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2.0 Introduction
Fluid mechanics is the study of the behavior of fluids at rest, fluid statics,
and in motion, fluid dynamics, and of the properties of fluids insofar as they
affect the fluid motion. A fluid may be either a gas or a liquid. The molecules
of a gas are much farther apart than those of a liquid. Hence a gas is compressible
while a liquid is relatively incompressible.
A vapor is a gas whose temperature and pressure are such that it is very
near the liquid phase. Steam is considered a vapor because its state is
normally not far from that of water. A gas may be defined as a highly super-
heated vapor, that is, its state is far removed from the liquid phase. Air is
considered a gas because its state is normally very far from that of liquid air.
The volume of a gas or vapor is greatly affected by changes in pressure or
temperature or both. It is usually necessary to take into account the changesin volume and temperature in dealing with gases or vapors. Whenever
significant temperature or phase changes are involved in dealing with vapors
and gases, the subject is largely dependent on heat phenomena, thermodynamics.
2
Fluid Mechanics
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The objective of this chapter is to introduce the reader to certain termi-nology, concepts, laws, and equations that are directly applicable to the
design of air-cooled heat exchangers and cooling towers.
2.1 Viscous Flow
Consider the flow of a fluid over a flat plate (Fig. 2.1.1).
Figure 2.1.1 Boundary Layer Development along a Flat Plate
Beginning at the leading edge of the plate, a region develops where the
influence of viscous forces is felt. These viscous forces are described in terms
of a shear stress, τ, between the fluid layers. If this stress is assumed to be pro-
portional to the normal velocity gradient, the defining equation for viscosi-
ty, known as Newton’s equation of viscosity, is
(2.1.1)
The constant of proportionality, µ, is called the dynamic viscosity. The
values of µ for some fluids are given in appendix A.
dv
d y τ = –µ
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The velocity or hydrodynamic boundary layer is the region of flow thatdevelops from the leading edge of the plate in which the effects of viscosity
are observed. The y-position where the boundary layer ends is arbitrarily
chosen at a point where the velocity becomes 99% of the free stream value.
The boundary layer thickness, δ, is defined as the distance between this point
and the plate.
Initially, the boundary layer development is laminar. At some critical
distance from the leading edge, small disturbances in the flow begin to
become amplified and a transition process takes place until the flow becomesturbulent. This depends on the flow field and fluid properties.
The physical mechanism of viscosity is one of momentum exchange. In
the laminar portion of the boundary layer, molecules move from one lamina
to another and carry momentum corresponding to the velocity of the flow.
There is a net momentum transport from regions of high velocity to regions
of low velocity, which creates a force in the direction of flow. This force may
be expressed in terms of the viscous shear stress as given by Equation 2.1.1.
The rate at which the momentum transfer takes place is dependent onthe rate at which the molecules move across the fluid layers. In a gas, the
molecules would move about with some average speed proportional to the
square root of the absolute temperature since we identify temperature with
the mean kinetic energy of a molecule in the kinetic theory of gases. The
faster the molecules move, the more momentum they will transport. Hence
we should expect the viscosity of a gas to be approximately proportional to
the square root of temperature, and this expectation is corroborated fairly
well by experiment.
The laminar velocity profile is approximately parabolic in shape. The
transition from laminar to turbulent flow occurs typically when
where
v ∞ = free stream velocity
x = distance from the leading edge of the plate
ν = µ/ρ, the kinematic viscosity of the fluid
qv ∞x
l
v ∞x
m
= ≥3.2x105
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This particular dimensionless group or ratio of inertial force to viscousforce is called the Reynolds number after the British scientist-engineer who
first did extensive research on flow in the late 1800s.
(2.1.2)
Although the critical Reynolds number for transition on a flat plate isusually taken as 3.2 x 105 for most analytical purposes, the critical value in a
practical situation is strongly dependent on the surface roughness conditions
and the turbulence level of the free stream. The normal range for the beginning
of transition is between 3.2 x 105 and 106. With very large disturbances
present in the flow, transition may begin with Reynolds numbers as low
as 105. For flows which are very free from fluctuations, it may not start until
Rex = 2 x 106 or more. In reality, the transition process covers a range of
Reynolds numbers. Completed transition and fully developed turbulent flow
usually is observed at Reynolds numbers twice the value at which transition began.
A qualitative picture of the turbulent flow process may be obtained by
imagining macroscopic chunks of fluid transporting momentum instead of
microscopic transport on the basis of individual molecules. The turbulent
boundary layer is more complex than the laminar boundary layer because the
nature of the flow in the former changes with distance from the plate surface.
The zone adjacent to the wall is a layer of fluid, which, because of the
stabilizing effect of the wall, remains laminar even though most of the flow
in the boundary layer is turbulent. This very thin layer is called the laminarsublayer, and the velocity distribution in this layer is related to the shear
stress and viscosity using Newton’s viscosity law.
The flow zone outside the laminar sublayer is turbulent. The turbulence
alters the flow regime so much that the shear stress, as given by τ = - µ dv/dy,
is not significant. The mixing action of turbulence causes small fluid masses
to be swept back and forth in a direction transverse to the mean flow direction.
As a small mass of fluid is swept from a low-velocity zone next to the sublayer
into a relatively high-velocity zone farther out in the stream, the mass has a
retarding effect on the high-velocity stream. This mass of fluid, through an
exchange of momentum, creates the effect of a retarding shear stress applied
to a high-velocity stream. A small mass of fluid originates farther out in the
boundary layer in a high-velocity flow zone and is swept into a region of
ρv ∞x
µ Rex =
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relatively low velocity. This has an effect on the low-velocity fluid much likeshear stress augmenting the flow velocity. In other words, the mass of fluid
with relatively higher momentum will tend to accelerate the lower velocity
fluid in the region into which it moves. Although the process described
previously is a momentum-exchange phenomenon, it has the same effect as
a shear stress applied to the fluid. In turbulent flow, these stresses are termed
apparent shear stresses or Reynolds stresses. The turbulent velocity profile has a
nearly linear portion in the sublayer and a relatively flat profile outside this region.
Consider the flow in a tube shown in Figure 2.1.2. A boundary layerdevelops at the entrance. Eventually the boundary layer fills the entire tube,
and the flow is said to be fully developed. If the flow is laminar, a parabolic
velocity profile is experienced as illustrated in Figure 2.1.2a. When the flow
is turbulent, a somewhat blunter profile is observed (Fig. 2.1.2b). In a tube,
the Reynolds number based on the mean fluid velocity and the tube diameter
is again used as a criterion for laminar and turbulent flow. For Red = ρvd/ µ ≤ 2300,
the flow is usually observed to be laminar, whereas for Red ≥ 10,000, it is turbulent.
Fig. 2.1.2 Velocity Profiles in a Tube: (a) Laminar Flow (b) Turbulent Flow
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Again, a range of Reynolds numbers for transition may be observeddepending on the roughness of the pipe and smoothness of the flow. The
generally accepted range for transition, also referred to as the critical region,
is 2000 < Red < 4000. Laminar flow has been maintained up to Reynolds
numbers of 25,000 in carefully controlled laboratory conditions.
The mass flow rate or continuity relationship for one-dimensional flow
in a tube is
(2.1.3)
where
m = mass rate of flow
v = mean velocity
A = cross-sectional area of the tube
The mass flux or mass velocity is defined as
(2.1.4)
so the Reynolds number may be written as
(2.1.5)
Similar flow patterns are observed in ducts that do not have a circular
cross section. In those cases, it is convenient to define the following equivalent
or hydraulic diameter for calculating the Reynolds number:
(2.1.6)
This particular grouping of terms is used because it yields the value of the
physical diameter when applied to a circular cross section.
d e =4 x cross-sectional flow area
wetted perimeter
Red = Gd /µ
G = m/ A = ρv
m = ρvA
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2.2 Flow in Ducts
Real flows in ducts experience boundary stresses due to frictional effects,
which cause a pressure drop to occur between any two cross sections.
Typically, a force due to such frictional effects acts on the incompressible
fluid in the elementary control volume shown in Figure 1.4.2, i.e., dF = - τapp P edx.
Here, τapp is the apparent shear stress at the fluid-wall interface, and P e is the
wetted perimeter of the duct according to Shames. If this force is substituted
into Equation 1.4.27 for flow in a round duct or pipe of length L and fixeddiameter d (v 1 = v 2), find
or (2.2.1)
Dimensional analysis shows that, for fully developed pipe flow, the
frictional pressure drop, ∆p, between any two sections is generally related to
the pipe geometry and fluid properties in the following way:
The quantity ρv 2 / 2 is known as the dynamic pressure. The term L/d
considers the geometry of the pipe and ε/d is a measure of the roughness of
the pipe surface.
