the vorticity to the change in pressure, DCp through Eq. 5.56:

DCp = Cpl− Cpu

= −2ul

V∞

⎛⎝⎜

⎞⎠⎟

− −2uu

V∞

⎛⎝⎜

⎞⎠⎟

= 2uu

V∞

−ul

V∞

⎛⎝⎜

⎞⎠⎟

(5.66)

which leads to: DCp (x)

2= γ (x) (5.67)

resulting in the expression for camber line slope in terms of design chord load:

8 Karamcheti, K., Principles of Ideal-Fluid Aerodynamics, 2nd Rev. Ed., Krieger Publishing, Melpourne, 1980.

14 Kuethe, A.M., and Chow, C-Y., Foundations of Aerodynamics, 5th Ed., John Wiley, New York, 1998, pp. 156-164.

15 Wauquiez, Christian, http://www.nada.kth.se/~chris/pablo/pablo.html, Pablo theory described as part of his Licentiate’s Thesis, “Shape Optimization of Low Speed Airfoils using MATLAB and Automatic Differentiation,” KTH, Stockholm, 2000.

16 Drela, M., “XFOIL: An Analysis and Design System for Low Reynolds Number Airfoils,” in Low Reynolds Number Aerodynamics, Mueller, T.J., ed., Lecture Notes in Engineering No. 54, Springer Verlag, 1989. http://web.mit.edu/drela/Public/web/xfoil/

21 Volpe, G., “Inverse Airfoil Design: A Classical Approach Updated for Transonic Applications,” in Applied Computational Aerodynamics, ed. by P.A. Henne, AIAA Progress in Astronautics and Aeronautics, Vol. 125, AIAA, New York, 1990, pp. 191-220.

22 Labrujere, Th. E., and Sloof, J.W., “Computational Methods for the Aerodynamic Design of Aircraft Components,” Ann. Rev. of Fluid Mech., 1993, Vol. 25, pp.183-214.

23 Bristow, D.R., “A New Surface Singularity Method for Multi-Element Airfoil Analysis and Design,” AIAA Paper 76-20, Jan. 1976.

24 Aidala, P.V., Davis, W.H., Jr., and Mason, W.H., “Smart Aerodynamic Optimization,” AIAA Paper 83-1863, July 1983.

25 PAN AIR User’s Class Short Course Presentation Material, 1981.26 Hess, J. L. “The Problem of Three-Dimensional Lifting Potential Flow and Its Solution by

Means of Surface Singularity Distributions,” Computer Methods in Applied Mechanics and Engineering, Vol. 4, 1974. pp. 283-319.

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dzdx

=−14p

DCp

x− ′x0

χ⌠

⌡⎮⎮ d ′x . (5.68)

Here dz/dx includes the slope due to the angle of attack. Note that the integral contains a

singularity, and this singularity introduces the extra complications that require special analysis

for numerical integration. The original Lan theory (Ref. Error: Reference source not found) was

27 Carmichael, R.L., and Erickson, L.L., "PAN AIR - A Higher Order Panel Method for Predicting Subsonic or Supersonic Linear Potential Flows About Arbitrary Configurations," AIAA Paper No. 81-1255, June 1981.

3 Hess, J. L., “Panel Methods in Computational Fluid Dynamics,” Ann. Rev. of Fluid Mech., Vol. 22, 1990, pp. 255-274.

4 Hess, J.L., “Linear Potential Schemes,” Applied Computational Aerodynamics, P.A. Henne, ed., AIAA, Washington, 1990. pp.21-36.

5 Katz, J., and Plotkin, A., Low-Speed Aerodynamics, 2nd Edition, Cambridge University Press. Cambridge, 2001.

13 Houghton, E.L., and Carpenter, P.W., Aerodynamics for Engineering Students, 4th Ed., Halsted Press, New York, 1993, pp. 257-265, 203-211. (code removed from the 5th Ed.)

