The Sears–Haack body is the shape with the lowest theoretical wave drag in supersonic flow, for a slender solid body or revolution with a given body length and volume. The mathematical derivation assumes small-disturbance (linearized) supersonic flow, which is governed by the Prandtl–Glauert equation. The derivation and shape were published independently by two separate researchers: Wolfgang Haack in 1941 and later by William Sears in 1947.[1] [2] [3]
The Kármán–Moore theory indicates that the wave drag scales as the square of the second derivative of the area distribution,
Dwave\sim[S''(x)]2
S(x)
The cross-sectional area of a Sears–Haack body is
S(x)=
16V | |
3L\pi |
[4x(1-x)]3/2=\pi
2[4x(1-x)] | |
R | |
max |
3/2,
its volume is
V=
3\pi2 | |
16 |
2 | |
R | |
max |
L,
its radius is
r(x)=
3/4 | |
R | |
max[4x(1-x)] |
,
the derivative (slope) is
r'(x)=
-1/4 | |
3R | |
max[4x(1-x)] |
(1-2x),
the second derivative is
r''(x)=
-5/4 | |
-3R | |
max\{[4x(1-x)] |
(1-2x)2+2[4x(1-x)]-1/4\},
where:
Rmax
From Kármán–Moore theory, it follows that:
Dwave=-
1 | |
4\pi |
\rhoU2
\ell | |
\int | |
0 |
\ell | |
\int | |
0 |
S''(x1)S''(x2)ln|x1-x2|dx1dx2,
alternatively:
Dwave=-
1 | |
2\pi |
\rhoU2
\ell | |
\int | |
0 |
S''(x)dx
x | |
\int | |
0 |
S''(x1)ln(x-x1)dx1.
These formulae may be combined to get the following:
Dwave=
64V2 | |
\piL4 |
\rhoU2=
| |||||||
4L2 |
\rhoU2,
C | |
Dwave |
=
24V | |
L3 |
=
| |||||||
2L2 |
,
where:
Dwave
C | |
Dwave |
\rho
According to Kármán–Moore theory, the wave drag force is given by
F=-
\rhoU2 | |
2\pi |
l | |
\int | |
0 |
l | |
\int | |
0 |
S''(\xi1)S''(\xi2)ln|\xi2-\xi1|d\xi1d\xi2
where
S(x)
x=0
x=l
S(x)
f(x)=S'(x)
f=-l
infty | |
\sum | |
n=2 |
An\sinn\theta, x=
l | |
2 |
(1-\cos\theta)
where
0\leq\theta\leq\pi
n=2
S(0)=S(l)=0
x | |
S(x)=\int | |
0 |
f(x)dx, V=
l | |
\int | |
0 |
S(x)dx=
\pi | |
16 |
l3A2.
Note that the volume of the body depends only on the coefficient
A2
To calculate the drag force, first we shall rewrite the drag force formula, by integrating by parts once,
F=p.
\rhoU2 | |
2\pi |
l | |
\int | |
0 |
l | |
\int | |
0 |
f(\xi1)f'(\xi
|
in which
p.v.
f
p.v.
\pi | |
\int | |
0 |
\cosn\theta2 | |
\cos\theta2-\cos\theta1 |
d\theta2=
\pi\sinn\theta1 | |
\sin\theta1 |
,
\pi | |
\int | |
0 |
\sinn\theta1\sinm\theta1d\theta1=
\pi | |
2 |
\begin{cases}1(m=n),\ 0,(m ≠ n).\end{cases}
The final result, expressed in terms of the drag coefficient
Cd=F/\rhoU2l2/2
Cd=
\pi | |
4 |
infty | |
\sum | |
n=2 |
n
2. | |
A | |
n |
Since
V
A2
F
An=0
n\geq3
Thus, setting
An=0
n\geq3
S=(1/3)l3A2\sin3\theta
Cd=
128 | \left( | |
\pi |
V | |
l3 |
| |||||
\right) | \left( |
Smax | |
l2 |
\right)2, R(x)=
8\sqrt2 | \left( | |
\pi |
V | |
3l4 |
\right)1/2[x(l-x)]3/4,
where
R(x)
x
The Sears–Haack body shape derivation is correct only in the limit of a slender body.The theory has been generalized to slender but non-axisymmetric shapes by Robert T. Jones in NACA Report 1284.[5] In this extension, the area
S(x)
x
x=constant
A superficially related concept is the Whitcomb area rule, which states that wave drag due to volume in transonic flow depends primarily on the distribution of total cross-sectional area, and for low wave drag this distribution must be smooth. A common misconception is that the Sears–Haack body has the ideal area distribution according to the area rule, but this is not correct. The Prandtl–Glauert equation, which is the starting point in the Sears–Haack body shape derivation, is not valid in transonic flow, which is where the area rule applies.