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Lecture 12 F. Morrison CM3110
10/27/2019
CM3110
Transport I
Part I: Fluid Mechanics
More Complicated Flows II:
External Flow
(or applying fluid-mechanics problemsolving to a new category of flows)
Professor Faith Morrison
Department of Chemical Engineering
Michigan Technological University
1
© Faith A. Morrison, Michigan Tech U.
More complicated flows II: From Nice to Powerful
r
Nice:
A
z
cross-section A:
r
z
Learning to solve one particular problem
(or a group of related problems)
L
vz(r)
fluid
R
Powerful:
Solving never-before-solved problems.
2
© Faith A. Morrison, Michigan Tech U.
1
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
A real flow problem
(external). What is the
speed of a sky diver?
(Morrison, Example 8.1)
3
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
A real flow problem
(external). What is the
speed of a sky diver?
Can we use anything we
learned from flow-throughconduits to tell us how to
solve this new problem?
(Morrison, Example 8.1)
4
© Faith A. Morrison, Michigan Tech U.
2
Lecture 12 F. Morrison CM3110
10/27/2019
Flow through Conduits
More complicated flows II
So far we have talked about internal flows
•ideal flows (Poiseuille flow in a tube)
•real flows (turbulent flow in a tube)
Strategy for handling real flows:
Dimensional analysis and data
correlations, 𝑓 Re
How did we arrive at correlations?
non-Dimensionalize ideal flow; use to
guide expts on similar non-ideal flows;
take data; develop empirical
correlations from data
What do we do with the correlations? use in MEB; calculate pressure-drop
flow-rate relations
5
© Faith A. Morrison, Michigan Tech U.
F. A. Morrison, An Introduction to Fluid Mechanics, Cambridge
University Press 2013.
6
© Faith A. Morrison, Michigan Tech U.
3
Lecture 12 F. Morrison CM3110
10/27/2019
Solve a wide variety
of practical problems
with data correlations.
Pumping loops, piping networks, pump
characteristic curves, non-circular cross
sections, flow through porous media, etc.
F. A. Morrison, An Introduction to Fluid Mechanics, Cambridge
University Press 2013.
7
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
A real flow problem
(external). What is the
speed of a sky diver?
We can apply the
conduit process to this
new problem.
(Morrison, Example 8.1)
8
© Faith A. Morrison, Michigan Tech U.
4
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
A real flow problem
(external). What is the speed
of a sky diver?
Drag
(fluid force)
Gravity
Apply the physics:
π‘šπ‘Ž
𝑓
(Morrison, Example 8.1)
9
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
A real flow problem
(external). What is the speed
of a sky diver?
π‘šπ‘Ž
𝑓
At terminal velocity π‘Ž
Drag
0
0
π‘šπ‘”
𝐹
(fluid force)
𝐹
Gravity
π‘šπ‘”
The fluids part of
the problem is,
what is 𝐹 ?
(drag in flow around an obstacle)
(Morrison, Example 8.1)
10
© Faith A. Morrison, Michigan Tech U.
5
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
A real flow problem
(external). What is the speed
of a sky diver?
Can we address
this new problem
(new to us) . . .
At terminal velocity π‘Ž
Drag
0
0
π‘šπ‘”
𝐹
(fluid force)
𝐹
Gravity
π‘šπ‘”
The fluids part of
the problem is,
what is 𝐹 ?
(drag in flow around an obstacle)
(Morrison, Example 8.1)
More complicated flows II
Flow through Conduits
So far we have talked about internal flows
•ideal flows (Poiseuille flow in a tube)
•real flows (turbulent flow in a tube)
Strategy for handling real flows:
Dimensional analysis and data
correlations, 𝑓 Re
How did we arrive at correlations?
non-Dimensionalize ideal flow; use to
guide expts on similar non-ideal flows;
take data; develop empirical
correlations from data
By using the same
approach as used for
pipe flow?
What do we do with the correlations? use in MEB; calculate pressure-drop
flow-rate relations
11
© Faith A. Morrison, Michigan Tech U.
Flow around Obstacles
More complicated flows II
Now, we will talk about external flows
•ideal flows (flow around a sphere)
•real flows (turbulent flow around a sphere, sky diver, other obstacles)
Strategy for handling real flows:
Dimensional analysis and data
correlations
How did we arrive at correlations?
non-Dimensionalize ideal flow; use to
guide expts on similar non-ideal flows;
take data; develop empirical
correlations from data
What do we do with the correlations? calculate drag – free-stream velocity
relations
12
© Faith A. Morrison, Michigan Tech U.
6
Lecture 12 F. Morrison CM3110
10/27/2019
Flow around Obstacles
More complicated flows II
Now, we will talk about external flows
•ideal flows (flow around a sphere)
•real flows (turbulent flow around a sphere, sky diver, other obstacles)
Let’s try
Strategy for handling real flows:
Dimensional analysis and data
correlations
How did we arrive at correlations?
non-Dimensionalize ideal flow; use to
guide expts on similar non-ideal flows;
take data; develop empirical
correlations from data
What do we do with the correlations? calculate drag – free-stream velocity
relations
13
© Faith A. Morrison, Michigan Tech U.
What is the steady state velocity
field around a sphere dropping
through an incompressible
Newtonian fluid
𝑔
14
© Faith A. Morrison, Michigan Tech U.
7
Lecture 12 F. Morrison CM3110
10/27/2019
(equivalent to
sphere falling
through a liquid)
Steady flow of an
incompressible, Newtonian
fluid around a sphere
What is the steady state velocity
field when an incompressible,
Newtonian fluid flows around a
stationary sphere? What is the
drag on the sphere? The
upstream velocity is 𝑣 .
𝑔
(Morrison, Example 8.2)
flow
𝒗
15
© Faith A. Morrison, Michigan Tech U.
(equivalent to
sphere falling
through a
liquid)
Steady flow of an
incompressible,
Newtonian fluid around a
sphere
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
•spherical coordinates
•symmetry in the πœ™ direction
•calculate 𝑣 and drag on sphere
•upstream 𝑣
𝑣
𝑔
𝑣
flow
𝒗
𝑣
𝑣
𝑣
(Morrison, Example 8.2)
16
© Faith A. Morrison, Michigan Tech U.
8
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
flow
17
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
Microscopic Balances
(Microscopic balances on an
arbitrary control volume)
S
dS
Continuity Equation (mass)
nΜ‚
V

