Lecture 6 Potential Flow

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SPC 307 Introduction to Aerodynamics Lecture 6 Potential Flow April 2, 2017 Sep. 18, 2016 1

Transcript of Lecture 6 Potential Flow

Page 1: Lecture 6 Potential Flow

SPC 307Introduction to Aerodynamics

Lecture 6Potential Flow

April 2, 2017

Sep. 18, 20161

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Stream Lines

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Stream Lines

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The Stream Function, (x,y)β€’ Consider the continuity equation for an incompressible 2D flow

β€’ Substituting the clever transformation, (x,y)

β€’ Defined as:

β€’ Gives

This is true for any smoothfunction (x,y)

satisfied be always willmass ofon conservati

unknow one unknows two functionstream using

v

ueq. continuity thesatisfies alwaysit that so

0)()(

xyyxy

v

x

u

0

y

v

x

u

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The Stream Function, β€’ Why do this?

β€’ Single variable replaces (u,v).

β€’ Once is known, (u,v) can be determined.

β€’ Physical significance

1. Curves of constant are streamlines of the flow

2. Difference in between streamlines is equal to

volume flow rate between streamlines

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The Stream Function: Physical Significance

Recall that the streamline equation is given by:

Change in along streamline is zero

1. Curves of constant are streamlines of the flow

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β€’ Let dq represent the volume rate of flow per unit width perpendicular to the x–y plane passing between the two streamlines.

β€’ From conservation of mass we know that the inflow, dq, crossing the arbitrary surface AC must equal the net outflow through surfaces AB and BC. Thus,

β€’ or in terms of the stream function

β€’ Thus, the volume rate of flow, q,

between two streamlines can be

determined by integration to yield

2. Difference in between streamlines is equal to volume flow rate between streamlines

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Prove

β€’ Volume flow rate per unit depth=

β€’ Now, in terms of velocity components

*)Λ†(*)Λ†( drnVareanVdq β€’β€’

jviuV Λ†Λ†

*)Λ†Λ†(*)Λ†Λ†(

β€’β€’

dvdxudy

dxjjvdyiiudq

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Example Stream Functionβ€’ The velocity components in a steady, incompressible, two-dimensional

flow field are

Determine the corresponding stream function and show on a sketch several streamlines.

Indicate the direction of flow along the streamlines.

4xv2yu

(y)fx2(x)fy 2

2

1

2

From the definition of the stream function

xx

vyy

u 42

Cyx 222

For simplicity, we set C = 022

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Example Solution

β€’ Streamlines can now be determined by setting =const. and plotting the resulting curve.

β€’ With the above expression for , the value of at the origin is zero so that the equation of the streamline passing through the origin is

0 = -2x2 + y2

β€’ For

22 yx2

Ξ¨=0

Ξ¨β‰ 0 12/

xy 22

which we recognize as the equation of a hyperbola

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Rate of rotation (angular velocity)

tan 𝛿𝛼 β‰ˆ 𝛿𝛼 =

πœ•π‘£πœ•π‘₯

𝛿π‘₯ 𝛿𝑑

𝛿π‘₯=πœ•π‘£

πœ•π‘₯𝛿𝑑

Consider the rotation about z-axis of the rectangular element x-y

The rotation of the side x

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Rate of rotation (angular velocity)

Angular Velocity of OA

πœ”π‘‚π΄ = lim𝛿𝑑→0

𝛿𝛼

𝛿𝑑= π‘™π‘–π‘šπ›Ώπ‘‘β†’0

πœ•π‘£πœ•π‘₯

𝛿𝑑

𝛿𝑑=πœ•π‘£

πœ•π‘₯

The rotation of the side y

πœ”π‘‚π΅ = lim𝛿𝑑→0

𝛿𝛽

𝛿𝑑= π‘™π‘–π‘šπ›Ώπ‘‘β†’0

πœ•π‘’πœ•π‘¦

𝛿𝑑

𝛿𝑑=πœ•π‘’

πœ•π‘¦

Angular Velocity of OB

tan 𝛿𝛽 β‰ˆ 𝛿𝛽 =

πœ•π‘’πœ•π‘¦

𝛿𝑦 𝛿𝑑

𝛿𝑦=πœ•π‘’