31 Margason, R.J., Kjelgaard, S.O., Sellers, W.L., Moriis, C.E.K., Jr., Walkley, K.B., and Shields, E.W., “Subsonic Panel Methods - A Comparison of Several Production Codes,” AIAA Paper 85-0280, Jan. 1985.

32 Ashby, D.L., Dudley, M.R., Iguchi, S.K., Browne, L., and Katz, J., “Potential Flow Theory and Operation Guide for the Panel Code PMARC,” NASA TM 102851, Jan. 1991.

33 Nathman, J.K., “Subsonic Panel Methods – Second (Order) Thoughts,” AIAA Paper 98-5563. Sept. 1998.

63 Lan, C.E., “A Quasi-Vortex-Lattice Method in Thin Wing Theory”, Journal of Aircraft, Vol. 11, No. 9, September 1974, pp. 518-527.

64 Mook, D.T., and Nayfeh, A.H., “Application of the Vortex-Lattice Method to High-Angle-of-Attack Subsonic Aerodynamics,” SAE Paper No. 851817, October, 1985.

65 Jacob Kay, W.H. Mason, W. Durham, F. Lutze and A. Benoliel, “Control Power Issues in Conceptual Design: Critical Conditions, Estimation Methodology, Spreadsheet Assessment, Trim and Bibliography,” VPI-Aero-200, November 1993. (software and report available, http://www.aoe.vt.edu/~mason/Mason_f/MRsoft.html )

69 Etkin, B., Dynamics of Flight—Stability and Control, 2nd Ed., John Wiley & Sons, New York, 1982.

71 Polhamus, E.C., “Prediction of Vortex Lift Characteristics by a Leading-edge Suction Analogy,” Journal of Aircraft, Vol. 8, No. 4, 1971, pp. 193-199.

73 Belotserkovskii, S.M., The Theory of Thin Wings in Subsonic Flow, Plenum Press, New York, 1967.74 Saunders, G.H., “Aerodynamic Characteristics of Wings in Ground Proximity,” Canadian

Aeronautics and Space Journal, June 1965, pp. 185-192.

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Classical Linear Theory Computational Aerodynamics 5-77

used to find DCp (in a slightly different form), but it can also be used to obtain dz/dx directly

from DCp . To do this, Lan derived a summation formula to obtain the slope. Once the slope is

known, it is integrated to obtain the camber line.

Lan showed that the integral in Eq. (5.68) can be found very accurately from the summation:

dzdx i

=−1N

DCp

4xκ(1−xκ)xi −xκκ=1

N

∑ (5.69)

where:

xk =12

1−χoσ2κ−1( )p2N

⎧⎨⎩⎫⎬⎭

⎡⎣⎢

⎤⎦⎥

κ=1,2,...,N (5.70)

and:

xi =12

1−χoσipN

⎧⎨⎩⎫⎬⎭

⎡⎣⎢

⎤⎦⎥

i =0,1,2,...,N . (5.71)

Here N + 1 is the number of stations on the camber line at which the slopes are obtained.

Given dz/dx, the camber line is then computed by integration using the trapezoidal rule

(marching forward starting at the trailing edge):

zi+1 =zi −xi+1 −xi

2⎡⎣⎢

⎤⎦⎥

dzdx i

+dzdx i+1

⎡⎣⎢

⎤⎦⎥

. (5.72)

The design angle of attack is then:

aDES = tan−1 z0(5.73)

The camber line can then be redefined in standard nomenclature, i.e., z(x=0) = z(x=1) = 0.0:

zi =zi −(1−xi)tanaDEΣ (5.74)

How well does this work? Program DesCam implements the method described here, and the

user’s manual is provided in App. C. Here we compare the results from DesCam with the

analytic formula given in Appendix A for the NACA 6 Series mean line with a = 0.4. The results

are shown in Figure 5.53 below. The camber scale is greatly enlarged to demonstrate the

excellent comparison. Even though the chord load is constructed by two straight-line segments,

the resulting required camber line is highly curved over the forward portion of the airfoil. Note

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that thin airfoil theory allows only two possible values for the pressure differential at the leading

edge, zero or infinity. A close examination of the camber line shape required to produce a finite

load reveals a singularity, since the slope is infinite. This feature is much easier to study using

the analytic solution, as given in Appendix A. This approach can easily be extended to three

dimensions. Notice that the design problem is direct, in that it does not require the solution of a

system of equations.

