Thwaites Solution
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Transcript of Thwaites Solution
Momentum Integral Equation
• In the previous lecture it was shown that
the momentum integral equation can be
written as
• or
xu2dy
0Ue x
udy0
Ue
Ue
x=
w (1)
d
dx+ H + 2( )
Ue
dUe
dx=c f2
(2)
Solutions
• In this lecture, solutions of the momentum integral will be presented.
• The equation has three unknowns: – Momentum thickness
– Displacement thickness
– Wall shear
• Additional information is needed in order to solve the equation.
• Two methods for obtaining such information will be discussed: – Pohlhausen’s polynomial solution
– Thwaites’ correlation method
Assumed profiles
• Both methods are based on the same
premise:
• A family of profile functions is chosen,
such that it can describe the entire
boundary layer velocity field, u(x,y):
u x,y( )Ue
= f ;P( )
=y
x( )
P is a profile
parameter that
determines the shape of the local velocity
profile
Pohlhausen polynomial
solution
• Ernst Pohlhausen (another one of
Prandtl’s researchers) used an
approximate fourth order polynomial
profile function.
• The boundary conditions are:
u x,y( )Ue
= f ( ) = a1 + a22+ a3
3+ a2
4
y = 0 : u = v = 0
y = : u =Ue, u
y= 0
= 0 : f 0( ) = 0
= 1: f 1( ) = 1, f 1( ) = 0or
More Conditions
• More conditions are needed in order to
calculate the unknown coefficients a1, a2 etc.
• Consider the case where y=0. The
boundary layer equation is:
• Then a further condition is:
u y = 0( )u
x y=0
+ v y = 0( )u
yy=0
=Ue
Ue
x+
2u
y 2y=0
2u
y 2y=0
=Ue Ue
x f 0( ) =
2 Ue
x=or
Even More Conditions
• Now differentiate the boundary layer
equation with respect to y:
• At y=0 this becomes:
• Additionally, continuity at y= requires
that:
u
y
u
x+ u
2u
x y+
v
y
u
y+ v
2u
y 2=
3u
y 3
3u
y 3 = 0 or f 0( ) = 0
= 1: f 1( ) = f 1( ) = f 1( ) = = f n( ) 1( ) = 0
Substitution
• Substituting the polynomial in these
conditions yields:
f 1( ) = a1 + a2 + a3 + a4 = 1
f 1( ) = a1 + 2a2 + 3a3 + 4a4 = 0
f 1( ) = 2a2 + 6a3 +12a4 = 0
f 1( ) = 6a3 + 24a4 = 0
f iv 1( ) = 24a4 = 0
f 0( ) = 2a2 =
f 0( ) = 6a3 = 0
Now there’s too many conditions.
We need to choose to satisfy only
four of them. The form of function f( ) is determined by the conditions
we choose.
Note: This choice is dictated by the
fact that the polynomial is 4th order.
For a 12th order polynomial we can
satisfy 12 conditions. The higher
the order the less approximate the
function.
Pohlhausen’s polynomial
• Pohlhausen chose to satisfy the
following conditions:
• With the following polynomial:
• For this polynomial:
f 0( ) = 0, f 0( ) = - , f 1( ) =1, f 1( ) = f 1( ) = 0
f ( ) = 2 2 3+
4+1
61( )
3
w =μ u
yy =0
=Ue f 0( ) =
Ue 2 +6
Substitution in
Momentum Integral • The momentum integral equation is
• In terms of f and :
• Or:
xu2dy
0Ue x
udy0
Ue
Ue
x=
w
xUe2 f 2d0
1
Ue xUe fd
0
1
Ue
Ue
x=
Ue f 0( )
d
dxf 1 f( )d
0
1+
d
dxf 1 f( )d
0
1
+ 2Ue
dUe
dxf 1 f( )d
0
1
+Ue
dUe
dx1 f( )d
0
1=
Ue
f 0( )
Substitution (2)
• Believe it or not, this equation can be
written as:
• Remembering that
ddx
=1
Ue
dUe
dxg( ) +
d2Ue
dx 2
dUe
dx2
g( ) = f 0( )
f 1 f( )d0
1 21 f( )d
0
1
f 1 f( )d0
1
=
2 Ue
x
Substitution (3)
• Evaluating the integrals and f’(0):
• And subbing back into g( ):
f 1 f( )d0
1=
2
9072 945+37315
1 f( )d0
1=3
10 120
f 0( ) = 2 +6
g( ) =90720 10512 + 282 2 10 3
5328 + 48 + 5 2
Substitution (4)
• So that, finally,
• Which is a non-linear differential equation in and Ue.
• The velocity distribution, Ue, is obtained from the inviscid solution.
• Then, the equation is a nonlinear ODE in only.
• It can be integrated numerically to yield .
• From that we can obtain , the thickness of the boundary layer.
d
dx=1
Ue
dUe
dx
90720 10512 + 282 2 10 3
5328 + 48 + 5 2 +
d2Ue
dx 2
dUe
dx2
Simple Example: Blasius
• For the Blasius flat plate, the inviscid
airspeed is constant, i.e. =0.
