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8/10/2019 Viscous Flows Introduction
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Viscous Flow
MECH5001(P01)
Edgar A. MatidaDepartment of Mechanical &
Aerospace Engineering
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Contents
1. Introduction 2. Equations of Motion 3. Boundary Layer Equations 4. Laminar Boundary Layers 5. Boundary Layer Stability and Transition 6. Turbulent Boundary Layers 7. Calculation of Turbulent Boundary Layers 8. Compressible Boundary Layers 9. 3-D Boundary Layers
10. Current Capabilities
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Objectives
Analytical and numerical methods for viscousflow analysis
Report findings (assignments & term project)
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Evaluation
60% - Homework Assignments (not all equallyweighted)
30% - Term Project
10% - Participation
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Recommended Literature
White, F. M., Viscous Fluid Flow, Third Edition,McGraw-Hill
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Accommodations
Students with disabilities requiring academicaccommodations in this course are encouragedto contact the Paul Menton Centre for Students
with Disabilities (500 University Centre) tocomplete the necessary forms. After registeringwith the Centre, make an appointment to meetwith me in order to discuss your needs at least
two weeks before the first in-class test or CUTVmidterm exam. This will allow for sufficient timeto process your request.
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Viscosity
Viscosity is important when
Velocity is very low (creeping flow)
Velocity gradients are changing rapidly (shear flows),for example
Boundary layers
Jets
Wakes Mixing Layers
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Basics Concepts
A) Solid versus fluid For a solid, stress is proportional to strain
For a fluid, stress is proportional to the rate of strain
For a simple parallel laminar shear flow (Couette flow)
Where is the shear stress, du/dy is the rate of shearstrain, and is the viscosity
yd
ud
Newtonian fluid: linear relationship
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Basic Concepts
B) Continuum
Fluid properties (P, , T, ) are treated ascontinuous even though they reflect molecule
properties Pressure is a measure of molecular momentum
Temperature is a measure of molecular kinetic energy
Continuum approach is valid except at very lowdensities
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Basic Concepts
C) Equation of State for Gases For gases, only 2 of P, T, and are independent
They are linked by the equation of state
The perfect gas law will be used in this course
Where M is the molecular weight of the gas
Kkg
J287
Kkmol
kJ314.8where
airR
RM
RR
TRP
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Basic Concepts
D) No-Slip Condition
Surface irregularities and intermolecular forcesprevent relative motion at a solid surface
Due to viscosity, velocity cannot changediscontinuouslythus a thin boundary layerdevelops over which the velocity varies from the
wall value to the freestream value
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Basic Concepts
Temperature dependence
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Role of Viscosity in High Reynolds
Number Flows
The Reynolds number is the ratio between
inertial ( u2) and viscous stresses ( u/ y) givenby
ULRe
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Role of Viscosity in Low Reynolds
Number Flows
Creeping Flow
Viscous forces are important everywhere in the fluid
Low velocities and high viscosities (liquid metal melts)
Very small length scales (micro-organisms, dispersion
of particulate matter, microfluidic devices)
)1(Re O
ULRe
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Role of Viscosity in High Reynolds
Number Flows
For most problems on a human scale:
Re = 2 x 104: water flow in a 2.5-cm-diameter bathroomsupply pipe
Re = 2 x 105
: for a baseball thrown by a major league pitcher Re = 1 x 107: car at highway speeds
Re = 5 x 107: modest river (Reynolds based on width)
Re = 2 x 108: commercial jet airplane wing (Reynolds based
on chord length)
Re~1012: For a typical atmospheric low pressure system
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Role of Viscosity in High Reynolds
Number Flows
For flows with Reynolds number much largerthan unity, viscous forces will be important onlyin the regions with small length scales or over
very long convective time scales
The length scale ratio (boundary layer thicknessversus height) for a channel flow is
)(Re 2/1OL
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Role of Viscosity in High Reynolds
Number Flows
Viscous forces are important everywhere in aturbulent flow, but only at small scales ofmotion
The ratio of the smallest to the largest lengthscales of a turbulent flow is
)(Re 4/3OL
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Viscous Flow Unsteady Simulation
Velocity field using LES (Large EddySimulation, Ilie, 2005)
2-D simulation using 16 processors during aweek (approximately 1.2 million elements)
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Review
Standard vector algebra
Mass, momentum, and energy conservations