0.00

0.02

0.04

0.06

0.08

0.10

0.12

-0.50

0.00

0.50

1.00

1.50

2.00

0.0 0.2 0.4 0.6 0.8 1.0

(Z-Z0)/C - DesCamZ/C - from Abbott & vonDoenhoff

z/cDCP

x/χ

Dσign ChordΛoading

(z-z0)/χ - DσCa

z/χ - ro thin airoil thory

Figure 5.53. Example and verification of camber design using DesCam.

5.3.5 Alternate and Advanced vlm MethodsMany variations of the vortex lattice method have been proposed over the years. They

address both the improvement in accuracy for the traditional case with a planar wake, and

extensions to include wake position and rollup as part of the solution. The traditional vortex

lattice approaches assume that the wing wake remains flat and aligned with the freestream. This

assumption is acceptable for most cases, although not technically correct. The effect of the wake

on the wing that generates it is small unless the wing is highly loaded. However, the interaction

between the wake from an upstream surface and a trailing lifting surface can be influenced by the

rollup and position.

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In the basic case where the wake is assumed to be flat and at a specified location, the primary

extensions of the method have been directed toward improving the accuracy using a smaller

number of panels. Hough75 demonstrated that improvement in accuracy could be achieved by

using a lattice that was slightly smaller than the true planform area. Basically, he proposed a 1/4

panel width inset from the wing tips.

Perhaps the most important revision of the vortex lattice method was proposed by LanError:

Reference source not found, and called the “quasi vortex lattice method.” In this method Lan

used mathematical methods, rather than the more heuristic arguments described above, to find an

approximation for the thin airfoil integral in the streamwise direction. The result was, in effect, a

method where the vortex and control point locations were established from the theory of

Chebychev polynomials to obtain an accurate value of the integrals with a small number of

panels. The mathematically based approach also led to an ability to compute leading edge

suction very accurately.

The wake rollup and position problem has been addressed by MookError: Reference source

not found among others, and his work should be consulted for details. A method similar to

Mook’s has been presented in the book by Katz and Plotkin.Error: Reference source not found

They propose a vortex ring method, which has advantages when vortices are placed on the true

surface of a highly cambered shapes.

5.3.6 Unsteady flow extension

Extensions to include unsteady flow have also been made. For the case of harmonically

oscillating surfaces and an assumed flat wake the extension was given by Albano and Rodden.76

In this case the vortex is augmented with an oscillating doublet, and the so-called doublet-lattice method is obtained. The doublet-lattice method is widely used for subsonic flutter

calculations. Kalman, Giesing, and RoddenError: Reference source not found provide additional

details and examples (they also demonstrated the highly nonplanar capability of the vlm method

as given above). A refinement to this method and an investigation of panel density requirements

was made by Rodden at al.77,78

A general unsteady flow calculation method, including wake rollup and incorporation of

leading edge vortices has been developed by Mook and co-workers.Error: Reference source not

found Katz and PlotkinError: Reference source not found also describe vlm methods for

unsteady motion in some detail, and biologically inspired interest in flapping flight has also led

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to the development of general unsteady methods.79 The resulting codes have the potential to be

used to model time accurate aerodynamics of vehicles in arbitrary maneuvering flight, including

the high angle of attack cases of interest in fighter aerodynamics. These methods are also

currently being used in studies where the aircraft aerodynamics is coupled with advanced control

systems as well as structural dynamics. In this case active control is incorporated and adverse

aeroelastic behavior can suppressed.

