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1- Fluid Mechanics, Victor L. Streeter and E. Benjamin Wylie, McGrawHill book Company.2- Mechanics of Fluids, Irving H. Shames, McGraw Hill book Company.3- Fluid Mechanics, F. M. White, McGraw Hill book Company.4- Introduction to Fluid Mechanics, A. T. McDonald, and R. W. Fox,John Wiley & Sons book Company.5- Elementary Fluid Mechanics, John K. Vennard & Robert L. Street,John Wiley & Sons book Company.
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1
REFERENCES
1- Fluid Mechanics, Victor L. Streeter and E. Benjamin Wylie, McGraw Hill book Company.
2- Mechanics of Fluids, Irving H. Shames, McGraw Hill book Company. 3- Fluid Mechanics, F. M. White, McGraw Hill book Company. 4- Introduction to Fluid Mechanics, A. T. McDonald, and R. W. Fox,
John Wiley & Sons book Company. 5- Elementary Fluid Mechanics, John K. Vennard & Robert L. Street,
John Wiley & Sons book Company. FLUID MECHANICS Is a branch of applied mechanics which deals with fluids. Statics MECHANICS Dynamics FLUID MECHANICS ⇔ Statics + Dynamicsof Fluids (Liquids and Gases) Fluids are classified into liquids and gases. The difference between the two is that LIQUIDS OCCUPY A DEFINITE VOLUME, whereas GASES EXPAND TO FILL THE ENTIRE VOLUME OF THE CONTAINER IN WHICH THEY ARE PLACED. FLUID is a substance that deforms continuously when subjected to a shear stress, no matter how small that shear stress may be.
F U
Fixed Plate
y
2
When a force F is applied to the upper plate, it exerts a shear stress F/A on the substance at the interface of the plate and the substance. If the force F causes the upper plate to move with a steady(nonzero) velocity, no matter how small the magnitude of F , one conclude that the substance between the two plates is a fluid. RELATIONSHIP BETWEEN STRESS AND DEFORMATION
ityVisofLawNewtonsdydv
dydv cos'µττ =⇒∝
µ is called viscosity , absolute or dynamic viscosity.
µ is defined as the proportionality factor between dydvandτ
dydv /τ
µ =
Considering two different fluids such as water and tar Applying the same τ for both fluids results in less deformation (dv/dy) for the tar. Hence, µ of the tar is greater than that of the water. So, the viscosity can also be expressed as the fluid characteristic that represent the resistance of the fluid against the shear stress. VISCOSITY IS A FUNCTION OF TEMPERATURE The magnitude of µ depends on:
1- Cohesive force between molecules. 2- Momentum interchange between colliding molecules.
The cohesive force is dominant for Liquids, So, as the temperature of a liquid is raised, the cohesive force between molecules decreases. This results in a decrease in viscosity. The momentum interchange is dominant for gases. So, as the temperature of the gas is raised, providing for greater momentum interchange, the viscosity of the gas increases.
3
RHEOLOGICAL DIAGRAM
Thin Liquids and Gases tend to be Newtonian Fluids. UNITS OF VISCOSITY
sPam
sN
msm
mNdydv
../
// 2
2
====τ
µ
In English units
2
.ft
slb=µ
Kinematic Viscosity
ρµ
ν =
Units s
mmkg
ms
smkg
mkgmsN 2
3
22
3
2
/
.
//.
====ρµ
ν
τ
dydv
Newtonian Fluids
Non-Newtonian Fluids Thixotropic Substance
Ideal Plastic
4
In English units s
ft 2
=ν
P.1.3 A Newtonian liquid flows down an inclined plane in a thin sheet of thickness t: The upper surface is in contact with air, which offers almost no resistance to the flow. Using Newton’s law of viscosity, decide what the value of dydu / , y measured normal to the inclined plane, must be at the upper surface. Would a linear variation Of u with y be expected?
Hence, a linear variation of u with y would not be expected. 1.5 A Newtonian fluid is in the clearance between a shaft and a concentric sleeve. When a force of 500 N is applied to the sleeve parallel to the shaft , the sleeve attains a speed of 1 m/s. If a 1500 N force is applied, what speed will the sleeve attain? The temperature of the sleeve remains constant.
Newtonian Fluid
0=τ
00
0
=⇒≠
==
dydu
dydu
µ
µτ
0≠dydu
5
smVNFsmVNF/?1500
/1500
22
11
=⇒==⇒=
dydV1
1 µτ =
Since the clearance thickness is very small, the velocity distribution can be assumed linear.
smVVV
VFF
VV
AFAFVV
tVt
Vt
Vdy
dV
/3
11500500
//
2
22
1
2
1
2
1
2
1
2
1
2
1
11
11
=⇒
=⇒=⇒=⇒
=⇒
=
=⇒=
ττ
µτ
µτ
1.16 A flywheel weighing 600 N has a radius of gyration of 300 mm. When it is rotating 600 rpm, its speed reduces 1 rpm/s owing to fluid viscosity between sleeve and shaft. The sleeve length is 50 mm; shaft diameter is 20 mm; and radial clearance is 0.05 mm. Determine the fluid viscosity. W = 600 N R = 300 mm=0.3 m
y Concentric Sleeve
Shaft
6
?
/60
21/1
/2.060
01.02600600
2
=
×==
=××
==
µ
πα
ππ
sradsrpm
smrpmV
The system is rotating with 600 rpm. When the power is disconnected, the velocity of the rotating system will be reduced by 1 rpm/s owing to fluid viscosity. In other words the frictional shear force between the rotating shaft and the fluid results in a torque equals to Fr
αµ
α
α
2
2
mRrAtV
mRFrIT
=
=
=
Where t = clearance thickness between shaft and sleeve, A = Shaft-Fluid interface surface area.
sPa.46.16023.0
806.9600)1010()1050()1020(
1005.02.0 2333
3
=
××=××
×××××
×−−−
−
µ
ππ
πµ
50 mm
20 mm V=600rpm 0.05 mm
shaft flywheel
sleeve
7
EXAMPLE -An oil of viscosity µ between the conical body and the container fills the clearance. Find the torque required to be applied on the conical body to produce an angular velocity w
Owing to the fact that the velocity at the surface of the conical body varies with radius of the cone at that point, the torque should be obtained by integration.
w
αw H
Conical Body
Container
Oil Film of thickness h
8
ααµπ
αµπ
αµπ
αµπ
sin2tan
sin24sin2
sin2 444
0
4
0
3
hHw
hRwx
hwdxx
hwT
RR
==
== ∫
w
αw H
Conical Body
Container
Oil Film of thickness t
dx
dy ds
α α
α
sin
sin
dxds
dsdx
=
=
απµ
απµ
πµ
τ
sin2
sin2
2
)(
dxxdsh
wxx
dxxdshVx
xdsdydVx
dAxxdFT
xdFdT
A
A
A
AA
∫
∫
∫
∫∫
×=
×=
×=
==
=
9
αµπ
sin2
4
1
21
tRwT
TTT
=
+=
H
R
w H =4” R = 2” t = 0.01”
25 .105.4
ftslb−×=µ
Find the torque T required to rotate the conical body with angular velocity w
r rdrdA π2=
10
BULK MODULUS OF ELASTICITY K For most purposes a liquid may be considered as incompressible, but for situations involving either sudden or great changes in pressure, its compressibility becomes important.
∀∀−=
/ddPK
The compressibility of a liquid is expressed by its bulk modulus of elasticity K. An increase of the pressure dP results in a liquid volume decrease of ∀d . The ratio
∀∀−
/ddP will be equal to K of that liquid.
Example In order to show the low compressibility of water let’s consider the application of 0.1 MPa (about one atmosphere) to a cubic meter of water:
3102.210)(
9999545.01 9
5)
meeKLnPP
dKdP
KPP
oo
o
P
Po o
=×=∀=∀⇒
∀∀
−=−
∀∀
=−
×
−−−
∀
∀∫ ∫
SURFACE TENSION Surface tension of a liquid is due to the forces of attraction between like molecules called COHESION and those between unlike molecules called ADHESION. In the interior of a liquid, the cohesive forces acting on a molecule are balanced out, since the molecule is surrounded by like molecules. Near a free surface however, since the cohesive force between liquid molecules is greater than that between air molecule and liquid molecules, there is a resultant force on a liquid molecule acting toward the interior of the liquid. This force is balanced out with the surface tension force formed in the membrane type surface. The surface tension force is proportional to the product of a surface tension coefficient σ and the length of the free surface. To illustrate, consider the equilibrium of a water droplet shown in cross-section in the figure:
11
BUBLE
JET
Po Pi
Interface of water and air
RPP
RRPP
oi
oi
σ
πσπ
22)( 2
=−
×=×−
RPP
LRLPP
oi
oi
σ
σ
=−
×=×− 22)(
12
BULB
JET RPP oi
σ=−
BUBLE RPP oi
σ2=−
BULB RPP oi
σ4=−
Po Pi
Two Interfaces of liquid and gas
RPP
RRPP
oi
oi
σ
πσπ
422)( 2
=−
××=×−
13
CAPILARITY When a liquid is in contact with a solid surface, adhesion forces between solid and liquid in addition to cohesive forces within the liquid should be taken into consideration.
Water meniscus
Glass tube
Liquid
Rh
hRR
γθσ
γπθσπcos2cos2 2
=
=
Adhesive Forces > Cohesive Forces
14
Cohesive Forces > Adhesive Forces Adhesive Forces > Cohesive Forces
15
CHAPTER 2 FLUID STATICS STRESS AT A POINT
The stress is the ratio of two vectors. So it is neither vector nor scalar.
kFjFiFF
kAjAiAA
zyx
zyx
∆+∆+∆=∆
∆+∆+∆=∆
x
zxz
x
yxy
x
xxx
AFAFAF
∆∆
=
∆
∆=
∆∆
=
τ
τ
σ
C
A∆ F∆
To obtain the stress at point C, let F∆ be the force vector acting on the surface element A∆ . Then
AFCatStress
A ∆
∆=
→∆lim
0
A∆
y
z
xyτ zA∆
x
xA∆
yA∆
xzτ
xxσ
16
==
zzzyzx
yzyyyx
xzxyxx
ijpoaatStressσττ
τστ
ττσ
τint
The stress is a second degree tensor, since it has two indices. Number of Components = 3degree = 32 = 9 Vector ⇒ Tensor of first degree ⇒ Number of Components = 31=3 Scalar ⇒ Tensor of zero degree ⇒ Number of Components = 30=1 In Fluid Statics there exists only pressure(Normal Stress) and there are no shere stresses. Hence,
==
z
y
x
ij
PP
PpoaatStress
00
00
00
int τ
PRESSURE AT A POINT At a point, a fluid at rest has the same pressure in all directions. To demonstrate this, a tetra-hydral element is considered in a fluid at rest as shown in the figure:
x
xA∆
yA∆
zA∆
xx AP ∆
y
z
zz AP ∆
yy AP ∆
AP∆
17
Direction cosines of PdA are l, m, n, respectively. ∑ =0xF
⇒=∆−∆⇒=∆−∆ 00 xxxxx APAPAlPAP Px = P ∑ = 0zF
⇒=∆−∆⇒=∆−∆ 00 zzzzz APAPAnPAP Pz = P ∑ = 0yF
⇒∆⇒=∆
−−
⇒=∆∆
−∆−∆⇒=∆∆
−∆−∆
zeroapproachesyyPP
yAAPAP
yAAmPAP
y
yyyy
yyy
03
03
03
γ
γγ
Py = P Px = Py = Pz = P BASIC EQUATIONS OF FLUID STATICS PRESSURE VARIATION IN A STATIC FLUID The forces acting on element of fluid at rest consist of surface forces and body forces. Surface forces are the forces that act on the element surfaces and body forces act on the particles of the body. Gravity force is the only body force.
18
amF vv=∑ (1)
kFjFiFF zyx
vvvv∑∑∑∑ ++=
dxdydzxPF
dydzdxxPPPdydzF
x
x
∂∂
−=
∂∂
+−=
∑
∑ )(
Similarly:
dxdydzdydzdxyPF
yγ−
∂∂
−=∑
dzdxdyzPF
y ∂∂
−=∑
Substituting in (1) results in:
)( EquationEulerajP
ajkzPj
yPi
xP
adxdydzkdzdxdyzPjdxdydzdydzdx
yPidxdydz
xP
vvv
vvvvv
vvvv
ργ
ργ
ργ
=−∇−
=−
∂∂
+∂∂
+∂∂
−
=∂∂
−
−
∂∂
−+∂∂
−
This equation is valid for invicid fluids in motion, or fluids so moving that the shear stress is everywhere zero. This equation will be used in the end of this chapter for a fluid which is in container moving with acceleration. For fluid statics 0=av
Hence, =−∇− jPvv
γ 0 ⇒ =−
∂∂
+∂∂
+∂∂
− jkzPj
yPi
xP vvvv
γ 0
Pdydz dydzdxxPP )(
∂∂
+
dx dz
dy
x
y
z
19
⇒ 0,,0 =∂∂
−=∂∂
=∂∂
zP
yP
xP
γ
00 =∂∂
=∂∂
zPand
xP states that two points at the same elevation in the same
continuous mass of fluid at rest have the same pressure. Using Differential Calculus:
dydP
dzzPdy
yPdx
xPdP
γ−=∂∂
+∂∂
+∂∂
=
The last equation holds for both compressible and incompressible fluids. Integrating this equation yields:
P is the absolute pressure and hγ represents the gage pressure. Absolute pressure is expressed as a difference between its value and a complete vacuum. Gage pressure is the difference between its absolute value and the local atmospheric pressure.
