of 142
Chapter 2
PIPE FLOW
2.1 Generalities
On both historical and pedagogical grounds, fully developed flow in
a smooth pipe of circular cross section is an ideal point of entry for
technical fluid mechanics. The reason is that a crucial quantity, the
friction at the wall, is proportional to the axial pressure gradient,
which is usually easily measured. More than a century ago, exper-
iments by Hagen, Poiseuille, Couette and others used this property
to confirm the hypothesis of Newton that the viscosity of ordinary
fluids, particularly water and air, is a real physical quantity that
depends on the state of the fluid but not on the particular motion.
These early experimenters encountered turbulence in larger facilities
at higher speeds, and the issue quickly became the need for a better
qualitative and quantitative appreciation of turbulence. In fact, it
was an investigation of transition in pipe flow by Reynolds that led
to the discovery of the fundamental dimensionless number that bears
his name.
Study of turbulent flow in smooth round pipes led about 1930
to development of the mixing-length model, which in some situa-
tions still represents the best available approach to the problem of
turbulent flow near a wall. An important mechanism, just beginning
to be understood, involves the effect of the no-slip condition at the
61
62
CHAPTER 2.
PIPE FLOW
wall on turbulent fluctuations. Pipe flow is the vehicle of choice for
exploring the effect of wall roughness and the effect of drag-reducing
polymers on turbulent flow. Pipe flow is also a useful vehicle for in-
vestigating heat transfer, with numerous practical applications. Sec-
ondary flow in non-circular pipes exposes the non-Newtonian nature
of the Reynolds stresses, unfortunately without exposing any plau-
sible constitutive relations. Other variations on pipe flow, such as
flow with curvature or flow with an abrupt change in cross section,
reveal strong effects on mixing processes. Similarity laws originally
developed for pipe flow provide a point of contact with the boundary
layer and the wall jet.
The main experimental disadvantage of pipe flow is difficulty of
access for instrumentation, particularly optical instrumentation. A
major source of experimental scatter in fundamental work is failure
to provide sufficient length for the flow to become fully developed.
2.1.1
Equations of motion
The Reynolds equations of mean motion were derived in SECTION
1.3.4 for the cylindrical polar coordinates sketched in FIGURE 2.1.
These equations are easily specialized for the case of steady flow in
a round pipe of radius
R
. To make the notation consistent with
that for plane flow, take the axial, radial, and azimuthal coordinates
as (
x,r,θ
) and the corresponding velocity components as (
u,v,w
).
Take the mean flow to be fully developed, which is to say rectilinear.
Thus
v
=
w
= 0, and
u
6
= 0. All derivatives of mean quantities
with respect to
θ
are zero, as are all derivatives with respect to
x
except
p/∂x
, this term being the engine that drives the flow. The
continuity equation is moot. For simplicity, the overbar indicating
a mean value will be suppressed hereafter except in the Reynolds
stresses. The three momentum equations are reduced to
0 =
∂p
∂x
+
1
r
d
d
r
r
(
μ
d
u
d
r
ρ
u
v
)
;
(2.1)
0 =
∂p
∂r
+
1
r
(
ρ
w
w
d
d
r
r ρ
v
v
)
;
(2.2)
2.1. GENERALITIES
63
Figure 2.1: Cylindrical polar coordinate system and
notation for pipe flow.
0 =
1
r
2
d
d
r
r
2
ρ
v
w
.
(2.3)
The fluctuations
u
,v
,w
vanish at the wall. The three equations
(2.1)–(2.3) are rigorously correct, and must be satisfied by the mean
flow under the specified conditions. The equations are obviously not
complete, since there are three equations for six unknown quanti-
ties. Two of the Reynolds stresses,
ρ
u
u
and
ρ
u
w
, fail to ap-
pear. Of these, the absence of the mean product
u
w
is expected
if the turbulent motion is random. Given a sampled value for the
axial fluctuation
u
, it is reasonable to suppose, in view of the axial
symmetry of the problem, that positive and negative values for the
azimuthal fluctuation
w
are equally probable. That this argument
can be dangerous will be demonstrated in SECTION 2.5.5, where it
leads to a wrong conclusion for the viscous sublayer near a wall. In
the case of
ρ
u
u
, the failure of the Reynolds equations even to con-
tain this streamwise normal stress is embarrassing. It appears that
nothing can be learned about this stress from the laws of mechanics
in Reynolds-averaged form. At the same time, it is this Reynolds
stress
ρ
u
u
that is most easily and most commonly measured.
64
CHAPTER 2.
PIPE FLOW
Consider the three equations of motion (2.1)–(2.3). The third
equation (2.3) has the integral
r
2
ρ
v
w
= constant, and the constant
is zero whether evaluated on the axis or at the wall. The second
equation (2.2) is more instructive. Formal integration from
r
to
R
,
with the boundary condition
p
=
p
w
at the wall, gives
p
+
ρ
v
v
=
p
w
ρ
R
r
(
w
w
v
v
)
r
d
r .