Based on this analysis, the pipe friction equation, also commonly
referred to as the Darcy-Weisbach equation for pressure drop in a circular
pipe, is obtained according to Weisbach, i.e.,
(2.2.2)∆ p = f D( L/d )(ρv 2/2)
= Function
(
), ,∆p
ρv 2 / 2
ρvd
l
ε
d
L
d
∆p = p1 – p2 = 4τapp L / d
∫ –τapp P edx / A = ∫ –τapp(πd )dx / (πd 2/4) = –4τapp L / d = p2 – p1
2
1
L
0
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The number of velocity heads, v 2 / 2, lost for a given pressure drop, ∆ p, isexpressed by the product of the Darcy friction factor f D and the geometric
factor L/d . The friction factor under consideration corresponds to fully developed
velocity profiles, both laminar and turbulent. These are encountered only
after 25 or more diameters downstream of a pipe inlet.
By equating Equations 2.2.1 and 2.2.2, find
or
Other definitions of the friction factor appear in the literature. In some
cases, the right side of this equation is divided by a factor of 4, giving a
friction factor f = f D
/4, also referred to as the Fanning friction factor. The
friction factor is a function of Re, the cross-sectional shape of the duct and,
in the turbulent flow regime, the relative roughness of the duct surface.
Equations 2.2.1 and 2.2.2 are also applicable to ducts other than circular
pipes, in which case d is replaced by d e.
Laminar flow
An extensive summary of Fanning friction factors for laminar flow in a
variety of ducts is presented by Shah. Using the Hagen-Poiseuille solution for
fully developed laminar flow in a circular duct or pipe, f = 16/ Re = f D/4
according to Shames. The friction factor is independent of the roughness of
the surface in the case of laminar flow.
The results for other duct shapes are shown in Figure 2.2.1. For the
rectangular duct, the friction curve in Figure 2.2.1 may be expressed as
(2.2.3)fRe = 24 [1–1.3553 ( ) + 1.9467 ( )
– 1.7012 ( )
b
a
b
a
b
a
b
a
b
a
2 3
4 5
+ 0.9564 (
) – 0.2537 ( ) ]
f D = 4τapp / (ρv 2/2)
4τapp L/d = f D( L/d )(ρv 2/2)
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Fig. 2.2.1 Friction Factors for Fully Developed Flow
In certain applications where very viscous fluids are to be cooled, e.g., oil
coolers, a twisted tape may be inserted into a circular heat exchanger pipe or
tube. Smooth heat exchanger pipes are usually referred to as tubes. The tape
is inserted to establish swirl flow, thereby increasing the heat transfer coefficientand is twisted around the longitudinal axis shown in Figure 2.2.2.
Fig. 2.2.2 A Tube with a Twisted Tape Insert
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Using Hong and Bergles, the friction factor for fully developed flow in atube with such an insert is given by
where
Re = m/[µ(πd/ 4-t t )]
m = mass flow rate
t t = tape thickness
A more recent equation for the friction factor was derived numerically by
Du Plessis and Kröger:
(2.2.4)
where
a1 = a2/[ Re(15.767 – 0.14706 t t /d )]
a2 = Ats d 2/(a3a42)
a3 = 2 P 2 (a6 – 1) /p – dt t
a4 = 4a3/a5
a5 = 2d – 2t t + πd /a6
a6 = [1 + (πd/ 2 P )2]0.5
Ats = πd 2/4
This equation is valid for 50 ≤ Re ≤ 2000 and for P/d ≥ 2.
In the case of hydrodynamically developing flow in a duct from an initial
uniform velocity distribution, an apparent Fanning friction factor is defined.
The factor takes into account both the skin friction and the change in
momentum rate caused by a change in the shape of the velocity profile in the
hydrodynamic entrance region. In a long duct , the apparent friction factor
may be expressed in terms of an incremental pressure drop number K ∞ as
f = a1 [1 + { Re/(70( P /d )1.3)}1.5]0.333
f = 45.9 / Re
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(2.2.5)
For a circular duct or pipe,
(2.2.6)
Du Plessis proposes the following general correlation which can beapplied to developing laminar flow in ducts of various cross sections:
(2.2.7)
where
fRe = the value for fully developed flow
n = an exponent dependent on the duct geometry
This correlation agrees well with similar ones by Shah.
For concentric annular ducts having inner and outer radii of r i and r o, values
of n are listed in Table 2.2.1.
Table 2.2.1 Values of Exponent for Annular Ducts
The case r i /r o = 0 corresponds to a pipe while r i /r o = 1 can be used for
parallel plates.
f app Re=[ (fRe)n+{3.44/( L/(d e Re))0.5}n
]1/n
f app Re=16+0.313dRe/ L for L/(dRe)≥0.06
f app Re = f Re + K ∞d e Re/4 L
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For rectangular ducts, fRe is determined using Equation 2.2.3. The valuesfor n are listed in Table 2.2.2.
Table 2.2.2 Values of Exponent for Rectangular Ducts
For isosceles triangular ducts having apex angles of 2θ degrees, the val-
ues of n are listed in Table 2.2.3.
Table 2.2.3 Values of Exponent for Isosceles Triangular Ducts
In general, the hydraulic entry length Lhy = x/(d e Re) is the dimensionless
length required for the centerline velocity to attain 99% of its fully developed
value. Values for Lhy and K ∞ for different duct sections are listed in Table 3.2.1.
When heat is transferred to or from the fluid, all physical properties are
evaluated at the mean fluid temperature. The latter is also referred to as the
bulk or mixing cup temperature according to Holman. For those problems
involving large temperature differences between the fluid and the duct wall,
Shah introduced corrections to provide for the temperature dependence of the fluid properties.
In the case of gases, the friction factor evaluated at the bulk mean
temperature is multiplied by one of the following factors:
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(T w /T) for 1 < (T w /T ) < 3 (heating) (2.2.8a)
(T w /T)0.81 for 0.5 < (T w /T) < 1 (cooling) (2.2.8b)
For liquids, the friction factor evaluated at the bulk mean temperature is
multiplied by one of the following factors to obtain the correct value.
(µw /µ)0.58 for µw /µ < 1 (heating) (2.2.8c)
(µw /µ)0.54 for µw /µ > 1 (cooling) (2.2.8d)
The subscript w refers to the mean value of the duct wall temperature and
the temperatures are in degrees Kelvin. These relationships are also applicable to
developing flow.
Example 2.2.1
Air at a pressure of p = 101,025 N/m2 and a temperature of T = 16.87 °C flows
uniformly into a rectangular duct with
a = 50 mm
b = 3.5 mm
at a rate of m = 6.403 x 10-4 kg/s
the duct length is L = 200 mm
Determine the pressure differential between the inlet and the outlet of the duct.
Solution
Using the perfect gas law given by Equation 1.4.13, the density of the air at
the specified conditions can be expressed as
where the gas constant for air is R = 287.08 J/kgK.
ρ = = = 1.2134 kg/m3 p
RT
101025
287.08x(273.15+16.87))
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Using Equation A.1.3, the dynamic viscosity of the air at 16.87 °C or (273.15+ 16.87) = 290.02 K is
The mean air speed in the duct follows from Equation 2.1.3, i.e.,
v = m/( ρab) = 6.403 x 10-4/(1.2134 x 0.05 x 0.0035) = 3.015 m/s
Using Equation 2.1.6, the hydraulic diameter of the duct is
The Reynolds number for the air flowing in the duct is, using Equation 2.1.5,
Re = ρv d e / µ = 1.2134 x 3.015 x 0.006542/(1.8007 x 10-5) = 1329.1
It follows from Equation 2.2.3 that for duct flow
For b/a = 0.0035/0.05 = 0.07, find n ≈ 2.3 from Table 2.2.2.
Substitute the values for fRe and n into Equation 2.2.7 to find
or
f app = 30.16/1329.1 = 0.02269
f app Re=[(21.938)2.3+{3.44/(0.2/0.006542x1329.1)0.5}2.3]1/2.3=30.16
fRe=24[1–1.3553(0.0035/0.05)+1.9467(0.0035/0.05) 2–1.7012(0.0035/0.05)3
+0.9564(0.0035/0.05)4–0.2537(0.0035/0.05)5]=21.938
d e= = = 0.006542 m4ab
2(a+b)
4x0.05x0.0035
2(0.05+0.0035)
µ=2.287973x10–6 +6.259793x10–8T –3.131956x10–11 T 2+8.15038x10–1 5T 3
=2.287973x10–6+6.259793x10–8 x 290.02–3.131956x10–1 1x290.022
+8.15038x10–15 x290.023=1.8007x10–5kg/sm
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Using Equation 2.2.2, the pressure drop between the inlet and the outlet of the duct is
Turbulent flow
With fully developed turbulent flow in ducts, the friction loss depends
on flow conditions as characterized by the Reynolds number and on the
nature of the duct wall surface. The quantity, ε, having the dimension of
length is introduced as a measure of the surface roughness. From dimensional
analysis, it follows that the friction factor is a function of the Reynolds
number and the relative roughness ε /d . The graphical representation of thisrelationship is known as the Moody diagram and is presented in Figure 2.2.3
according to Moody.