CyP +−= γ
•
h Depth of point from fluid free surface
y Choosing origin for the coordinates is arbitrary. For simplicity, the origin has been chosen at the free surface. y=0 , P = Patm ⇒ C= Patm y=-h ⇒
.atmPhP += γ
20
EXAMPLE Find the pressure at depth 6 m of water. Then calculate the absolute pressure. The barometer reads 760 mmHg. SHg = 13.57
.24.15996710113158826.24.10113176.0806.9100057.13
).(588266806.91000
.
.
PaPpPPahgP
gagePahp
atm
HgHgatm
=+=+=
=×××===××==
ργ
h=760mm
vacuum
21
PRESSURE VARIATION IN A COMPRESSIBLE FLUID When the fluid is a perfect gas at rest at constant temperature (isothermal conditions), the following can be introduced:
RTP
PPP
PRTP
oo
o
o
oo
ρ
ρρ
ρρ
ρ
=
=⇒=⇒
=
(1)
gdydydP ργ −=−= (2)
Substituting for ρ from Eq.(1) in Eq.(2) results in:
dyP
gP
dPPgdyP
dPy
y o
oP
Po
o
oo
∫∫ −=⇒−=ρρ
[ ] [ ]yy
o
oPP oo
yP
gLnP ρ−=
)(
)(
oo
o yyP
g
o
oo
o
o
ePP
yyP
gPPLn
−−
=
−−=
ρ
ρ
The atmosphere frequently is assumed to have a constant temperature gradient expressed by:
yTT o β+= For standard atmosphere, mCo /00651.0−=β
)( yTRP o βρ += EXAMPLE Assuming isothermal conditions to prevail in the atmosphere, compute the pressure and density at 2000 m elevation if 35 /24.1.10 mkgPaP oo == ρ at sea level.
P,y
Po,yo
datum
22
.).(4.78.7841210)2000(
10806.924.1
5
)(
5 absPaPaeP
ePP
o
oo
o yyP
g
o
===
=×
−
−−ρ
35 /972.078412
1024.1 mkgP
Po
o =×==ρ
ρ
EXAMPLE Find the gage pressure at depth 1500 m of an ocean, assume: a) Incompressible fluid, 3/10050 mN=γ b) Compressible fluid, .1007.2 9 PaK ×=
23
EXAMPLE Cross sections at A and B are equal to 0.004 m2 and 0.4 m2 respectively. WB=40 kN., S = 0.75, Find F. Neglect cylinder A weight A general procedure should be followed in working all manometer’s problems (U type problems):
1- Start at one end and write the pressure there in an appropriate unit. 2- Add to this the change in pressure from one meniscus to the next (plus
if the next meniscus is lower, minus if higher). 3- Continue until the other end of the gage and equate the expression to the
pressure at that point.
F
5 m B NF
FAreaWh
AreaF
B
Bf
A
2534.0
40000
5980675.0004.0
=
=××+
=+γ
A
24
EXAMPLE
A
h1=0.6m
h2=0.9 m water
Mercury
SHg=13.57 Find the pressure at A
.11387709.0980657.136.09806
021
PaPP
hhP
A
A
HgwA
==××−×+
=−+ γγ
25
EXAMPLE
.37.246722.0980612.0980657.131.098068.0075.0980657.1325.09806
65421
PaPPPP
PdddddP
BA
BA
BwHgoilHgwA
=−
=×−××−××+××−×−
=−−+−+ γγγγγ
ASSIGNMENTS Assignment #2 2.15, 2.16, 2.21 Assignment #3 2.28, 2.32, 2.35, 2.55, 2.63 Assignment #4 2.69, 2.78, 2.82, 2.85, 2.90 Assignment #5 2.91, 2.123, 2.133
A
B
water
Mercury
Oil water
Mercury
d1 d2 d3
d4 d5
d6 SHg =13.57 Soil = 0.8 d1 = 0.25 m d2 = 0.075 m d3 = 0.1 m d4 = 0.1 m d5 = 0.12 m d6 = 0.2 m PA – PB = ?
26
FORCES ON PLANE AREAS HORIZONTAL SURFACES
To find the line of action of the resultant:
areatheofcentroidtheofxXA
xdAX
xPdAPAXxdFXF
GA
P
AP
AP
==
=⇒=
∫
∫∫ )()(
Similarly:
areatheofcentroidtheofzZA
zdAZ
zPdAPAZzdFZF
GA
P
AP
AP
==
=⇒=
∫
∫∫ )()(
Hence, for a horizontal area subjected to static fluid pressure, the resultant passes through the centroid of the area.
z
z
F = PA
⊗
zP
xP
APdAPPdAF
PdAdF
A A∫ ∫ ===
=
x
dF
x
y
27
INCLINED SURFACES
In the figure a plane surface is indicated by trace A’B’. It is inclined oθ from the horizontal plane. The intersection of the plane of the area and the free surface is taken as the x-axis. y-axis is taken in the plane of the inclined area with origin O, as shown in the free surface. The xy plane portrays the arbitrary inclined area. The magnitude, direction, and line of action of the resultant force due to the liquid, acting on one side of the area, are sought.
y
x
y
y
x
h h
x
y
O
O
Gx
Gy
28
For an element with area dA
dAyhdAPdAdF θγγ sin=== All force components (dFs) are parallel. Therefore, the resultant force will be equal to the algebraic summation of these components, i. e., the resultant F equals to the integral of dF:
APF
AhAyydAdAydFF
G
GAAA
=
===== ∫∫∫ γθγθγθγ sinsinsin
In other words, the magnitude of force exerted on one side of a plane area submerged in a liquid is the product of the area and the pressure at its centroid. As all force elements are normal to the surface, the line of action of the resultant also is normal to the surface. Any surface may be rotated about any axis through its centroid without changing the magnitude of the resultant if the total area remains submerged in the static liquid. CENTER OF PRESSURE The line of action of the resultant force has its piercing point in the surface at a point called the pressure center, with coordinates (xP, yP). Unlike that of the horizontal surface, the center of pressure of an inclined surface is not at the centroid. To find the pressure center, the moments of the resultant FyFx PP , are equated to the moments of the distributed forces about the y and x axes, respectively; thus:
29
AyxIyy
AyyxIxx
yAy
xIAy
AyxIAy
IxAy
dAyy
xAyyxI
AyAyxyxI
AyI
xAy
dAyxx
dAyyAyyyPdAFy
dAyxAyxxPdAFx
GP
GP
GGx
PA
P
GGGxy
PA
P
AGP
AP
AGP
AP
+=
+=
+=+
==⇒=
+=+
==⇒=
=⇒=
=⇒=
∫
∫
∫∫
∫∫
22
.
.
sinsin
sinsin
θγθγ
θγθγ
When either of the centroidal axes, xx = or yy = is an axis of symmetry for the surface, yxI vanishes and the pressure center lies on xx = . Since yxI may be either positive or negative, the pressure center may lie on either side of the line xx = .
tyeccentriciAy
xIyyAy
xIyy GPGP ==−+=
Py is always below the centroid of the surface.
30
EXAMPLE The triangular gate CDE in the figure is hinged along CD and is opened by a normal force P applied at E. It holds oil, relative density 0.8, above it and is open to the atmosphere on its lower side. Neglecting the weight of the gate, find a) the magnitude of force exerted on the gate. b) the location of pressure center.
31
N
AhAPF G
8.47068
)2
23(30sin498068.0
=
××××=== γ
mxx GP 667.03/2 ===
mAy
xIyy GP
09375.4)2/23(4
125.122
4
3
=××
××
+=+=
D
⊗ G
O
D
⊕
y y
C
O
TOP VIEW
x C
3 m
2m
Center of Pressure
30o
E
SIDE VIEW
x
2.5m
32
EXAMPLE Considering 3ft length of the tank perpendicular to the paper, Calculate the water force and the location of this force on the wall AD.
A
D 30o
Water 6ft
6ft
33
ADedgethefromftx
lb
AhAPF
P
G
5.1
8424
)63()2
30sin66(4.62
=
=
××+×=== γ
ft
AyxIyyG
GP
2.15
)63)(330sin
6(
1263
330sin
6
3
=
×+
×
++=+=
A
B
C
D
O
y
30o
⊗
x
y
Water 6ft
6ft
3ft
x
34
THE PRESSURE PRISM
olumeVismdFForceResultant
dPdAdF
∫ ∀=∀=
∀==
Pr
∀
∀=
∀
∀=
∫∫∀∀
ydy
xdx PP
This indicates that the resultant passes through the centroid of the pressure prism volume.
P=γh
35
EXAMPLE
lb
ftft
ftftPPF
8424
362
)30sin66(4.6264.62
362
21
=
××+×+×
=
××+
=∀=
The influence point of the resultant pressure force is the centroid of the pressure prism volume.
ftPPPP
y
ftx
8.269
629362
36
5.1
12
12 =
×+×
××+×=
+
+=
=
γγγγ
B
C
D
O
y
30o
x
y
Water 6ft
6ft
3ft
x
11 hp γ=
22 hp γ=
36
EXAMPLE
The width of the bate AB (Normal to the gate is 2 m). The gate weight is 15 kN. The gate is hinged at B. Find h so that the gate will start to open. Integration Method
dlyydAPPdAPdAPdF 2)()( 212121 ×−=−=−= γγ y1 and y2 are the depths of the element at left and right of the gate, respectively.
o 1.5 m
2 m W
A
B
Water Water
1.5 m
h
37
25.10
25.2)5.1(2
2)5.1(2
)5.1(2)()(
)5.1(2)(22)(
25.2
0
2
5.2
0
2121
×=
−−=
−=
−==⇒=
−=−=×−=
∫∫
WhlhM
dllhldFMldFdM
dlhyydlyydF
γγ
γ
γγγγ
mh
h
683.125.1150
25.2)5.1(806.92
2
=
×=
−−××
Second Method
122575)25.2()15.1()1(49030)25.2()1(
222
111
=××+==+=××+==
γγ
APFhhAPF
G
G
)25.2)(25.125.1(52.025.125.1
)25.2(25.2
45
12/5.2225.2
45 3
1
111 ×+
++=×
+
×+
+=+=
hh
hh
AyxIyy
GGP
)25.2)(25.125.1(52.0
×+h is e1
16667.0125.3)25.2(
25.25.1
45
12/5.2225.25.1
45 3
2
222 +=
×
+×
×+
+×=+=
AyxIyy
GGP
o 1.5 m
2 m W
A
B
Water Water
1.5 m
h
P1 P2
y1
y2
l
y
38
0.16667 is e2
Hence, )25.2)(25.125.1(52.0
25.2
25.2
11 ×+−=−=
hel
ml 08333.116667.0
25.2
2 =−=
∑ =−×−⇒= 025.10 2211 lFWlFM B
mh
hh
hh
683.132
05.53405.205.2
005.505.23
00833.112257525.115000
)25.2)(25.125.1(52.0
25.2)1(49030
2
2
=×
××+±=
=−−
=×−×−
×+
−×+
It has to remember that this example can also be solved as a curved surface.
39
CURVED SURFACES When the elemental forces PdA vary in direction, as in the case of a curved surface, they must be added as vector quantities; i.e., their components in three mutually perpendicular directions are added as scalors, and then three components are added victorially.
xxx PdAPdAdFPdAdF
===
θcos
P is the pressure on dA
∫ =⇒=xA
xGxxxxx APFequalaredAanddAonPPdAF ,
Similarly, it can be proved that:
zGzz APF = But,
z
x
y
PdA
dAy
dAx
dAz h
⊗ ⊗ Gx
Gz
40
yGyy
Ayyy
APF
equalnotaredAanddAonPessuresPdAFy
≠
⇒= ∫ Pr,
∫ ∫∫ ∀===
yy Ay
Ayy dhAPdAF γγ
∀d is the volume of the small prism of height h and base dAy or the volume
of liquid vertically above the areaelement. Hence, ∀=∀= ∫ γγ dFy The vertical component of pressure force on a curved surface is equal to the weight of liquid vertically above the curved surface and extending up to the free surface. The horizontal component of pressure force exerted on a projection of the curved surface. The vertical plane of projection is normal to the direction of the component. EXAMPLE The equation of an ellipsoid of revolution submerged in water is
1944
222
=++zyx . The center of the body is located 2m below the free surface.
