Chap.5 Flow of an Incompressible Ideal Fluidocw.snu.ac.kr/sites/default/files/NOTE/10109.pdf · 5.8...

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Chap.5 Flow of an Incompressible Ideal Fluid

• Ideal fluid (or inviscid fluid) → viscosity=0

→ no friction b/w fluid particles

or b/w fluid and boundary walls

• Incompressible fluid → ρ=const, 0/ =dtdρ

5.1 Euler’s Equation (1-D steady flow)

- pressure force: dpdAdAdpppdA −=+− )(

- body force: gdAdzdsdzgdsdA ρρ −=⎟⎠⎞

⎜⎝⎛−

- acceleration: dsdVV

sVV

tV

dtdVa =

∂∂

+∂∂

==

Newton’s 2nd law: maF =

dsdVdAdsVgdAdzdpdA ρρ =−−

0=++ VdVgdzdpρ

← 1-D Euler’s equation

0=++ dVgVdzdp

γ

02

2

=⎟⎟⎠

⎞⎜⎜⎝

⎛++

gVzpd

γ → const

2

2

=++g

Vzpγ

5.2 Bernoulli’s Equation with Energy and Hydraulic Grade Lines

For 1-D steady flow of incompressible and

uniform density fluid, integration of the Euler

equation gives the Bernoulli equation as follows:

{ {{ { )streamline a (alongconst

2headtotal

headelevation

headvelocity

2

headpressure

==++ Hzg

Vpγ

정지유체 )0( =V : const=+ zpγ

(2.6)

Assumption: The stream tube is infinitesimally

thin, so that it can be assumed to be a streamline.

Hg

Vpz =++=2

EL2

γ

γpz +=HGL

gV2

HGLEL2

=−

5.3 1-D Assumption for Streamtubes of Finite Cross Section

Assumptions:

1. Streamlines are straight and parallel. 2. constant=V across a cross section

(ideal fluid → no friction)

Straight and parallel streamlines

→ No cross-sectional velocity

→ No cross-sectional acceleration

Newton’s 2nd law in x-sectional direction:

0forcebody force pressure =+=cF

(Q no x-sectional acceleration) Read text

22

11 zpzp

+=+γγ

or constant=+ zpγ

across the x-section

Ex) Ideal fluid flowing in a pipe (IP 5.1)

gVzp

gVzp B

BBA

AA

22

22

++=++γγ

(Qsame streamline)

gVzp

gVzp C

CCB

BB

22

22

++=++γγ

( CB VV =Q )

Therefore, the Bernoulli’s equation can be

applied not only between A and B (on the same

streamline) but also between A and C (on

different streamlines) in the pipe shown below.

5.4 Applications of Bernoulli’s Equation

(1) If const≈z , const2

2

≈+g

Vpγ

∴ high velocity → low pressure

(2) Torricelli’s equation

Bernoulli equation b/w 1 and 2:

2

222

1

211

22z

gVpz

gVp

++=++γγ

Using 21 zz = , hp γ=1 , 02 =p , 01 ≈V ,

g

Vh2

22= → ghV 22 = ← Torricelli equation

For application of Torricelli’s equation, see IP

5.2 in text.

Note:

In the reservoir ( 0=V ),

Water surface = EL ( zg

Vp++=

2

2

γ)

= HGL ( zp+=

γ)

= const. in static fluid (reservoir)

= )surfaceat0(|surface =pz Q

(3) Cavitation

Cavitation occurs if vpppp ≤+= atmgageabs

or )( atmgage vppp −−≤

At initiation of cavitation,

)( atmgage vppp −−=

cp (critical gage pressure in text p. 134)

0=

(4) Pitot tube (for measuring velocity)

)EL(22

22

==++=++ Hzg

Vpzg

VpS

SSO

OO

γγ

⎟⎠

⎞⎜⎝

⎛−=γγ

OSO

ppgV 2

can be measured

∴ OV can be known.

(5) Overflow structure (e.g. spillway of a dam)

Pressure and velocity on the spillway surface at 2?

