Aerodynamic Note

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    Introduction Review of prerequisite elements

    Perfect gas

    Thermodynamics laws

    Isentropic flow

    Conservation laws

    Speed of sound Analogous concept

    Derivation of speed of sound Mach number

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    Review of prerequisite elements

    Perfect gas:Equation of state

    For calorically perfect gas

    T

    qds

    =

    RTP =

    v

    p

    vp

    v

    p

    c

    c

    Rcc

    dTcdu

    dTcdh

    RTuhTuu

    =

    +=

    =

    =+==

    )(

    Entropy

    Entropy changes?

    =

    +

    =

    1

    2

    1

    212

    2

    1

    1

    212

    lnln

    lnln

    P

    PR

    T

    Tcss

    RT

    Tcss

    p

    v

    p

    v

    cR

    p

    cR

    v

    P

    P

    c

    ss

    T

    T

    c

    ss

    T

    T

    =

    =

    1

    212

    1

    2

    1

    212

    1

    2

    exp

    exp

    T

    vdPdh

    T

    Pdvduds

    =

    +=

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    Review of prerequisite elementsCont.

    Forms of the 1st law

    dpdhTds

    pddeTds

    ewq

    =+==+

    T

    qds

    The second law

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    Review of prerequisite elements Cont.

    =

    =

    =

    1

    2

    1

    2

    1

    1

    2

    1

    1

    2

    1

    2

    P

    P

    P

    P

    T

    T

    For an isentropic flow

    1

    1

    2

    1

    2

    1

    2

    1

    1

    2

    1

    2

    1

    2

    =

    =

    =

    =

    P

    P

    P

    P

    T

    T

    T

    T

    p

    v

    c

    R

    c

    R

    If ds=o

    constant=

    P

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    Review of prerequisite elements Cont.

    Conservation of mass (steady flow):

    Rate of mass

    enters control

    volume

    Rate of mass

    leaves control

    volume

    =

    1 2dAA

    dVV

    d

    ++

    +

    A

    V

    dx

    flow

    A

    dA

    V

    dV

    A

    dA

    V

    dVd

    VdAAdVVAd

    dAAdVVdVA

    AVAV

    mm

    =

    =++

    =++

    +++=

    =

    =

    0

    0

    ))()((

    222111

    21

    Ifis constant (incompressible):

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    Review of prerequisite elements Cont.

    Conservation of momentum (steady flow):

    Rate momentum

    leaves control

    volume

    Rate momentum

    enters control

    volume

    -

    Net force on

    gas in control

    volume

    =

    ( ) ( )12 VmVmFF p =+

    Euler equation (frictionless flow):

    =+constant

    2

    2

    dpV

    1 2

    dAA

    dVV

    d

    dpp

    +++

    +

    A

    V

    p

    dx

    flow

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    Review of prerequisite elements Cont.

    ++

    +++= e

    eeei

    iii

    CV gzV

    umgzV

    umWQdt

    dE

    22

    22

    heat transfer energy transfer due to mass flowwork transfer

    Basic principle:

    Change of energy in a CV is related to

    energy transferby heat, work, and energy inthe mass flow.

    Conservation of energy for a CV (energy balance):

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    Review of prerequisite elements Cont.

    iep

    pCV

    WWW

    WWW

    =

    +=

    ( )

    ++

    +++=

    +=

    +++

    ++++=

    ++

    +++=

    e

    e

    eei

    i

    iiCV

    CV

    ee

    eeeeii

    iiiiCVCV

    ee

    eeii

    iiiiieeeCVCV

    gzV

    hmgzV

    hmWQdt

    dE

    pvuh

    gzV

    vpumgzV

    vpumWQdt

    dE

    gzV

    umgzV

    umvpmvpmWQdt

    dE

    22

    22

    22

    22

    22

    22

    pvmW

    AVvmAVm

    VFWpAF

    p

    ppp

    =

    ==

    ==

    Most important form

    of 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.

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    Review of prerequisite elements Cont.

    ( )( )

    2

    22

    22

    22

    ieie

    i

    ii

    e

    ee

    VVhhdwdq

    Vhm

    VhmWQ

    +=

    +

    +=

    1 2dVVdhh

    dTT

    ++

    +

    Vh

    T

    dx

    flowTch p=

    For adiabatic flow (no heat transfer)

    and no work:

    For calorically perfect gas (dcp=dcv=0):

    0=+VdVdTcp

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    Conservation of mass

    (compressible flow):

    Conservation of

    momentum

    (frictionless flow):

    Conservation of energy

    (adiabatic):

    021 =++=A

    dA

    V

    dVdmm

    ( ) ( ) 012 =+=+ VdVdP

    VmVmFF p

    ( ) ( ) 02

    22 =++= VdVdTcVVhhdwdq pie

    ie

    Review of prerequisite elements Cont.

    Conservation laws

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    Group Exercises 1

    1. Given that standard atmospheric conditions for air at 150C are a

    pressure of 1.013 bar and a density of 1.225kg, calculate the gasconstant 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=174

    0

    C.