Fig. 2.2.3 Friction Factors for Pipe Flow
∆ p=4f app( ) =4x0.02269( )( ) =15.3 N /m2 L
d e
ρv 2
2
0.2
0.006542
1.2134x3.0152
2
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As shown, the laminar friction factor for pipe flow is a single straight line andis not influenced by the relative roughness. Reynolds numbers in the range from
2000 to 4000 lie in a critical region where flow can be either laminar or turbulent.
For Reynolds numbers larger than those in the critical region, turbulent
flow exists. The two regions into which the turbulent zone is divided, transition
and complete turbulence, categorize the state of the viscous sublayer as
influenced by roughness.
Based on Nikuradse’s data, the following implicit relationship is applicable
to turbulent flow in smooth pipes
(2.2.9)
or according to Filonenko,
(2.2.10)
Inspection indicates, for high Reynolds numbers and relative roughness,
the friction factor becomes independent of the Reynolds number in the
region of complete turbulence. Then
(2.2.11)
Transition between this region and the smooth wall friction factor is
represented by an empirical implicit transition function developed by Colebrook.
(2.2.12)
For purposes of computation, the following explicit relationship from
Benedict is of value:
(2.2.13)
Haaland recommends an equation that yields results comparable to the
implicit Colebrook equation:
0.9 Re5.74 +
3.7/d log0.25 = f 10
-2
Dε
f Re
2.51 +
3.7
/d log =
f
10.5
D
-2
100.5 D
ε
]/d)(n0.86-[1.14=f -2
D ε
)1.64- Relog = (1.82f -2
10 D
0.8-)f ( Ren= 0.86f /1 0.5 D
0.5 D
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For ε/d > 10-4
(2.2.14)
For situations where ε /d is very small, Haaland proposes
(2.2.15)
The curves in the turbulent and transitional zones in Figure 2.2.3 were
drawn employing Equation 2.2.11 and the Haaland relations, respectively.
An approximate indication of the relative roughness of typical pipe surfaces
encountered in practice is shown in Figure 2.2.4 according to Kirschmer.
Fig. 2.2.4 Surface Roughness in Pipes
3.75
/d +
Re
7.7 log2.7778=
f
3.333
10
-2
D
ε
1.11
3.7
/d +
Re
6.9log0.3086 =f 10
-2
D
ε
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Dimensional analysis does not relate the performance of ducts havingcircular and noncircular cross sections. The fully turbulent friction factor for
noncircular cross sections (annular spaces, rectangular and triangular ducts,
etc.) may be evaluated from the data for circular pipes. This applies if the pipe
diameter is replaced by an equivalent diameter, also referred to as the
hydraulic diameter , defined by Equation 2.1.6.
The equivalent or hydraulic diameter for an annulus of inner and outer
diameter d i and d o is
(2.2.16)
For a rectangular duct having sides a and b, it is
(2.2.17)
Launder and Ying show, for a rectangular duct, the secondary velocity
distribution gives rise to an increase in the friction factor of about 10%. Even so,
their full theory slightly underestimates the measurements of Hartnett et al.
According to White, the friction factor for turbulent flow between parallel
plates as given by the following equation is higher than the value that would
be obtained if the equivalent diameter were substituted into the equation for
pipe flow.
(2.2.18)
where Re is based on the hydraulic diameter which is equal to twice the
distance between the plates.
For developing turbulent flow near the entrance of a duct, the friction factor
is considerably higher than for fully developed flow according to Deissler.
When heat transfer occurs in turbulent duct flow, changes in thermo-
physical properties should be considered. This effect is taken into consideration
by multiplying the friction factor, evaluated at the bulk temperature of the
fluid, by one of the following appropriate correction factors from Petukhov:
( ) 1.19- Ref log2=f /1 0.5D10
0.5 D
b)+/(aab2=d e
d -d )d +d (
)d -d 4)(/4(d io
io
2i
2o
e ππ
= =
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(7 – µ/µw )/6 for (µw /µ) < 1 (heating) (2.2.19a)
(µw /µ)0.24 for (µw /µ) > 1 (cooling) (2.2.19b)
for 1.3 < Pr < 10 and where µw is evaluated at the duct wall temperature.
For air and hydrogen—temperature in degrees Kelvin
(2.2.20a)
(2.2.20b)
Example 2.2.2
Calculate the approximate mean Darcy friction factor when air
• at a pressure of pa = 1.013 x 105 N/m2
• a bulk temperature of T = 93.33 °C
• flows at a speed of 6.096 m/s through a smooth pipe having an inside
diameter of 25.4 mm
• T w = 426.67 °C is the inside pipe wall temperature• µaw = 3.355 x 10-5 kg/ms is the dynamic viscosity of air at 426.67 °C
Solution
Evaluate the Reynolds number of the airstream at bulk temperature.
Using Equation A.1.1, the density of the air at the bulk temperature of
(273.15 + 93.33) = 366.48 K is
m3kg/0.9628=93.33)+(273.15x287.08
x1.013 =
T 287.08
p =
105a
aρ
[ ](cooling) )/T T ( )/ Re0.79(+-0.6
w
-0.11w w ρρ
[ ](heating) )/T T ( )/ Re(5.6+-0.6
w
-0.38w w ρρ
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The dynamic viscosity of the air at this temperature follows from Equation A.1.3.
µa = 2.287973 x 10-6 + 6.259793 x 10-8 x 366.48 - 3.131956 x 10-11 x 366.482
+ 8.15038 x 10-15 x 366.483 = 2.14236 x 10-5 kg/ms
Thus,
The flow is turbulent, and the friction factor for the smooth tube may be
determined at the bulk temperature using Equation 2.2.10, i.e.,
This factor must be corrected by multiplying it by Equation 2.2.20a, which
includes the Reynolds number of the air evaluated at the wall temperature
T w = 426.67 °C
or
(273.15 + 426.67) = 699.82 K
The air density at this temperature is
With this density and the specified dynamic viscosity of the air evaluated at
the pipe wall temperature, find the Reynolds number
The corrected friction factor is thus
0.03019=)366.48/(699.820.03489=
)/T T (f =f
])0.9628/0.5042x(2326.965.6+[-0.6
])/ Re(5.6+[-0.6w D Dc
0.38-
-0.38aaw w ρρ
2326.96= x3.355
0.0254x6.096x0.5042 = Re 510
-w
kg/0.5042=699.82x287.08
x1.013 = m
3105
aw ρ
0.03489=)1.64-6958.61log(1.82=f -2
10 D
6958.61= x2.14236
0.0254x6.096x0.9628 =
vd = Re
10-5
a
aµ
ρ
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Transition laminar-turbulent flow In the critical zone where transition from laminar to turbulent flow takes
place, the friction factor is uncertain, and there is an uncertainty in pressure
drop estimates if the Reynolds number falls in this range, i.e., 2000 ≤ Re ≤ 4000.
A single correlating equation that covers the entire range from the laminar
through the critical region to turbulent flow in smooth pipes or tubes is
proposed by Churchill:
(2.2.21)
A more comprehensive equation including the effect of surface roughness
is also presented by Churchill.
(2.2.22)
where
and(37530) 16
a2 = [ Re ]
2.3 Losses in Duct Systems
As a result of the frictional resistance experienced during flow in ahorizontal duct, the mechanical energy (the p/ ρ + αev 2/2 terms in Equation
1.4.4) between any two sections of the duct is reduced, i.e., converted to
thermal energy. Similar reductions or losses in mechanical energy may
occur at inlets, outlets, abrupt changes in duct cross-sectional area, valves,
bends, and other appurtenances.
/d 0.27+0.9/ Re)(7
1n 2.457 = a
16
1 ε
1.5)a+a(
1 +
12
Re
88 = f D
21
0.0833
10
7
Ren2.21+
20
36500
Re +
10
Re
8
18f D =
0.5
-0.2
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A dimensionless loss coefficient, in general, can be defined between twocross sections in a horizontal duct as
(2.3.1)
where v is usually based on conditions at either section 1 or section 2.
Since most loss coefficients are determined experimentally, it is important tospecify the velocity on which a loss coefficient for a particular duct element
is based, i.e., inlet, outlet, or some mean condition.
If the flow is incompressible and the velocity distribution at sections 1
and 2 is uniform, as is approximately the case in turbulent flow, the kinetic
energy coefficient is αe ≈ 1, and Equation 2.3.1 can be written as
(2.3.2)
or
where
pt 1 = total pressure at section 1
pt 2 = total pressure at section 2
K is also referred to as the total pressure loss coefficient
A static loss coefficient is sometimes defined as
(2.3.3)
This loss coefficient is equivalent to K if there is no change in velocity
between sections 1 and 2.
( ) ( )2/v / p- p= K 2
21s ρ
( ) ( )2/v /t 2 p-t 1 p= K 2ρ
( ) ( )2/v
2/v + p-2/v + p
= K 2
222
211
ρρρ
( ) ( )2/v
2/v +/ p-2/v +/ p = K
2
222e22
211e11 αραρ
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For frictional, fully developed, incompressible flow in a pipe of constantdiameter, the pressure drop is given by the empirical Darcy-Weisbach
Equation 2.2.2. A loss coefficient, using Equation 2.3.2, may be expressed as
K f = ∆ p/(ρv 2/2) = f D L/d (2.3.4)
The region of influence for a component can be determined experimentally.
