Gas Dynamics 1 An Introduction to Compressible Flow
Gas Dynamics 1
An Introduction to Compressible Flow
Gas Dynamics
The Course Outcomes
Understand the definition and fundamental aspects of
compressible flow
Understand the definitions and types of shock and
expansion waves: oblique-shock waves, shock-
expansion interaction, and unsteady expansion waves.
Be able to do simple calculations related to
applications of compressible flow on variations in
geometry
Understand the concept of generalization of subsonic
and supersonic flows
Aims
To provide and introductory to the theories of compressible flows as part ofthe curriculum requirement and as a fundamental background to aerospacepropulsion courses
Gas Dynamics
Course Contents• Introduction to compressible flows
– Definitions and equations of compressible flow, Conservation laws, Sonic velocity and Mach number
• Isentropic Flow (IF)– Equations of isentropic flows and stagnation properties, IF in a converging
and converging-diverging nozzle, and application• Normal shock waves
– Stationary and moving normal shock wave, Working equations and shocks in nozzles, and application
• Oblique shock wave– Working equations, Oblique shock analysis
• Prandt-Meyer Flow– Analysis of Prandtl-Meyer flow – Shock-expansion interaction
• Adiabatic flow– Working equations, nozzle operation, and analysis of Fanno flow
• Flow with heat transfer– Analysis of Rayleigh subsonic & supersonic flow.
Gas Dynamics
Recommended Text booksn Fundamentals of Gas Dynamics by Robert D. Zucker : ISBN 0-916460-12-6n Gas Dynamics by James John and Theo Keith : ISBN 0-13-202331-8n Fundamental of Aerodynamics by John D. Anderson, Jr : ISBN 0-07-
001656-9n Dr Zulfa lecture notes – Gas dynamics
Course Assesment
n Midterm 30%n Final Exam 70%
Gas Dynamics 5
De Laval Nozzle• High Speed flows often seem “counter-intuitive” whenCompared with low speed flows
• Example: Convergent-Divergent Nozzle (De Laval)
In 1897 Swedish Engineer Gustav De Laval designedA turbine wheel powered by 4- steam nozzles
De Laval Discovered that if the steam nozzle first narrowed, and then expanded, the efficiency ofthe turbine was increased dramatically
Furthermore, the ratio of the minimum areato the inlet and outlet areas was critical for achievingmaximum efficiency … Counter to the “wisdom” of the day
flow
Convergent / Divergent Nozzle
Credit: NASA GSFC
Gas Dynamics 6
De Laval Nozzle (cont’d)
• Mechanical Engineers of the 19’th century werePrimarily “hydrodynamicists” .. That is they wereFamiliar with fluids that were incompressible … liquidsand Low speed gas flows where fluid density wasEssentially constant
• Primary Principles are Continuity and Bernoulli’s Law
Gas Dynamics 7
De Laval Nozzle (cont’d)
AeA I At
pIVIAIρ
peVeAeρ
ptVtAtρ
• When Continuity and Bernoulli are applied to a De Laval Nozzle and density is Assumed constant
At Throat
ContinuityBernoulli
• Pressure Drop• Velocity Increases
“classic” Venturi
High Pressure Inlet
Gas Dynamics 8
De Laval Nozzle (cont’d)
AeA I At
pIVIAIρ
peVeAeρ
ptVtAtρ
• When Continuity and Bernoulli are applied to a De Laval Nozzle and density is Assumed constant
At Exit
BernoulliContinuity
• Pressure Increases• Velocity Drops
High Pressure Inlet
Gas Dynamics 9
De Laval Nozzle (concluded)
AeA I At
pIVIAIρ
peVeAeρ
ptVtAtρ
• But De Laval Discovered that when the Nozzle throatArea was adjusted downward until the pressure ratio becamept / pI < 0.5484 -> then the exit Pressure dropped (instead ofRising … compared to the throat pressure)And the exit velocity rose (instead of dropping)… Which is counter to What Bernoulli’s law predicts … he had inadvertently ,,, Generated supersonic flow! …
High Pressure Inlet
• fundamental principle that makes rocket motors possible
Review of prerequisite elements
10
Perfect gasThermodynamics lawsIsentropic flowConservation laws
Gas Dynamics
constant area duct
quasi one-dimensional flow
compressible flow
steady flow
isothermal flow
ideal gas
Diameter (D) 4/2DA π= is a constant
speed (u)
x
u varies only in x-direction
Density (ρ) is NOT a constant
Temperature (T) is a constant
Obeys the Ideal Gas equation
uAm ρ=&Mass flow rate is a constant
Gas Dynamics
Friction factor: (shear stress acting on the wall)
For laminar flow in circular pipes:
where Re is the Reynolds number of the flow defined as follows:
For lamina flow in a square channel:
For the turbulent flow regime:
Re/16=f
µρuD
=ReµD
Am&
=µπD
Dm
24 &
=µπD
m&4=
Re/227.14=f
=
εD
f7.3log0.41
10
Quasi one-dimensional flow is closer to turbulent velocity profile than to laminar velocity profile.