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    Speed of sound

    0=VT

    P

    dVV

    dTT

    d

    dPP

    =+++

    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

    =

    dVaV

    dTT

    d

    dPP

    =+

    ++

    Sound wave

    Sound wave moving

    through stationary gas

    Gas moving through

    stationary sound wave

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    Derivation of speed of sound

    Speed of sound cont.

    ( ) ( )

    adVd

    AdVadaAm

    =

    +==

    ( ) ( )

    adVdP

    amdVamAdPPPA

    ==+

    d

    dpa =

    constant

    1

    2

    1

    2

    =

    =

    P

    PP

    RTP

    a

    P

    d

    dP

    ==

    =

    Conservation of mass

    Conservation of momentum

    Combination of mass and momentum

    For

    isentropic flow

    Finally

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    Mach Number

    M=V/a

    Source of

    disturbance

    Distance traveled =

    speed x time = 4at

    Zone of

    silence

    Region of

    influence

    If M=0

    M1 Supersonic

    M>5 HypersonicDistance traveled = at

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    Mach Numbercont.

    Source of

    disturbance

    If M=0.5

    Original location

    of source ofdisturbance

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    Mach Numbercont.

    Source of

    disturbance

    If M=2

    Original location

    of source of

    disturbanceutut

    ut

    ut

    Mut

    at 1sin ==

    Mach wave:

    Direction

    of motion

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    Normal and Oblique

    Shock

    A shock wave (also called shock front or

    simply "shock") is a type of propagatingdisturbance. Like an ordinary wave, it carries

    energy and can propagate through a medium

    (solid, liquid, gas or plasma) or in some

    cases in the absence of a material medium,through a field such as the electromagnetic

    field.

    http://en.wikipedia.org/wiki/File:Schlierenfoto_Mach_1-2_Pfeilfl%C3%BCgel_-_NASA.jpg
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    Shock waves are characterized by an abrupt,nearly discontinuous change in thecharacteristics of the medium. Across ashock there is always an extremely rapid risein pressure, temperature and density of theflow. In supersonic flows, expansion is

    achieved through an expansion fan. A shockwave travels through most media at a higherspeed than an ordinary wave.

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    Unlike solutions (another kind of nonlinear wave), the

    energy of a shock wave dissipates relatively quickly

    with distance. Also, the accompanying expansionwave approaches and eventually merges with the

    shock wave, partially canceling it out. Thus the sonic

    boom associated with the passage of a supersonic

    aircraft is the sound wave resulting from thedegradation and merging of the shock wave and the

    expansion wave produced by the aircraft.

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    Thus the sonic boom associated with the

    passage of a supersonic aircraft is the soundwave resulting from the degradation and

    merging of the shock wave and the

    expansion wave produced by the aircraft.

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    When a shock wave passes through matter,

    the total energy is preserved but the energywhich can be extracted as work decreases

    and entropy increases. This, for example,

    creates additional drag force on aircraft with

    shocks.

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    Oblique Shock

    An oblique shock wave, unlike a normal shock, isinclined with respect to the incident upstream flow

    direction.

    It will occur when a supersonic flow encounters acorner that effectively turns the flow into itself andcompresses.

    http://en.wikipedia.org/wiki/File:X-15_Model_in_Supersonic_Wind_Tunnel.jpg
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    The upstream streamlines are uniformly deflectedafter the shock wave. The most common way to

    produce an oblique shock wave is to place a wedgeinto supersonic, compressible flow. Similar to anormal shock wave, the oblique shock wave consistsof a very thin region across which nearlydiscontinuous changes in the thermodynamic

    properties of a gas occur. While the upstream anddownstream flow directions are unchanged across anormal shock, they are different for flow across anoblique shock wave.

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    It is always possible to convert an oblique

    shock into a normal shock by a Galileantransformation.

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    EXPANSIONWAVES,RAYLEIGH AND

    FANNO FLOW

    A Prandtl-Meyer expansion fan is a centered expansionprocess, which turns a supersonic flow around a convexcorner.

    The fan consists of an infinite number ofMach waves,diverging from a sharp corner. In case of a smooth corner,these waves can be extended backwards to meet at a point.

    http://en.wikipedia.org/wiki/Convex_sethttp://en.wikipedia.org/wiki/Mach_wavehttp://en.wikipedia.org/wiki/Mach_wavehttp://en.wikipedia.org/wiki/Convex_set
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    Each wave in the expansion fan turns the flowgradually (in small steps). It is physically impossible to

    turn the flow away from itself through a single "shock"wave because it will violate the second law ofthermodynamics. Across the expansion fan, the flowaccelerates (velocity increases) and the Mach numberincreases, while the static pressure, temperature and

    density decrease. Since the process is isentropic, thestagnation properties remain constant across the fan.