 v οƒ—  ο€½ ο€­   οƒ— v 
ο‚Άt
Equation of Motion (momentum)
Newtonian
οƒΆ
 ο‚Άv
 v οƒ—  v οƒ· ο€½ P   2 v   g fluid
οƒΈ
 ο‚Άt

Navier-Stokes Equation
18
© Faith A. Morrison, Michigan Tech U.
9
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
Continuity
(spherical coordinates)
19
www.chem.mtu.edu/~fmorriso/cm310/Navier.pdf
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
Navier-Stokes
(spherical coordinates)
20
www.chem.mtu.edu/~fmorriso/cm310/Navier.pdf
© Faith A. Morrison, Michigan Tech U.
10
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
Gravity
𝑔
𝑧
π‘Ÿ, πœƒ, πœ™

𝑒̂
sin πœƒπ‘’Μ‚
(See inside back cover;
do some algebra)
𝑦
𝑔
𝑔
cos πœƒπ‘’Μ‚
𝑔𝑒̂
𝑔cos πœƒπ‘’Μ‚
𝑔sin πœƒπ‘’Μ‚
𝑔cos πœƒ
𝑔sin πœƒ
0
(Morrison, Example 8.2)
flow
𝒗
21
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
Because the flow is
not unidirectional, we
have to consider the
left-hand-side of the
Navier-Stokes
Steady flow of an
incompressible,
Newtonian fluid
around a sphere
Equation of Motion:
 ο‚Άv
οƒΆ
 v οƒ— v οƒ· ο€½ P   2 v   g
 ο‚Άt
οƒΈ