)fluidideal(2 QVVV bs ==

Bernoulli equation at points s and b :

bbb

sss z

gVpz

gVp

++=++22

22

γγ ←

)( bsb zzp −=∴ γ

Continuity: 2211 yVyV =

Bernoulli equation at water surfaces at 1 and 2

szg

Vpyg

Vp++=++

22

222

1

211

γγ

2 equations for 2 unknowns ( 1y and 1V )

→ can be solved for 1y and 1V .

See also § 5.3

const/ =+ zp γ

across a x-section

5.5 Work-Energy Equation

• Addition or extraction of energy by flow machines

- pump: add energy to flow system (or a pump does work on fluid)

- turbine: extract energy from flow system (or fluid does work on a turbine)

• Mechanical work-energy principle

Work done on a fluid system is equal to the change in the mechanical energy (potential + kinetic energy) of the system

dtdE

dtdWdEdW =→=

Note: Work, energy, and heat have the same unit (J=N⋅m)

• Control volume analysis (Reynolds transport theorem)

Reynolds transport theorem for mechanical energy:

⎥⎦

⎤⎢⎣

⎡⎟⎟⎠

⎞⎜⎜⎝

⎛+−⎟⎟

⎞⎜⎜⎝

⎛+=

⎟⎟⎠

⎞⎜⎜⎝

⎛+−⎟⎟

⎞⎜⎜⎝

⎛+=

⎟⎟⎠

⎞⎜⎜⎝

⎛+−⎟⎟

⎞⎜⎜⎝

⎛+=

⋅⎟⎟⎠

⎞⎜⎜⎝

⎛++⋅⎟⎟

⎞⎜⎜⎝

⎛++

⎟⎟⎠

⎞⎜⎜⎝

⎛⎟⎟⎠

⎞⎜⎜⎝

⎛+

∂∂

=

∫∫∫∫

∫∫∫

gVz

gVzQ

AgVg

VzAgVg

Vz

AVVgzAVVgz

dAnvVgzdAnvVgz

VdVgztdt

dE

inout CSCS

CV

22

22

22

22

2

21

1

22

2

11

21

122

22

2

11

21

122

22

2

22

2

γ

ρρ

ρρ

ρρ

ρ

Rate of work done on the flow system ⎟⎠⎞

⎜⎝⎛ = ?

dtdW

1. flow work rate done by pressure force

∫∫ ⎟⎠

⎞⎜⎝

⎛−=−=⋅=

CS

ppQVApVApdAvpγγ

γ 21222111

2. machine work rate done by pumps or turbines

( )tp EEQ −= γ

=tp EE , work rate per unit weight of fluid

3. Shear work rate done by shearing forces on the

control surface = 0 (Q ideal fluid)

⎟⎠

⎞⎜⎝

⎛−+−=∴ tp EEppQ

dtdW

γγγ 21

Since dtdE

dtdW

= , we get

gVzpEE

gVzp

tp 22

22

22

21

11 ++=−+++

γγ

Work-energy equation (per unit weight of fluid)

• Power of pump or turbine

Power = rate of work done

=tp EE , rate of work done per unit weight of fluid

∴ Power of pump or turbine

( ) γQEE tp ×= or (ft⋅lb/s or J/s=W)

total weight of fluid passing the

x-section per unit time

5.6 Euler’s Equations (2-D Steady Flow)

Newton’s 2nd law:

x-direction:

⎟⎠⎞

⎜⎝⎛

∂∂

+∂∂

+∂∂

=⎟⎠⎞

⎜⎝⎛

∂∂

+−⎟⎠⎞

⎜⎝⎛

∂∂

−zuw

xuu

tudxdzdzdx

xppdzdx

xpp ρ

22

zuw

xuu

xp

∂∂

+∂∂

=∂∂

−ρ1

z-direction:

⎟⎠⎞

⎜⎝⎛

∂∂

+∂∂

+∂∂

=−⎟⎠⎞

⎜⎝⎛

∂∂

+−⎟⎠⎞

⎜⎝⎛

∂∂

−zww

xwu

twdxdzgdxdzdxdz

zppdxdz

zpp ρρ

22

gzww

xwu

zp

+∂∂

+∂∂

=∂∂

−ρ1

Continuity: 0=∂∂

+∂∂

zw

xu

3 equations for 3 unknowns ),,( wup

5.7 Bernoulli’s Equation

Euler’s equations:

dxzuw

xuu

xp

×⎟⎠

⎞⎜⎝

⎛∂∂

+∂∂

=∂∂

−ρ1

dzgzww

xwu

zp

×⎟⎠

⎞⎜⎝

⎛+

∂∂

+∂∂

=∂∂

−ρ1

+

( ) gdzzu

xwwdxudz

dzzwwdz

zuudx

xwwdx

xuu

gdzdzzwwdz

xwudx

zuwdx

xuudz

zpdx

xp

+⎟⎠⎞

⎜⎝⎛

∂∂

−∂∂

−+

⎟⎠⎞

⎜⎝⎛

∂∂

+∂∂

+⎟⎠⎞

⎜⎝⎛

∂∂

+∂∂

=

+∂∂

+∂∂

+∂∂

+∂∂

=⎟⎠⎞

⎜⎝⎛

∂∂

+∂∂

−ρ1

Using

dzzpdx

xpdp

∂∂

+∂∂

=

dzzwwdz

zuudx

xwwdx

xuu

dzz

wudxx

wuwud

∂∂

+∂∂

+∂∂

+∂∂

=∂+∂

+∂+∂

=+

2222

)()()(2222

22

we get

ξρ

)(12

)( 22

udzwdxg

dzg

wudg

dp−=+

++

Let ),( 111 zxX = and ),( 222 zxX = .

Integrating from 1X to 2X ,

∫ −=⎟⎟⎠

⎞⎜⎜⎝

⎛+

++ 2

1

2

1

)(12

22 X

X

X

X

udzwdxg

zgwup ξ

γ

If the path between 1X and 2X is a streamline

( dtdxu /= , dtdzw /= ), the RHS vanishes so that

02

2

1

22

=⎟⎟⎠

⎞⎜⎜⎝

⎛+

++

X

X

zgwup

γ

Therefore,

)(const2

22

Czgwup

=++

along a streamline.

But, in general, the constant(C ) may be different for

different streamlines.

On the other hand, for an irrotational flow, 0=ξ , thus

02

2

1

22

=⎟⎟⎠

⎞⎜⎜⎝

⎛+

++

X

X

zgwup

γ

for any two points in the flow. Thus

)const(2

2

Hzg

Vp=++

γ

over the whole flow field for irrotational flow.

5.8 Applications of Bernoulli’s Equation

For irrotational flow of ideal incompressible fluid, the

Bernoulli’s equation applies over the whole flow field

with a single energy line.

zg

VpH ++=2

2

γ

We are interested in p and V at a point.

Exact velocity field → Exact pressure

Difficult to solve

Semi-quantitative (approximate) approach

(1) Tornado or bathtub vortex: Higher pressure and

lower velocity outwards from the center (Read text)

(2) Flow in a curved section in a vertical plane (Fig.

5.12)

- gravity effect >> centrifugal force (low velocity)

- outer wall: sparse streamlines → lower velocity

→ higher pressure

- inner wall: dense streamlines → higher velocity

→ lower pressure

(3) Flow in a convergent-divergent section

At section 2:

Center: sparse streamlines → lower velocity

→ higher pressure

Wall: dense streamlines → higher velocity

→ lower pressure

gVzp

gVzp L

LLU

UU

22

22

++=++γγ

LU VV = → LL

UU zpzp

+=+γγ

UL zz < → LU pp <

If cavitation occurs, it will occur first at the upper wall.