Find the horizontal force components acting on the curved surface that is located in the first octant. Consider the x-z plane to be horizontal and y to be positive upward.
41
N
APF xGxx
53200
)4
23)(3
242(
−=
×××−−=
−=π
πγ
N
APF zGzz
35400
)42)(
3242(
2
−=
××−−=
−=
ππ
γ
×××−×
×××−=
−×××
×−=
∀−=
8
32234
24
329806
834
4
ππ
ππγ
γ
abcbca
Fy
The influence line of Fy passes through the centroid of the volume ∀ .
2m
2m
3m
Gz Gx
Fz
Fx
42
Liquid pressure force when the liquid is below the curved surface
∀ is the volume above the curved surface and extending up to the free surface or the extension of it. Unlike the previous case yF direction is upward and the influence line passes through the centroid of ∀ . EXAMPLE A cylindrical barrier holds water as shown. The contact between cylinder and wall is smooth. Considering a 1m length of cylinder, determine a) its gravity force and b) the force exerted against the wall.
θ
PdA
dAx
Extension of free surface
h
∀=∀=
==
=
=
=
==
∫
∫∫
∫
γγ
γ
θ
dF
hdAPdAF
PdAdFAPF
PdAF
PdAdFPdAdF
y
yyy
yy
xGxx
Axx
x
x
cos
43
a) In equilibrium: ∑ = 0yF
ABy
BCDy
BCDy
ABy
FFW
FWF
−=
=+−− 0
γπγπ )4(1
4
22 −=××
−=
rrF ABy
A
B
C
D r=2m
44
γπ
γπ
)82(
122
22
+=
××
+= rrF BCD
y
NW 51032.1)43()4()82( ×=+=−−+= γπγπγπ b)
1m
2m
NAPF Gh 19600221 ==××== γγ
⊗ G
45
TENSILE STRESS IN A PIPE AND SPHERICAL SHELL A circular pipe under the action of an internal pressure is in tension around periphery. A section of pipe of unit length is considered. If one-half of the ring is taken as a free body, The horizontal component of force acts through the pressure center of the projected area and is 1×× dDP , in which P is the pressure at the center line.
∑ =⇒= TPdDFx 20
σσ
22 PdeePd =⇒=
EXAMPLE A 100 mm-ID steel pipe has a 6 mm wall thickness. For an allowable tensile stress of 70 MPa., what is the maximum pressure?
PaPPPde 66 102.4
107021.0006.0
2×=⇒
×××
=⇒=σ
46
For a spherical shell
It can be noted that spherical shells with half thickness compared to cylindrical shells can tolerate the same internal pressure.
σ
σππ
4
4
2
Pde
dedP
TPA
=
=×
=
47
EXAMPLE Calculate the force F required to hold the gate in a closed position
θ
θd
r
θcosr
θsinr
F
PdA
∫=×
=×
dMrF
essureinsideofMrF Pr
)1(sin3.1
sin
∫∫
××=×
×=×
θθ
θ
rrdPrF
rPdArF
o
)2(5295.24cos-17650.806.09806398062.1cos6.098069.0
036.06.0cos
θθ
γγγθγ
==××−×+××+
=−++×+
PP
RrP wwwoil
F
S=3.0
o
48
Substituting for P from Eq. (2) in Eq. (1) yields:
[ ]
[ ] [ ]{ }NF
F
dF
ddF
ddrF
drrF
rrdrF
604.22942/2cos62.2647cos0/2cos-17650.86.03.1
2sin62.2647cos-17650.86.03.1
cossin22
5295.24-sin17650.86.03.1
sin5295.24cos-sin17650.83.1
sin)5295.24cos-17650.8(3.1
sin3.1)5295.24cos-17650.8(
2/0
2/
0
2/0
2/
0
2/
0
2/
0
2/
0
2/
0
2
=
−−+××=
−××=
××=
=
×=×
××=×
∫
∫ ∫
∫ ∫
∫
∫
π
ππ
π π
π π
π
θπ
θθθ
θθθθθ
θθθθθ
θθθ
θθθ
BUOYANT FORCE The resultant force exerted on a body by a static fluid in which it is submerged or floating is called the buoyant force. The buoyant force always acts vertically upward. There can be no horizontal component of the resultant because the projection of the submerged body or submerged portion of the floating body on a vertical plane is always zero. The buoyant force on a submerged body is the difference between the vertical component of pressure force on its underside and the vertical component of pressure force on the upperside.
49
∀=∀−∀=∀−∀=
−=
γγ
γγ)( 12
12
)1()2( VVB FFF
∀ is the volume of fluid displaced and γ is the unit gravity force of fluid. Buoyant force BF = Weight of Displaced Fluid The same relationship holds for floating bodies. The buoyant force acts through the centroid of the displaced volume of fluid. The centroid of the displaced volume of fluid is called the center of buoyancy. EXAMPLE A piece of ore having gravity force 1.1 N when submerged in water. What is the volume in cubic centimeters and what is its relative density?
50
75.398060000408.0/5.1/
8.400000408.0
98064.04.01.15.1
33
==∀
=
==∀
∀×∀=⇒=−=
w
w
B
WS
cmm
F
γ
γ
Buoyant force of a body submerged between two fluids
2211 ∀+∀= γγBF The center of buoyancy is located at the centroid of the displaced combined fluid.
2∀
1∀ 1γ
2γ
51
STABILITY OF SUBMERGED AND FLOATING BODIES
A body has stable equilibrium when a small disturbance results in forces tending to return it to its initial position. A body has unstable equilibrium when a small disturbance results in forces tending to increase displacement from its initial position. A body has neutral equilibrium when a small disturbance results in no forces. For floating bodies
Stable Equilibrium Unstable Equilibrium Neutral Equilibrium
52
A light piece of wood with a metal mass at its bottom is stable because a small disturbance (rotation) results in a couple that tends to return it to its initial position.
The metal mass is at the top. A small disturbance results in a couple that tend increase displacement (angular displacement) from its initial position.
⊗ × B
G G ⊗ B ×
⊗ ⊗ × × B
B
G G
53
FLOATING PRISMATIC OBJECTS If G is below B, stable equilibrium will govern. If B is below G, two conditions may occur: - The metacenter M lies above G. This results in stable equilibrium. The intersection of the buoyant force vector and the centerline is called metacenter
- The matacenter M lies below G. This results in unstable equilibrium
× ⊗ ×
⊗
B’ G G
B
M
Metacenter
54
Summary G is below B ⇒ Stable Equilibrium G is above B ⇒ -Metacenter is above G ⇒ Stable Equilibrium -Metacenter is below G ⇒ Unstable Equilibrium - Metacenter is on G ⇒ Neutral Equilibrium
RELATIVE EQUILIBRIUM When a fluid is being accelerated so that no layer moves relative to an adjacent one, i.e., when the fluid moves as if it were a solid, no shear stresses occur and variation in pressure can be determined by writing the equation of motion for an appropriate free body.
× ⊗
× ⊗
B’
G G B
M
55
UNIFORM LINEAR ACCELERATION By selecting a Cartesian coordinate system with y vertical and x such that the acceleration vector a is in the xy plane, the z axis is normal to a and there is no acceleration component in that direction:
ajP vvvργ =−∇−
The pressure gradient P∇
v is then the vector sum of avρ− and j
vγ− as shown
below:
Since P∇
v is in the direction of maximum change in P (the gradient), at right
angles to P∇v
there is no change in pressure. Surfaces of constant pressure, including the free surface must therefore be normal to P∇
v.
)(,
)(
yyx
yx
yx
agayPa
xP
jaiajyPi
xP
jaiajjyPi
xP
+−=−−=∂∂
−=∂∂
+=
+
∂∂
−∂∂
−
+=−
∂∂
+∂∂
−
ρργρ
ρργ
ργ
vvvv
vvvvv
dyagdxa
dyyPdx
xPdP
yx )( +−−=∂∂
+∂∂
=
ρρ
Integrating for an incompressible fluid, yields:
56
)1()( CyagxaP yx ++−−= ρρ Equation of free surface can be obtained by setting P=0:
SurfaceFreeofSlopeag
adxdy
Cyagxa
y
x
yx
+−
=
++−−= )(0 ρρ
In Eq.(1) C can be determined by choosing the origin of coordinates at the intersection of the vertical line passing through the point we want to obtain its pressure and free surface (surface of zero pressure):
hagPCPyx
y )(00,0,0
+==⇒===
ρ
h ×
O x
y
57
EXAMPLE The tank in the figure is filled with oil, relative density 0.8, and accelerated as shown. There is a small opening in the tank at A. Determine the pressure at B and C ; and the acceleration xa required to make the pressure at B zero.
5.0tan
5.00806.9
903.4tan
=⇒
−=+
−=
+−
==
α
θy
x
aga
dxdy
.18.11.11179425.1)0806.9(10008.0)(
425.12/15.02.115.0.35.2.44.2353
3.0806.910008.)(3.09.02.19.08.15.0'
kPaPaPhagP
mhkPaPaP
oghhagPmhmAA
C
CyC
C
B
BByB
B
==
×+××=+=
=++===
×××==+==−=
=×=
ρ
ρρ
For zero pressure at B 667.0
8.12.1tan / ==⇒ α
2
'
/537.6
0806.9667.0tan
sma
aag
adxdy
x
x
y
x
=⇒
+−
=+
−==−=θ
Zero pressure surface
hB
θ α A’
58
EXAMPLE A closed box with horizontal base 6 6× units and a height of 2 units is half filled with liquid. It is given a constant linear acceleration
4/,2/ gaga yx −== . Find the pressure at A.
32tan
32
4/2/tan
=⇒
−=−
−=
+−
=
α
θgg
gag
a
y
x
Fluid Volume = 6)26(
2162
2)3(
×××=××++ xx
ggghagP
x
AyA ρρρ49)5.1
322()
4()(
5.1
=×+×−=+=
=⇒
g/2
A
x
x 3
59
UNIFORM ROTATION ABOUT A VERTICAL AXIS Rotation of a fluid, moving as a solid, about an axis is called forced-vortex motion Every particle of fluid has the same angular velocity. This motion is to be distinguished from free vortex, motion, in which each particle moves in a circular path with a speed varying inversely as the distance from the center. A liquid in a container, when rotated about a vertical axis at a constant angular velocity, moves like a solid after some time interval. No shear stress exist in the liquid, and the only acceleration that occurs is directed radially inward toward the axis of rotation.
60
CrgyP
rdrgdydrrPdy
yPdP
++−=
+−=∂∂
+∂∂
=
2
22
2
ρωρ
ρωρ
Take the origin at the vertex of the paraboloid of revolution, then:
2
00,0,022rgyP
CPyrρω
ρ +−=
=⇒===
The zero pressure surface can be obtained by setting P=0:
gryrgy oo 22
02222 ωρω
ρ =⇒+−=
PdA dAdrrPP )(
∂∂
+ dr r
gyPmaF
rrP
rdAdrdAdrrPPPdA
maF
yy
rr
ρ
ρω
ωρ
−=∂∂
⇒=
=∂∂
−=∂∂
+−
=
∑
∑
2
2 )()(
61
In forced vortex ως 2= , while in free vortex the vorticity is equal to zero.
oy
1y ×
h ghP
yygPgygyP
grggyP
rgyP
o
o
ρ
ρρρ
ωρρ
ρωρ
=
+=+=
+=
+−=
)(
2
2
1
1
22
1
22
r
y
Volume of displaced fluid =Ah =Volume of fluid in the periphery of the paraboloid = 1/2 (Volume of the cylinder ) = 1/2 (AH)
2Hh = h
H
62
EXAMPLE A liquid, relative density 1.2, is rotated at 200 rpm about a vertical axis. At one point in the fluid 1 m from the axis, the pressure is 70 kPa. What is the pressure at a point B, which is 2m higher than A and is 1.5 m from the axis.
EXAMPLE A straight tube 2m long, closed at the button and filled with water, is inclined 30o with the vertical and rotated about a vertical axis through its midpoint 6.73 rad/s. Draw the paraboloid of zero pressure, and determines the pressure at the bottom and midpoint of the tube.
r ×A
×B
2m
1.5m
1m
mymy
y
rgyP
PaP
BA
A
AAA
A
42.18242.1642.16
2/160
220010002.1
806.910002.1700002
70000
22
22
=+=⇒=
×
×
××+
×××−=
+−=
=
π
ρωρ
.44.375424
2/5.160
220010002.142.18806.910002.1 22
PaP
P
B
B
=
×
×
××+×××−=π
y
63
?,? == AB PP
yA
1 m
1 m
64
.1698030cos2806.91000.2830
)]577.030cos1([806.910002
577.0806.92
)30sin1(73.6806.92
73.62
22
22
2222
PahgPPa
rygP
m
y
rgry
CC
BB
A
=××===
−−××−=
+−=
=×
=
×==
ρ
ρωρ
ω
65
FLUID DYNAMICS SYSTEM A system refers to a definite fixed mass of material and distinguishes it from all other matter, called its surroundins.