2/2ufw ρτ =
Gas Dynamics
Ideal Gas equation of state:
mRTpV =pressure
volume
mass
specific gas constant(not universal gas constant)
temperature
RTVmp =
Ideal Gas equation of state can be rearranged to give
RTp ρ=
kg/m3 J/(kg.K)
K
Pa = N/m2
Gas Dynamics
Review of prerequisite elements
• Perfect gas:Equation of state
For calorically perfect gas
Tqds δ
=RTP ρ=
v
p
vp
v
p
cc
RccdTcdu
dTcdhRTuh
Tuu
=
+==
=+=
=
γ
)(
Entropy
Entropy changes?
−
=−
+
=−
1
2
1
212
2
1
1
212
lnln
lnln
PPR
TTcss
RTTcss
p
v ρρ
p
v
cR
p
cR
v
PP
css
TT
css
TT
−=
−=
1
212
1
2
1
212
1
2
exp
expρρ
TvdPdh
TPdvduds −
=+
=
Gas Dynamics
Review of prerequisite elements Cont.
Forms of the 1st law
dpdhTdspddeTdsewq
υυ
δδδ
−=+=
=+
Tqds δ
≥
The second law
Gas Dynamics
Review of prerequisite elements Cont.
γ
γγ
γ
ρρ
ρρ
=
=
=
−−
1
2
1
2
1
1
2
1
1
2
1
2
PP
PP
TT
For an isentropic flow
γγ
γ
ρρ
ρρ
1
1
2
1
2
1
2
1
1
2
1
2
1
2
−
−
=
=
=
=
PP
PP
TT
TT
p
v
cR
cR
If ds=o
constant=γρP
Gas Dynamics
Review of prerequisite elements Cont.
Conservation of mass (steady flow):
Rate of massenters controlvolume
Rate of massleaves controlvolume
=
1 2dAAdVVd
+++ ρρ
AVρ
dx
flow
AdA
VdV
AdA
VdVd
VdAAdVVAd
dAAdVVdVA
AVAV
mm
−=
=++
=++
+++=
=
=
0
0
))()((
222111
21
ρρ
ρρρ
ρρρ
ρρ
&&
If ρ is constant (incompressible):
Gas Dynamics
Review of prerequisite elements Cont.
Conservation of momentum (steady flow):
Rate momentumleaves controlvolume
Rate momentumenters controlvolume
-Net force ongas in controlvolume
=
( ) ( )12 VmVmFF p && −=+µ
Euler equation (frictionless flow):
∫ =+ constant2
2
ρdpV
1 2
dAAdVVddpp
++++
ρρ
AV
pρ
dx
flow
Gas Dynamics
Review of prerequisite elements Cont.
++−
+++−= e
eeei
iii
CV gzVumgzVumWQdt
dE22
22
&&&&
heat transfer energy transfer due to mass flowwork transfer
Basic principle:• Change of energy in a CV is related to energy transfer by heat, work,
and energy in the mass flow.
Conservation of energy for a CV (energy balance):
Gas Dynamics
Review of prerequisite elements Cont.
iep
pCV
WWW
WWW&&&
&&&
−=
+=
( )
++−
+++−=
+=
+++−
++++−=
++−
+++−−−=
ee
eeii
iiCVCV
ee
eeeeii
iiiiCVCV
ee
eeii
iiiiieeeCVCV
gzVhmgzVhmWQdt
dE
pvuh
gzVvpumgzVvpumWQdt
dE
gzVumgzVumvpmvpmWQdt
dE
22
22
22
22
22
22
&&&&
&&&&
&&&&&&
pvmWAVvmAVm
VFWpAF
p
ppp
&&&&
&
=
=⇒=
=⇒=
ρ
Most important formof energy balance.