Attach straight pipes to the exit and entry of the component to attain fullydeveloped conditions upstream and downstream.
Consider the pressure distribution along a pipeline containing a bend for
incompressible turbulent flow shown in Figure 2.3.1. The variations in static
pressure, present across a section within the bend, extend for a diameter or
two into the straight pipes upstream or downstream. The constant pressure
gradient associated with fully developed flow in a straight pipe is not re-
established until fifty or more diameters downstream from the bend.
Fig. 2.3.1 Pressure Distribution in Horizontal Pipeline Containing a Bend
For most other pipework components, the variations in static pressure at
a cross section are far less marked than for bends, and the fully developed
velocity profile is recovered more quickly. For example, the flow recovers after
about five diameters downstream of a sudden enlargement according to Hall.
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When the flow upstream and downstream of a component is fullydeveloped, the component is said to be free of interference effects, since
its performance is independent of the flow beyond the regions of fully
developed flow. In the calculation of system pressure losses, it may be
necessary to approximate the real situation by using data obtained from
tests in interference-free flow. This approach should not lead to large
errors, provided that a spacer length of at least 5 diameters or, in the case
of bends, 10 diameters separates one component from another.
In many practical systems, interference exists between the componentsof the pipe system. This occurs when the regions of influence of two
components overlap. According to ESDI, the pressure loss through combinations
may be higher or lower than the sum of the losses of the components in
interference-free flow.
There are so many possible combinations of components that, at
present, the prediction of the performance of a system with interferences
cannot be made with any accuracy except in special circumstances. If the
interference in the system is confined to the interactions between a few
of the components for which data are available, the principles outlined
for interference-free flow can be applied by considering these components
as single entities. In some circumstances, it may be possible to deduce,
by broad physical arguments, that the interference effects will not be
important. Consequently, the performance of the system can be estimated
quite accurately using data obtained under interference-free conditions.
Alternatively, there may be one or two particularly large sources of pressure
loss in the system, and a much lower order of accuracy is acceptable for the
other components—if their magnitudes are known with reasonable accuracy.
However, these situations must be regarded as special cases. With the
present state of knowledge, it is necessary to resort to model tests or
computer analysis if an accurate assessment is required of the performance
of a duct flow system in which interferences occur.
Extensive data for loss coefficients of different components in pipe
and duct systems is presented in the literature in works by Miller, Holms,
Crane, Idelchik, and Fried.
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Abrupt contractions and expansionsHead or mechanical energy losses occur at abrupt changes in duct flow
cross-sectional areas. Consider incompressible flow in the duct shown in
Figure 2.3.2, which includes a contraction at the inlet and a sudden enlargement
at the outlet.
Fig. 2.3.2 Static Pressure Distribution in a Duct
From Equation 2.3.2 for uniform velocity distributions, the total inlet
pressure drop due to a reduction in the flow area resulting in an acceleration
of the flow and a loss due to separation of the boundary layer can be
expressed as
=- 2/v K 22c ρ( )2/v + p 2
22 ρ( )2/v + p 211 ρ
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80
The static pressure drop is
(2.3.5)
where
σ21 = A2/ A1
K c = the contraction coefficient containing the irreversible loss
At the outlet of the duct, there will be a rise in static pressure owing to
the increase in flow area, whereas a loss will occur due to boundary layer
separation and momentum changes following the abrupt expansion.
The resultant change in pressure is
(2.3.6)
where
K e = expansion coefficient
σ34 = A3/ A4
The loss coefficients K c and K e refer to the kinetic energy of the flow in the
smaller cross-sectional area. For highly turbulent flow, Kays expressed thesecoefficients using the following two equations:
(2.3.7)
and
Ke
= (1 – σ34
)2 (2.3.8)
( )σσσ c 22
c c c /1-1=/1+/2-1= K
[ ])-(1- K 2)/v ( p- 2
34e2343 σρ=
[ ] K +)-(12) / v (= p- c 221
2221
σρ
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Equations 2.3.7 and 2.3.8 apply to square-edged abrupt changes in crosssection for single tubes or for tube bundles.
The contraction ratio σc = Ac / A2 , shown in Figure 2.3.3 for two-dimen-
sional and three-dimensional circular contractions, is usually determined
experimentally according to Weisbach. The minimum area of the jet between
sections 1 and 2, Ac , is referred to as the vena contracta.
Fig. 2.3.3 Contraction Ratio for Round Tubes and Parallel Plates
The curves shown in Figure 2.3.3 are approximated by the following
empirical relations for round tubes
(2.3.9)
and for parallel plates according to Rouse.
(2.3.10)
σσσ6
21
5
21
4
21 3.558944+5.963169-2.672041+
σσσσ 321
22121c 0.4082743+0.336651-0.04566493+0.6144517=
σσσσ 32122121c 0.51146+0.26095-0.13318+0.61375=
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It is possible to reduce the contraction loss coefficient for a tube significantlyby rounding off the inlet edge. This is illustrated in Fig. 2.3.4 and Table 2.3.1,
according to Fried.
Fig. 2.3.4, Table 2.3.1 Contraction Loss Coefficient for Rounded Inlet
For tubes penetrating into a manifold, Fried shows a higher loss coefficient
is applicable (Fig. 2.3.5 and Table 2.3.2).
Fig. 2.3.5, Table 2.3.2 Contraction Loss Coefficient for Penetrating Tube
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Example 2.3.1
A heat exchanger bundle consists of tubes having an inside diameter of 22.09 mm
and a total length of 15,024 mm. The tubes are arranged in a staggered pattern
and are welded into tube sheets (Fig. 2.3.6).
Water at 52.5 °C flows through each tube at a rate of 0.4015 kg/s. The tube
inlet has a square edge. Determine the difference in static pressure between theheaders for a smooth tube and for the case where ε/d i = 10-3.
Fig. 2.3.6 Tube Dimensions and Layout
Solution
The thermophysical properties of water are listed in appendix A. Evaluate
properties at 52.5 °C (325.65 K).
Density of water from Equation A.4.1:
ρw = (1.49343 x 10–3 – 3.7164 x 10–6 x 325.65 + 7.09782 x 10–9 x 325.652
– 1.90321 x 10–20 x 325.656)–1 = 986.9767 kg/m3
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Dynamic viscosity of water from Equation A.4.3:
µw = 2.414 x 10–5 x 10247.8/(325.65 – 140) = 5.21804 x 10–4 kg/ms
The Reynolds number for the water flowing in the tube is
The flow in the tube is turbulent, e.g., transition zone. The mean velocity of
the water in the tube is determined from
The frictional pressure drop may be determined using Equation 2.2.2.
For a smooth tube, the friction factor follows from Equation 2.2.10:
f D = (1.82 log10 44349.9 – 1.64)–2 = 0.021516
The frictional pressure drop is thus
For the rough pipe, it follows from Equation 2.2.14 that
f D = 0.3086/[log10 {6.9/44349.9 + (10-3/3.7)1.11 }]2 = 0.0241234
The resultant frictional pressure drop is
m N/9122.122
061441.x986.9767
22.09
15024 0.0241234 p
2
2
f
∆ ==
m N/8136.152
061441.x986.9767
22.09
15024 0.021516 p
22
f
∆ ==
2v d
L f = p
2
w
i
Df
ρ
∆
m/s1.06144 = )(0.02209x986.9767
0.4015x4 =
d
m4 = v
22iw πp q
44,349.95.21804x 22.09x
10x0.4015x4
d
m4d v Re
7
w iw
iw
πµπµρ
= = = =
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For the particular tube layout, the area ratio for the entering water stream is
σ = π x 22.092/(4 x 58 x 50.22) = 0.13158
whereas the jet contraction ratio is, using Equation 2.3.9,
σc = 0.61375 + 0.13318 x 0.13158 – 0.26095 x 0.131582 + 0.51146 x
0.131583 = 0.628
For turbulent flow, the inlet contraction loss coefficient may be approximated
by Equation 2.3.7, i.e.,
K c = 1 – 2/0.628 + 1/0.6282 = 0.351
The static pressure drop at the inlet to the tube follows from Equation 2.3.5:
∆ pi = 0.5 x 986.9767 x 1.061442 [(1 – 0.131582) + 0.351] = 741.5 N/m2
The outlet expansion loss coefficient is approximated by Equation 2.3.8:
K e = (1 – 0.13158)2 = 0.7542
The static pressure drop at the outlet of the tube follows from Equation 2.3.6:
∆ pe = 0.5 x 986.9767 x 1.061442 [0.7542 – (1 – 0.131582)] = –127.0 N/m2
For a smooth tube, the total static pressure differential between the headers is
∆ p = 8136.15 + 741.5 – 127.0 = 8751 N/m2
For the rough tube, the pressure drop is
∆ p = 9122.12 + 741.5 – 127.0 = 9737 N/m2
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Reducers and diffusersWhen the duct flow area is reduced gradually (Figs. 2.3.7a and b), the
number of velocity heads lost is very small. Based on the smaller flow area, a
loss coefficient of K red = 0.04 or less is commonly quoted.