SYSTEMS LAGRANGIAN APPROACH The Lagrangian approach is used wherein the basic equations are derived for a given mass. In this approach we follow the given mass (system) With a reference to Fig. 2 to obtain position, velocity, momentum, energy or acceleration of the car, the Lagrangian approach in which the mass is followed is used.
The relative position of various particles comprising the mass of a solid stays in the same relative position during subsequent motion. Therefore, in order to
t1 t2 to
Solid Brick Fluid Flow in apipe
66
obtain position, velocity and acceleration of all particles or points of a solid it is sufficient to determine these unknowns at one point such as the center of gravity of the solid. Solid Mechanics Lagrangian Approach System Let’s try the lagrangian approach in fluid mechanics:
Since the relative position of various particles comprising the mass of the system does not stay in the same relative position during subsequent motion, knowing the situation of one point will not help to determine other other points situations. Unless, infinite number of equations for infinite number of particles is used. This approach is not reasonable. Therefore, another approach called Eulerian approach is adopted for most analyses in fluid dynamics. CONTROL VOLUME A fixed volume in space is called a control volume. In the Eulerian approach a control volume is adopted, and equations are described to express changes in mass, momentum, and energy as the fluid passes through or by the fixed volume or point (very small control volume). The boundary of a control volume is its control surface. The size and shape of the control volume are entitrly arbitrary but frequently they are made to coincide with the solid boundaries.
System System
67
To calculate the point by point variation of the fluid variable over the whole domain, the field approach is used. This approach essentially allows the domain to consist of a large number of control volumes or systems such that when they shrink to zero a series of nonlinear partial differential equations result. These equations are so difficult that a general solution for the three-dimensional distribution of relevant variables for the type of complex geometries encountered in practice has not yet been achieved, not even on the most powerful parallel processing super computers. THE GENERAL CONTROL VOLUME CONSERVATION EQUATION Consider some general flow situation in which the velocity of a fluid is given relative to an xyz coordinate system. At time t consider a certain mass of fluid that is contained within a system, having the dotted line boundaries indicated. Also consider a control volume, fixed relative to the xyz axes, that exactly coincide with the system at time t. At t+Δt the system has moved somewhat, since each mass particle moves at the velocity associated with its location. Let N be the total amount of some property (e.g., mass, energy, or momentum) within the system at time t, and let η be the amount of this property, per unit unit mass, throughout the fluid. The time rate of increase of N for the system is now formulated in terms of the control volume:
68
tN
tN
tN
tN
tN
tNN
tNNNN
tNN
dtdN
ttC
t
ttB
t
VC
ttC
t
ttB
t
tVCttVC
t
tVCttBCVC
t
tstts
tsystem
∆−
∆+
∂∂
=
∆−
∆+
∆−
=
∆−−−
=
∆−
=
∆+
⇒∆
∆+
⇒∆
∆+
⇒∆
∆+
⇒∆
∆+
⇒∆
∆+
⇒∆
∆+
⇒∆
)(lim
)(lim
)(lim
)(lim
)()(lim
)()(lim
)()(lim
00
.
00
...
0
...
0
0
Consider a small element with mass of dm, then
∫ ∫ ∀==⇒=.. ..VC VC
ddmNdmdN ηρηη
∫ ∀
∂∂
=∂
∂
..
.
VC
VC dtt
Nηρ
69
tN ttB
t ∆∆+
⇒∆
)(lim
0= time rate of flow of N out of the control volume
= ∫∫ ∀
=∆
∀ ∆+
⇒∆SBC
ttB
t dtd
t
d
.0
)(lim ηρ
ηρ
∫∫∫
=∀
=∆
∀=
∆
∆+
⇒∆
∆+
⇒∆)(..
00.
)(lim
)(lim
areaoutflowSBCSBC
ttB
t
ttB
tAdV
dtd
t
d
tN rr
ηρηρηρ
Similarly, for inflow to the control volume:
AdV
dAV
dAdtdl
dtd
dldAd
rr.
cos
cos
cos
=
=
=∀
=∀
α
α
α
dl
αcosdA
70
∫∫∫
−=∀
=∆
∀=
∆
∆+
⇒∆
∆+
⇒∆)(inf..
00.
)(lim
)(lim
arealowSCCSCC
ttC
t
ttC
tAdV
dtd
t
d
tN rr
ηρηρηρ
∫∫
∫∫∫
+∀∂∂
=
++∀∂∂
=
SCVCsystem
arealowSCCareaoutflowSBCVCsystem
AdVdtdt
dN
AdVAdVdtdt
dN
...
)(inf.)(...
.
..
rr
rrrr
ηρηρ
ηρηρηρ
The last equation states that the time rate of increase of N within a system is just equal to the time rate of increase of the property N within the control volume (fixed relative to xyz coordinate sytem) plus the the net rate of efflux of N across the control volumeboundaries. CONSERVATION OF MASS
∫∫ +∀∂∂
=
SCVCsystem
AdVdtdt
dN
...
.rr
ηρηρ
N =Property=m , η =Property per unit mass=1 Then:
∫∫ +∀∂∂
=
SCVCsystem
AdVdtdt
dm
...
.rr
ρρ
0.0...
=+∀∂∂
⇒=
∫∫SCVCsystem
AdVdtdt
dm rrρρ (conservation of mass or continuity
equation) The continuity equation states that the time rate of change of mass in the control volume plus the net rate at which mass leaves through the control surface equals zero.
71
Consider the cylindrical tube in the figure, flow enters the tube atstation 1 and exists at station 2. No flow is permitted through the solid surface comprising the tube. The application of the conservation of mass proceeds as follows:
1- The control volume is defined to include all the fluid in the tube out to the solid wall and from station 1 to station 2. If at all possible the inlet and outlet stations should be defined or placed in regions where the stream lines (or tubes) are parallel to the boundary such that the entrance and exit fluid velocities are perpendicular to the respective areas.
2- For steady flow:
0..0.2.
2221.
111.
=+⇒= ∫∫∫SCSCSC
dAVdAVAdVrrrr
ρρρ
3- If the inlet and outlet velocity vectors are at each inlet and outlet,
perpendicular to their respective areas; 4- - 0
2.222
1.111 =+ ∫∫
SCSC
dAVdAV ρρ
5- If average velocities are used; mAVAVAVAV &==⇒=+− 222111222111 0 ρρρρ
72
m& is the mass flow rate in kg/s or slug/s. If the discharge Q (also called the volumetric flow rate, flow or discharge) is defined as VAQ = For incompressible, steady flow:
2211 AVAVQ == Go back to the general equation:
0....
=+∀∂∂
∫∫SCVC
AdVdt
rrρρ
For incompressible fluids:
0..
=∫SC
AdVrr
which states that the net volume efflux is zero. This implies that
the control volume is filled with liquid at all times:
22112211 0 AVAVAVAV =⇒=+− EXAMPLE Apply the steady continuity equation for the figure:
73
0
0.0.
222333111
....
=+−−
=⇒=+∀∂∂
∫∫∫AVAVAV
AdVAdVdt SCSCVC
ρρρ
ρρρrrrr
For incompressible fluid flow ( tcons tan=ρ ):
223311
223311 0AVAVAVAVAVAV
=++=+−−
CONTINUITY DIFFERENTIAL EQUATION
0....
=+∀∂∂
∫∫SCVC
AdVdt
rrρρ Continuity Equation
dxdydzt
dxdydzt
dt VC ∂
∂=
∂∂
=∀∂∂
∫ρ
ρρ )(..
zyxSC
mmmAdV &&&rr
++=∫.
.ρ (Summation of net effluxes in x, y and z directions)
dxdydzxudydzdx
xuuudydzmx ∂
∂=
∂∂
++−=ρρ
ρρ&
Similarly, it can be proved that:
udydzρ dydzdxxuu )(
∂∂
+ρ
ρ
dx dz
dy
x
y
z
74
dzdxdyzwm
dydzdxyvm
z
y
∂∂
=
∂∂
=
ρ
ρ
&
&
Hence;
0).(
0
0
=∇+∂∂
=∂
∂+
∂∂
+∂
∂+
∂∂
=∂
∂+
∂∂
+∂
∂+
∂∂
Vt
Or
zw
yv
xu
t
dzdxdyzwdydzdx
yvdxdydz
xudxdydz
t
rrρ
ρ
ρρρρ
ρρρρ
For steady flow 0).( =∇⇒ V
rrρ
For incompressible fluid flow 0. =∇⇒ Vrr
75
CONTINUITY DIFFERENTIAL EQUATION IN CYLINDRICAL COORDINATES
0....
=+∀∂∂
∫∫SCVC
AdVdt
rrρρ Continuity Equation
zrSC
mmmAdV &&&rr
++=∫ θρ.
. (Summation of net effluxes in r, θ and z directions)
dzrdrdt
dzddrt
dzrdrdt
drdzddrrrdtt
m
θρ
θρθ
ρ
θθρ
∂∂
=
∂∂
+∂∂
=
++
∂∂
=∂∂
2)(
2)(
2
dzdrrdrVdzdrdV
dzddrrVdzdrrd
rVdzdrdVdzrdVdzrdV
dzddrrdrrVVdzrdVm
rr
rrrrr
rrrr
θρ
θρ
θρ
θρ
θρθρθρ
θρ
ρθρ
∂∂
+=
∂∂
+∂
∂+++−=
+
∂∂
++−=
2)(
)(&
rVρ
DrVV r
r ∂∂
+ρ
ρ
θρV θ
ρρ θ
θ ∂∂
+VV
zVρ
zVV z
z ∂∂
+ρ
ρ
76
drdzdV
drdzdVVdrdzVm
θθ
ρ
θθ
ρρρ
θ
θθθθ
∂∂
=
∂
∂++−=&
drdzrdzV
ddrdrrddzzVVddrdrrdV
drddrrrddzzVVdrddrrrdVm
z
zzz
zzzz
θρ
θθ
ρρ
θθρ
θθρρ
θθρ
∂∂
=
+
∂∂
++
+−=
++
∂∂
++
++
−=
2)(
2)(
2)(
2)(
22
&
Hence;
01
0
=∂
∂+
∂∂
+∂
∂++
∂∂
=∂
∂+
∂∂
+∂
∂++
∂∂
zVV
rrV
rV
t
drdzrdzVdrdzdVdzdrrd
rVdzdrdVdzrdrd
tzrr
zrr
ρθ
ρρρρ
θρ
θθ
ρθ
ρθρθ
ρ
θ
θ
FLUID FLOW CLASSIFICATION Flow can be classified in many ways such as laminar versus turbulent; steady versus unsteady; uniform versus non-uniform. Laminar Flow
Laminar Flow
Turbulent Flow
77
In laminar flow, fluid particles move along smooth paths in laminas, or layers, with one layer gliding smoothly over an adjacent layer. Laminar flow is governed by Newton’s law of viscisity. TURBULENT FLOW In turbulent flow the fluid particles (small molar masses) move in very irregular, swirling paths, causing an exchange of momentum from portion of the fluid to another. The turbulent swirls continuously range in size from very small (say a few thousand fluid molecules) to very large (a large swirl in a river or in an atmospheric gust). The turbulent sets up greater shear stresses through out the fluid and causes more irreversibilities or less.
ityviseddythecalledisdydV cos, ηητ =
The eddy viscosity is not a property of the fluid, varies from time to time and point to point. The eddy viscosity is not constant and it is function of flow characteristics (velocity, velocity gradient, fluid density and distance from wall)
kyldydul
=
= 2ρη
STEADY FLOW Steady flow is the flow that does not change with time:
00,0 =∂∂
=∂∂
=∂∂
tPand
tQ
tV
78
UNSTEADY FLOW Unsteady flow is the flow that changes with time:
00,0 ≠∂∂
≠∂∂
≠∂∂
tPand
tQ
tV
Changes with time
Fixed
79
UNIFORM FLOW Uniform flow occurs when at every point, the velocity vector or any of the other fluid variables is identically the same for any given instant:
0=∂∂
tVr
Uniform over the cross section means that the velocity is the same at all points over the cross section: NON-UNIFORM FLOW Non-uniform flow is the flow in which the velocity vector varies from place to place at any instant.
