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Compressible Flow Introduction

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Title: Compressible Flow Introduction


1
Compressible Flow Introduction
  • Objectives
  • Indicate when compressibility effects are
    important.
  • Classify flows with Mach Number.
  • Introduce equations for adiabatic, isentropic
    flows.
  • Larry Baxter
  • Ch En 374

2
Flow Classifications
Flow Regime Density Gradient Shock Waves
Incompressible Negligible None
Subsonic Small None
Transonic Significant First appear
Supersonic Significant Significant
Hypersonic Dominant Dominant
3
Property Changes
For isentropic (?s0), constant-heat-capacity
conditions
4
Speed of Sound
C
C
pressure wave ?xn?
5
Speed of Sound in Materials
Most (perfect) gas conditions
High frequency waves (isothermal rather than
isentropic expansion)
Solids and liquids (actually gases as well),
where K is bulk modulus
Bulk modulus, not heat capacity ratio
6
Typical Sound Speeds (STP)
Generally, sound travels faster in solids than
liquids and faster in liquids than gases.
7
Sound Speed vs. Molecular Speed
Molecular theory of gases indicates that the
average molecular speed is
Therefore, the average velocity of a molecule
(speed in any specified direction) is
In the case of a sound wave, molecules dont have
time to adjust their temperatures to the rapid
change in pressure, so their temperature changes
slightly inside the wave. If this change is
completely adiabatic generally a good
assumption the specific heat ratio accounts for
the temperature change. Thus, the speed of sound
is identically equal to the speed at which
molecules travel in any one direction under
conditions of a propagating wave.
8
Sound Travels in Longitudinal Waves
Light, cello strings, and surfing waves are
transverse waves.
Sound travels in a longitudinal or compression
wave.
9
Ideal and Perfect Gases
Ideal Gas
Good approximation for most conditions far from
critical points and at atmospheric pressure or
lower.
Perfect Gas
Reasonable approximation for many gases.
Generally also assume that the gas is
non-dissociating.
10
Gas Flows
Perfect Gas
11
Mach-Number Relations
Isentropic Expansion
Isentropic Expansion
12
Graphical Representation
13
Critical Properties
0.8333 for k 1.4 (air)
0.9129 for k 1.4 (air)
0.5283 for k 1.4 (air)
0.6339 for k 1.4 (air)
14
Blunt Body Flows
Ma 2.2
15
Sonic Flows
Ma 1.7
Ma 3.0
16
Compressible Flow Essentials
  • Know what a Mach number is and the regimes of
    flow as indicated by the Mach number. (Mach
    number is ratio of velocity to the speed of sound
    at the same conditions. Mach numbers of 0.3, 0.8,
    1.2, and 3 separate incompressible, subsonic,
    transonic, supersonic, and hypersonic regimes,
    respectively).
  • Know how pressure, temperature, density, and
    velocity change across a normal shock wave.
    (First three all increase in direction of
    decreasing velocity, with pressure increasing the
    most. Velocity decreases from supersonic to
    subsonic value, with post-shock velocity
    decreasing as pre-shock velocity increases).

17
Supersonic vs. Subsonic Flows
18
Area Changes Differ with Ma
19
Critical Area
20
Mass Flow Relationships
Choked flow
All flows
21
Normal Shock Wave
22
Shock Waves
23
Normal Shock Wave
24
Nozzle Performance
25
Compressible Flow Essentials
  • Be able to explain on a molecular level the
    origin of the changes in pressure, temperature
    and density. (Molecules collide into one another
    or a surface, exchanging kinetic energy for
    pressure or temperature. Ideal gas law still
    applies to give relationship between density,
    pressure, and temperature).
  • Know how streamlining designs differ for
    compressible flows compared to incompressible
    flows. (Leading edges are relatively sharp edges
    rather than rounded corners and heat dissipation
    is a major issue).

26
Three Classes of CFD
  • Finite Difference
  • Original and still widely used formulation for
    CFD describes flow fields as values of velocity
    vectors at discrete points.
  • Finite Volume
  • Close cousin to finite difference, but discrete
    points represent average values of velocities in
    a volume rather than at a point.
  • Finite Element
  • Most commonly used for heat transfer and stress
    calculations in solid bodies rather than fluid
    mechanics (because of stability issues).
  • Much easier to describe general/complex
    geometries than FD/FV techniques.
  • Solves for dependent variable (velocity,
    temperature, stress) with variations across
    element by minimizing an objective function

27
First Derivative FD Formulas
central O(?x2)
backward O(?x)
forward O(?x)
backward O(?x2)
forward O(?x2)
28
First Derivative FV Formulas
General Formula
central O(?x2)
backward O(?x)
forward O(?x)
backward O(?x2)
forward O(?x2)
29
Second Derivative FD Formulas
central O(?x2)
backward O(?x)
forward O(?x)
30
First Derivative FV Formulas
General Formula
central O(?x2)
backward O(?x)
forward O(?x)
31
Navier-Stokes Cartesian Coord.
x component
y component
z component
32
Outline of CFD model
33
Stoker Geometry and Surface Areas
Super heater 2 194 m2 / 2090 ft2
Super heater 1 364 m2 / 3920 ft2
Boiler
Boiler Bank 1181 m2 / 12700 ft2
Super heater 1
Super heater 2
Economizer 330 m2 / 3550 ft2
Econo.
y
Secondary air
8 kg/s, 175 ºC
Secondary air
x
8 kg/s, 175 ºC
z
Spreader stokers
Grate air
9 kg fuel/s
24 kg/s, 175 ºC
34
Computational mesh
35
Cloud (Particle) Trajectories
36
Oxygen Mass Fraction Contours
37
Velocity and Heat Release Vary
38
Initial Deposition Rates Vary
39
Temporal Deposition Variation
40
Gas Temperature Field
41
CFD Essentials
  • Know the distinguishing characteristics of finite
    difference, finite volume, and finite element
    approaches to numerical methods differ.
  • Know where to find (in these notes) common
    algebraic approximations for first and second
    derivatives for FD and FV approaches and the
    accuracy of the approximation.
  • Know (conceptually) how the algebraic
    approximations are substituted into the partial
    differential equations and how these are then
    solved.
  • Recognize that entire careers are dedicated to
    small fractions of CFD problem solving because of
    issues of convergence, stability, non-uniform
    grids, turbulence, etc.
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