Fig. 2.3.7 Reducers (a) (b) (c)
For the conical reducer shown in Figure 2.3.7(c), the loss coefficient
based on the smaller area may be obtained from the following equation
according to Fried:
(2.3.11)
where
σ21 = A2/ A1
θ is in radians
The loss coefficient is based on the velocity at 2.
( )θθπθ 20-4-8x 23
( )0.00745-0.00444+0.00723-0.0224+0.0125-= K 21221
321
421red σσσσ
a b c
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Whenever it is necessary to increase the flow area of a pipe gradually, theconical diffuser shown in Figure 2.3.8 may be used.
Fig. 2.3.8 Conical Diffuser
Ideally, in the absence of losses, the total pressure remains constant, i.e.,
and the pressure recovery is
(2.3.12)
where
σ12 = A1 /A2
id = ideal conditions
In practical diffusers, only a part of this pressure recovery is possible, and
a diffuser efficiency is defined as
(2.3.13)( ) 2/-1v
p- p
p- p
p- p2
1221
12
1id 2
12dif
σρη = =
( ) ( ) 2/-1v =2/v -v = p-2
1221
22
211id 2 σρρ
2/v + p=2/v +211
22id 2 ρρ
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For relatively small expansion angles, the diffuser efficiencies have been
determined by Patterson, whose results are shown in Figure 2.3.9.
The loss coefficient of a diffuser with uniform inlet and outlet flow is
(2.3.14)
Fig. 2.3.9 Conical Diffuser Efficiencies
Substitute Equation 2.3.13 into Equation 2.3.14 and find
(2.3.15)
For practical applications, Daly suggests it may be convenient to employ
Figure 2.3.10.
( )( )ση 212dif dif -1-1= K
( ) ( )2/v
2/v + p-2/v + p =
2/v
p- p = K 2
1
222
211
21
2t 1t dif
ρ
ρρ
ρ
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Fig. 2.3.10 Losses in Duct Diffusers
The losses for open-outlet diffusers are shown in Figure 2.3.11. A uniform
approach velocity, such as a venturi nozzle flow meter, allows more rapid
expansion and lower loss, shown by the broken lines. Extensive data on flat
and conical diffusers is presented by Runstadler et al.
Fig. 2.3.11 Losses in Open Outlet Diffusers
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Three-leg junctionsPressure loss data for dividing flows through planar three-leg junctions
are cited in various references such as Engineering Sciences Data Unit (ESDU),
Verein Deutscher Ingenieure-Wärmeatlas, the General Electric Fluid Flow
Data Book, and Miller.
The total pressure differences across pairs of inlet and outlet legs of a
junction (Fig. 2.3.12) are calculated from
pt 3 – pt 1 = K 31ρv 32/2 + f D3 L3ρv 3
2/2d 3 + f D1 L1ρv 12/2d 1 (2.3.16)
and
pt 3 – pt 2 = K 32ρv 32/2 + f D3 L3ρv 3
2/2d 3 + f D2 L2ρv 22/2d 2 (2.3.17)
Fig. 2.3.12 Variation of Total Pressure in the Vicinity of a Junction
The last two terms on the right side of Equations 2.3.16 and 2.3.17 are
the straight-pipe friction losses over lengths L3, L1 , and L2.
The loss coefficient for a 90° junction, K j90 = K 31, with Re3 ≥ 2 x 105
between leg 3 and leg 1 is given in Figure 2.3.13 for square corners (r 31 = r 12 = 0)
as a function of A1/ A3 and V 1/V 3.
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Fig. 2.3.13 Loss Coefficient for a 90° Junction with Square Corners
With rounded corners, the loss coefficient may be reduced, i.e.,
(2.3.18)
for r 12/d 1 < 0.15 and r 31/d 1 < 0.15, and
(2.3.19)
for r 12/d 1 > 0.15 and r 31/d 1 > 0.15.
The information strictly applies to junctions where the inlet flow is fullydeveloped and where there is a long downstream duct length. However, in practice
it can be applied without significant error when there are 15 or more equivalent
diameters upstream and at least 4 diameters downstream of the junction. It is
possible to reduce the loss coefficient by installing suitable guide vanes.
A / A
V / V 0.45- K = K = K
31
31
2
90 jr 90 jr 31
d
r
A / A
V / V 0.26 –
d
r
A / A
V / V 0.9- K = K = K
1
12
0.5
31
31
2
1
31
0.5
31
31
2
90 jr 90 jr 31
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The loss coefficient between leg 3 and 2 can be assumed to be unaffect-ed by the geometry of leg 1 and is given in Figure 2.3.14 as a function of the
flow ratio only. There is no significant change in the loss coefficient, K 32, due
to rounding of the junction corners.
Fig. 2.3.14 Loss Coefficient K32 for a 90° Junction
In the case of a square-edged T-junction, ( K T = K 31, the loss coefficient is
shown in Figure 2.3.15.
Fig. 2.3.15 Loss Coefficient for a T-Junction with Square Corners
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Curved ducts or bendsA few common types of curved ducts or bends are shown in Figure 2.3.16.
Pressure loss data for flow through such bends are available from ESDU.
Fig. 2.3.16 Bends (a) Circular-Arc Bend (b) Single Miter Bend (c) Composite Miter Bend
The pressure loss due to a square bend and, in particular, a miter bend
may be reduced by fitting guide vanes. It is common practice to use a num-
ber of guide vanes in a cascade in a miter bend. The vane geometry is not
fixed by the bend geometry, and a number of designs exist. One example of
such a miter bend is shown in Figure 2.3.17.
Fig. 2.3.17 Miter Bend with Cascade and Circular-Arc Guide Vanes
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a b c
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Insufficient systematic data exist to provide detailed information onpressure losses in miter bends with cascades shown in Figure 2.3.18. The
probable range of the loss coefficient, K bm, is between 0.15 and 0.4, the lower
values requiring very careful construction for their achievement. These values
compare with a loss coefficient equal to approximately 1.1 for a similar bend
without a cascade.
Fig. 2.3.18 Miter Bends Kbm = 0.28, Kbm = 0.25, Kbm = 0.4 (Jorgensen)
2.4 Manifolds
The design of manifolds for the distribution or division of a fluid
stream into several branching streams is of importance in the design of
different types of heat exchangers. The same is true for the formation of
a single main stream by the collection or confluence of several smaller
streams. A manifold basically consists of a main channel, a header, towhich several smaller conduits, tubes, or laterals are attached at right
angles. Manifolds commonly used in flow distribution systems can be
classified in the following five categories (Fig. 2.4.1).
• simple distributing or dividing
• collecting or combining
• cocurrent flow or parallel flow
• countercurrent flow or reverse flow
• mixed flow or combined flow
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The cocurrent or countercurrent flow configurations are also referred toas Z or U type heat exchangers.
Fig. 2.4.1 Types of Manifolds
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Often, the objective of the design is to provide equal flow rates throughthe branches or laterals. This can be achieved if the cross-sectional area of the
header is designed such that the fluid velocity and the pressure in the header
remain constant.
The variations in fluid pressure in the header are due to frictional effects
and changes in momentum. The frictional loss is always in the direction of
the flow. The momentum changes cause an increase in pressure in the direction
of flow in the distributing header and a decrease in pressure in the direction
of flow for the collecting header.
By applying the energy equation to the flow in the header, Miller
and Hudson quantified the flow and pressure distribution in the header.
Enger and Levy, Keller, Acrivos et al., Markland and Bassiouny, and
Martin based their continuous mathematical model on local momentum
balance considerations in the header. Discrete mathematical models
based on local momentum balances are derived by Kubo and Euda,
Majumdar and Datta, and Majumdar. Bajura and Bajura and Jones
derived continuous mathematical models based on integral momentum
balances of the fluid in the header. They integrated the momentum
equation in vector form over a control volume to quantify the flow and
pressure distribution. A discrete mathematical model based on an integral
momentum balance is due to Nujens.
To find the approximate flow distribution and pressure change in a
manifold, consider a section of a header of uniform cross section, Ah, and
wetted perimeter, P eh, fitted with closely spaced laterals shown in Figure
2.4.2.
Fig. 2.4.2 Header Control Volume (a) Dividing Header (b) Combining Header
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By applying a mass balance to an incompressible fluid in an elementarycontrol volume, Ah∆x, in a header, find
ρ Ah(dv h/dx)∆x + ρv A
= 0 (2.4.1)
where the subscripts h and
refer to the header and the laterals, for a
header of length Lh and n
laterals, ∆x = Lh/n.
The approximate momentum balance applicable to the control volumemay be written as
(2.4.2)
where the factor c = 1 for v h > 0 and c = -1 for v h < 0. The momentumcorrection factors, αmh and αm
provide for nonuniformities in local header
and lateral inlet velocity distributions.