(do we have to?)
22
© Faith A. Morrison, Michigan Tech U.
11
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
𝑣
𝑣
𝑣
𝑣
Eqn of
Continuity:
Eqn of
Motion:
𝑔cos πœƒ
𝑔sin πœƒ
0
𝑔
𝑝
𝑝 π‘Ÿ, πœƒ
 
Steady flow of an
incompressible,
Newtonian fluid
around a sphere
 1 ο‚Ά r 2vr
1 ο‚Άv sin  οƒΆ
 2
οƒ·ο€½0
 r ο‚Άr  r sin 
 οƒ·οƒΈ

Creeping Flow
 ο‚Άv
οƒΆ
 v οƒ— v οƒ· ο€½ P   2 v   g
 ο‚Άt
οƒΈ

steady
state
SOLVE
neglect
inertia
BC1: no slip at sphere surface
BC2: velocity goes to 𝑣 far from sphere
23
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
SOLUTION: Creeping Flow
οƒΆ
  3 R 1  R οƒΆ3οƒΉ
οƒ·
 v οƒͺ1 ο€­
cos


οƒΊ

οƒ·
οƒ·
 ο‚₯οƒͺ 2 r 2  r οƒΈ οƒΊ

οƒ·
 
 3 R 1  R οƒΆ3οƒΉ
οƒ·

v ο€½  ο€­ vο‚₯οƒͺ1 ο€­
ο€­  οƒ· οƒΊ sin  οƒ·
οƒͺ 4 r 4  r οƒΈ 
οƒ·

0
οƒ·

οƒ·

0
οƒ·

οƒΈr

2
3 vο‚₯  R οƒΆ
P ο€½ P0 ο€­ gr cos ο€­
 οƒ· cos
2 R rοƒΈ
Morrison, Example 8.2; complete solution steps in
Denn, Process Fluid Mechanics (Prentice Hall, 1980)
around a sphere
(we neglected inertia, i.e.
LHS of Navier-Stokes; this
has consequences)
all the stresses can be
calculated from 𝑣
πœΜƒ
πœ‡ 𝛻𝑣
Π
𝛻𝑣
𝑝𝐼̳
πœΜƒ
(see the usual handout
for stress components)
24
© Faith A. Morrison, Michigan Tech U.
12
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
SOLUTION: Velocity Field for
Creeping Flow around a sphere
• No slip at the walls
of the sphere
• Far from the sphere
the flow does not
feel the presence of
the sphere
(we neglected inertia, i.e.
LHS of Navier-Stokes; this
has consequences)
25
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
To get the force on the
sphere (drag), we ask,
What is the total
z-direction force
on the sphere?
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
𝐹
𝑛⋅Π
𝑑𝑆
flow
26
© Faith A. Morrison, Michigan Tech U.
13
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
To get the force on the
sphere, we ask,
𝑧
π‘Ÿ, πœƒ, πœ™

Let’s
try
What is the total
z-direction force
on the sphere?
𝑦
𝐹
𝑛⋅Π
𝑑𝑆
flow
27
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
𝐹
𝑛⋅Π
𝑑𝑆
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
flow
28
© Faith A. Morrison, Michigan Tech U.
14
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
𝐹
𝑛⋅Π
𝑑𝑆
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
𝑛
?
surface
𝑑𝑆
Π
flow
?
?
?
𝑛⋅Π
?
29
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
SOLUTION: Creeping Flow
around a sphere
What is the total z-direction
force on the sphere?
integrate over
the entire
sphere surface
vector stress on a
microscopic surface of
unit normal 𝑒̂
total vector
force on
sphere
2 
Fο€½
total z-direction
force on the
sphere 𝒆𝒛 ⋅ 𝑭
  eˆ οƒ—  Μƒ ο€­ PI 
r
0 0
total stress
at a point in
the fluid
r ο€½R
R 2 sin d dοͺ
evaluate at the
surface of the
sphere
30
© Faith A. Morrison, Michigan Tech U.
15
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
𝐹
𝑛⋅Π
𝑑𝑆
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
flow
31
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
𝐹
𝑛⋅Π
𝑑𝑆
𝑝 𝑅, πœƒ sin πœƒ
flow
𝐹
𝑅
3πœ‡π‘£ sin πœƒ
2𝑅
π‘‘πœƒπ‘‘πœ™
0
32
© Faith A. Morrison, Michigan Tech U.
16
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
𝑧
π‘Ÿ, πœƒ, πœ™