5.3.7 Summary

The summary provided above illustrates the current state of affairs. Classical vortex lattice

methods, per se, are not currently being developed. However, unsteady methods continue to be

developed. The steady flow methods are continuously used in a variety of applications for

conceptual design trade studies and in advanced simulation methods where several disciplines

are being studied simultaneously and an affordable model of the aerodynamics is required. They

are also widely used in conceptual design and the early stages of aircraft preliminary design.

5.4 Project

Use WinVorView to solve the aerodynamics of the T-38 aircraft at a variety of conditions. WinVorView is a GUI program written to run VorlaxError: Reference source not found on a PC; Vorlax is a vortex lattice program. You should do the following prior to starting your project in order to become familiar with the program and its use.

Drag the WinVorView folder onto the top level of your C: drive (i.e. C:\WinVorView; DO NOT run from from your Desktop!)

The folder has a hermite file for the T-38 (a hermite file is a simplified geometry file). Double click on the program and open the T-38 file (the view is not to scale, so resize the

window to make the T-38 look better). Try the different views (View, Hermite, etc.). The first thing to do is slice the geometry (Actions, Slice Geometry) . . . make sure you

have enough slices to adequately model the inlet, etc. The number of slices must be an odd number—at least 51 slices should be used. Reslicing the control surfaces is OK. Treat the geometry as “flat”.

Now run Vorlax (Actions, Run Vorlax, Create). You need to go through the wizard and input the required geometric variables (be sure to tab through the input boxes, otherwise you won’t be able to proceed to the next window). Specify “symmetric” geometry/flight conditions and use cosine chordwise panel spacing. Once the input file is complete, run the cases. Note: make sure you are saving the results in the same directory as your hermite file and name the output files with the same name as the hermite file. The digital output will be in “t-38.cof”. 

The basic geometric parameters for the T-38 are:

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Wing area, S: 170 ft2Aspect ratio, AR: 3.75Taper ratio, l : 0.30

Other geometric dimensions for the T-38 can be found in Introduction to Aeronautics, Appendix B.80 You will need this information to properly predict the aerodynamic coefficients. Set the X and Z moment reference centers and the height above the ground to 0.0.

The first thing you should do is perform a “panel sensitivity study” on the configuration. Run WinVorView at α = 10o and M = 0.4 with 100 vortex panels and find the resulting CL and CD. Now rerun with 200 panels, 300 panels, etc., until you find the number of panels that give you “converged” results. You may need to continue this up to 1500 or more panels! Graph your results (CL and CD vs. # panels) and comment on the results as appropriate.

Now run the program for the following combination of conditions: M = 0.0, 0.4, 0.8 and α = 0o, 2o , 4o , 6o , 8o, 10o, 12o, 14o, 16o, 18o. Graph the results for CL and CD as a function of angle of attack, with one graph for each Mach number (you can plot both coefficients on one graph by using two vertical scales if you want). Since the vortex lattice program only predicts drag due to lift, you should add the experimental value of zero-lift drag coefficient to your results. For the CL

and CD results at M = 0.4, compare with the actual aircraft data. Also for M = 0.4 compare your results with the theoretical values you obtain using the theoretical lift-curve slope for a wing:81

CLa=

2pAR

2 + 4 + AR 2b 2(1+tan2 Λb 2 )

Where the 2p term in the numerator is the classical 2D thin airfoil theory lift curve slope per radian, AR is the aspect ratio, b2/Sref, b = 1− M∞

2 , and Λ is the sweep of the max thickness line. You should correct the theoretical lift-curve slope and for compressibility using the Prandtl-Glauert rule (Ref. Error: Reference source not found):

21

)0(

==

M

MCC Λ

Λa

a

Data for the T-38 are given below.

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from Brandt, et al (Ref. Error: Reference source not found)

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from Brandt,

from Brandt, et al (Ref. Error: Reference source not found)

Comment on how well the vortex lattice program was able to predict the aerodynamics of the vehicle. What did it do well? What didn’t it do well? What didn’t it do at all? How well did the results of the program compare with both the aircraft data and the theoretical values? Comment on the shortcomings relative to the assumptions for a potential flow method.