(2.4)
When the lower limit is taken at the pipe axis,
r
= 0, the integral
diverges unless
v
v
=
w
w
on the axis. The equality is intuitively
obvious. If two traverses are made along a diameter of the pipe
to measure in one case the radial velocity fluctuation
v
along the
traverse direction and in the other case the azimuthal velocity fluc-
tuation
w
normal to it, the two measurements must be statistically
equivalent on the axis.
As the lower limit
r
in equation (2.4) approaches the upper
limit
R
, the definite integral is eventually small compared with the
term
ρ
v
v
on the left. In some vicinity of the wall, therefore, a useful
approximation suggests itself;
p
+
ρ
v
v
=
p
w
= constant
.
(2.5)
This approximation will be examined more closely in SECTION X
1
.
Finally, the quantity in parentheses in the first momentum
equation (2.1) is evidently the total shearing stress
τ
, here defined
with a change in sign in the derivative and in
v
because
y
=
R
r
is a more natural independent variable for an observer viewing the
flow from the wall;
τ
=
(
μ
d
u
d
r
ρ
u
v
)
.
(2.6)
At the wall of the pipe, where all velocity fluctuations vanish, the
corresponding value is
τ
w
=
μ
(
d
u
d
r
)
w
.
(2.7)
1
Unclear reference, possibly 5.2.1
2.1. GENERALITIES
65
By assumption, the terms in parentheses in equations (2.1) and
(2.2) do not depend on
x
, so that
2
p
∂x
2
=
2
p
∂r∂x
= 0
.
(2.8)
It follows that
∂p/∂x
is a constant, independent of
x
and
r
, although
p
itself depends on
x
and also on
r
if the flow is turbulent, according
to equation (2.4). Equation (2.1) in the form
0 =
∂p
∂x
1
r
d
d
r
(2.9)
can therefore be integrated from
r
to
R
, with the boundary condition
τ
=
τ
w
when
r
=
R
, to obtain
w
=
(
R
2
r
2
)
2
∂p
∂x
.
(2.10)
On putting
r
= 0, this becomes
τ
w
=
D
4
∂p
∂x
,
(2.11)
where
D
= 2
R
is the diameter. The last expression is also easily
obtained from a global momentum balance on a length of the pipe,
given that
∂p/∂x
is constant. Elimination of
∂p/∂x
between equa-
tions (2.10) and (2.11) yields finally the linear stress profile shown in
FIGURE 2.2,
τ
τ
w
=
r
R
.
(2.12)
So far, the flow has usually not been specified to be either
laminar or turbulent. In either case, equation (2.11) provides an
accurate and unambiguous method for determining
τ
w
for fully de-
veloped flow, and this property is the main reason that pipe flow is
discussed here before all other flows involving walls. In a real pipe,
there will be problems with entrance flow and development length,
to be discussed in SECTION 2.2.1. The fact that the stress
τ
de-
fined by equation (2.6) is linear in
r
also provides an opportunity for
proof and calibration of instruments, such as hot-wire anemometers,
66
CHAPTER 2.
PIPE FLOW
Figure 2.2: The parabolic mean-velocity profile and
the linear shearing-stress profile for steady laminar
flow in a circular pipe.
commonly used for measurement of the Reynolds shearing stress.
See, for example, NEWMAN and LEARY (1950), KJELLSTR
̈
OM
and HEDBERG (1970), and PATEL (1974). A more cogent use of
equation (2.12), as one criterion for equilibrium at second order of a
developing turbulent flow, will be taken up in SECTION 2.5.1.
2.1.2
Laminar flow
If the flow is laminar,
p
is independent of
r
, according to equation
(2.2), so that
∂p/∂x
becomes d
p/
d
x
. The velocity profile is the
integral of equation (2.12), given
τ
=
μ
d
u/
d
r
, that takes the value
u
=
u
c
(
c
for centerline) at
r
= 0 and satisfies the boundary condition
u
= 0 at
r
=
R
. In dimensionless form, this profile is the parabola
shown in FIGURE 2.2,
u
u
c
= 1
r
2
R
2
,
(2.13)
2.1. GENERALITIES
67
where the centerline velocity
u
c
is related to the other parameters of
the problem by
τ
w
= 2
μ
u
c
R
.
(2.14)
This solution (2.13) of the Navier-Stokes equations for laminar pipe
flow, like solutions of the Stokes approximation for low Reynolds
numbers, represents a balance between pressure forces and viscous
forces. However, the transport terms vanish here because of the
special geometry, not because the Reynolds number is necessarily
small.