𝑦
𝐹
𝑛⋅Π
𝑑𝑆
𝑝 𝑅, πœƒ sin πœƒ
flow
𝐹
3πœ‡π‘£ sin πœƒ
2𝑅
𝑅
π‘‘πœƒπ‘‘πœ™
0
Note:
𝑒 , 𝑒 , 𝑒 are a function of πœƒ, πœ™
(see text page 614)
33
© Faith A. Morrison, Michigan Tech U.
Slow flow around a sphere (Stokes Flow)
Force on a sphere (creeping flow limit)
comes from pressure
comes from shear stresses
form drag
eˆz οƒ— F ο€½ Fz ο€½
4
 R 3  g  2 Rv ο‚₯  4 Rv ο‚₯
3
buoyant
force
stationary terms
0 when 𝑣 0
(this is famous)
See Morrison, p613-17
friction drag
kinetic terms
Stokes law:
kinetic force ≡ 𝐹
6πœ‹πœ‡π‘…π‘£
34
© Faith A. Morrison, Michigan Tech U.
17
Lecture 12 F. Morrison CM3110
10/27/2019
Slow flow around a sphere (Stokes Flow)
Force on a sphere (creeping flow limit)
comes from pressure
comes from shear stresses
form drag
eˆz οƒ— F ο€½ Fz ο€½
4
 R 3  g  2 Rv ο‚₯  4 Rv ο‚₯
3
friction drag
buoyant
force
kinetic terms
stationary terms
0 when 𝑣 0
Stokes law:
kinetic force ≡ 𝐹
(this is famous)
6πœ‹πœ‡π‘…π‘£
35
See Morrison, p613-17
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
A real flow problem
(external). What is the speed
of a sky diver?
Back to our
problem:
Drag
(fluid force)
𝑧
π‘₯
Gravity
π‘šπ‘Ž
𝑓
(Morrison, Example 8.1)
36
© Faith A. Morrison, Michigan Tech U.
18
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
A real flow problem
(external). What is the speed
of a sky diver?
π‘šπ‘Ž
0
𝑓
π‘šπ‘”
𝐹
Drag
(fluid force)
𝑧
𝐹
We can get this from the
creeping flow solution
(Stokes flow)
π‘₯
Gravity
π‘šπ‘”
Creeping flow drag:
𝑒̂ ⋅ 𝐹
4
πœ‹π‘… πœŒπ‘”
3
𝐹
6πœ‹πœ‡π‘…π‘£
37
(Morrison, Example 8.1)
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
π‘šπ‘Ž
0
0
0
4πœ‹π‘… 𝜌
3
𝑔
𝑓
π‘šπ‘”
4πœ‹π‘… πœŒπ‘”
3
𝑣
𝜌
π‘₯
𝐹
0
0
6πœ‹π‘…πœ‡π‘£
𝜌 𝐷 𝑔
18πœ‡
0
0
0
From the creeping
flow solution
(see inside front cover)
(Morrison, Example 8.1)
𝑧
Gravity
38
© Faith A. Morrison, Michigan Tech U.
19
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
Gravity
𝑣
𝜌
𝜌 𝐷 𝑔
18πœ‡
𝑧
π‘₯
𝑣
14,000π‘šπ‘β„Ž
From the creeping
flow solution
(Stokes flow, no
inertia)
39
(Morrison, Example 8.1)
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
Gravity
𝑣
𝜌
𝜌 𝐷 𝑔
18πœ‡
From the creeping
flow solution
(Stokes flow, no
inertia)
(Morrison, Example 8.1)
𝑧
π‘₯
𝑣
14,000π‘šπ‘β„Ž
(wrong)
(oh well, nice try)
40
© Faith A. Morrison, Michigan Tech U.
20
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
Gravity
𝜌
𝑣
𝑧
π‘₯
𝜌 𝐷 𝑔
18πœ‡
𝑣
14,000π‘šπ‘β„Ž
(wrong)
From the creeping
flow solution
But, wait! . . .
41
(Morrison, Example 8.1)
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
Gravity
π‘šπ‘Ž
0
π‘šπ‘”
Now, we will talk about external flows
•ideal flows (flow around a sphere)
•real flows (turbulent flow around a sphere, other obstacles)
Strategy for handling real flows:
Dimensional analysis and data
correlations
How did we arrive at correlations?
non-Dimensionalize ideal flow; use to
guide expts on similar non-ideal flows;
take data; develop empirical
correlations from data
What do we do with the correlations? calculate drag - superficial velocity
relations
(Morrison, Example 8.1)
π‘₯
𝑓
Flow around Obstacles
More complicated flows II
𝑧
𝐹
How about if we do
dimensional analysis,
measure data correlations
for non-creeping flow, and
then use the correlations to
determine 𝐹 ?
42
© Faith A. Morrison, Michigan Tech U.
21
Lecture 12 F. Morrison CM3110
10/27/2019
Fast flow around a sphere (dimensional analysis)
•Nondimensionalize eqns of change:
 ο‚Άv* * * * οƒΆ
1 *2 * 1 *
 *  v οƒ—  v οƒ· ο€½ *P* 
 v 
g
 ο‚Άt
οƒ·
Re
Fr