Using Equations 2.2.1 and 2.2.2, the header shear stress can be expressed
in terms of the Darcy friction factor, i.e.,
(2.4.3)
Substitute Equations 2.4.1 and 2.4.3 into Equation 2.4.2, and simplify to find
(2.4.4)
where the overall momentum correction factor αmh = 2αmh - αmand
d e = 4 Ah/ P eh. Bajura et al. graphically present some values for overall momentum
correction factors.
0=d 2v f c
+dxdv v +
dx
dp
e
2h Dh
hmhh ρα
8/v f =2h Dh ρτ
( )[ ] Av -v Av + Ax/dxdv +v = h2hmhhmhhh
2mh ραραα δρ
( )[ ] x P c - Axdx/dp+ p- A ehhhhhhh ∆∆ τ
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If a lateral is located between a dividing and a combining header, the staticpressure difference between these headers can be expressed as
(2.4.5)
In this equation, K i and K o are the lateral inlet and outlet loss coefficients
while αed
and αec
are the header energy correction factors. In a conventional
single phase heat exchanger, the lateral velocity v i = v
o; however, in a
condenser, the inlet velocity is greater than the outlet velocity.
Bassiouny and Martin, after making some simplifying assumptions,
present solutions for the manifold momentum equations for single phase
flow in U or Z type configurations.
The more complicated problem of flow distribution in an air-cooled
steam condenser was analyzed by Zipfel and Kröger. While the lateral inlet
loss in a single-phase heat exchanger is usually negligible, this is not the casein a condenser. They show, under certain circumstances, backflow of vapor
can occur in some of the laterals.
2.5 Drag
Drag is defined as the force component, parallel to the relative approach
velocity exerted on the body by the moving fluid. Mathematically it can be
expressed as
F D = C D A ρ v 2/2 (2.5.1)
where
A = the characteristic projected area normal to the flow
ρv 2/2 = the dynamic pressure of the main stream
C D = the drag coefficient
[ ] ( ) /v v /v + K +2 2/v K +v /v - K = p-2o
2o
2hc ec o
2ii
2hd ed ihc hd ραρα
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The drag coefficient is found by dimensional analysis to be a function of thegeometrical configuration of the immersed body, the Reynolds number, the
turbulence characteristics of the incoming free stream, and the surface roughness
of the body. Experimental data on drag coefficients versus Reynolds numbers for
several different two-dimensional bodies are plotted in Figure 2.5.1.
Fig. 2.5.1 Coefficient of Drag for Two-Dimensional Bodies
A summary of results on forces associated with flow across circular
cylinders is reported by the Engineering Sciences Data Unit (ESDU). As
shown in Figure 2.5.1, the drag coefficient remains almost constant at a
value of 1.2 for 104 < Re < 2 x 105 in the case of infinitely long cylinders.
The drag coefficient is not significantly affected by surface roughness or
free-stream turbulence for Re < 3 x 104. Above this value, these effects do
become important according to ESDU.
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If the cylinder axis is rotated through an angle θ D with respect to thenormal approach flow direction, the drag coefficient may be calculated
approximately from
C Dθ = C D (cos θ D)3 (2.5.2)
for 0° < θ D < 45°.
Empirical equations based on experimental data have been developed byHoerner for predicting the drag coefficient about elliptical sections for different
Reynolds numbers, i.e.,
C D = 2.656 (1 + a/d ) Re–0.5 + 1.1 (d /a) (2.5.3)
for 103 < Re < 106 and where a and d are the dimensions of the major and
the minor axes. This relationship is plotted in Figure 2.5.1.
If the elliptical section is inclined relative to the flow, the drag coefficient
is corrected in the same way as the circular cylinder, i.e. Equation 2.5.2.
The drag coefficient for an infinitely long square section is C D = 2 for
Re > 104 (Fig. 2.5.1). An extensive study on square and rectangular sections
is presented by the ESDU.
The drag coefficients for other two-dimensional structural shapes are listed
in Table 2.5.1 according to Simiu.
Table 2.5.1 Two-Dimensional Drag Coefficients for Structural Shapes
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The drag coefficient for all objects with sharp corners is independent of the Reynolds number because the separation points are fixed by the geometry
of the object.
A more detailed list of drag coefficients is presented by Sachs. Data for
estimating the mean fluid forces acting on lattice frameworks are presented
in ESDU Item Number 75011.
According to Turton and Levenspiel, the drag coefficient for a sphere is
given by
C D = 24(1 + 0.173 Re0.657)/ Re + 0.413/(1 + 16300 Re-1.09) (2.5.4)
for Re ≤ 200000.
2.6 Flow through Screens or GauzesA screen may be defined as a regular assemblage of elements forming a
pervious sheet, which is relatively thin, in the direction of flow through the
screen. Screens of various types may be installed in systems to:
• remove foreign objects from the fluid stream
• protect equipment (e.g., against hailstones)• reduce fouling or clogging in heat exchangers
• smooth flow
• produce turbulence
In such cases, the prediction of the total pressure loss caused by the
screen is of interest.
An expression for the loss coefficient across a plane screen has been
deduced by Cornell for a compressible fluid. Since the losses across screens
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employed in air-cooled heat exchangers are normally small, the loss coefficientcan be expressed approximately in terms of the pressure difference across the
screen and mean, free, stream velocity, i.e.,
K s = 2( pt 1 – pt 2)/ρv 2 = 2( p1 - p2)/ρv 2 (2.6.1)
A round-wire screen or gauze of square mesh shown in Figure 2.6.1 is
usually specified by the mesh, defined by the number of openings per unit
length, 1 /P s, and by the diameter, d s, of the wires.
Fig. 2.6.1 Geometry of a Square-Woven Screen
An example of standard mesh data is listed in Table 2.6.1.
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Table 2.6.1 Standard Mesh Data
The porosity of the screen is defined as
βs = area of holes/total area = (1 – d s / P s)2 (2.6.2)
According to Simmons, the following equation holds for a screen placed atright angles to an airstream at velocities above 10 m/s under ambient conditions:
K s = (1 – βs)/βs2 (2.6.3)
This equation can be recommended for application in the case of most
screens of practical interest where screen Reynolds numbers exceed 300.
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The screen Reynolds number is defined as
Res = ρvd s /(βs µ) (2.6.4)
According to Wieghardt, the loss coefficient may be expressed as
K s = 6(1 – βs)βs –2 Res
–0.333 (2.6.5)
for 60 < Res < 1000.
In Figure 2.6.2, Equations 2.6.3 and 2.6.5 are compared with the
experimental results obtained by various investigators. Since the screen
geometry can have a significant influence on the loss coefficient, specific
tests should be performed when these losses are of importance.
Fig. 2.6.2 Screen Loss Coefficient
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For cases where ds/Ps << 1, the effective drag force per screen area may beexpressed as follows. This corresponds to one screen opening and uses
Equation 2.5.1
F D/ A = F D/[d s (2 P s – d s)] ≈ C D ρ v 2/2 (2.6.6)
Using Equation 2.6.1, the loss coefficient is
K s = 2F D/ ( P s2 ρ v 2) (2.6.7)
Substitute Equation 2.6.6 into Equation 2.6.7, and find
K s = C D (2 d s / P s – d s2/ P s2) = C D (1 – βs) (2.6.8)
Equation 2.6.8 can also be written as
K s βs2/ (1 – βs) = C D βs
2 ≈ C D (2.6.9)
for d s / P s << 1.
With the drag coefficient, C D, known for an infinitely long cylinder, the
approximate relationship (Eq. 2.6.9) can be applied over a wide range of
Reynolds numbers (Fig. 2.6.2).
Fan guards consisting of expanded metal or wire woven mesh are
required in most air-cooled heat exchangers. According to the American
Petroleum Institute, the recommended openings in the petrochemical industry
for woven mesh are usually not more than 2600 mm2 with a wire diameterof not less than 2.8 mm or 12 Birmingham wire gage (BWG).
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2.7 Two-Phase Flow
Two-phase flows are found in many industrial processes. Gas-liquid flow,
which occurs in condensation and boiling operations, is of particular interest
in the design of heat exchangers. Generally, these flows are more complicated
physically than single-phase flow. In addition to the usual inertia, viscous,
and pressure forces present in single-phase flow, two-phase flows are also
affected by interfacial tension forces, the wetting characteristics of the liquid
on the tube wall, and the exchange of momentum between the liquid andthe vapor phases in flow.
Two-phase flow patterns
In gas-liquid or vapor-liquid flow, the two phases can adopt various
geometric configurations known as flow patterns or flow regimes. Many flow
patterns are present during flow in tubes, including those observed by bothCollier and Hewitt, and a few of the more important ones will be described.