Finally, the volume flow
Q
in the pipe can be calculated, and
a mean velocity
̃
u
defined, from
Q
=
R
0
2
πru
d
r
=
πR
2
̃
u
(2.15)
(the tilde, here and elsewhere, is intended as a mnemonic for an
integral mean value). Given equation (2.13) for
u
, it follows on inte-
gration that
̃
u
=
u
c
2
.
(2.16)
Several of the earliest experiments with pipe flow and with
flow between concentric rotating cylinders in the 19th century were
undertaken primarily for a reason that may now seem almost unnat-
ural. The equations of NAVIER (1823) and STOKES (1849) inde-
pendently incorporate a hypothesis first proposed by NEWTON in
his
Principia Mathematica
, published in 1687. According to STAN-
TON and PANNELL (1914), the proper attribution to Newton was
first pointed out by Sir George Greenhill, who would presumably
have been at home in both the subject and the Latin language. The
relevant passage introduces Section IX, “The circular motion of flu-
ids,” in Book II, “The motion of bodies.” In the elegant prose of the
revised translation by Cajori (1934):
Hypothesis: The resistance arising from the want of lu-
bricity in the parts of a fluid is, other things being equal,
68
CHAPTER 2.
PIPE FLOW
proportional to the velocity with which the parts of the
fluid are separated from one another.
This hypothesis is explicit in the tensor relation
τ
=
μ
def
~u
in the introduction. The scalar constant of proportionality, the vis-
cosity, is assumed to be an intrinsic or state property of the fluid (it
may, for example, vary significantly with temperature), independent
of the motion. In the case of pipe flow, the technique was and is
used to show the existence of such a fluid property by showing that
the quantity
μ
, expressed theoretically for the case of fully developed
laminar pipe flow by a combination of equations (2.11), (2.14), and
(2.16),
μ
=
D
2
32
̃
u
d
p
d
x
,
(2.17)
is experimentally independent of particular choices for
D
and
̃
u
, since
these must be precisely compensated for by variations in d
p/
d
x
. As
a practical matter, it is usually not the mean velocity
̃
u
that is mea-
sured, but the volume flux
Q
defined by equation (2.15). Equation
(2.17) is therefore better expressed as
μ
=
πD
4
128
Q
d
p
d
x
(2.18)
to emphasize that in capillary-tube viscometry the diameter
D
needs
to be very accurately known. Many common fluids, including air and
water, possess the property of viscosity in the sense just defined and
are therefore referred to as Newtonian fluids. A second important is-
sue, the validity of the no-slip boundary condition at the wall, has for
practical purposes been resolved experimentally in favor of no slip.
Residual doubts about this condition for the case of non-wetting
combinations, such as mercury on glass, or water on tetrafluoroethy-
lene (teflon), have been mostly quieted by BINGHAM and THOMP-
SON (1928) and by BROCKMAN (1956), respectively. Exceptions
to Newtonian behavior are known, and these present formidable dif-
ficulties in formulating a constitutive relationship between the stress
and rate-of-strain tensors. The relatively unstructured literature of
rheology and of turbulence modeling testifies, in a familiar idiom,
that Newton is a hard act to follow.
2.1. GENERALITIES
69
The Reynolds number for both laminar and turbulent pipe flow
is commonly defined in terms of the mean velocity
̃
u
and the pipe
diameter
D
;
Re
=
̃
uD
ν
.
(2.19)
Usage varies in defining a dimensionless friction coefficient (see
SECTION X).
2
In mechanical and aeronautical engineering, where
the boundary layer and its global momentum balance are in the fore-
ground, the usual form for the dimensionless friction, and the one
that I will adopt here, is
C
f
=
τ
w
ρ
̃
u
2
/
2
.
(2.20)
This quantity is also denoted by
f
and called the Fanning factor
by mechanical engineers. For laminar flow, equations (2.14), (2.16),
(2.19), and (2.20) imply
C
f
=
16
Re
.
(2.21)
To the extent that pipe flow can be viewed as a boundary layer
on the inside of a cylindrical body, it might be more consistent to
use
u
c
and
R
instead of
̃
u
and
D
in the definition (2.19) for the
Reynolds number, and
u
2
c
instead of
̃
u
2
in the definition (2.20) for
the friction coefficient. Probably the usage described here has sur-
vived because no value for
u
c
is available for most of the existing
pipe data. In practice, the definition of dimensionless coefficients to
characterize pipe flow over a large range of Reynolds numbers has
been preempted by the turbulent case, for which the wall friction is
only weakly dependent on the viscosity, and the dynamic pressure is
the important reference quantity.
In principle, both
τ
w
and
̃
u
are easily measured for fully de-
veloped pipe flow, the former in terms of
∂p/∂x
and the latter by a
variety of methods. These include direct evaluation from the integral
definition (2.15), if a velocity profile is available; or measurement of
volume flow rate, by weighing or by use of a calibrated volume if
2
Possibly section 2.4.1
70
CHAPTER 2.