(4) Stagnation points

Sharp corner of a surface → 0=V (stagnation point)

At stagnation point, EL = HGL ( 0=VQ )

(5) Sharp-crested weir

At upstream side, pressure is hydrostatic.

ypA γ=∴ '

At point ''A (stagnation point), g

VypA

2

2'' +=

γ

Pressure distribution above the weir:

Near free streamlines: dense streamlines

→ higher velocity

→ lower pressure

Near center: sparse streamlines → lower velocity

→ higher pressure

Note: 0=p along free streamlines

(6) Flow past a circular cylinder

θcos1 2

2

⎟⎟⎠

⎞⎜⎜⎝

⎛−=

rRUvr , θsin1 2

2

⎟⎟⎠

⎞⎜⎜⎝

⎛+−=

rRUvt

At windward stagnation point:

0=→= rvRr , 0=→= tvπθ

At leeward stagnation point:

0=→= rvRr , 00 =→= tvθ

At surface of the cylinder ( Rr = ):

θsin2,0 Uvv tr −==

gUzpz

gUp

oo

2)sin2(

2

22 θγγ

−++=++∴

),,,( θγ

Uzpfnzpoo=+∴

(7) Flow through an orifice

Streamlines are straight and parallel in the vena

contracta. 0=p everywhere in the jet, but v varies

across the jet (Read page 131).

5.9 Stream Function and Velocity Potential

• Bernoulli equation → Relationship b/w p , V and z

• z is known. Therefore, if V ( u and v ) can be

calculated, then p can be calculated by the Bernoulli

equation.

• Introduce stream function (ψ ) and velocity potential (φ ),

which are related to the velocity field (u and v ).

• PDE for ),( yxψ or ),( yxφ + boundary conditions →

solve for ψ or φ → u and v → p

(1) Stream function

• ψ = flowrate b/w 0 and a streamline

• Flowrate ψ b/w 0 and any point on streamline A is the

same (Q no flow across a streamline) → ψ = const on

streamline A

• Flowrate b/w 0 and streamline ψψ dB += →

)( dqd =ψ = flowrate b/w streamlines A and B

physically

dyy

dxx

vdxudyd∂∂

+∂∂

=−=ψψψ

by definition

xv

yu

∂∂

−=∂∂

=∴ψψ ,

Now 022

=∂∂

∂−

∂∂∂

=∂∂

+∂∂

xyyxyv

xu ψψ

∴ ψ (stream function) satisfies continuity equation for

incompressible fluid.

For irrotational flow, 0=∂∂

−∂∂

=yu

xvξ

or 022

2

2

2=∇=

∂∂

+∂∂ ψψψ

yx ← Laplace equation for ),( yxψ

),( yxψ can be solved with proper boundary conditions.

(2) Velocity potential

Define the velocity potential, ),( yxφ , so as to satisfy

yv

xu

∂∂

−=∂∂

−=φφ ,

Plug in continuity equation:

2

2

2

2

0yxy

vxu

∂∂

−∂∂

−==∂∂

+∂∂ φφ

022

2

2

2

=∇=∂∂

+∂∂

∴ φφφyx

← Laplace equation for ),( yxφ

Vorticity:

022

=∂∂

∂+

∂∂∂

−=∂∂

−∂∂

=xyyxy

uxv φφξ → irrotational flow

∴ φ (velocity potential) is defined only in the

irrotational flow.

Note:

1. irrotational flow = potential flow

(Q velocity potential exists in irrotational flow)

2. ψ satisfies continuity for incompressible fluid

→ For irrotational flow, 02 =∇ ψ

3. φ satisfies irrotationality

→ For incompressible fluid, 02 =∇ φ

(3) Relationship between φ and ψ

⎪⎪⎭

⎪⎪⎬

∂∂

=∂∂

→∂∂

−=∂∂

−=

∂∂

−=∂∂

→∂∂

=∂∂

−=

xyxyv

yxyxu

ψφψφ

ψφψφ

Streamlines ( ψ =const) and equipotential lines

(φ =const) are orthogonal (Read text p. 167-168).

Cauchy-Riemann

Conditions