The total mass flow rate through a tube is equal to the sum of the mass
flow rates of gas, m g , and liquid, m.
m = m g + m
(2.7.1)
The ratio of the mass flow rate of gas to the total mass flow rate is known
as the dryness factor or quality, i.e.,
(2.7.2)
where G is the mass flux based on the total cross-sectional area of the
tube—also referred to as the superficial mass velocity. The subscript g refers to
the gas.
The void fraction, α is defined as the ratio of the gas flow cross-section-al area, A g , to the total cross-sectional area, Ats.
(2.7.3) A/ A= ts g α
/GG=/mm=x g g
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When both phases are flowing upwards in a tube, cocurrent flow,possible flow patterns obtained are shown in Figure 2.7.1 for increasing
gas flow or quality.
Fig. 2.7.1 Flow Patterns in Vertical Upflow in Tube
• Bubble flow. At low gas or vapor flow rate and low to moderate liquid
flow rates, the gas phase tends to become distributed throughout theliquid continuum as bubbles.
• Slug flow (also called plug flow). If the gas flow rate of a dispersed
bubble flow is increased, the bubbles coalesce to form large bullet
shaped bubbles, which approach the tube diameter in size. The
bubbles are separated by slugs of liquid containing small entrained
gas bubbles.
• Churn flow. With a further increase in gas flow rate, the liquid slugs
break down and give rise to this unstable flow of an oscillatory
nature according to Jayanti, Mao, and Hewitt.• Annular flow. At high gas velocities and low liquid flow rates, the
liquid travels partly as wavy annular film on the wall of the tube and
partly as small drops distributed in the gas, which flows in the
center of the tube.
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• Mist flow. At a gas velocity much higher than that of annular flow,there is an increase in the number of liquid droplets being sheared
away from the film flow until nearly all liquid is entrained in the gas
core flow.
More details of vertical cocurrent upward flow are given in the literature
from sources such as Oschinowo, Taitel, Hewitt, McQuillan, and Cindric.
Vertical cocurrent downward flow patterns have been described by
Oschinowo and Charles, Barnea et al., Crawford et al., and Mukherjee andBrill. A few of these patterns are shown in Figure 2.7.2 for increasing gas flow rate.
Fig. 2.7.2 Flow Patterns in Vertical Downflow in Tube
• Bubble flow. At very low gas flow rates and high liquid flow rates, the
gas phase flows as discrete bubbles in a downward flowing continu-
um. Shear stresses decrease from the tube wall to a minimum at thetube center, therefore the resultant imbalance in shear force acting
on each bubble causes it to migrate towards the center of the tube.
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• Slug flow. At higher gas flow rates, the dispersed bubbles coalesce toform larger bubbles separated by liquid slugs.
• Falling film flow . At low liquid and gas flow rates, the liquid flows in
the form of a thin film. The gas core flow entrains very few or no liq-
uid droplets. There is a tendency for dry spots to develop on the tube
wall. This flow pattern is sometimes classified as an annular flow
although its nature is different.
• Churn flow. If the gas flow rate in a slug flow pattern is increased, a
point is reached where the high gas concentration in the liquid slug
causes the slug to collapse. As this happens, the liquid slug falls then
regroups with other liquid drops until it is able to bridge the tube
again. The mixture is turbulent but much less agitated than for ver-
tical upward churn flow.
• Annular flow. At high gas flow rates and moderate liquid flow rates,
the liquid flows as an annular film while the gas forms a continuous
core flow at the center of the tube. The high velocity gas core flow
may entrain a portion of the wavy liquid film.
• Mist flow. At very high gas flow rates, all or most of the liquid film isentrained into the gas core flow in the form of small droplets.
The results of many studies of countercurrent two-phase flows in vertical
tubes have been reported by sources such as Wallis and Taitel. Flow patterns
include bubble, slug, and annular flow or falling film.
Horizontal two-phase flows in tubes generate patterns which are more
complex than vertical flow patterns because the gravitational influence is no
longer in the axial direction of flow. The horizontal flow pattern descriptionshown in Figure 2.7.3 are combinations of the categorization of a number of
researchers such as Taitel, Hewitt, Mukherjee, and Cindric.
• Stratified flow. This flow pattern occurs at low gas and liquid volume
flow rates. The liquid phase flows along the bottom of the tube, and
its surface is relatively smooth—also referred to as stratified smooth
flow. Increasing gas flow causes the liquid surface to become wavy—
also referred to as stratified wavy flow.
• Bubble flow. Bubble flow occurs at low gas flow rates and moderate
liquid flow rates. Bubbles tend to concentrate near the top of the
tube due to buoyancy forces.
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• Slug flow. At higher gas flow rates than for dispersed bubble flow, coa-lescence of bubbles occurs forming large bubbles separated by slugs
of liquid.
• Annular flow. At high gas flow rates, shear forces at the vapor-liquid
interface may be large compared to gravitational forces. The interaction
between these forces and the waves on the liquid surface causes the
liquid to flow up the tube wall until the liquid film flows as an
eccentric annulus according to James and Lin. The effect of gravity
causes the liquid film to be thicker at the bottom than at the top of
the tube.
• Mist flow. At very high gas flow rates, all the liquid film tends to be
entrained into the gas core as small droplets or mist.
Fig. 2.7.3 Flow Patterns in Horizontal Flow in Tube
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Flow patterns for inclined tubes are a superposition of the flow patternsfor horizontal and vertical flows. However, a quantitative prediction of flow
pattern transition for inclined tubes is more difficult according to Hewitt.
More detailed studies of two-phase flows in inclined tubes have appeared
in the literature from authors such as Spedding, Crawford, Mukherjee,
Stanislav, and Barnea.
Numerous attempts have been made to present different flow patterns
on a two-dimensional graph having different areas that correspond to the
different flow patterns. Such flow pattern maps may use the same axesfor all flow patterns and transitions, or they may employ different axes
for different transitions.
Baker was the first to develop a horizontal tube-side flow pattern map
that could be used for any fluid. His map was subsequently modified by Scott
(Fig. 2.7.4) and further evaluated by Bell et al. The map is plotted in terms of
G g /λ and Gψ where G g = m g / Ats and G
= m
/Ats are the superficial mass
velocities of the gas and liquid, and the factors λ and ψ are given by
(2.7.4)
(2.7.5)
where
σ = surface tension
a = physical properties of air
w = physical properties of water
= properties of the liquid flowing in the tube
g = properties of the gas flowing in the tube
ρw
= 1000 kg/m3
ρa = 1.23 kg/m3
( ) ( )( )[ ]///= w
2
w
0.333
w ρρµµσσψ
( )( )[ ]//= w a g
0.5ρρρρλ
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Fig. 2.7.4 Modified Baker Flow Pattern Map for Horizontal Flow in a Tube
The dynamic viscosity of water is taken as µw = 10-3 kg/ms, and the
surface tension is σw = 0.072 N/m. The Baker map works reasonably well for
water/air and oil/gas mixtures in small diameter (< 0.05 m) tubes.
One of the disadvantages of the Baker map is the parameters are
dimensional and empirical, so it is not possible to relate the map boundaries
theoretically to any known physical characteristics of the flow. Taitel and
Dukler approach the flow regime transitions theoretically and present a more
complex type of flow pattern map. Other graphical presentations have
been proposed by Breber, with some based on studies conducted during
condensation of vapors in horizontal tubes.
The Hewitt and Roberts map shown in Figure 2.7.5 is a widely used chart
for vertical upflow in a tube, while a map proposed by Oschinowo andCharles is applicable to downflow in a vertical tube. The Hewitt and Roberts
map works reasonably well for water/air and water/steam systems, again in
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small diameter tubes. Note that wispy annular flow is a subcategory of annularflow, which occurs at high mass flux when the entrained drops are said to
appear as wisps or elongated droplets.
Fig. 2.7.5 Hewitt and Roberts Map for Vertical Upflow in a Tube
Maps for patterns in inclined tubes have been presented by various
authors such as Spedding, Crawford, Mukherjee, Stanislav, and Barnea.
A systematic and practical approach for determining changes in pressure
in two-phase flows is presented by Carey.
FloodingThe flooding process is illustrated in Figure 2.7.6, and a description
found in Hewitt and Bankoff is summarized in the following.
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Fig. 2.7.6 Flow Regime Transitions during the Flooding Process inside a Vertical Tube (a-h)
Liquid enters the top of the tube through a porous section and isremoved through a porous section at the bottom of the tube. At low gas flow
rates, a stable counterflow exists (Fig. 2.7.6a). As the gas flow rate is increased,
the interface becomes wavy, liquid is entrained, and the film starts creeping
up past the liquid inlet (Fig. 2.7.6b). This flow transition is defined as flooding
and is also sometimes referred to as the onset of flooding or limiting condition
for countercurrent flow . Eventually, liquid flows up past the liquid inlet
(Fig. 2.7.6c), and a state of partial liquid delivery exists. With a further
increase in gas flow, the liquid flow below the inlet porous section changes
to a climbing film flow (Fig. 2.7.6d), and a state of cocurrent annular or churnupward flow above the liquid inlet porous section is reached (Fig. 2.7.6e).