PIPE FLOW
the fluid is a liquid; or by blowdown techniques if the fluid is a gas.
Other methods include use of a calibrated venturi, orifice plate, or
other type of flow meter; or, for best regulation, use of a constant-
displacement pump or even a piston-cylinder displacement mecha-
nism.
2.1.3
An extremum principle
It was pointed out by LIN (1952), in a short paper whose roots
lie in work by HELMHOLTZ (1868) and KORTEWEG (1883) on
arbitrarily slow steady viscous motions, that the parabolic laminar
profile in a round pipe can be obtained from an extremum principle.
Consider all possible axisymmetric rectilinear motions
u
(
r
) satisfying
the no-slip condition at the wall, and minimize the total rate of
energy dissipation,
̃
Φ =
μ
R
0
2
πr
(
d
u
d
r
)
2
d
r ,
(2.22)
subject to the constraint of a constant volume flux,
Q
=
R
0
2
πru
d
r
=
πR
2
̃
u
= constant
.
(2.23)
The notation
̃
Φ means a volume integral of the local rate of dissi-
pation over the pipe cross section and over unit length in the flow
direction.
The problem just formulated is an example of what COURANT
and HILBERT (1953, Vol. 1, Chapter IV) call the simplest problem
in the variational calculus. This is to find the function
u
(
r
) that
minimizes the integral
̃
Φ =
R
0
F
(
r, u, u
)d
r ,
(2.24)
2.1. GENERALITIES
71
subject to the constraint
Q
=
R
0
G
(
r, u, u
)d
r
= constant
.
(2.25)
The prime here indicates differentiation with respect to
r
. The Euler
equation for the problem is
(
u
′′
2
∂u
∂u
+
u
2
∂u∂u
+
2
∂r∂u
∂u
)
(
F
+
λG
) = 0
,
(2.26)
where
λ
is a Lagrange multiplier. In the present case, with
F
= 2
πμr
(
u
)
2
, G
= 2
πru ,
(2.27)
equation (2.26) becomes
2
μ
d
d
r
(
r
d
u
d
r
)
λr
= 0
.
(2.28)
The indefinite integral of this equation is
u
=
1
2
μ
(
λr
2
4
+
A
ln
r
+
B
)
,
(2.29)
where
A
and
B
are constants of integration. A logarithmic term
appears in equation (2.29), but not in equation (2.13), because the
earlier derivation already required
τ
(i.e., d
u/
d
r
) to be linear in
r
.
The logarithmic term is needed if the no-slip boundary condition is
to be satisfied for the more general case of axial flow in an annulus.
For flow in a pipe, the boundary conditions
u
=
u
c
at
r
= 0 and
u
= 0 at
r
=
R
require
A
= 0 and
B
= 2
μu
c
=
λR
2
/
4. Equation
(2.14) is recovered,
u
u
c
= 1
r
2
R
2
,
(2.30)
with now
λ
=
8
μu
c
R
2
.
(2.31)
72
CHAPTER 2.
PIPE FLOW
Use of the three equations (2.31), (2.14), and (2.11) implies
λ
= 2
d
p
d
x
,
(2.32)
as does a direct comparison of equation (2.28) with the laminar ver-
sion of the momentum equation (2.1).
For the parabolic profile in a pipe, therefore, the rate of dissi-
pation is an extremum. That the extremum is a minimum is easily
shown by adding to the parabolic profile an arbitrary axisymmetric
perturbation that vanishes at the wall and does not contribute to
the volume flux. The result (2.32), derived here for a very special
motion of an incompressible viscous fluid, should be read in the same
sitting as SOMMERFELD’s argument (1950, pp. 89–92) that for an
incompressible inviscid fluid the pressure
p
can be interpreted as a
Lagrange multiplier representing the constraint of incompressibility.
Finally, the pressure gradient and the rate of dissipation can
be related directly for fully developed pipe flow, whether laminar or
turbulent. The general form for energy loss from the mean flow per
unit time and per unit volume is
(cite introduction)
τ
·
grad
~u
, so
that equation (2.22) can be written
̃
Φ =
R
0
2
πrτ
d
u
d
r
d
r .
(2.33)
Integration by parts, with
τ
= 0 at
r
= 0 and
u
= 0 at
r
=
R
, gives
̃
Φ =
2
π
R
0
u
d
d
r
d
r .
(2.34)
Use of equation (2.12) for
τ
, (2.15) for the volume flow
Q
, and (2.11)
for
τ
w
then gives
̃
Φ =
Q
∂p
∂x
.
(2.35)
The point of this exercise in the calculus of variations for lam-
inar pipe flow is that a similar principle may hold for turbulent flow.
If so, it would not be surprising if the resulting mean velocity profile
turned out to be logarithmic.