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5.5 Exercises

1. Program PANEL (or an equivalent 2D panel method).

a) Obtain a copy of program PANEL and the sample case.b) Convert PANEL to run on your PC.c) Run the sample case: NACA 4412, 20 pts. upper, 20 pts. lower, a = 4° , and verify

against sample case.d) Document

i) compile time required on your PC(cite computer and compiler used)

ii) the execution time for the sample caseiii) the accuracy relative to the sample case.iv) the exact modifications required to make the code

work on your computer

2. Start work on program PANEL

a) Save a reference copy of the working code!b) Check convergence with panels (NLOWER+NUPPER must be less than 100

currently). How many panels do you need to get results independent of the number of panels? What happens to the computer time as the number of panels increases?

c) Check the coordinates generated by the airfoil routine vs. exact (consider using the NACA 0012, see App. A for geometry definition), including examination of the coordinates at the trailing edge. This is best done by making a table of exact and computed values at selected values of x/c. What did you find out?

d) Locate the source strengths, and sum the source strengths x panel lengths to get the total source strength. Does it sum to zero? Should it?

e) Where is the moment reference center in this code?Submit an assessment of your findings.

3. Modify program PANEL:

You need a version of PANEL that will allow you to compute the pressure distribution on arbitrary airfoils. This exercise will give you this capability. Modify the code to interpolate input airfoil points to the program defined surface points, x/c. The resulting code should:a) accept arbitrary airfoil input datab) echo all the input data on the outputc) generate an output file for post processing (both for plotting and as the input to a boundary layer code)d) output Cm about the airfoil quarter chord point.Hint: Don’t alter the panel distribution. The paneling scheme should be independent of the input distribution of airfoil coordinates. This produces a much more general and accurate program. This problem is usually solved by finding both the x/c and y/c values as functions of the airfoil arc length, starting at the lower surface trailing edge. A spline fit is usually used to interpolate the values along the arc length.

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Check your modified code. Run the airfoil you ran previously with internal coordinate generation. This time use an input file with the same coordinates as external inputs. Submit a description of your work, and assess your results.

4. Assess the accuracy of incompressible potential flow theory. Run your modified PANEL code using the airfoil you selected in the exercise in Chap. 1. (What happens if your airfoil has a trailing edge with finite thickness? What do you do now?)

- compare the computed pressure distribution with the experimental data- compare the computed force and moment results with the data (over a range of angles of attack

Turn in a CONCISE report describing the results of your work. Include a plot showing the pressure distribution comparison, and a plot(s) showing comparison with forces and moments. What do you conclude about the accuracy of this method?

5. Airfoil design using program PANEL

Take your reference airfoil:

a) add thickness on the bottom (mid chord)- what happens? b) shave some thickness off the bottom (mid chord) - ? c) add thickness on the top (mid chord)- what happens? d) deflect the trailing edge down a couple of degrees (how sensitive is the airfoil to changes at the TE?)

Hint: use smooth d's to the reference foil employing analytic formulas.

Turn in a CONCISE report comparing the effects on the pressure distribution due to the above modifications.

6. How good is thin airfoil theory? Compare the thin airfoil DCp for a flat plate with program PANEL.

Recall thin airfoil theory for an uncambered flat plate:

DCp = 4α1− x/c( )

x/c.

a) pick an NACA 0012 airfoil at a = 2° and 12° and run PANEL.b) plot DCp/a as a function of x/c.c) how many panels do you need to get a converged solution from PANEL?d) what conclusions do you reach?

7. Obtain a copy of XFOIL and compare the results you obtained in Exercise 6.

8. Get a copy of VLMpc from the web site, or an equivalent 3D vlm method. Install the program on your personal computer and repeat the sample case, checking that your output is the same as the sample output files. Study the output to familiarize yourself with the variety of information generated. Turn in a report describing your efforts (not the output), including any mods required to make the code run on your computer.

