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