8.5 Applications of the Integral Form of the Basic Equations 241
velocity U
A
= {(U
1
)
A
, (U
2
)
A
, 0} comprising two components, i.e. the U
3
component of the oncoming flow field is assumpt to be zero. Because of the
deflection of the flow by the blade, the departing velocity differs from the
approach velocity, so that the following holds:
U
B
= {(U
1
)
B
, (U
2
)
B
, 0} = U
A
. (8.91)
The assumed features of U
A
and U
B
, for which it always holds that (U
3
)
A
=
(U
3
)
B
= 0, make it clear that the flow field remains “two-dimensional” and
also has only two components. Thus for the inflow and outflow the following
equation can be derived from the continuity equation, where b is the width
of the blade in the x
3
direction:
ρ(U
1
)
A
tb = ρ(U
1
)
B
tb. (8.92)
For the inflow and outflow the same velocity components in the x
1
direction
thus result. This makes it clear that the purpose of the blades is to change
the velocity component (U
2
)
A
of the approaching flow.
For the computation of the force on a row of blades, a control volume
(a, b, c, d). is chosen, as shown in Fig. 8.9. In the flow direction, two flow
lines are chosen as boundaries of the control volume which are positioned
along (a − b)and(d − c), with the distance of the blades being t. Hence
the inflow and outflow to the chosen control volume take place only over the
areas (d − a)b and (c − d)b.
When one neglects gravitational effects, the Bernoulli equation yields the
following relationship between the velocity and pressure fields:
P
A
ρ
+
1
2
(U
1
)
2
A
+(U
2
)
2
A
entire kinetic energy in (A)
=
P
B
ρ
+
1
2
(U
1
)
2
B
+(U
2
)
2
B
.
entire kinetic energy in (B)
(8.93)
For the computation of the force on the blade, the integral form of the
momentum equation is used:
∂
∂t
⎛
⎝
#
V
K
ρU
j
dV
⎞
⎠
+
#
O
K
ρU
i
U
j
dA
i
= −
#
O
K
P dA
j
−
#
O
K
τ
ij
dA
i
+
#
V
K
ρg
j
dV +
F
j
.
(8.94)
With the following assumptions, one obtains from (8.94)
∂
∂t
#
V
K
ρU
j
dV
p
=0, as there is a stationary flow
#
O
K
τ
ij
dA
i
=0, as the flow is that of a viscosity-free fluid
#
V
K
ρg
j
dV =0, as gravitational forces are negligible,
(8.95)