0≠∂∂
tVr
1Vr
2Vr
Velocity is the same over cross section
1Vr
2Vr
80
EXAMPLES -Liquid flow through a long pipe at a constant rate is steady uniform flow. - Liquid flow through a long pipe at a decreasing rate is unsteady uniform flow. -Flow through an expanding tube at a constant rate is steady non-uniform flow. -Flow through an expanding tube at an increasing rate is unsteady non-uniform flow. STREAM LINE A stream line is a continuous line drawn through the fluid so that it has the direction of the velocity vector at every point. There can be no flow a cross a stream line. If a particle of a fluid which moves along a stream line has a displacement dS , its displacement components in xyz directions will be: dx, dy and dz:
dx
dy
dz
dS
A stream line
81
wdzdt
dtdzw
wdz
vdy
udx
vdydt
dtdyv
udxdt
dtdxu
dtdSV
=⇒=
==⇒=⇒=
=⇒=
=r
EXAMPLE A three-dimensional velocity distribution is given by u=-x , v=2y , w=5-z Find the equation of the stream line through (2,1,1).
yx
Cyx
Cyx
CyLnx
LnCLnyLnxLny
dyx
dxv
dyudx
22/11,2
1)()1()()(21)(
22/12/1
=
=⇒==
=⇒=⇒+=−⇒=−
⇒=
82
252
2521,2
51)
5()1()()5()(5
1
111
zy
x
zxCzx
zC
xzCLn
xLnCLnzLnxLnz
xdx
wdz
udx
−==∴
−=⇒=⇒==
−=⇒
−=⇒+−=−⇒−=
−⇒=
EULER EQUATION ALONG A STREAM LINE A prismatic control volume of very small size (a bar element) with cross sectional area dA and length of dS , is selected along a stream line as shown in the figure:
Assuming that the viscosity is zero, i.e., the flow is frictionless, the only forces acting on the element in the s-direction are end forces and the weight. Other pressure forces are acting perpendicular to s.
ss maF =∑
Z
83
sZ
agsP
dAdsdAdsagdAdsdsdAsP
dAdsagdAdsdAdssPPPdA
s
s
s
∂∂
=
=++∂∂
÷
=−
∂∂
−
=−∂∂
+−
θ
θρ
ρρθρ
ρθρ
cos
)1(0cos1
cos
cos)(
V
sV
tV
ts
sV
tV
dttsdVas ∂
∂+
∂∂
=∂∂
∂∂
+∂∂
==),(
Substiyuting in equation (1) yields:
01=
∂∂
+∂∂
+∂∂
+∂∂
sVV
tV
sZg
sP
ρ Euler Equation for Unsteady Flow
For steady flow:
01=
∂∂
++∂∂
+∂∂
sVV
sZg
sP
ρ
Now s is the only independent variable. Therefore, total differentials can replace the partials:
0
01
=++
×
=+++
VdVdPgdZ
dsdsdVV
dsdZg
dsdP
ρ
ρ
The last equation is The Euler equation for steady flow. Assumptions used in the derivation
1- The equation holds along a stream line. 2- Frictionless flow ( 0=µ ) 3- Steady flow
84
THE BERNOULLI EQUATION Integrating of Euler equation for constant density yields the Bernoulli equation:
tconsVPgZ tan2
2
=++ρ
The last equation represents energy per unit mass. Dividing the equation by g yields:
Cg
VPZ =++2
2
γ
This can be interpreted as energy per unit weight in Newton.meter per Newton or Pound.feet per pound. This equation is derived by applying the momentum equation on a small element.
⊗ 2
⊗ 1 g
VPZg
VPZ
EE
22
222
2
211
1
21
++=++
=
γγ
85
INTERPRETATION OF BERNOULLI EQUATION’S TERMS
EnergyKineticEnergyPotential
mVmgHEmg
gVHmgEmg
gVH
gVhZE
gVPZE
+=
+=
+=
+=++=
++=
2
2
22
2
21
2
22
2γ
γPZ + = Potential Energy per unit weight of fluid
gV2
2
= Kinetic Energy per unit weight of fluid
h= H
86
Units⇒
ftlb
ftlb
or
mNmN
Newtonjoul
fluidofWeightEnergy
==
===
.
.
EXAMPLE Water is flowing in an open channel as shown in the figure at a depth of 2 m and a velocity of 3 m/s . It then flows down a chute into another channel where the depth is 1 m and the velocity is 10 m/s. Assuming frictionless flow, determine the elevation of the channel floors. The velocities are assumed to be uniform over the cross sections, and the pressures hydrostatic.
The points 1 and 2 may be selected on the free surface, as shown, or they could be selected at other depths. If the difference in elevation of floors is y, Bernouli’s equation is:
gVPZ
gVPZ
EE
22
222
2
211
1
21
++=++
=
γγ
87
my
y
64.3
806.921010
806.9232
22
=
×++=
×++
EXAMPLE a) Determine the velocity of efflux from the nozzle in the wall of the reservoir of the figure b) find the discharge through the nozzle.
The jet issues as a cylinder with atmospheric pressure uniformly distributed a cross the outlet and around its periphery. The energy equation without losses
88
is applied between a point on the water surface and a point downstream from the nozzle:
gVPZ
gVPZ
EE
22
222
2
211
1
21
++=++
=
γγ
gV2
21 is negligible compared to
gV2
22
sLsmAVQ
smghVg
Vh
/70/07.041.086.8
/86.84806.9222
0000
32
22
2
22
==×==
=××==⇒++=++∴
π
If losses are to be considered, then :
ghCV 2= C is called the orifice coefficient.
1<C EXAMPLE Find the discharge of the previous example by integration assuming non-uniform outflow.
4 m h
dh x .
sm
dhhghQ
dhhRgh
xdhghVdAdQ
hRx
hxR
/0695.0
)4(05.022
)4(22
22
)4(
)4(
3
05.4
95.3
22
22
22
222
=
−−××=
−−××=
×==
−−=
−+=
∫
89
EXAMPLE Calculate the time required to lower the water surface in the tank from elevation 4 m to 2 m. The tank cross sectional area is 50 m2.
y
dy 1
2
Let’s assume that the water surface level at time t is y. Then:
gyVEE 2221 =⇒= Continuity 2211 AVAV =⇒
[ ]4
22
2
42
2
21
2)05.0(50
22)05.0(50
2)05.0(50
)05.0(2
yg
ydy
gt
ygdydt
gyAdtdy
××−
=
××−
=
××−=
××=−
∫
π
π
π
π
90
EXAMPLE
A hydroelectric plant as shown in the figure has a difference in elevation from headwater to tailwater of H=50 m and a flow Q=5 m3/s of water through the turbine. The turbine shaft rotates at 180 rpm and the torque in the shaft is measured to be mNT .1016.1 5×= . The output of the generator is 2100 kW. Determine:
a) the reversible power for the system b) losses in the system c) losses and efficiency in the turbine d) losses and efficiency in the generator
Solution a) mHEHE TT 5021 =⇒=− For perfect conversion, the reversible power is :
kWNmNQHT 5.2451/.24515005059806 ==××=γ b) Lost power in the system is the difference between the power into and out of the system, or:
91
2451.5-2100=351.5 kW c) The rate of work by the turbine is the product of the shaft torque and the rotational speed:
kWT 5.218660
21801016.1 5 =×
×=π
ω
Lost power through the turbine = 2451.5-2186.5 = 265 kW Head loss through the turbine = lost power per unit fluid weight m
QPower 4.5
5806.9265
=×
==γ
The generator power loss = 2186.5-2100 = 86.5 kW The generator head loss = m
QPower 76.1
5806.95.86
=×
==γ
Efficiency of the turbine = %19.89100
504.550
=×−
Efficiency of the generator = %05.96100
4.55076.14.550
=×−
−−
KINETIC ENERGY CORRECTION FACTOR α Often the flow entering or leaving a port is not strictly one-dimensional. In particular, the velocity may vary over the cross section. In this case the kinetic energy term for a given port should be modified by a correction factor α : Kinetic energy per unit time by integration = α × Kinetic energy per unit time using average velocity
dAVv
A
gVVA
gvdAv
A
A3
22
1
22
∫
∫
=
=
α
αγγ
Find α for the velocity distribution of flow in a pipe, given below:
92
−= 2
2
max 1RrVv Ans. 2=α
EXAMPLE In the figure, a pump with a water horsepower (WHP) rating of 10 hp draws water from the reservoir as indicated and delivers water to an outlet 15 ft higher than the reservoir surface for crop irrigation. What is the outlet discharge? Total system losses from the pump to the outlet are parametrized
as g
V2
82
, but there are no losses from the reservoir inlet to the pump. The
delivery pipe diameter is 4.67 in.
93
sftVAQsftVg
VVg
V
gV
QgV
gVPZHh
gVPZ
EHhE
Pf
Pf
/83.1/4.1524/)12/67.4(4.62
550102
8
201555010
28000
22
3
2
2
2
22
222
221
211
1
2211
==⇒=
=××
×+−
++=×
+−++
++=+−++
=+−
−
−
π
γ
γγ
EXAMPLE A venturimeter, consisting of a converging portion followed by a throat portion of constant diameter and then a gradually diverging portion, is used to determine rate of flow in a pipe. The diameter at section 1 is 0.15 m and at section 2 it is 0.1 m. Find the discharge through the pipe when
.9.0.,200021 ==− SPaPP
94
21
12
2
2
2
1
22
2
21
1
2211
)1(25.24
1.04
15.044
EE
VVVV
DVDV
AVAVQ
=
=⇒×
×=×
×
×=×
==
ππ
ππ
sLsmAVQ
smVVV
VV
gVVPP
gVPZ
gVPZ
/4.58/0584.0415.031.3
/31.3806.92
)25.2(98069.0
20000)2(),1(
)2(806.9298069.0
20000
20
22
32
11
1
21
21
21
22
21
2221
222
2
211
1
==××==
=⇒×
−=
×⇒
×−
=×
−=
−+
++=++
π
γ
γγ
Assignments Chapter1 1.18, 1.20 plus class assignment Chapter 2 2.3, 2.5, 2.15, 2.17, 2.35, 2.50, 2.51, 2.52, 2.69, 2.78, 2.82, 2.91, 2.94, 2.100, 2.124, 2.133 Chapter 3 3.19, 3.29, 3 .34, 3.36, 3.46, 3.61, 3.62, 3.73 Chapter 4 4.13, 4.16, 4.19
95
THE CONTROL VOLUME LINEAR-MOMENTUM EQUATION
∫∫
∫∫
+∀∂∂
=
====
+∀∂∂
=
SCVCsystem
SCVCsystem
AdVVdVtdt
Vdm
VmVm
mNVmN
AdVdtdt
dN
...
...
.
,
.
rrrrr
rr
r
rr
ρρ
η
ηρηρ
∫∫∑ +∀∂∂
=SCVC
AdVVdVt
F...
.rrrrr
ρρ
∫∫∑
∫∫∑
+∀∂∂
=
+∀∂∂
=
SCy
VCyy
SCx
VCxx
AdVVdVt
F
AdVVdVt
F
...
...
.
.
rr
rr
ρρ
ρρ
96
EXAMPLE
Water flows in the pipe D1=25 cm D2=15 cm Q=50 L/s P1=8.5 kPa P2=5.83 kPa W=2.0 N (total fluid weight in the pipe) Find the horizontal and vertical forces required to hold the pipe in place.
∑∑∫∫∫∑
∑∑∫∫∫∑
===+∀∂∂
=
===+∀∂∂
=
QVAdVVAdVVAdVVdVt
F
QVAdVVAdVVAdVVdVt
F
yySC
ySC
yVC
yy
xxSC
xSC
xVC
xx
ρρρρρ
ρρρρρ
rrrrrr
rrrrrr
...
...
....
....
∑∑ = QVF xx ρ
NR
R
QVQVRAPAP
x
x
x
4.801
)05.0(30cos4/15.0
050.01000
)05.0(45cos4/25.0
050.0100030cos415.0583045cos
425.08500
)(cos)(coscoscos
2
2
22
2211222111
=
+××
×
+−××
×=+××−××
++−=+−
π
πππ
θρθρθθ
Rx
Ry
97
∑∑ = QVF yy ρ
NR
R
QVQVWRAPAP
y
y
y
2.963
)05.0(30sin4/15.0
050.01000
)05.0(45sin4/25.0
050.01000230sin415.0583045sin
425.08500
)(sin)(sinsinsin
2
2
22
2211222111
=
+××
×
+−××
×=−+××−××
++−=−+−
π
πππ
θρθρθθ
EXAMPLE Find the reaction force exerted on a fixed vane when a jet discharging 60 L/s of water at 50 m/s is deflected through 135o. The frictional resistance between jet and vane is neglected. The velocity is assumed to be uniform throughout the jet upstream and downstream from the vane, that is, the control volume. When the small change in elevation between ends, if any, is neglected, application of the energy equation shows that the magnitude of the velocity is unchanged for fixed vanes.
Ry
Rx
uV −0
uV −0
98
kNN
QVQVRQVF
x
xx
121.55121)06.0(135cos501000)06.0(501000
)(135cos)( 00
==+×××+−××=
+×+−=−
= ∑∑ρρ
ρ
kNN
QVRQVF
y
yy
121.22121)06.0(135sin501000
)(135sin0
==+×××=
+×=
= ∑∑ρ
ρ
EXAMPLE Fluid issues from a long slot and strikes against a smooth inclined flat plate. Determine the division of flow and the force exerted on the plate, neglecting losses due to impact.