When the gas flow rate is reduced, the liquid begins to creep below the
liquid feed (Fig. 2.7.6f). This point is known as flow reversal. A further
decrease in gas flow rate results in a state of simultaneous climbing and
falling film flow (Fig. 2.7.6g). Finally, the initial state of countercurrent flow
is obtained (Fig. 2.7.6h). The last transition has been termed the deflooding
point by Clift et al.
There are various mechanisms by which flooding is said to occur. They
fall into two fundamental categories, namely: film flow theory assuming a
smooth gas-liquid interface and flow instability/wave growth theory.
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McQuillan and Whalley studied air-water flow experiments in vertical tubeswith porous wall liquid injection and removal. They concluded the following
concerning flooding:
• The gas-liquid interface is wavy when the flooding point is
approached.
• These waves grow in amplitude as they travel downwards.
• The velocity of the falling waves decreases as they fall. At the floodinggas flow rate, the wave reaching the lower porous wall becomes
stationary and grows rapidly in size. The result is a large disturbance
wave, which moves upwards and causes flooding.
• Prior to the formation of the large disturbance wave, there is very
little entrainment of liquid droplets into the gas stream.
• For an airflow rate just below the flooding rate, an artificially injected
wave grows to form a disturbance wave, which is indistinguishable
from the flooding disturbance.
It is known that the geometry of liquid and gas entry can affect the gas
velocity at which flooding occurs. According to Hewitt, a square edged gas
inlet introduces more turbulence than a rounded inlet, promotes wave
growth on the liquid film, and reduces the gas velocity where flooding
occurs. If the turbulence level is low, the tube length has an effect on the gas
velocity necessary to initiate flooding. In longer tubes, Whalley found the
liquid waves have more time to build up, so the flooding occurs at lower values
of the gas velocity.
Reviews of the flooding literature are presented by numerous researchers
such as Tien, McQuillan, Bankoff, and Stephan. There tends to be a consid-
erable amount of scatter in the available data. In part this can be ascribed to
the fact that different definitions for flooding exist.
Many correlations have been proposed for predicting the onset of flooding .
The method based on the semiempirical correlation of Wallis is widely used
to predict flooding, i.e.,
(2.7.6)a= Fr a+ Fr 20.25 D1
0.25 Dg
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where the superficial densimetric Froude numbers for the gas and theliquid are defined as
(2.7.7)
(2.7.8)
The superficial velocities are defined as follows:
(2.7.9)
(2.7.10)
where
Ats = total cross-sectional area of the tube
The constants a1 and a2 depend upon the liquid inlet and outlet flow
condition and geometric characteristics. For turbulent air-water flow, the constant
a1 is close to unity while the approximate value chosen for the other constant
generally is as follows:
• a2 ≈ 1.00 for very smooth liquid inlet and outlet, e.g., porous, withminimal flow disturbance
• a2 ≈ 0.88 for very smooth liquid inlet and outlet, e.g., porous, with
high flow disturbance
• a2 ≈ 0.88 for rounded or tapered inlet and outlet flanges
• a2 ≈ 0.725 for sharp or square-edged inlet and outlet flanges
A significant increase in pressure drop is measured when flooding occurs.
Zapke and Kröger conducted adiabatic counterflow experiments to investigatethe effect of the duct geometry, duct inclination, and the liquid and gas physical
properties on flooding. Typical flooding data generated during the course of
the experiment for air-water flow in a flattened tube having a square-edged
(90°) inlet is shown in Figure 2.7.7 as a function of the duct inclination.
( ) A/m=/G=v tss ρρ
( ) A/m=/G=v ts g g g g gs ρρ
2 Fr D = ρ v s / [(ρ - ρ g )gd ]
2 Fr Dg = ρ g v gs / [(ρ - ρ g )gd ]
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Fig. 2.7.7 Flooding Data for Air-Water Flow in an Inclined Duct
As a result of the different flow patterns encountered during counterflow
in inclined ducts as opposed to vertical ducts, a significant decrease in the
flooding gas velocity was observed as the duct inclination changed from just
off the vertical to the vertical. Separate correlations were developed by Zapke
for flooding in inclined and vertical ducts.
For inclined round and flattened tubes with a square-edged gas inlet,
where a3 and a4 are functions of the duct inclination ϕ, i.e.,
(2.7.11)
where ϕ is in degrees and
ϕϕϕ 3-42-24 10x5.3227-10x6.7058+1.9471-18.149=a
ϕϕϕ 3-62-4-3-23 10x1.9852-10x1.5183+10x4.9705+10x7.9143=a
( )Oh Fr a-exp a= Fr 0.20.6
D43 Dg
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The Ohnesorge number is a dimensionless parameter that accounts forthe effect of the liquid properties on flooding and in this case is defined as:
where
d e = the hydraulic diameter of the duct
In the case of flattened or elliptical tubes, Fr Dg is based on the inside
height, while Fr Dis based on the hydraulic or equivalent diameter.
Equation 2.7.11 is based on tests conducted within these ranges:
10 mm ≤ W (inside duct width) ≤ 20 mm (flattened tubes)
50 mm ≤ H (inside duct height) ≤ 150 mm (flattened tubes)
d = 30 mm (tubes)
2° ≤ ϕ ≤ 80° (duct inclination to the horizontal)
For vertical round and flattened tubes with a square-edged gas inlet,
(2.7.12)
within the ranges:
10 mm ≤ W (inside duct width) ≤ 20 mm (flattened tubes)
50 mm ≤ H (inside duct height) ≤ 100 mm (flattened tubes)
d i = 30 mm (tubes)
ϕ = 90°
( )Oh Fr 0.0055= Fr
0.30.2
D
-1
Dg
0.04Oh Fr 0.20.6
D ≤
( )σρ l d /=Oh e0.5
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Limited extrapolation outside the geometric ranges specified is possible.
Pressure drop in two-phase flow
During two-phase flow in inclined ducts, the total pressure gradient,
dptp/dz, can be considered to be composed of three components arising from:
• friction losses, dpf /dz
• acceleration of the fluid, dpm /dz
• change of pressure or static head due to gravitational forces, dps /dz
A momentum balance on an element of the duct leads to the followingexpression for the various terms:
(2.7.13)
The normal procedure for using Equation 2.7.13 is to make some arbitrary
assumption about the nature of the flow. One such assumption would be to
treat the flow as a homogeneous mixture of the phases with constant phasecontent and constant and equal velocities for the two phases across the
whole duct. This is called the homogeneous model for two-phase flow. Usually
this model is not very satisfactory.
An alternative to the homogeneous model is to consider the flow to be
completely separated into two zones within the duct, one occupied by the
first phase and the other by the second phase.
In the separated flow models, a knowledge of phase content is essential
to calculate the accelerational and gravitational terms. The most common
way of correlating the frictional term is to express it in terms of a friction
dz
dp +
dz
dp +
dz
dp =
dz
dpsmf tp
0.02Oh Fr 0.110.30.2
D ≥≥
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multiplier . This is defined as the ratio of the frictional pressure gradient tothat for one or the other phase flow alone or for a flow at the same total mass
flux having gas or liquid properties.
(2.7.14)
(2.7.15)
where
ϕ, ϕ g , ϕ
o, and ϕ go = two-phase frictional multipliers
The literature contains a large number of two-phase flow correlations for
predicting the frictional pressure drop during cocurrent flow such as those
from Lockhart, Baroczy, Chisholm, and Friedel. Whalley tentatively recommends
the use of the following correlations:
• For µ/µ g < 1000, the Friedel correlation should be used.
• For µ/u g > 1000 and G > 100 kg/m2s, the Chisholm correlation
should be employed.
• For µ/µ g > 1000 and G < 100 kg/m2s, the Martinelli correlationshould be used.
The pressure gradient due to acceleration or deceleration effects may be
expressed as
(2.7.16)
ραρα g
222m x
+
-(1
)
)
x-(1
dz
d G=
dz
dp
/dzdp=/dzdp=/dzdp go
2
goo
2
of ϕϕ
/dzdp=/dzdp=/dzdp g 2
g 2
f ϕϕ
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where the term in brackets is the local effective specific volume and x isthe vapor mass fraction. The void fraction, α, can be determined using
Premoli’s correlation.
The static or geodetic pressure gradient is given by
(2.7.17)
where ϕ is the angle of the tube with respect to the horizontal plane with
downward flow.
The homogeneous and separated flow models tend to give an inadequate
representation of many real two-phase flows, and the detailed physics of the
flow, including the flow pattern, are important. By employing flow pattern
related frictional pressure drop correlations, it is possible to predict, stepwise,the pressure gradient along the tube according to Olujic. A systematic and
practical approach for determining changes in pressure in two-phase flows is
presented by Carey.
Correlations on counterflow pressure drops are presented by a few
researchers such as Feind, Dukler, Bharathan, and Stephan.
The pressure drop for nonadiabatic flow is discussed in more detail in
chapter 3.
( )[ ] ϕραρα sin g -1+=dz
dp g
s
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References
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