• The full momentum integral equation
• Becomes simply:
• Integrating:
d
dxf 1 f( )d
0
1+
d
dxf 1 f( )d
0
1
+ 2Ue
dUe
dxf 1 f( )d
0
1
+Ue
dUe
dx1 f( )d
0
1=
Ue
f 0( )
d
dxf 1 f( )d
0
1=
Ue
f 0( ) or d
dx
37
315=
2
Ue
x( ) =5.836x
Rex
Wedge flow
• Flow around a wedge: Inviscid flow:
Airspeed is zero at stagnation
point, Ue(0)=0.
Downstream of
this point the airspeed
increases
according to:
Ue(x)=U1xm
where U1 and m
are constants.
Potential flow
around a wedge • The potential flow around a wedge is
modelled using the following potential or stream functions:
• Notice that (r, ) satisfied Laplace’s equation:
• The radial and tangential velocities are:
r,( ) = Crm+1 cos m +1( ) , r,( ) = Crm+1 sin m +1( )
2
r2+1
r2
2
2 +1
r r= 0
qr = r= m +1( )Crm sin m +1( ) , q =
1
r= m +1( )Crm cos m +1( )
Velocity parallel to surface
• Therefore, the total velocity component
at any point in the flow is:
• Along the surface of the wedge:
q = m +1( )Crm = m +1( )C x 2 + y 2( )m
q = m +1( )Cnm
x
y
nTo calculate the boundary layer,
change variable in directions
parallel and perpendicular to the surface. n is called x, t is
called y and q is called Ue
t
Boundary layer solution
• Using Ue(x)=U1xm and
• We can substitute into:
• Which yields a long equation of the form:
• Where h is a nonlinear function of both
and x. Numerical integration gives:
=
2 Ue
x
d
dxf 1 f( )d
0
1+
d
dxf 1 f( )d
0
1
+ 2Ue
dUe
dxf 1 f( )d
0
1
+Ue
dUe
dx1 f( )d
0
1=
Ue
f 0( )
d
dx= h ,x( )
More about wedge flows
• In fact, wedge flows also have an exact treatment, similar to that applied to the Blasius flow.
• The governing equation is
• Where =2m/(m+1). It is called the Falkner-Skan equation and has boundary conditions
• It is clear that the Blasius equation is the special case =0.
f + f f + 1 f 2( ) = 0
f 0( ) = f 0( ), f ( ) = 0
Effect of value of m
For wedge
flows, m
represents the pressure
gradient. It
determines
whether the
pressure drops or
increases with
x.
Correlation method by
Thwaites
• This is another method for solving the
momentum integral equation.
• It is called correlation because it is
based on correlation with known
analytical and experimental results.
• It uses the non-dimensional version of
the momentum integral equation:
d
dx+ H + 2( )
Ue
dUe
dx=c f2
Shape factor
• Rewrite the equation in the form:
• And define a shape parameter as:
• Such that H=H( ) and S=S( ). The
equation becomes:
Ue d
dx+ H + 2( )
2 dUe
dx= w
μUe
= S
=
2 dUe
dx
Ue
d
dx dUe /dx
= 2 S( ) H( ) + 2( )( ) F( )
Correlation • The equation is not very useful because F( ) is unknown.
• Thwaites used known analytical solutions and experimental results to show that, for a laminar boundary layer,
• Now the equation can be integrated to yield:
F( ) = 0.45 6.0
2=
0.45
Ue6 x( )
Ue5 x( )dx
0
x
S =0.22 + 1.57 1.80 2 for 0 < < 0.1
0.22 + 1.402 + 0.018+ 0.107
for - 0.1 < < 0
H =2.61 3.75 + 5.24 2 for 0 < < 0.1
2.088 +0.0731
+ 0.14for - 0.1 < < 0
Blasius example
• As an example, apply the method to
Blasius’s flow. For this flow,
Ue=constant, =0, S=0.22, H=2.61.
• Then,
• The solution of the exact equations
gives
• So the Thwaites solution is not bad.
2=0.45
Ue
x =0.6708
Rex
*=1.7507x
Rex
*=1.7208x
Rex
Boundary layer at the
trailing edge
• What happens to the boundary layer on
a flat plate at the trailing edge?
The upper and lower
boundary layers merge
to create a single wake.
Methods for airfoils
• In practice, the viscous flow over 2D airfoils is solved using an iterative method.
• The method is called viscous-inviscid interaction.
• The boundary layer solution requires an inviscid solution.
• However, once the boundary layer is calculated, it has a thickness that changes slightly the shape of the airfoil.
• Then, the inviscid solution must be recalculated for the airfoil + boundary layer.
• The new inviscid solution is used to calculate a new boundary layer.
• The new airfoil+boundary layer give rise to a new inviscid solution.
• Eventually the method converges.
Viscous-Inviscid Interaction A better approach is to
leave the shape of the
airfoil unchanged. Calculate an Equivalent
Inviscid Flow (EIF) whose
boundary condition at the
wall is:
i.e. the normal flow at the
wall is not 0.
Such solutions can be
extended beyond the
trailing edge and simulate the wake.
n=d Ue
*( )dx
y
uI,vI
u,v
v(x,0) 0