πœ•π‘¦π›Ώπ‘‘

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Rate of rotation (angular velocity)β€’ The rotation of the element about the z axis is defined as the average of the angular velocities of the two mutually perpendicular lines OA and OB. If counterclockwise rotation is considered to be positive, then:

β€’ Average rotation about z-axis

β€’ Average rotation about x-axis,

β€’ Average rotation about y-axis,

β€’ Rotation Vector

y

u

x

vz

2

1

z

v

y

wx

2

1

x

w

z

uy

2

1

k

y

u

x

vj

x

w

z

ui

z

v

y

wkji zyx

Λ†Λ†Λ†2

1Λ†Λ†Λ†

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Rotational and Irrotational Flows

β€’ The vorticity is defined as:

= 2πœ”=

ky

u

x

vj

x

w

z

ui

z

v

y

w Λ†Λ†Λ†

For irrotational flow = = 0

Examples: Rotational flow:

Solid-Body Rotation (Forced Vortex): u = r

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Rotational and Irrotational Flowsβ€’ Examples: Irrotational flow:

β€’ Free Vortex: u = K/r

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Mathematical Representation

β€’ Vorticity is the curl of the velocity vector

β€’ For 3-D vorticity in Cartesian coordinates:

y

u

x

vk

x

w

z

uj

z

v

y

wi

wvu

zyx

kji

V

The horizontal relative vorticity (about z axis) is found byeliminating terms with vertical () components:

β€’

y

u

x

v

wvu

zyx

kji

Vk

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Potential Function, β€’ Irrotational approximation: vorticity

is negligibly small

β€’ In general, inviscid regions are also irrotational, but there are situations where inviscid flow are rotational, e.g., solid body rotation.

What are the implications of irrotational approximation. Look at continuity and momentum equations.Use the vector identity where is a scalar functionSince the flow is irrotational where

is a scalar potential function

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Irrotational Flow Approximation

β€’ Therefore, regions of irrotational flow are also called regions of potential flow.

β€’ From the definition of the gradient operator

β€’ Substituting into the continuity equation for incompressible flow gives:

Cartesian

Cylindrical

zw

yv

xu

, ,

zu

ru

ru zr

,

1 ,

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Irrotational Flow Approximationβ€’ This means we only need to solve 1 linear scalar equation to determine

all 3 components of velocity!

β€’ Luckily, the Laplace equation appears in numerous fields of science, engineering, and mathematics. This means there are well developed tools for solving this equation.

Laplace Equation

Momentum equationIf we can compute from the Laplace equation (which came from continuity) and velocity from the definition , why do we need the NSE? the answer: To compute Pressure.To begin analysis, apply irrotational approximation to viscous term of the incompressible NSE

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Irrotational Flow Approximationβ€’ Therefore, the NSE reduces to the Euler equation for irrotational flow

β€’ Instead of integrating to find P, use vector identity to derive Bernoulli equation

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Irrotational Flow Approximationβ€’ This allows the steady Euler equation to be written as

β€’ This form of Bernoulli equation is valid for inviscid and irrotational flow since we’ve shown that NSE reduces to the Euler equation.

β€’ However, Inviscid

Irrotational ( = 0)35

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Irrotational Flow Approximationβ€’ Therefore, the process for irrotational flow

1. Calculate from Laplace equation (from continuity)

2. Calculate velocity from definition

3. Calculate pressure from Bernoulli equation (derived from momentum equation)

Valid for 3D or 2D

gz

Vpgz

Vp

22

22

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Irrotational Flow Approximation2D Flows

β€’ For 2D flows, we can also use the stream function

β€’ Recall the definition of stream function for planar (x-y) flows

β€’ Since vorticity is zero for irrotational flow,

β€’ This proves that the Laplace equation holds for the stream function and the velocity potential

xv

yu

0

y

u

x

vz

= 2

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Irrotational Flow Approximation2D Flows

β€’ Constant values of : streamlines

β€’ Constant values of : equipotential lines

β€’ and are mutually orthogonal

β€’ is defined by continuity; 2 results from irrotationality

β€’ is defined by irrotationality;2 results from continuity

Flow solution can be achieved by solving either 2 or 2, however, BCs are easier to formulate for

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Relation between and linesβ€’ If a flow is incompressible, irrotational, and two dimensional, the velocity

field may be calculated using either a potential function or a stream function.