οƒΈ
•Nondimensionalize eqn for 𝐹 ,
define dimensionless
kinetic force f ο€½ C
D
•conclude f=f(Re) or
CD=CD(Re)
Steady flow of an
incompressible, Newtonian
fluid around a sphere
Turbulent Flow
:
ο€½
drag
coefficient
Fz,kinetic
D2  1 2 οƒΆ
 vο‚₯ οƒ·
4 2
οƒΈ
•take data, plot, develop correlations
43
© Faith A. Morrison, Michigan Tech U.
Fast flow around a sphere (dimensional analysis)
Steady flow of an
incompressible, Newtonian
fluid around a sphere
What does this look like
in Creeping flow?
(we have the solution)
Creeping flow:
𝑓
𝐢
𝐹,
Creeping Flow
Stokes law
6πœ‹πœ‡π‘…π‘£
πœ‹π·
1
πœŒπ‘£
4
2
24
𝑅𝑒
From the creeping
flow solution
44
© Faith A. Morrison, Michigan Tech U.
22
Lecture 12 F. Morrison CM3110
10/27/2019
Fast flow around a sphere (dimensional analysis)
Steady flow of an
incompressible, Newtonian
fluid around a sphere
How do we apply to
Turbulent flow?
(we need to take data)
Turbulent flow:
Turbulent Flow
Calculate 𝐢 from terminal velocity of a falling sphere
(see Figure 8.13)
At terminal speed the net
weight is exactly
balanced by the viscous
retarding force.
𝐹
𝑓
𝑓
𝐢
𝐢
𝜌
𝜌
all
measurable
quantities
𝜌 4 𝐷𝑔
3 𝑣
(see Example 8.4)
45
© Faith A. Morrison, Michigan Tech U.
Fast flow around a sphere (dimensional analysis)
•take data, plot, develop correlations
Steady flow of an
incompressible, Newtonian
fluid around a sphere
Creeping Flow
Steady flow of an
incompressible, Newtonian
fluid around a sphere
Turbulent Flow
Data of 𝐢 Re ?
46
© Faith A. Morrison, Michigan Tech U.
23
Lecture 12 F. Morrison CM3110
10/27/2019
Fast flow around a sphere (dimensional analysis)
Steady flow of an incompressible, Newtonian
fluid around a sphere
graphical correlation
24
Re
47
McCabe et al., Unit Ops of Chem
Eng, 5th edition, p147
© Faith A. Morrison, Michigan Tech U.
Fast flow around a sphere (dimensional analysis)
Steady flow of an incompressible, Newtonian
fluid around a sphere
graphical correlation
24
Re
We see the
creeping-flow result
for Re 2
McCabe et al., Unit Ops of Chem
Eng, 5th edition, p147
48
© Faith A. Morrison, Michigan Tech U.
24
Lecture 12 F. Morrison CM3110
10/27/2019
Fast flow around a sphere (dimensional analysis)
correlation equations
creeping
vortices
wake flow
Steady flow of an incompressible, Newtonian
fluid around a sphere
24
𝑅𝑒
18.5𝑅𝑒
𝑓 0.44
𝑓
𝑓
𝑅𝑒
.
2
500
0.10
𝑅𝑒
𝑅𝑒
500
200,000
BSL, p194
•use correlations in engineering practice
•particle settling
(See Denn, Bird et al., Perry’s)
•entrained droplets in distillation columns
•particle separators
•drop coalescence
Dr. Morrison developed a
single, combined correlation
Denn, Process Fluid Mechanics, 1980