2.2. DEVELOPMENT LENGTH
73
Figure 2.3: A schematic diagram of flow in the
laminar development region of a circular pipe with
uniform entrance flow.
2.2 Development length
In any attempt to define the properties of a hypothetical fully de-
veloped or equilibrium flow experimentally, a useful first step is to
observe the rate of approach to equilibrium from a disturbed ini-
tial condition. In the case of pipe flow, the process most commonly
observed is the evolution of the flow downstream from the pipe en-
trance. The response to other disturbances, such as a step change in
diameter, can also provide estimates of a characteristic time scale or
spatial scale for approach to equilibrium.
2.2.1
Laminar flow
The parabolic profile requires some distance to develop in the en-
trance region of a real pipe, especially at large Reynolds numbers,
and the need for adequate development length is not always recog-
nized by experimenters. Let this development length be estimated
approximately in terms of the inward growth of internal laminar
boundary layers that start at the pipe entrance at
x
= 0, as shown
in FIGURE 2.3. Note that the artist was apparently not told of the
doubling of the velocity on the pipe axis during laminar develop-
74
CHAPTER 2.
PIPE FLOW
ment. Global parameters available for making the estimate dimen-
sionless are the kinematic viscosity
ν
, the pipe diameter
D
, and the
mean velocity
̃
u
. That the latter quantity is independent of
x
in the
development region can be shown by reinstating the axisymmetric
continuity equation in the form
∂u
∂x
+
1
r
∂rv
∂r
= 0
(2.36)
and calculating the derivative of
̃
u
from the definition (2.15); thus
πR
2
d
̃
u
d
x
=
R
0
2
πr
∂u
∂x
d
r
=
R
0
2
π
∂rv
∂r
d
r
= 0
,
(2.37)
since
v
vanishes at both limits.
A qualitative estimate of development length in terms of dif-
fusion time and transport time can be obtained by using the device
of a moving observer applied to a growing internal boundary layer.
Assume that the entrance is cut square with the axis so that the
origin for
x
is well defined. Take the flow to be uniform at the pipe
entrance; i.e.,
u
=
̃
u
at
x
= 0. Vorticity generated at the wall by
the axial pressure gradient diffuses inward through a distance
δ
in a
time
t
δ
2
(see the Rayleigh problem in the introduction)
.
An observer following the mean flow travels a distance
x
in a time
t
=
x/
̃
u
. At equal times,
x/δ
̃
uδ/ν
. If the development length
X
is defined as the value of
x
when
δ
=
D/
2, then
X
is proportional to
DRe
and
x/X
is proportional to
x/DRe
.
Since the first papers by BOUSSINESQ (1890a,b,c; 1891a,b),
work on the problem of laminar flow development in a round pipe
has become almost a cottage industry. Of more than forty exper-
imental, analytical, or numerical papers on this topic, about half
aim at estimates of a particular constant
m
belonging to the art
of capillary-tube viscometry (see the next SECTION 2.2.2). The
remainder view the problem as an exercise in classical fluid mechan-
ics. The first analysis using boundary-layer theory was carried out
by SCHILLER (1922). This paper was a natural application of the
integral method of Karman and Pohlhausen, published a year ear-
lier. The model combined parabolic profiles near the wall with a
2.2. DEVELOPMENT LENGTH
75
X/(R&)D
FIGURE
3.25.
SOme
analytical
results
for
laminar
flow
development
in
a
smooth
pipe.
The
dependent
variable
uc/u
has
an
asymptotic
limit
of
2
.
-
Figure 2.4: Some analytical results for laminar flow
development in a smooth pipe. The dependent variable
u
c
/
̃
u
has an asymptotic limit of 2.
flat profile near the centerline. The predicted evolution of the axial
velocity on the pipe axis is one of the curves shown in FIGURE 2.4.
The analysis ignores the fact that a boundary-layer approach is com-
plicated by effects of lateral curvature and by interaction between
the axial pressure gradient in the inviscid core flow and the grow-
ing displacement thickness of the boundary layer, each affecting the
other. Moreover, the boundary-layer approximation fails before the
flow development is complete, and an asymptotic analysis is even-
tually required. The growing power of computers now allows the
laminar problem to be treated by numerical integration of the full
Navier-Stokes equations for quite large Reynolds numbers.
The other data in FIGURE 2.4 are chosen from the work of
DORSEY (1926)
M
̈
ULLER (1936) figure 4
ATKINSON and GOLDSTEIN (1938)
LANGHAAR (1942) figure 1
ASTHANA (1951)
TATSUMI (1952)
SIEGEL (1953)
76
CHAPTER 2.