β€’ Using the potential function, the velocity components in Cartesian coordinates are

β€’ And

β€’ For lines of constant potential (d = 0), which are called equipotential lines:

β€’ Since a streamline is everywhere tangent to the local velocity, the slope of a streamline, which is a line of constant , is

yv

xu

,

vdyudxdyy

dxx

d

v

u

dx

dy

c

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Relation between and lines

β€’ Comparing equations of slopes yields:

β€’ The slope of an equipotential line is the negative reciprocal of the slope of a streamline.

β€’ Therefore, streamlines ( = constant) are everywhere orthogonal (perpendicular) to equipotential lines ( = constant).

β€’ This observation is not true, however, at stagnation points, where the components vanish simultaneously.

u

v

dx

dy

c

cc dxdydx

dy

)(

1

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Irrotational Flow Approximation2D Flowsβ€’ Similar derivation can be performed for cylindrical coordinates (except for 2 for axisymmetric flow)β€’ Planar, cylindrical coordinates: flow is in (r,) plane

β€’ Axisymmetric, cylindrical coordinates : flow is in (r,z) plane

Planar Axisymmetric

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Irrotational Flow Approximation2D Flows

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Potential flows Visualization

β€’ For such a system, dye injected upstream reveals an approximate potential flow pattern around a streamlined airfoil shape.

β€’ Similarly, the potential flow pattern around a bluff body is shown. Even at the rear of the bluff body the streamlines closely follow the body shape.

β€’ Generally, however, the flow would separate at the rear of the body, an important phenomenon not accounted for with potential theory.

Flow fields for which an incompressible fluid is assumed to be frictionless and the motion to be irrotational are commonly referred to as potential flows.

Paradoxically, potential flows can be simulated by a slowly moving, viscous flow between closely spaced parallel plates.

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Irrotational Flow Approximation2D Flows

β€’ Method of Superposition

1. Since 2 is linear, a linear combination of two or more solutions is

also a solution, e.g., if 1 and 2 are solutions, then (A1), (A+1), (1+2),

(A1+B2) are also solutions

2. Also true for in 2D flows (2 =0)

3. Velocity components are also additive

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Irrotational Flow Approximation2D Flows

β€’ Given the principal of superposition, there are several elementary planar irrotational flows which can be combined to create more complex flows.

β€’ Elementary Planar Irrotational Flowsβ€’ Uniform stream

β€’ Line source/sinkβ€’ Line vortexβ€’ Doublet

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Elementary Planar Irrotational FlowsUniform Stream

β€’ u = U=constant , v = 0, w = 0

β€’ In Cartesian coordinates

β€’ = U x , = U y

β€’ Conversion to cylindrical coordinates can be achieved using the transformation

β€’ = U r cos , = U r sin

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β€’ The flow is an incoming far field flow which is perpendicular to the wall, and then turns its direction near the wall

β€’ The origin is the stagnation point of the flow. The velocity is zero there.

Stagnation Flow

x

y

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Application: Stagnation Flow

β€’ For a stagnation flow,

β€’ Hence,

β€’ Therefore,

β€’ And

β€’ Therefore

2 cos22

222 rB

)yx(B

Byvy

Bxux

,

jByiBx Λ†Λ† V

2sin 2

2rB

Bxy

Byvx

Bxuy

,

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Elementary Planar Irrotational FlowsLine Source/Sink β€’ Let’s consider fluid flowing

radially outward from a line through the origin perpendicular to x-y plane

β€’ from mass conservation:

β€’ The volume flow rate per unit thickness is K

β€’ This gives velocity components

rrv

rrr

Kvr

0

2

and

0 2

vr

Kvr and

K

vr

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Stream function and potential function