As there are no changes in the elevation or pressure before and after impact, the magnitude of the velocity leaving is the same as the initial speed of the jet. The plate surface is assumed to be smooth. Therefore, there is no shear force exerted on the surface.
R
99
)2(
)1(cos0))(()()(cos0
210
210
201000
QQQContinuity
QQQQVQVQV
QVF xx
+=⇒
−+−=
+−+++−=
= ∑∑
θ
ρρθρ
ρ
Equations (1) and (2) yields: )cos1(2
01 θ+=
QQ , )cos1(2
02 θ−=
The force R exerted on the plate must be normal to it.
00
00
sin
))(sin(
QVQVR
QVF yy
θρ
θρ
ρ
=
−−=
= ∑∑
100
101
MOVING VANES To analyse the problem, it is reduced to steady state by superposition of vane velocity u to the left. The control volume relationship has been proved with respect to fixed coordinates. Therefore, in order to be able to use the same relationship, the coordinate system has to be moved with the vane velocity u to the right. By this way the control volume will have a stationary position with respect to the coordinate system. EXAMPLE The vane in the figure is moving with a velocity u= 30 ft/s. Determine the force components due to the water jet and the rate of work done on the vane.
Vo Vo-u
Vo-u Vo
θ
u
θ
Rx
Ry
x
y
z x
y
z
u
102
sftu
sftVftA
/3060
/10004.0
0
0
20
==
==
θ
lbR
AuV
AuVuVAuVuVRQVF
x
x
xx
569
)5.01(04.0)30100(17.324.62)cos1()(
])(][cos)([])()[(
20
20
000000
=⇒
+××−−=+−−=
−+−−+−−−=−
= ∑∑
θρ
θρρ
ρ
lb
AuV
AuVuVRQVF
y
yy
329
60sin04.0)30100(17.324.62sin)(
])][(sin)[(
20
20
000
=
×−=−=
−−=
= ∑∑
θρ
θρ
ρ
The power exerted on the vane is sftlbuRx /.1707056930 =×=
103
THE MOMEN OF MOMENTUM EQUATION The general unsteady linear momentum equation applied to a control volume:
∫∫∑ +∀∂∂
=SCVC
AdVVdVt
F...
.rrrrr
ρρ
Taking the cross, or vector, product of the equation and the position vector r of a point on the line of action of the vector from any point O, yields:
∫∫∑ ×+∀×∂∂
=×SCVC
AdVVrdVrt
Fr...
.rrrvrvrv ρρ
Moment of the resultant force = Summation of moments of components; Hence:
∫∫∑ ×+∀×∂∂
=×SCVC
AdVVrdVrt
Fr...
.rrrvrvrv ρρ
For steady flow and uniform average flow on the cross section:
∑∑∑∑∑
×=
×=×=×
QVrM
QVrAVVrFrrv
rvrrrvrv
ρ
ρρ ).(
104
105
lbftT
T
AVhVAVhVhAPhAPTQVrM
A
A
A
.455
)4
)12/3(40)(12/1040(94.1)4
)12/3(40)(12/240(94.1
1210
4)12/3(14480
122
4)12/3(144100
))(())((
22
2222221111222111
=⇒
×+××+×−××
=××××−××××+
++−=−+
×= ∑∑
ππ
ρρ
ρrv
3.79 In Fig. 3.66, a jet, 3/2 ftslug=ρ , is deflected by a vane through 1800. Assume that the cart is frictionless and free to move in a horizontal direction. The cart weighs 200 lb. Determine the velocity and the distance traveled by the cart 10 s after the jet is directed against the vane A0 = 0.02 ft2 and V0 = 100 ft/s.
V0
106
2100
010001010
)(2
])()][([])()[(
VVAFAVVuVAVVVVF
QVF
x
x
xx
−=⇒
−+−−+−−−=−
= ∑∑
ρ
ρρ
ρ
Fx is variable. It varies with respect to V1. For the cart:
21
1
121
2100
)100(71.77
17.32200)100(02.022
)(2
VdVdt
dtdVV
dtdVmVVAmaF xx
−=
=−××
=−⇒= ρ
ftxsttLntxCxt
CtLntxtdt
dxV
sftVstt
VV
t
CVtCV
t
796103.19)7771.0(71.771003.190,0
)7771.0(71.771007771.071.77100
/79.92107771.071.771007771.0
10071.77
7771.00,0,100
71.77
2
21
1
11
1111
=⇒=−+−=⇒−=⇒==
++−=⇒+
−==
=⇒=+
−=⇒−−
=
−=⇒==+−
=
V0-V1
V0-V1
Fx
107
DIMENSIONAL ANALYSIS AND DYNAMIC SIMILITUDE Solving practical design problems in fluid mechanics usually requires both theoretical developments and experimental results. By grouping significant quantities into dimensionless parameters, it is possible to reduce the number of variables and make this compact result (equations or data plots) applicable to all similar situations. Dimensions Quantity Symbol Dimension Length l L Time t T Mass m M Force F F or MLT-2 Velocity V LT-1 Acceleration a LT-2 Area A L2 Discharge Q L3/s Pressure P FL-2 or ML-1T-2 Density ρ ML-3 Specific weight γ FL-3 or ML-2T-2 Dynamic viscosity µ ML-1T-1 Kinematic viscosity ν L2T-1 EXAMPLE Obtain an equation for distance traveled by a body in a free fall after time t. Assume distance =S Gravity acceleration = g
),( tgfS = According to dimensional homogeneity:
batKgS = Where K is a dimensionless coefficient.
108
202,1)( 22
=⇒=+−=⇒=⇒= +−−
bbaaTLLTLTL baaba
2KgtS =∴
K can be determined by experiment. EXAMPLE Determine the power P of a pump as a function of discharge Q, total dynamic head H and fluid specific weight γ .
HQKPccbaab
TLFLFLTLFLT
HKQP
acbab
cba
cba
γ
γ
==⇒=+−==⇒
=
=
=
−+−
−−−
1133,1,1
)()(33
3131
In S.I. units K=1 which can be determined by experiment. EXAMPLE Find a relationship for the drag force FD exerted by a fluid on a sphere in terms of flow velocity V, sphere diameter D, fluid viscosity µ , and fluid density ρ . Method 1 Obtain the relationship for FD versus D by keeping other variables as constants. 10 points may be appropriate for obtaining a curve. These curves should be plotted for various cases including combinations of 10 µ , 10 V and 10 ρ . Similar curves for FD versus other variables can be obtained. Hence, number of required experiments will be: 10×10×10×10=104 and number of
curves should be 103. If it is assumed to spend half an hour for every experiment and work 8 hours daily, then it takes 2.5 years to prepare the data of the mentioned 1000 curves.
109
Method 2
dcbaD VDF µρ=
To obtain the unknowns a, b, c, and d four equations are required, while only three equations can be written. Method 3 Grouping significant variables into dimensionless parameters by using the pai theorem (Buckingham П theorem) as explained in the following:
1- Select repeating variables. Repeating variables should have the following characteristics:
• Number of them should be equal to number of dimensions. • They should be significant. • They should not be dependant variable. • They should not have similar dimensions. • They should altogether include all dimensions in the problem.
⇒ According to the above-mentioned characteristics DandV ,,ρ are selected as repeating variables.
2- µρπ 1111
zyx DV= In which 1π is dimensionless.
µρ
πρ
µπ
VDOrVD
zyxTLMTMLLLTMLTLM yzyxxzyx
==
−=−=−=⇒==∴ −−−++−+−−−−
11
1111113111111113000
11,11,11)()()(
A dimensionless parameter can be inverted if desired. Similarly:
Dzyx FDV 111
1 ρπ =
222
221222312222123000
22,22,12)()()(
DVF
zyxTLMMLTLLTMLTLM
D
yzyxxzyx
ρπ =
−=−=−=⇒==∴ −−+++−+−−−
110
2/
2/4
(Re)8(Re)
(Re))(),(
0),(
2
22
1
221
112222
21
AVCF
VDfF
DVfF
fVDfDV
FDV
FVDf
f
DD
D
D
DD
ρ
ρππ
ρ
µρ
ρρµρ
ππ
=
=
=
==⇒
=
Where CD is a function of Re..
EXAMPLE The losses hf in turbulent flow through a smooth pipe depend on pipe length L, flow velocity V, diameter D, dynamic viscosity µ , g, and density ρ . Use dimensional analysis to determine the general form of the equation.
0),,,,,/(0),,,,,,(
=
=
gDVLhFgDVLhF
f
f
µρ
µρ
hf/L is a dimensionless parameter, say Lh f /1 =π . Select repeating variables among other variables. The repeating variables will be similar to those of the previous example. Repeating variables are DV ,,ρ
µρ
πµρπVDDV zyx =⇒=∴ 2
2222
gDV zyx 333
3 ρπ =
gDV
VgD
zyxTLMLTLLTMLTLM yzyxxzyx
2
323
23133333233133000
13,23,03)()()(
=⇒=
=−==⇒==∴ −−+++−−−−
ππ
111
gV
DLfh
gV
DLfh
gDVf
Lh
gDVVDf
Lh
gDVVD
Lh
F
f
f
f
f
f
2
2(Re)2
(Re
,
0,,
2
2
2
2
2
2
1
2
=
=
=
=
=
∴
µρ
µρ
The last equation is called the Darcy-Weisbach equation. For rough pipes with absolute roughness ε , another dimensionless parameter
Dε
π =4 will be added . Hence, the equation will be as follows:
gV
DL
Dfh f 2
Re,2
=
ε
Second Method -Select Repeating Variables:
LDLTVML === −− ,, 13ρ -Obtain dimensions in terms of repeating variables:
33,, DLM
VD
VLTDL ρρ =====
-Obtain non-repeating variables in terms of repeating variables:
µρ
πρρµVDVDVDDDTML =⇒=== −−−−
111311 )/)()((
gDVDVVDDLTg
2
2222 /)/( =⇒=== −− π
112
DlDLl =⇒== 3π
Dh
DLh ff =⇒== 4π
DDL ε
πε =⇒== 5
lh
DlDh ff ===
//
3
46 π
ππ
gV
Dl
Dfh
gV
Dl
Dfh
gDV
DVDf
lh
Dlh
gDVVDF
F
f
f
f
f
2)(Re,
2)(Re,2
),(
0),,,(
0),,,(
2
2
1
2
1
2
5621
ε
ε
εµ
ρ
εµ
ρ
ππππ
=
=⇒
=
=
=
DIMENSIONLESS PARAMETRS Reynold’s Number
ForceViscousForceInertial
Ama
LLV
TLL
LLV
LTL
LLV
LVVLVLVDVD
=====×==τµ
ρ
µ
ρ
µ
ρµ
ρµ
ρ2
23
2
22
2
2
22
Re
Froude Number
ForceGravityForceInertial
gLLV
LL
gLVFr
gLVFr ==×=⇒= 3
22
2
222
ρρ
ρρ
Mach Number
ForceElasticForceInertial
CLLV
LL
CVMa
CVMa ==×=⇒= 22
22
2
2
2
22
ρρ
ρρ
113
MODEL STUDIES AND SIMILITUDE Model studies of proposed hydraulic structures and machines are frequently undertaken as an aid to the design. Geometric Similitude The ratios of all corresponding dimensions must be the same.
rprototype
el LLL
=mod =constant
Dynamic Similitude The ratios of the various types of forces must be the same at corresponding points.