PIPE FLOW
RIVAS and SHAPIRO (1956)
BOGUE (1959)
TOMITA (1961)
CAMPBELL and SLATTERY (1963)
COLLINS and SCHOWALTER (1963)
LUNDGREN et al. (1964)
SPARROW et al. (1964) figure 3
CHRISTIANSEN and LEMMON (1965) figures 2, 3
HORNBECK (1965) figures 3, 6
McCOMAS and ECKERT (1965)
VRENTAS et al. (1966) figures 3–8
McCOMAS (1967)
FRIEDMANN et al. (1968) figures 1–4
LEW and FUNG (1968) tables
SCHMIDT and ZELDIN (1969)
FARGIE and MARTIN (1971) figure 4
CHEN (1973) figure 1
KESTIN et al. (1973) figure 8
KANDA and OSHIMA (1986) figures 5–8
The main imperfection of these contributions lies in the fre-
quent assumption of a flat velocity profile at the station
x
= 0, with
an unphysical upstream flow that is often left undefined. However,
there is general agreement that the independent variable
x/DRe
is
a natural and appropriate one in the laminar development region,
whether a boundary-layer model is used or not.
A few experiments include the work of
BOND (1921)
RIEMAN (1928)
ZUCROW (1929)
KLINE and SHAPIRO (1953)
SHAPIRO et al. (1954)
KREITH and EISENSTADT (1957)
WELTMANN and KELLER (1957)
RESHOTKO (1958) figure 9
PFENNINGER (1961) figure 12
2.2. DEVELOPMENT LENGTH
77
McCOMAS and ECKERT (1965) figure 3
ATKINSON et al. (1967) figure 4
DAVIS and FOX (1967) figure 11
EMORY and CHEN (1968)
BERMAN and SANTOS (1969) figures 3–7
BURKE and BERMAN (1969) figures 3–6, 8
FARGIE and MARTIN (1971) figure 4
WYGNANSKI and CHAMPAGNE (1973)
MESETH (1974)
MOHANTY and ASTHANA (1979)
(
Why does nobody plot
̃
τ
w
? Mention honeycombs. No calcula-
tions for square-cut entrance with bubble.)
From all of this work, the evidence is persuasive that develop-
ment is complete for practical purposes when
1
Re
x
D
0
.
07
1
14
,
(2.38)
provided that the Reynolds number
Re
is not less than about 100.
For a pipe of given diameter and length, the largest Reynolds number
for which a parabolic profile can be established is about 14
L/D
. For
a given Reynolds number, the smallest
L/D
is about
Re/
14. Con-
sequently, to identify the record holder for highest Reynolds number
with fully developed laminar flow, it is necessary only to look for
large values of
L/D
and to test the state of the exit flow. By this
criterion, the record is about
̃
uD/ν
= 13
,
000 and is held by LEITE
(1958).
With sufficient care, it is possible to maintain laminar flow
in relatively short pipes up to very large Reynolds numbers, 50,000
or more. However, the parabolic profile is never fully developed in
such cases, and the decisive element for transition becomes the dis-
turbance level outside the boundary layer in the early development
region. In any contest to establish the highest achievable laminar
Reynolds number in short pipes, the results are a measure of the de-
gree of care taken to avoid such disturbances, rather than of any di-
rectly useful physical quantity. For example, blowdown methods can
reduce disturbance levels far below the best obtainable in flows driven
78
CHAPTER 2.
PIPE FLOW
by an upstream pump or compressor, and a gas flow can be quieted
by use of a sonic orifice to isolate the test section from a downstream
pump. As far as I know, the record here is held by PFENNINGER
and MEYER (1953), who used a long conical contraction fitted with
13 screens, as well as elaborate vibration isolation, to obtain a flow
free of turbulence at a Reynolds number
̃
uD/ν
= 88
,
000. The corre-
sponding number
̃
ux/ν
was about 50
×
10
6
, an order of magnitude
higher than the number that can be obtained on flat plates in con-
ventional wind tunnels. The boundary layer in Pfenninger’s pipe
occupied about 60 percent of the area at the pipe exit. To obtain a
fully developed parabolic profile in air under these conditions would
need a length of about 140 meters, together with heroic measures
to minimize disturbances in the flow and to account for changes in
density. Even if this could be done, I see no particular profit from
an attempt.
Finally, several experimenters have found that it is not safe to
assume that a laminar pipe flow in the laboratory will automatically
be axisymmetric. LEITE (1958), RESHOTKO (1958), HOULIHAN
(1969), WYGNANSKI and CHAMPAGNE (1973), and BREUER
(1985), all working on difficult questions of stability and transition,
and all working with air in pipes having a diameter of a few centime-
ters, describe problems in obtaining axisymmetric fully-developed
flow. Some of their results are illustrated in FIGURE 2.5. They
comment in particular on the need for close control of thermal in-
homogeneities, pipe alignment, and axial symmetry of conditions far
upstream. Most other experimenters have had a better experience
or have not tested their flows for symmetry.