2

0r

K

rr

and

By integration:

rln 2

K

2

2

0

K

r

K

r

r

and

By integration:

2

K Equations are for a source/sink

at the origin

K

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Elementary Planar Irrotational FlowsLine (potential) Vortex

β€’ A potential vortex is defined as a singularity about which fluid flows with concentric streamlines

β€’ Vortex at the origin. First look at velocity components

β€’ These can be integrated to give and Equations are for a line vortexat the origin where the arbitrary integration constants are taken to be zero at (r,)=(1,0)

π‘£πœƒ =1

π‘Ÿ

πœ•βˆ…

πœ•πœƒ= βˆ’

πœ•πœ“

πœ•π‘Ÿ=

2πœ‹π‘Ÿ

π‘£π‘Ÿ =πœ•βˆ…

πœ•π‘Ÿ=1

π‘Ÿ

πœ•πœ“

πœ•πœƒ= 0

v

&

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β€’ The potential represents a flow swirling around origin with a constant circulation .

β€’ The magnitude of the flow decreases as 1/r.

Free Vortex

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Line Vortex

β€’ now we consider situation when the stream lines are concentric circles i.e. we interchange potential and stream functions:

ln

K

K r

β€’ circulation

0C C C

ds ds d V

β€’ in case of vortex the circulation is zero along any contour except ones enclosing origin

2

0

( ) 2

ln2 2

Krd K

r

r

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Shape of the free surface

2

2

2

p Vgz const

2 2

1 2

2 2

V Vz

g g

at the free surface p=0:

2

2 28z

r g

π‘£πœƒ =1

π‘Ÿ

πœ•βˆ…

πœ•πœƒ=

2πœ‹π‘Ÿ

Bernolli’s equation

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Elementary Planar Irrotational FlowsLine Vortex

β€’ If vortex is moved to (x,y) = (a,b)

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Source and Sinkβ€’ Consider a source of strength K at (-a, 0) and a sink of K at (a, 0)

β€’ For a point P with polar coordinate of (r, ). If the polar coordinate from (-a,0) to P is (r2, 2) and from (a, 0) to P is (r1, 1),

β€’ Then the stream function and potential function obtained by superposition are given by:

12

12

lnln2

, 2

rrK

K

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Source and Sink

β€’ Hence,

β€’ Since

β€’ We have

β€’ We have

12

1212

tantan1

tantantan

2tan

K

22

sin22tan

ar

ar

K

ar

r

ar

r

cos

sintan

cos

sintan 12 and

22

1- sin2tan

2 ar

arK

πœ“ =𝐾

2πœ‹(πœƒ1βˆ’πœƒ2)

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Source and Sink

β€’ We have

β€’ Therefore,

β€’ The velocity component are:

cos2cossin

cos2cossin

22222

1

22222

2

arararrr

arararrr

cos2

cos2ln

2 22

22

arar

ararK

πœ™ =𝐾

2πœ‹(ln π‘Ÿ1 βˆ’ ln π‘Ÿ2)=

𝐾

2πœ‹(ln

π‘Ÿ2

π‘Ÿ1)

sin2

sin

sin2

sin

2

cos2

cos

cos2

cos

2

2222

2222

arar

r

arar

rKv

arar

ar

arar

arKvr

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Doubletβ€’ The doublet occurs when a source and a sink of the same strength are

collocated the same location, say at the origin.

β€’ This can be obtained by placing a source at (-a,0) and a sink of equal strength at (a,0) and then letting a 0, and K , with Ka kept constant, say aK/2=B

β€’ For source of K at (-a,0) and sink of K at (a,0)

and sin2

tan2 22

1-

ar

arK

cos2

cos2ln

2 22

22

arar

ararK

Under these limiting conditions of a 0, K , we have

cos2

cos2

cos2lnlim

sin2sin2tanlim

22

22

0a

22

1-

0a

r

a

arar

arar

r

a

ar

ar

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Doublet (Summary)

β€’ Adding 1 and 2 together, performing some algebra, Therefore, as a0 and K with aK/2=B then:

B is the doublet strength

ψ = βˆ’π΅π‘ π‘–π‘›πœƒ

π‘Ÿ

πœ™ = π΅π‘π‘œπ‘ πœƒ

π‘Ÿ

The velocity components for a doublet may be found the same way we found them for the source

π‘£π‘Ÿ =πœ•βˆ…

πœ•π‘Ÿ= βˆ’

π΅π‘π‘œπ‘ πœƒ

π‘Ÿ2π‘£πœƒ =

1

π‘Ÿ

πœ•βˆ…

πœ•πœƒ=π΅π‘ π‘–π‘›πœƒ

π‘Ÿ2&

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Examples of Irrotational Flows Formed by Superposition

Superposition of sink and vortex : bathtub vortex

β€’ Superposition of sink and vortex : bathtub vortex

Sink Vortex

Ψ =𝐾

2πœ‹πœƒ βˆ’

Ξ“

2πœ‹ln π‘Ÿ

π‘£πœƒ = βˆ’πœ•πœ“

πœ•π‘Ÿ=

2πœ‹π‘Ÿ

π‘£π‘Ÿ =1

π‘Ÿ

πœ•πœ“

πœ•πœƒ=

𝐾

2πœ‹π‘Ÿ

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Superposition of Source and Uniform Flowβ€’ Assuming the uniform flow U is in x-direction and the source of K stregth at(0,0),

the potential and stream functions of the superposed potential flow become:

πœ“ = π‘ˆβˆžπ‘Ÿπ‘ π‘–π‘›πœƒ +𝐾

2πœ‹πœƒ βˆ… = π‘ˆβˆžπ‘Ÿπ‘π‘œπ‘ πœƒ +

𝐾

2πœ‹ln π‘Ÿ&

π‘£π‘Ÿ =1

π‘Ÿ

πœ•πœ“

πœ•πœƒ= π‘ˆβˆžπ‘π‘œπ‘ πœƒ +

𝐾

2πœ‹π‘Ÿπ‘£πœƒ = βˆ’

πœ•πœ“

πœ•π‘Ÿ= βˆ’π‘ˆβˆžπ‘ π‘–π‘›πœƒ&

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Superposition of Source and Uniform Flowβ€’ Assuming the uniform flow U is in x-direction and the source of K stregth at(0,0),

the potential and stream functions of the superposed potential flow become:

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Source in Uniform Stream

β€’ The velocity components are:

β€’ A stagnation point (vr=v=0) occurs at

Therefore, the streamline passing through the stagnation point when

β€’ The maximum height of the curve is

sin

2cos

U

rv

r

KU

rvr and

22

KUr

U

Kr ss

and

UrK

ss 2

2

Ks

and as rU

Krh 0

2sin

πœ“ = π‘ˆβˆžπ‘Ÿπ‘ π‘–π‘›πœƒ +𝐾

2πœ‹πœƒ

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Source in Uniform Stream

2

mψ

2

mψ

0ψStag. point

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Superposition of basic flows

β€’ Streamlines created by injecting dye in steadily flowing water show a uniform flow.

β€’ Source flow is created by injecting water through a small hole.

β€’ It is observed that for this combination the streamline passing through the stagnation point could be replaced by a solid boundary which resembles a streamlined body in a uniform flow.

β€’ The body is open at the downstream end and is thus called a halfbody.

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Rankine Ovalsβ€’ The 2D Rankine ovals are the results of the superposition of equal strength

(K) sink and source at x=a and –a with a uniform flow in x-direction.

πœ“ = π‘ˆβˆžπ‘Ÿπ‘ π‘–π‘›πœƒ +𝐾

2πœ‹(πœƒ2βˆ’πœƒ1)

βˆ… = π‘ˆβˆžπ‘Ÿπ‘π‘œπ‘ πœƒ +𝐾

2πœ‹(π‘™π‘›π‘Ÿ2βˆ’ln π‘Ÿ1)

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Rankine Ovalsβ€’ Equivalently,

β€’ The velocity components are given by:

β€’ The stagnation

points occur at

where V = 0 with

corresponding s = 0

22

1

22

22

sin2tan

2sin

cos2

cos2ln

2cos

ar

raKrU

raar

raarKrU

sin2

sin

sin2

sin

2

cos2

cos

cos2

cos

2

2222

2222

arar

r

raar

rK

rv

arar

ar

raar

arK

rvr

0

12

1

2

1

2

s

ss

y

aU

K

a

xa

U

Kax

i.e., ,

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Rankine Ovalsβ€’ The maximum height of the Rankine oval is located at

when = s = 0 ,i.e.,

which can only be solved numerically.