.mod constFF
prototype
el =
pviscous
pinertial
p
pm
pviscous
mviscous
pinertial
minertial
pviscous
pinertial
mviscous
minertial
p
m
mviscous
minertial
m
FF
FF
FF
FFFF
FF
=
=⇒===⇒
=
Re
ReRe1ReRe
Re
Similarly, it can be proved that pmpm MaMaFrFr == , and all dimensionless parameters should be equal when a dynamic similitude exists. In order to achieve exact similitude between model and prototype, the scale ratio should be 1:1(Strict fulfillment of these requirements (equality of the dimensionless parameters) is generally impossible to achieve unless the scale ratio is 1:1
114
Therefore, the dominant forces and consequently the corresponding dimensionless number is considered to be equal for model and prototype. Pipe Flow⇒ Rem =Rep Hydraulic structures ⇒ Frm=Frp Very high velocities of compressible flow, i.e., sonic and super-sonic velocities ⇒ Mam=Map
λ==⇒
=⇒=
m
p
m
p
p
p
m
mpm
LL
VV
gLV
gLVFrFr
2222
λ
λλ
=
×=×=⇒==
m
p
p
m
m
p
m
p
p
pp
m
mm
tt
VV
LL
tt
VL
tVLt 1,
( )
2/52
2/533
3
3
//
//
λλλ
λλ
λ
=×==
====
mm
pp
m
p
mp
mp
mm
pp
m
p
AVAV
ttLL
tLtL
Force ratio, for example, on gates:
3λγ
γ==
mm
pp
m
p
AhAh
FF
Assignment#5 5.6.1, 5.6.2, 5.2
115
VISCOUS FLOW This chapter deals with real fluids, that is, situations in which irreversibilities (losses) are important, viscosity is the fluid property that causes shear stresses in a moving fluid, viscosity is also one mean by which losses are developed. In turbulent flows random fluid motions, superposed on the average; create apparent shear stresses that are more important than those due to viscous shear. Turbulent flow, however, has very erratic motion of fluid particles, with a violent transverse interchange of momentum. We have used continuity and Euler equations which was integrated to Bernoulli equation to solve problems without viscous effects. In order to solve problems with viscous effects continuity and Navier-Stokes equations should be used. Navier-Stokes Equations
x-component ∑ = xx maF
xViscousx
essurex
Gravityx adFFF ∀=++ ρPr
116
zuw
yuv
xuu
tu
dtdz
zu
dtdy
yu
dtdx
xu
tu
dtduax
∂∂
+∂∂
+∂∂
+∂∂
=
∂∂
+∂∂
+∂∂
+∂∂
==
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
+
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
∂∂
+∂∂
+∂∂
+∂∂
=∂
∂+
∂
∂+
∂∂
−
2
2
2
2
2
2
2
2
2
2
2
2
1
1
zu
yu
xu
xp
zuw
yuv
xuu
tu
gzu
yu
xu
xp
zuw
yuv
xuu
tu
zuw
yuv
xuu
tu
zyxpg
x
xzxyx
νρ
νρ
ρττ
ρ
Or
uxp
zuw
yuv
xuu
tu 21
∇+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
νρ
Similarly: y-component
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
+
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
2
2
2
2
2
2
2
2
2
2
2
2
1
1
zv
yv
xv
yp
zvw
yvv
xvu
tv
gzv
yv
xv
yp
zvw
yvv
xvu
tv
y
νρ
νρ
vyp
zvw
yvv
xvu
tv 21
∇+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
νρ
z-component
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
+
∂∂
+∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
2
2
2
2
2
2
2
2
2
2
2
2
1
1
zw
yw
xw
zp
zww
ywv
xwu
tw
gzw
yw
xw
zp
zww
ywv
xwu
tw
z
νρ
νρ
wzp
zww
ywv
xwu
tw 21
∇+∂∂
−=∂∂
+∂∂
+∂∂
+∂∂
νρ
117
Two Dimensional Navier Stokes equations
y
x
gy
vxv
yp
yvv
xvu
tv
gyu
xu
xp
yuv
xuu
tu
+
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
+
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
2
2
2
2
2
2
2
2
1
1
νρ
νρ
Or
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
2
2
2
2
2
2
2
2
1
1
yv
xv
yp
yvv
xvu
tv
yu
xu
xp
yuv
xuu
tu
νρ
νρ
EXAM PLE Derive an expression for the flow past a fixed cross section of the figure for laminar flow between the two moving plates. Find the shear stress at each plate.
x
y
118
)(0
)0(0
0
)0(0
)(0
)(0
1
2
2
2
2
2
2
directionxtheincomponentnohasggxu
xu
xp
vyuv
continuityxu
FlowSteadytu
gyu
xu
xp
yuv
xuu
tu
x
x
−=
=∂∂
=∂∂
=∂∂
==∂∂
=∂∂
=∂∂
+
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
νρ
12
2
2
2
00 CCyuCdydu
dyud
yu
+=⇒=⇒=⇒=∂∂
Boundary Conditions y=0, u=-V 1CV =−⇒
y=a, u=Ua
VUVCaU +⇒−=⇒
Vya
VUu −+
=
aVU
yu +
=∂∂
= µµτ
EXAM PLE In the figure one plate moves relative to the other as shown; sPa.08.0=µ and
3/850 mkg=ρ . Determine the velocity distribution, the discharge, and the shear stress exerted on the upper plate.
y
119
xp
yu
yu
xp
yu
xu
xp
yuv
xuu
tu
∂∂
=∂∂
∂∂
+∂∂
−=
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
µ
νρ
νρ
1
10
1
2
2
2
2
2
2
2
2
At point 1 pa
hPP264053806.98501400 =×××=
+= γ
At point 2 pahPP
800=+= γ
1m/s
P1=1.4kpa
P2=0.8kpa
3m
3m
x 6 mm
120
212
1
2
2
2
2
3771808.0
603508.0
6035603508.01
/603523
26405800
CyCyu
Cydydu
dyud
yu
mpadxPd
++−=
+−=
−=⇒−×=∂∂
∴
−=−
=
Boundary Conditions
yyuCsmuy
Cuy
646.5937718
646.59/1,006.000,0
21
2
+−=∴
=⇒−===⇒==
smdyyyudyQudydQ /00164.0)646.5937718(1 3006.0
0
2006.0
0
−=+−==⇒×= ∫∫
pay
yu
y 44.31)646.59377182(08.0 006.0 −=+−××=∂∂
= =µτ
EXAMPLE For the fluid flowing downward on the inclined surface, find u , Q and the shear stress at the bed. Fluid viscosity = µ , fluid specific gravity = γ.
θ
b
y
x
121
1
2
2
2
2
2
2
2
2
sin
sinsin0
1
Cygdydu
gdy
udgyu
gyu
xu
xp
yuv
xuu
tu
x
+−
=⇒
−=⇒+
∂∂
=
+
∂∂
+∂∂
+∂∂
−=∂∂
+∂∂
+∂∂
µθρ
µθρ
θν
νρ
Boundary Conditions
22
1
2sin
sin00,0
Cyu
ygdydu
Cuy
+−
=
−=
=⇒==
µθγµ
θρ
2
2 2sin0, bCuby
µθγ
=⇒==
22
2sin
2sin byu
µθγ
µθγ
+−
=
)(2sin 22 ybu −=
µθγ
µθγ
µθγ
3sin)(
2sin 3
0
22
0
bdyybudyQbb
=−== ∫∫
bg
ygygyu
bed θρτ
θρµ
θρµµτ
sin
sinsin
−=
−=−
=∂∂
=
122
LAMINAR FLOW THROUGH CIRCULAR PIPES Cylindrical Coordinates
z-Component
∂∂
+∂∂
+
∂∂
∂∂
+∂∂
−=
∂
∂+
∂∂
+∂
∂+
∂∂
2
2
2
2
2
110zVV
rrVr
rrzP
zVVV
rV
rVV
tV zzzz
zzz
rz
θµ
θρ θ
123
1
2
2
11
10
Cdr
dVrdzPdr
drdVr
drd
dzPdr
drdVr
drd
rdzPd
rVr
rrzP
z
z
z
z
+=
=
=
∂∂
∂∂
+∂∂
−=
µ
µ
µ
µ
At r=0 , Vz =Vmax ,i.e. , 00 1 =⇒= Cdr
dVz
2
2
2
4
22
CdzPdrV
dzPdr
drdV
drdVr
dzPdr
z
zz
+=
=⇒=
µ
µµ
EquationPoiseuilleHagenRr
dzPdRV
dzPdRCC
dzPdRVRr
z
z
−
−−=∴
−=⇒+=⇒==
2
22
2
22
2
14
4400,
µ
µµ
−=⇒−= 2
2
max
2
max 14 R
rVVdzPdRV zµ
Average Velocity V
)1(82
2122
max
02
2
max0 dz
PdRVrdrRrVrdrVdAVV
RR
zz µππ −==×
−=×== ∫∫∫
Darcy-Weisbach Equation
)2()/
2()/
2(
)/()/()/()(
2
2
1
2
12
Lh
L
ZPg
VZPg
V
dzPd
LZPZPZP
dzdZP
dzd
dzPd
fγγγ
γ
γγγγγγ
−=++−++
−=
+−+=+=+=
Substituting for dzPd from equation (2) in equation (1) yields:
124
)3(32888 22
22
DV
RVh
LhR
dzPdRV f
f
γµ
γµ
γµµ
==⇒−×−=−=
It should be noted that in laminar flow Vh f ∝ On the other hand the Darcy-Weisbach equation is as follows:
)4(2
2
gV
DLfh f =
Comparing equations (3) and (4), it can be concluded that :
Re64
=f
EXAMPLE Find the discharge in the pipe shown below.
gV
gV
gVPZE
gV
gV
gVPZE
25.37
280003000000
2
230
280002000005
2222
2222
22211
11
+=++=++=
+=++=++=
γ
γ
E2 >E1 Hence, flow direction should be from 2 to 1.
125
mg
Vg
VEEh f 5.7)2
30()2
5.37(22
12 =+−+=−=
gV
DLfh f 2
5.72
==
Assuming laminar flow (which is the opposite in practice);
gV
V
gV
DL
VDgV
DLfh f
201.010
04.0
01.0806.9
8000645.7
2/64
25.7
2
22
××
××=
===µρ
V= 0.47 m/s 6.9504.0
01.047.0806.9
8000
Re =××
==⇒µ
ρVD
Hence, the assumption of laminar flow is correct. REYNOLD’S EXPERIMENT
Glass tube
dye
126
Laminar flow is defined as flow in which the fluid moves in layers, or laminas, one layer gliding smoothly over an adjacent layer with only a molecular interchange of momentum. Any tendencies toward instability and turbulence are damped out by viscous shear forces that resist relative motion of adjacent fluid layers. Turbulent flow, however, has very erratic motion of fluid particles, with a violent transverse interchange of momentum. The nature of the flow, that is, whether laminar or turbulent, and its relative position along a scale indicating the relative importance of turbulent to laminar tendencies are indicated by the Reynolds number. For small flows, the dye stream moved as a straight line through the tube, showing that the flow was laminar. As the flow rate increased, the Reynolds number increased, since D, ρ and μ were constant and V was directly proportional to the rate of flow. With increasing discharge a condition was reached at which the dye stream wavered and then suddenly, broke up and was diffused or dispersed throughout the tube. The flow had changed to turbulent flow with its violent interchange of momentum that had completely disrupted the orderly movement of laminar flow. By careful manipulation Reynolds was able to obtain a value Re=12000 before turbulence set in. A later investigator, using Reynolds’ original equipment, obtained a value of 40000 by allowing the
127
water to stand in the tank for several days before the experiment and by taking precautions to avoid vibrations of the water or equipment. These numbers, referred to as Reynolds upper critical numbers, (lately, Re=1000000 was obtained before turbulence at Brown university) have no practical significance in that an ordinary pipe installation has irregularities that cause turbulent flow at a much smaller value of the Reynolds number. Starting with turbulent flow in the glass tube, Reynolds found that it always becomes laminar when the velocity is reduced to make Reynolds’ number less than 2000. This is the Reynolds lower critical number for pipe flow and is of practical importance. With the usual piping installation, the flow will change from laminar to turbulent in the range of Reynolds’ numbers from 2000 to 4000. For the purpose of this treatment it is assumed that the change occurs at Re=2000. In laminar flow the losses are directly proportional to the average velocity, while in turbulent flow the losses are proportional to the velocity to a power varying from 1.7 to 2.
Starting with low Reynolds’ number (laminar flow), the upper critical value was 12000, 40000, and 1000000. Starting with high Reynolds’ number (turbulent flow), the lower critical value was always 2000. This can be interpreted due to stability principles. Stable flow is the flow in which the disturbance energy is damped. Laminar flow with Reynolds’ number less than 2000 is stable, i.e., disturbance energy damps.
106 105 12000 10000 5000 2000 1000 100
106 105 12000 10000 5000 2000 1000 100
128
Laminar flow with Reynolds’ number greater than 2000 is unstable, i.e., disturbance energy does not damp and changes the laminar flow to turbulent. At Brown university, disturbance and vibrations were avoided by using more fixed equipments. MOODY DIAGRAM
Laminar Zone (Re =0-2000)
Re64
=f which plots a straight line with slope equals to -1 on a log-log chart.
Head-loss hf is independent of roughness. Critical Zone (Re=2000-4000) The flow may be either laminar or turbulent.
129
Transition Zone The zone in which hf is a function of Re and
Dε . Colebrook formula in this
zone holds:
+−=
fDLn
f Re51.2
7.3/86.01 ε
Complete Turbulent Zone In this zone all curves are almost horizontal which means that hf is a function of
Dε only and is not a function of Re.