2.2.2
Capillary-tube viscometry
Numerous devices are commercially available for measuring the vis-
cosity of fluids used in laboratory experiments or manufacturing pro-
cesses. They include cone-plate, rotating-cylinder, falling-ball, and
capillary-tube viscometers. The choice is usually governed by the
range of viscosity involved, by the volume of the sample committed
to the measurement, and occasionally by special conditions such as
2.2. DEVELOPMENT LENGTH
79
Figure 2.5: Several examples from the experimental
literature showing non-axisymmetric laminar flow in
circular pipes. The most likely cause is secondary flow
due to thermal inhomogeneity in a gravitational field or
asymmetry of the upstream channel.
80
CHAPTER 2.
PIPE FLOW
a need in process work to immerse the device in the bulk fluid. Typ-
ically, such viscometers are calibrated by the manufacturer or the
user, using fluids of known viscosity, to take into account various
effects of finite geometry.
The question of how a known viscosity comes to be known is
far from trivial. This question is the business of standards labora-
tories. For example, SWINDELLS, COE, and GODFREY (1952)
describe a painstaking program in capillary-tube viscometry, carried
on from 1931 to 1941 and from 1947 to 1952 at the U.S. National
Bureau of Standards (now the U.S. National Institute of Standards
and Technology), whose singular result was to establish the value
μ
= 0
.
010019
±
0
.
000003 poise for pure water at 20
C
. This value is
still the cornerstone of viscosity tables for water that are constructed
from more extensive but less accurate measurements. The geometry
in capillary viscometry at the standards level is apparently stan-
dardized, requiring a square-cut entrance and exit, although other
geometric details, such as the tube outer diameter, are usually left
open. The need for close control of several variables is self-evident. In
order to obtain four significant figures in the viscosity, according to
equation (2.18), the absolute temperature, the volume flow rate, the
tube length, the pressure difference, and especially the tube diameter
must all be known to better accuracy, with a further allowance for
errors introduced by differentiation of experimental data. It may be
necessary, for example, to represent the cross section of a real tube
by an ellipse rather than by a circle, with a corresponding adjust-
ment in the theory. A long tube of small diameter provides an easily
measurable pressure difference, although this pressure difference is
necessarily global rather than local if pressure taps cannot be pro-
vided along the length of the tube. At the same time, the diameter
must not be so small that it cannot be measured with the necessary
accuracy. The length is also limited in practice by the need to main-
tain the flow system at constant temperature in a bath of practical
size without having to coil the tube and accept a much more complex
theory.
The expected pressure distribution in a finite tube is shown
schematically in FIGURE 2.6. Certain general relationships that
2.2. DEVELOPMENT LENGTH
81
Figure 2.6: A schematic representation of the
pressure distribution along a tube of length
L
with
uniform entrance flow at
x
= 0. The flow may be laminar
or turbulent and the cross section need not be circular.
emerge from the figure do not depend on the shape of the tube cross
section or the shape of the tube entrance, as long as these are fixed.
Suppose for convenience that entrance and exit are cut square, so
that
L
is well defined. The quantities
p
0
and
p
2
are the static pres-
sures in the entrance and exit reservoirs. The quantity
p
1
is the
static entrance pressure associated with a fictitious fully developed
flow over the full length of the tube. Anomalous pressure effects at
both entrance and exit are included in principle, although exit effects
are not treated explicitly. It is not necessary to distinguish between
laminar and turbulent flow, or even mixed flow at Reynolds numbers
in the transition regime.
The strategy associated with FIGURE 2.6 is one of experi-
mental differentiation. Suppose that the Reynolds number is held
constant as the length of the tube is varied, and suppose that the
shortest tube is long enough to achieve fully developed flow. Then
a unit increment in the length of the tube will give rise to a unit
82
CHAPTER 2.
PIPE FLOW
increment in total pressure drop. Begin with the identity
p
0
p
2
= (
p
0
p
1
) + (
p
1
p
2
)
.
(2.39)
For the general case, define an ideal friction coefficient for fully de-
veloped flow,
C
f
=
D
(
p
1
p
2
)
2
̃
u
2
,
(2.40)
where
̃
u
=
Q/A
is again a mean velocity over the cross section
A
.
For the special case of a circular tube, the definition (2.40) reduces
through equation (2.11) to equation (2.20). Define also a global
friction coefficient,
̂
C
f
=
D
(
p
0
p
2
)
2
̃
u
2
,
(2.41)
where the circumflex over
C
f
denotes a mean value over the entire
length of the tube, reservoir to reservoir. Equation (2.39) then takes
the form
̂
C
f
L
D
=
(
p
0
p
1
)
2
ρ
̃
u
2
+
C
f
L
D
.