Analyzing more about Rate of Work Transfer:• work can be separated into 2 types:
• work associated with fluid pressure as mass entering or leaving the CV.• other works such as expansion/compression, electrical, shaft, etc.
Work due to fluid pressure:• fluid pressure acting on the CV boundary creates force.
Gas Dynamics
Review of prerequisite elements Cont.
( ) ( )2
22
22
22
ieie
iii
eee
VVhhdwdq
VhmVhmWQ
−+−=−
+−
+=− &&&&
1 2dVVdhhdTT
+++
VhT
dx
flowTch p=
For adiabatic flow (no heat transfer)and no work:
For calorically perfect gas (dcp=dcv=0):
0=+VdVdTcp
Gas Dynamics
Conservation of mass(compressible flow):
Conservation of momentum(frictionless flow):
Conservation of energy(adiabatic):
021 =++→=A
dAVdVdmm
ρρ&&
( ) ( ) 012 =+→−=+ VdVdPVmVmFF p ρµ &&
( ) ( ) 02
22
=+→−
+−=− VdVdTcVVhhdwdq pie
ie
Review of prerequisite elements Cont.
Conservation laws
Gas Dynamics
Exercises 11. Given that standard atmospheric conditions for air at 150C are a
pressure of 1.013 bar and a density of 1.225kg, calculate the gas constant for air. Ans: R=287.13J/kgK
2. The value of Cv for air is 717J/kgK. The value of R=287 J/kgK. Calculate the specific enthalpy of air at 200C. Derive a relation connecting Cp, Cv, R. Use this relation to calculate Cp for air using the information above. Ans: h=294.2kJ/kgK,Cp=1.004kJ/kgK
3. Air is stored in a cylinder at a pressure of 10 bar, and at a room temperature of 250C. How much volume will 1kg of air occupy inside the cylinder? The cylinder is rated for a maximum pressure of 15 bar. At what temperature would this pressure be reached? Ans: V=0.086m2, T=1740C.
Gas Dynamics
Sound Speed and Mach Number
24
Gas Dynamics
Speed of sound
0=VT
Pρ
dVVdTTddPP
=+++
ρρ
Sound wave
Sounds are the small pressure disturbances in the gas around us, analogous to the surface ripples produced when still water is disturbed
aVT
P
=
ρ
dVaVdTTddPP
−=+++
ρρ
Sound wave
Sound wave movingthrough stationary gas
Gas moving throughstationary sound wave
Gas Dynamics
Derivation of speed of sound
Speed of sound cont.
( )( )
adVd
AdVadaAm
=
−+==
ρρ
ρρρ&
( ) ( )adVdP
amdVamAdPPPAρ=
−−=+− &&
ρddpa =
constant
1
2
1
2
=
=
γ
γ
ρ
ρρ
PPP
RTPa
PddP
γρ
γ
ργ
ρ
==
=
Conservation of mass
Conservation of momentum
Combination of mass and momentum
For
isentropic flow
Finally
Gas Dynamics
What is a Mach number?
Definition of Mach number (M):
M ≡Speed of the flow (u)
Speed of sound (c) in the fluid at the flow temperature
Incompressible flow assumption is not valid if Mach number > 0.3
RTc γ=For an ideal gas,
specific heat ratiospecific gas constant (in J/kg.K)absolute temperature of the flow at the point concerned (in K)
Gas Dynamics
For an ideal gas,
Unit of c = [(J/kg.K)(K)]0.5
= [m2/s2]0.5 = m/s
= [kg.(m/s2).m/kg]0.5
M =u u
RTγc=
Unit of u = m/s
= [J/kg]0.5 = (N.m/kg)0.5
Gas Dynamics
Mach Number
M=V/a
Source of disturbance
Distance traveled = speed x time = 4at
Zone of silence
Region of influence
If M=0
M<1 Subsonic
M=1 Sonic
M>1 Supersonic
M>5 Hypersonic Distance traveled = at
Gas Dynamics
Mach Number cont.
Source of disturbance
If M=0.5
Original location of source of
disturbance
Gas Dynamics 31
• As the object approaches the speed of sound, it begins to catch up withthe pressure waves and creates an infinitesimally weak flow discontinuityjust ahead of the aircraft
Mach Number cont.
Gas Dynamics
Mach Number cont.
Source of disturbance
If M=2
Original location of source of
disturbance
utut
utut
Mutat 1sin ==α
Mach wave:
Directionof motion