20

,r

a

r

K

aU

a

r

a

r

ar

arKrU

o0

2tan1

2

1

02

tan2

2

0

22

0

01

0

or

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Flow around a Cylinder: Steady Cylinderβ€’ Flow around a steady circular cylinder is the limiting case of a Rankine

oval when a0.

β€’ This becomes the superposition of a uniform parallel flow with a doublet in x-direction.

β€’ Under this limit and with B = a.K /2 =constant, the radius of the cylinder is:.

2

1

U

BrR s

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β€’ The stream function and velocity potential become:

β€’ The radial and circumferential velocities are:

sin1sin

sin

cos1cos

cos

2

2

2

2

r

RrU

r

BrU

r

RrU

r

BrU

and

sin1 cos1

2

2

2

2

r

RU

rrv

r

RU

rrvr and

Flow around a Cylinder: Steady Cylinder

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Steady Cylinder

On the cylinder surface (r = R)

Normal velocity (vr) is zero, Tangential velocity (v) is non-zero slip condition.

sin2 0 Uvvr and

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Pressure Distribution on a Circular Cylinderβ€’ Using the irrotational flow approximation, we can calculate and plot the

non-dimensional static pressure distribution on the surface of a circular cylinder of radius R in a uniform stream of speed U .

β€’ The pressure far away from the cylinder is p

β€’ Pressure coefficient:

β€’ Since the flow in the region of interest is irrotational, we use the Bernoulli equation to calculate the pressure anywhere in the flow field. Ignoring the effects of gravity

β€’ Bernoulli’s equation:

β€’ Rearranging Cp Eq. , we get

2

2

1

U

ppC p

2tan

2

22

Up

tconsVp

2

2

2

1

2

1

U

V

U

ppC p

79

Page 80: Lecture 6 Potential Flow

Pressure Distribution on a Circular Cylinder

β€’ We substitute our expression for tangential velocity on the cylinder surface, since along the surface V2 = v2

; the Eq. becomes

β€’ In terms of angle , defined from the front of the body, we use the transformation = - to obtain Cp in terms of angle :

β€’ We plot the pressure coefficient on the top half of the cylinder as a function of angle , solid blue curve.

2

2

22

sin41)sin2(

1

U

UC p

2sin41pC

80

Page 81: Lecture 6 Potential Flow

Pressure distribution on a fishβ€’ Somewhere between the front stagnation point and the aerodynamic

shoulder is a point on the body surface where the speed just above the body is equal to V, the pressure P is equal to P , and Cp = 0. This point is called the zero pressure point

β€’ At this point, the pressure acting normal to the body surface is the same (P = P), regardless of how fast the body moves

β€’ through the fluid.

β€’ This fact is a factor in the location of fish eyes .

81

Page 82: Lecture 6 Potential Flow

β€’ If a fish’s eye were located closer to its nose, the eye would experience an increase in water pressure as the fish swimsβ€”the faster it would swim, the higher the water pressure on its eye would be. This would cause the soft eyeball to distort, affecting the fish’s vision. Likewise, if the eye were located farther back, near the aerodynamic shoulder, the eye would experience a relative suction pressure when the fish would swim, again distorting its eyeball and blurring its vision.

β€’ Experiments have revealed that the fish’s eye is instead located very close to the zero-pressure point where P = P , and the fish can swim at any speed without distorting its vision.

β€’ Incidentally, the back of the gills is located near the aerodynamic shoulder so that the suction pressure there helps the fish to β€œexhale.”

β€’ The heart is also located near this lowest pressure point to increase the heart’s stroke volume during rapid swimming.

Pressure distribution on a fish

82