Bird, Stewart, Lightfoot, Transport Phenomena, 1960 and 2006
49
© Faith A. Morrison, Michigan Tech U.
Fast flow around a sphere (dimensional analysis)
Morrison Correlation
F. A. Morrison An Introduction to Fluid Mechanics,
Cambridge 2013, Figure 8.13, p625
50
© Faith A. Morrison, Michigan Tech U.
25
Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
Drag
(fluid force)
A real flow problem
(external). What is the speed
of a sky diver?
(Instead of creeping
flow, use π‘ͺ𝑫 Re for
noncreeping flow)
0
0
π‘‰πœŒ
π‘šπ‘Ž
0
𝑔
𝑓
π‘šπ‘”
π‘‰πœŒπ‘”
π‘₯
𝐹
0
0
πœŒπ‘£ 𝐴 𝐢
2
4 𝜌
𝑣
𝑧
Gravity
𝜌 𝐷𝑔
3𝜌𝐢
0
0
0
Applicable in
NON-creeping flow
51
(Morrison, Example 8.5)
© Faith A. Morrison, Michigan Tech U.
More complicated flows II
Drag
A real flow problem
(external). What is the speed
of a sky diver?
(fluid force)
Gravity
𝑣
4 𝜌
𝑧
𝜌 𝐷𝑔
π‘₯
3𝜌𝐢
𝑣
107π‘šπ‘β„Ž
Right!
(or close, anyway)
(Morrison, Example 8.5)
52
© Faith A. Morrison, Michigan Tech U.
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Lecture 12 F. Morrison CM3110
10/27/2019
More complicated flows II
Powerful:
Solving never-before-solved problems.
Left to explore:
• What is non-creeping flow like?
(boundary layers)
• Viscosity dominates in creeping flow, what about
the flow where inertia dominates?
(potential flow)
• What about mixed flows (viscous+inertial)?
(boundary layers)
• What about really complex flows (curly)?
(vorticity; irrotational+circulation)
53
© Faith A. Morrison, Michigan Tech U.
Fast flow around a sphere (dimensional analysis)
F. A. Morrison An Introduction to Fluid Mechanics,
Cambridge 2013, Figure 8.23, p650
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© Faith A. Morrison, Michigan Tech U.
27
Lecture 12 F. Morrison CM3110
10/27/2019
Fast flow around a sphere (dimensional analysis)
a)
c)
b)
d)
e)
55
© Faith A. Morrison, Michigan Tech U.
We have learned
somethings that
are very powerful.
More complicated flows II: From Nice to Powerful
r
Nice:
A
z
cross-section A:
r
z
Learning to solve one particular problem
(or a group of related problems)
L
vz(r)
1. External flows⇒
use drag
coefficient for
real external
flows
fluid
R
Powerful:
Solving never-before-solved problems.
2. In general, “simple” problems can
lead to solutions to “complex”
problems through dimensional
analysis (and data correlation)
End of Exam 3
topics; see
Homeworks to apply
56
© Faith A. Morrison, Michigan Tech U.
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Lecture 12 F. Morrison CM3110
10/27/2019
One more essential topic in Fluid
Mechanics: Boundary Layers
57
© Faith A. Morrison, Michigan Tech U.
29
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