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9. How good is thin airfoil theory? Compare the thin airfoil theory DCp for a 2D flat plate airfoil with program VLMpc.

Flat plate thin airfoil theory:

DCP = 4α1− x /c( )

x /c

i. Pick an aspect ratio 10 unswept wing at a = 3° and 12° and run VLMpc.ii. Plot (DCp)/a as a function of x/c at the wing root. iii. How many panels do you need to get a converged solution from VLM?iv. What conclusions do you reach?

10. Compare the validity of an aerodynamic strip theory using VLMpc. Consider an uncambered, untwisted wing, AR = 4, l = .4, Λle = 50°, at a lift coefficient of 1. Plot the spanload, and the DCp distribution at approximately the center section, the midspan station, and the 85% semispan station. Compare your results with a spanload constructed assuming that the wing flow is approximated as 2D at the angle of attack required to obtain the specified lift. Also compare the chordloads, DCp, at the three span stations. How many panels do you need to obtain converged results. Document your results. Do you consider this aerodynamic strip theory valid based on this investigation? Comment.

11. Compare the wing aerodynamic center location relative to the quarter chord of the mac for the wing in exercise 10, as well as similar wings. Consider one wing with zero sweep on the quarter chord, and a forward swept wing with a leading edge sweep of -50°. Compare the spanloads. Document and analyze these results. What did you learn from this comparison?

12. For the wings in exercise 11, compare the section lift coefficients. Where would each one stall first? Which wing appears to able to reach the highest lift coefficient before the section stalls.

13. For the problem in exercise 12, add twist to each wing to obtain near elliptic spanloads. Compare the twist distributions required in each case.

14. Pick a NASA or NACA report describing wind tunnel results for a simple one or two lifting surface configuration at subsonic speeds. Compare the lift curve slope and stability level

75 Hough, Gary R., “Remarks on Vortex-Lattice Methods,” Journal of Aircraft, Vol. 10, No. 5, 1973, pp. 314-317.

76 Albano, E., and Rodden, W.P., “A Doublet-Lattice Method for Calculating Lift Distributions on Oscillating Surfaces in Subsonic Flows,” AIAA J., Vol. 7, No. 2, February 1969, pp. 279-285; errata AIAA J., Vol. 7, No. 11, 1969, p. 2192.

77 Rodden, W.P., Taylor, P.F. and McIntosh, S.C. Jr., “Further Refinement of te Subsonic oublet-Lattice Method,” Journal of Aircraft, Vol. 35, No. 5, Sept-Oct 1998, pp. 720-727.

78 Rodden, W.P., Taylor, P.F., McIntosh, S.C., Jr. and Baker, M.L., “Further Convergence Studies of the Enhanced Doublet-Lattice Method,” Journal of Aircraft, Vol. 36, No. 4, July-Aug 1999, pp. 682-688.

79 Fritz, T.E., and Long, L.N., “Object-Oriented Unsteady Vortex Lattice Method for Flapping Flight,” Journal of Aircraft, Vol. 41, No. 6, Nov-Dev 2004, pp. 1275 –1289.

80 Brandt, S.A., Stiles, R.J., Bertin, J.J., and Whitford, R., Introduction to Aeronautics: A Design Perspective, Reston, VA: AIAA, 1997.

81 Nicolai, L.M., Fundamentals of Aircraft Design, METS, Inc., San Jose, 1975

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predicted by VLMpc with wind tunnel data. Submit a report describing your work and assessing the results.

15. Add a canard to the aft and forward swept wings analyzed in exercise 11. Plot the sum of the spanloads. How does the canard effect the wing spanload.

16. Consider the wings in exercise 15. How does lift change with canard deflection? Add an equivalent tail. Compare the effect of tail or canard deflection on total lift and moment. Did you learn anything? What?

17. Construct a design code using the 1/4 - 3/4 rule and compare with DESCAM.18. Construct a little 2D code to study ground effects.19. Compare wing and wing/tail(canard) results for CLa with standard analytic formulas.

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5.6 References

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