(2.42)
For fully developed flow at the exit, the first term on the right is a
constant that is characteristic of the complete development process
for particular entrance conditions and Reynolds number. Without
the factor of 2 in the denominator, this constant is usually denoted
by
m
in the literature of capillary-tube viscometry;
m
=
(
p
0
p
1
)
ρ
̃
u
2
,
(2.43)
so that
̂
C
f
L
D
=
m
2
+
C
f
L
D
.
(2.44)
Except possibly for a square-cut entrance, the development parame-
ter
m
, defined graphically in figure 2.6, will depend on the entrance
geometry and flow conditions for a particular tube. A plot of
̂
C
f
L/D
against
L/D
is a straight line whose slope
C
f
and intercept
m/
2 are
characteristic for the Reynolds number in question. In particular,
C
f
=
(
̂
C
f
L/D
)
(
L/D
)
.
(2.45)
2.2. DEVELOPMENT LENGTH
83
A simple implementation of this differentiation scheme was
proposed and used by COUETTE (1890), but has since been used
only rarely, and then mostly by professionals such as Swindells
et al
.
The technique is to construct two capillary viscometers by connect-
ing two tubes in series with a third reservoir inserted between them.
The two tubes are assumed to be identical in diameter and all other
geometrical details except length. When in equilibrium, they have
the same flow rate. The two parameters
C
f
and
m
are then readily
evaluated from a single experiment.
Discuss
m
from
p
(
x
)
. Cite bibliography.
Equation (2.44) is usually cast in a more direct and more literal
form for use in viscometry with a round tube. From equation (2.39),
with
p
1
p
2
=
L
d
p/
d
x
= 4
w
/D
= 8
μ
̃
uL/R
2
, and with
̃
u
=
Q/πR
2
, this form is
π
2
R
4
(
p
0
p
2
)
ρQ
2
=
m
+
8
πμL
ρQ
.
(2.46)
For constant
Q
and
R
and variable
L
, a dimensional plot of (
p
0
p
2
)
against
L
yields a straight line whose slope is proportional to
μ
and
whose intercept is proportional to
m
. Such a plot is a practical
realization of FIGURE 2.6.
A different form, appropriate for a single tube with changing
flow rate, is obtained on multiplying by
Q
and making the important
assumption that
m
is independent of Reynolds number;
π
2
R
4
(
p
0
p
2
)
ρQ
=
mQ
+
8
πμL
ρ
.
(2.47)
Now, for constant
L
and
R
and variable
Q
, a plot of (
p
0
p
2
)
/Q
against
Q
yields a straight line whose slope is proportional to
m
and
whose intercept is proportional to
μ
. This formulation is the one used
by Swindells et al. Such a plot is sometimes called a Knibbs plot,
after KNIBBS (1895). The assumption that the entrance parameter
m
defined by equation (2.44) is independent of Reynolds number in
some range of
Re
needs verification for both smooth and square-cut
entrances, since the parameters
̃
u
,
D
, and
ν
define two lengths,
D
and
ν/
̃
u
, together with their ratio
Re
.
84
CHAPTER 2.
PIPE FLOW
Finally, still for a single tube, multiplication of equation (2.47)
by
ρQ
yields
π
2
R
4
(
p
0
p
2
) =
ρmQ
2
+ 8
πμLQ .
(2.48)
The conclusion that the overall pressure drop should be the sum of
a term in
Q
(or
̃
u
) and a term in
Q
2
(or
̃
u
2
) was noted by HAGEN
(but not by Poiseuille) and is probably the reason that the term
containing
m
is often referred to, not quite correctly, as a kinetic-
energy correction.
For the case of a circular tube, it is also possible to calculate
p
0
p
1
in FIGURE 2.6 from first principles, given a suitable model
of the flow in the development region. By definition,
m
=
(
p
0
p
1
)
ρ
̃
u
2
=
(
p
0
p
1
) + (
p
1
p
2
)
(
p
1
p
2
)
ρ
̃
u
2
.
(2.49)
Visualize an ideal entrance, for which the velocity profile at an initial
station
x
= 0 is uniform, with velocity
̃
u
and pressure
p
1
that do not
depend on
r
. Assume frictionless acceleration from rest upstream of
this station. The Bernoulli equation then determines the first term
on the right in equation (2.49);
p
0
p
1
=
1
2
ρ
̃
u
2
.
(2.50)
The middle term can be partially evaluated for laminar flow.
For steady axisymmetric laminar flow in the development region,
the equations of motion
(see introduction)
can be written, with
no boundary-layer approximation, as
∂ru
∂x
+
∂rv
∂r
= 0 ;
(2.51)
ρ
(
∂ruu
∂x
+
∂ruv
∂r
)
=
r
∂p
∂x
+
μr
(
2
u
∂x
2
+
1
r
∂r
r
∂u
∂r
)
.
(2.52)
When both equations are integrated over a cross section of a tube of
constant diameter, the result can be reduced to a simple momentum