It should be noted that the relative roughness curves 001.0<
Dε approach the
smooth pipe curve for decreasing Reynolds’ numbers. This can be explained by the presence of a laminar film at the wall of the pipe that decreases in thickness as the Reynolds’ number increases. For certain ranges of Reynolds’ number in the transition zone the film completely covers small roughness projections, and the pipe has a friction factor the same as that of a smooth pipe. The larger Reynolds’ numbers projections protrude through the laminar film, and each projection causes extra turbulence that increases the head loss. For the zone marked “complete turbulent rough pipes”, the film thickness is negligible compared with the height of roughness projections and each projection contributes fully to the turbulence. Viscosity does not affect the head-loss in this zone, as evidenced by the fact that the friction factor does not change with the Reynolds’ number. In this zone 2Vh f ∝
130
SIMPLE PIPE PROBLEM Type 1 fh⇒ is unknown Type 2 QorV⇒ is unknown Type 3 D⇒ is unknown EXAMPLE TYPE 1 Q=140 L/s
sm /00001.0 2=ν L = 400 m D = 200 mm cast iron pipe mm25.0=⇒ ε
8912700001.0
2.0456.4Re
/456.44/2.0
140.04/ 22
=×
==
=×
==
ν
ππVD
smD
QV
00125.0
20025.0
==mmmm
Dε
⇒ Colebrook Formula
+−=
fDLn
f Re51.2
7.3/86.01 ε
⇒
×+−=
fLn
f 8912751.2
7.300125.086.01 023.0=f
mg
VDLfh f 58.46
806.924/2.0
140.0
2.0400023.0
2
2
22
=×
×××== π
EXAMPLE TYPE 2 T =150C water flow D = 300mm riveted steel pipe
mhmm
f 63
==ε
L = 300 m Q =?
131
termondtheneglectingequationColebrookgumm
mmD
secsin01.0300
3⇒==
ε
04.007.301.086.01
=⇒
+−= fLn
f
Darcy-Wesbach equation
smVV /715.1806.923.0
30004.062
=⇒×
=
From appendix C , sm /1013.1 26−×=ν
01.0,4550001013.1
3.0715.1Re 6 ==×
×==
− DVD εν
Colebrook formula 038.0=f ⇒ smVV /76.1806.923.0
300038.062
=⇒×
=
⇒==××
==−
01.0,4672561013.1
3.076.1Re 6 DVD εν
Colebrook formula 038.0=f
V= 1.76 m/s
Q=VA = sm /1244.043.076.1 3
2
=××π
EXAMPLE TYPE 3 Determine the size of clean wrought iron pipe ( 00015.0=ε ) required to convey 8.93 cfs oil, sft /0001.0 2=ν , for 10000 ft with a head-loss of 75 ft. Try 02.0=f in the middle of the diagram
ftDDD
398.1806.92
4/93.8
1000002.075
2
2
=⇒×
×××= π
00011.0398.1
00015.0,814000001.0
398.14/398.1
93.8
Re2
===×
×==D
VD επν
inftDfformulaColebrook 6.16382.1019.0 ==⇒=⇒
132
NON-CIRCULAR CROSS SECTIONS
gV
DLfh
hf 2
2
= ,
+−=
fDLn
fh
Re51.2
7.3/
86.01 ε , ν
hVD=Re
Where
pA
perimeterwettedareationalcrossDh 4sec4 ==
,
Where EXAMPLE
gV
DLfh
hf 2
2
=
+−=
fDLn
fh
Re51.2
7.3/86.01 ε
νhVD
=Re
pA
perimeterwettedareationalcrossDh 4sec4 ==
133
gV
gV
DLfh
gVPZ
gV
DLf
gVPZ
EhE
h
h
f
200
200
22222
222
2
2211
1
21
++=−++
++=−++
=−
γγ
134
MINOR LOSSES Losses which occur in pipe lines because 0f bends, elbows, joints, valves, etc., are called local or minor losses. In almost all cases the minor loss is determined by experiment. However, one important exception is the head-loss due to a sudden expansion in a pipe line. Sudden Expansion in A pipe line
gV
DD
gVV
gVKhm 2
12
)(2
21
22
2
12
212
−=
−==
135
Continuity:
)1(2211 AVAV = Energy:
)2(22
222
211
gVPhm
gVP
+=−+γγ
Momentum:
)3()( 212212111 QVQVAPAAPAP ρρ +−=−−+ Having known P1, A1, A2, Q , the unknowns V2, P2, hm by solving equations (1), (2) and (3), simultaneously can be obtained:
22
2
1
21
22
2
12
21
1
21
2)(
−=⇒
−=
−=
DDK
gV
DD
gVVhm
For the joint of a pipe and a reservoir , D1/D2 approaches zero and hence, K=1 This means that all kinetic energy will be dissipated. Head-loss due to Gradual Expansion
gVVKhm 2
)( 221 −
=
136
Head loss due to a sudden contraction
The head-loss from section 1 to the vena contrata ( the section of greatest contraction of the jet) is small compared with the loss from section 0 to section 2 , where velocity head being reconverted into pressure head (expansion):
137
gVK
gV
Cg
VCV
h
CV
AAVV
AAVAVAV
gVVh
C
Cm
C
m
2211
2
/
2)(
22
22
2
2
22
2
20
22
0
202200
220
=
−=
−
=
===⇒=
−=
K
K K
K K
K
138
EXAMPLE Find the discharge through the pipe line in the figure for H=10 m and determine the head-loss for Q =60 L/s.
200C
60 m 30 m
10 m
12 m
150mm
139
)1(2
)6803.13(
200
210
29.02
25.0
215.010200
2210
29.02
25.0
22
2
22222
222
2
2222211
1
2211
gVfH
gV
gV
gV
gV
gVfH
gVPZ
gV
gV
gV
gV
DLf
gVPZ
EhE f
+=
++=
+××++−++
++=
+××++−++
=− −
γγ
sLsmVAQsmV
fColebrookD
smVfD
/9.45/0459.0415.06.2/6.2)1(
023.00017.0,3910001001.1
15.063.2Re
/63.2)1(022.00017.0
32
6
==××==⇒=⇒⇒
=⇒⇒==××
=⇒
=⇒⇒=⇒=
−
π
ε
ε
For the second part, with Q = 60 L/s , the solution is straight forward:
mH
fD
smAQV
06.17)1(
023.00017.0,505000Re/4.34/15.0
06.02
=⇒⇒
=⇒==⇒=×
==ε
π
Assignment 6.3.1, 6.3, 6.14, 6.20, 6.21, 6.28, 6.34, 6.78, 6.79, 6.100, 6.110
140
BOUNDARY LAYER Consider flow over a flat plate as shown in the figure:
The flow approaching the plate is of uniform velocity, U0 . From the no-slip condition, we know the velocity at the plate must be zero. The plate exerts a retardation force on the flow; it slows the fluid in the neighborhood of the surface. At , the flow will not be influenced by the presence of the plate. At some intermediate point, the velocity has a value lies between zero and U0.
The flow field can be divided into two general regions. In the region adjacent to the boundary, shear stresses are present; the region is called the boundary layer. Outside the boundary layer the velocity gradient is zero and hence the shear stresses are zero.
U0 y=δ
y=δ
141
is the boundary layer thickness. The plate would influence a greater region of the flow field as we move farther down the plate. DRAG FORCE ON IMMERSED BODIES In the region between A and B, the pressure force behind fluid particles is sufficient to overcome the resisting shear force and the motion in the flow direction is maintained. Now consider an element of fluid inside the boundary layer on the back of the cylinder beyond point B. Since the pressure increases in the direction of flow, the fluid element experiences a net pressure force opposite to its direction of motion. Finally the momentum of the fluid in the boundary layer is insufficient to carry the element further into the region of increasing pressure. The fluid layers adjacent to the solid surface will be brought to rest and the flow will separate from the surface. The point at which this occurs is called the point of separation.
δ
A
Stagnation Point V=0
B Velocity increases Pressure decreases 0>
dxdP
MaximumVelocity
Velocity decreases Pressure increases 0<
dxdP
142
Boundary layer separation results in the formation of a relatively low pressure region behind a body; this region which is deficient in momentum, is called the wake. Thus, for separated flow over a body, there is a net unbalanced of pressure forces in the direction of flow; this results in a pressure drag on the body. The greater the size of the wake behind a body, the greater is the pressure drag.
143
Reducing the size of wake results in reducing the pressure drag. Since a large wake results from boundary layer separation, which in turn is related to the pressure of an adverse pressure gradient (increase of pressure in the direction of flow), reducing the adverse pressure gradient should delay the onset of separation and hence, reduce the drag. STREAMLINING A BODY REDUCES THE ADVERSE PRESSURE GRADIENT. Streamling the body delays the onset of separation; although the surface area of the body and, hence, the total shear force acting on the body is increased, the drag is reduced significantly.
Wake
A
Stagnation Point V=0
B Velocity increases Pressure decreases 0>
dxdP
MaximumVelocity
Velocity decreases Pressure increases
Wake
Boundary Layer
144
COMPRESSIBLE FLOW Flows in which variation in density are not negligible are termed compressible. For many practical cases liquids are incompressible. However, water hammer and cavitation are examples of the importance of compressibility effects in liquid flows. Gas flows also may be considered incompressible provided the flow speeds are small relative to the speed of sound; the ratio of flow speed V, to the local speed of sound, a, in the gas is defined as the Mach number,
145
For values of M <0.3, the maximum density variation is less than 5 percent. Thus gas flows with M<0.3 can be treated as incompressible; a value of M =0.3 in air at standard conditions corresponds to a speed of approximately 100 m/s. Compressibility effects are very important in the design of modern high-speed aircraft and missiles, power plants, fans, and compressors.
RTuPuh +=+= ρ/ h is the enthalpy of the gas and u is the internal energy
vv T
uC
∂∂
= specific heat at constant volume ,
p
p ThC
∂∂
= specific heat at constant pressure
v
p
CC
k = k is the ratio of specific heats
kRTa = a is the sound speed CONTINUITY EQUATION
.consVA =ρ ENERGY EQUATION When there is no heat transfer and no work done by pumps and turbines in the flow of an ideal fluid, the motion is isentropic (Adiabatic[dQ=0] + reversible[dS=0]) and the steady flow energy equation for the streamline becomes:
.2
2
constVPu =++ρ
, .2
2
constVh =+ or .2
2
constVTC p =+
146
EULER EQUATION
0=++ VdVdPgdZρ
For compressible flow, however, the term gdZ is usually dropped (change of elevation is negligible) and the Euler equation written:
0=+VdVdPρ
INTEGRATION OF THE EULER EQUATION When the Euler equation is integrated along the streamline for isentropic flow of a perfect gas, it becomes:
∫=− 1
2
21
22
2
P
P
dPVVρ
Obtaining ρ from kk
PP
1
1
ρρ= and substituting in the above integral,
yields:
−
−=
−−k
k
PP
kkPVV
1
1
2
1
12
12
2 112 ρ
Or obtaining ρ from kk
PP
2
2
ρρ= and substituting in the above
integral, yields:
−
−
=−
−
112
1
2
1
2
22
12
2k
k
PP
kkPVV
ρ
147
EXAMPLE An airplane flies at 644 km/h (179 m/s) through still air at 90 kPa and -20oC. Calculate pressure, temperature, and air density at the stagnation point (On nose of fuselage of the wings).
31
1
111
/24.1)27320(8.286100090
mkg
RTP
=
+−××=×=
ρ
ρρ
smkRTa /3192538.2864.111 =××==
562.0319179
1 ==M
CKT
T
VTCVTC
o
pp
4269
010032
1792531003
22
2
2
2
22
2
21
1
−==
+=+×
+=+
kPaP
P
PP
kkPVV k
k
5.111
901
14.14.1
24.1100090
21790
112
2
4.114.1
22
1
1
2
1
12
12
2
=
−
−×
=−
−
−=
−
−
−
ρ
31
2
222
/45.1)2734(8.28610005.111
mkg
RTP
=
+−××=×=
ρ
ρρ
SUBSONIC AND SUPERSONIC VELOCITIES Taking the differential of the continuity equation .consVA =ρ and dividing by VAρ yields:
148
)1(0=++VdVd
AdA
ρρ
And considering the Euler equation:
22 00
00
aVdVdVdVdaVdVd
ddP
VdVdddPVdVdP
−=⇒=+⇒=+×
=+×⇒=+
ρρ
ρρ
ρρ
ρ
ρρ
ρρ
Substituting the last expression for
ρρd in equation (1) gives:
( )12 −= MVdV
AdA
Subsonic Flow 001,0 2 >⇒<−<
VdVM
AdA Velocity increases
Convergent Nozzle
149
001,0 2 <⇒<−>
VdVM
AdA Velocity decreases
Supersonic Flow 001,0 2 <⇒>−<
VdVM
AdA Velocity decreases
Divergent Nozzle
Convergent Nozzle
150
001,0 2 >⇒>−>
VdVM
AdA Velocity increases
THROAT 0<
AdA 0>
AdA
0=
AdA throat
⇒= 0
AdA Either 12 −M ; 1=M or 1≠M , Velocity
VdV
⇒= 0 is either
minimum or Maximum. Accordingly it can be concluded that if the throat velocity is not sonic it will be a maximum in subsonic flow and a minimum in supersonic flow. For flow at sonic speed (M=1) the rate of change of area must be zero; that is, this might occur at a maximum or minimum cross section; use of the preceding conclusions will show this to be restricted to a minimum section (a throat) only. SONIC VELOCITY (M=1) OCCURS ONLY AT A THROAT.
Divergent Nozzle