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Vector Algebra
A+B=C, A-B=D
Scalar product
Note that the scalar product of two vectors is a scalar
Vector product (cross product)
Where G is perpendicular to the plane of A and B andin a direction which obeys the right-hand rule
Note that the vector product of two vectors is a vector
cos|||| BABA
GeBABA )sin|||(|
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Orthogonal Coordinate System
A point P in space is located by specifying the threecoordinates (x,y,z)
The point can also be located by the position vector r
Where i, j, and k are unit vectors
If A is a vector, then
kjir zyx
kjiA zyx AAA
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Scalar and Velocity Fields
Pressure, density, and temperature are scalarquantities
A scalar quantity given as a function ofcoordinate space and time t is called a scalarfield
),,,(
),,,(
),,,(
1
1
1
tzyxTT
tzyx
tzyxpp
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Scalar and Velocity Fields
Velocity is a vector quantity
Where
is the vector field for V in the Cartesian space
kjiV zyx VVV
),,,(
),,,(
),,,(
tzyxVV
tzyxVV
tzyxVV
zz
yy
xx
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Scalar and Velocity Fields
The scalar and vector products can be written interms of the components of each vector
Having
AndThen
And
kjA zyx AAA i
kjiB zyx BBB
zzyyxx BABABABA
)()()( xyyxzxxzyzzy
zyx
zyx BABABABABABA
BBB
AAA kji
kji
BA
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Gradient of a Scalar Field
The gradient of p, , at a given point in spaceis defined as a vector such that
Its magnitude is the maximum rate of change of p
per unit length of the coordinate space at the givenpoint
Its direction is that of maximum rate of change of p
at the given point
p
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Gradient of a Scalar Field
The magnitude of is the rate of change of p perunit length in the direction from this point along whichp changes the most.
A line along which sigma p is tangent at every point isdefined as a gradient line.
At any point, the gradient line is perpendicular to theisoline.
p
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Gradient of a Scalar Field
Consider a gradient of p at a point (x,y). The rate ofchange of p per unit length in some arbitrary s directionis
Here n is a unit vector in the s direction
The expression for the gradient of p is
np
ds
dp
),,( zyxpp
kjiz
p
y
p
x
pp
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Divergence of a Vector Field
Consider a fluid element of fixed mass movingalong a streamline with velocity V
As the fluid element moves through space, itsvolume will, in general, change
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Divergence of a Vector Field
The time rate of change of the volume of amoving fluid element of fixed mass, per unitvolume of that element, is equal to thedivergence ofV
kjiVV zyx VVVzyx ),,(
zV
yV
xV zyxV
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Curl of a Vector Field
Consider the same fluid element of fixed massmoving along a streamline with velocity V
It is possible that this fluid element is rotating
with an angular velocity as it translates alongthe streamline
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Curl of a Vector Field
The angular velocity, , is equal to one-half ofthe curl of V
kjiVV zyx VVVzyx ),,(
y
V
x
V
x
V
z
V
z
V
y
V
VVV
zyx
xyzxyz
zyx
kji
kji
V
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Line Integrals
Consider a vector field Consider a curve C connecting two points a and b
Let ds be the elemental length of the curve and n be aunit vector tangent to the curve
Then the line integral from point a to b is
),,( zyxAA
dsnds
a
b dsA
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Line Integrals
If the curve C is closed
Where the counterclockwise direction around Cis positive
CdsA
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Surface Integrals
Consider an open surface S bounded by a closed curve C At point P, let dS be an elemental area of the surface and n
be a unit vector normal to the surface
The orientation of n is in direction according to the right-
hand rule for a movement along C The vector elemental area is dSndS
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Surface Integrals
The surface integral can be defined in three ways
1) Surface integral of a scalar p over the opensurface S (the result is a vector)
2) Surface integral of a vector Aover the opensurface S (the result is a scalar)
3) Surface integral of a vector Aover the opensurface S (the result is a vector)
dSS
p
dSAS
dSA
S
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Surface Integrals
If the surface S is closed (spheres, cubes, etc.), nwill point out of the surface, and
dSS
p
S
dSA
S
dSA
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Relations
Stokes theorem
Divergence theorem
Gradient theorem
dSAdsAS
C)(
VS
dV)( AdSA
VS
dVpp dS
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Models of Fluid
Infinitesimal Fluid Element Infinitesimal fluid element fixed in space with the
fluid moving through it
Infinitesimal fluid element moving along astreamline with the velocity V equal to the local flow
velocity at each point
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