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    Prandtl-Meyer Function

    2 1 = (M2) (M1)

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    Rayleigh flow

    Rayleigh flow refers to diabetic flow through a

    constant area duct where the effect of heat addition or

    rejection is considered. Compressibility effects oftencome into consideration, although the Rayleigh flow

    model certainly also applies to incompressible flow.

    For this model, the duct area remains constant and no

    mass is added within the duct. Therefore, unlikeFanno flow, the stagnation temperature is a variable.

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    Rayleigh flow

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    The heat addition causes a decrease in stagnationpressure, which is known as the Rayleigh effect and is

    critical in the design of combustion systems. Heataddition will cause both supersonic and subsonicMach numbers to approach Mach 1, resulting inchoked flow. Conversely, heat rejection decreases asubsonic Mach number and increases a supersonic

    Mach number along the duct. It can be shown that forcalorically perfect flows the maximum entropy occursat M = 1. Rayleigh flow is named after John Strutt, 3rdBaron Rayleigh.

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    Solving the differential equation leads to the relation shownbelow, where T0* is the stagnation temperature at the throatlocation of the duct which is required for thermally choking theflow.

    These values are significant in the design of combustionsystems. For example, if a turbojet combustion chamber has amaximum temperature of T0* = 2000 K, T0 and M at theentrance to the combustion chamber must be selected so

    thermal choking does not occur, which will limit the mass flowrate of air into the engine and decrease thrust. For the Rayleigh flow model, the dimensionless change in

    entropy relation is shown below.

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    Fanno flow

    Fanno flow refers to adiabatic flow through a constant areaduct where the effect of friction is considered.Compressibilityeffects often come into consideration, although the Fanno flowmodel certainly also applies to incompressible flow. For thismodel, the duct area remains constant, the flow is assumed tobe steady and one-dimensional, and no mass is added withinthe duct. The Fanno flow model is considered an irreversibleprocess due to viscous effects. The viscous friction causes theflow properties to change along the duct. The frictional effect ismodeled as a shear stress at the wall acting on the fluid withuniform properties over any cross section of the duct.

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    Fanno flow

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    For a flow with an upstream Mach number greaterthan 1.0 in a sufficiently long enough duct,

    deceleration occurs and the flow can become choked.On the other hand, for a flow with an upstream Machnumber less than 1.0, acceleration occurs and theflow can become choked in a sufficiently long duct. Itcan be shown that for flow of calorically perfect gas

    the maximum entropy occurs at M= 1.0. Fanno flowis named after Gino Girolamo Fanno.

    http://en.wikipedia.org/wiki/Mach_numberhttp://en.wikipedia.org/wiki/Mach_number
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    DIFFERENTIAL EQUATIONS OFMOTION FOR STEADY

    COMPRESSIBLE FLOWS

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    TRANSONIC FLOW OVER WING

    In aerodynamics, the critical Mach number

    (Mcr) of an aircraft is the lowest Mach

    number at which the airflow over a small

    region of the wing reaches the speed of

    sound.

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    Critical Mach Number (Mcr)

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    For all aircraft in flight, the airflow around the aircraft

    is not exactly the same as the airspeed of the aircraft

    due to the airflow speeding up and slowing down totravel around the aircraft structure. At the Critical

    Mach number, local airflow in some areas near the

    airframe reaches the speed of sound, even though the

    aircraft itself has an airspeed lower than Mach 1.0.This creates a weak shock wave. At speeds faster

    than the Critical Mach number:

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    drag coefficient increases suddenly, causing

    dramatically increased drag

    in aircraft not designed for transonic or

    supersonic speeds, changes to the airflow

    over the flight control surfaces lead to

    deterioration in control of the aircraft.

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    In aircraft not designed to fly at the Critical Mach

    number, shock waves in the flow over the wing and

    tail plane were sufficient to stall the wing, makecontrol surfaces ineffective or lead to loss of control

    such as Mach tuck. The phenomena associated with

    problems at the Critical Mach number became known

    as compressibility. Compressibility led to a number ofaccidents involving high-speed military and

    experimental aircraft in the 1930s and 1940s.

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    Drag Divergence Mach Number

    The drag divergence Mach numberis the

    Mach number at which the aerodynamic drag

    on an airfoil or airframe begins to increase

    rapidly as the Mach number continues to

    increase. This increase can cause the drag

    coefficient to rise to more than ten times itslow speed value.

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    The value of the drag divergence Machnumber is typically greater than 0.6; therefore

    it is a transonic effect. The drag divergenceMach number is usually close to, and alwaysgreater than, the critical Mach number.Generally, the drag coefficient peaks at Mach

    1.0 and begins to decrease again after thetransition into the supersonic regime aboveapproximately Mach 1.2.

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    The large increase in drag is caused by the

    formation of a shock wave on the upper

    surface of the airfoil, which can induce flow

    separation and adverse pressure gradients

    on the aft portion of the wing. This effect

    requires that aircraft intended to fly atsupersonic speeds have a large amount of

    thrust.

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    In early development of transonic and supersonicaircraft, a steep dive was often used to provide extraacceleration through the high drag region aroundMach 1.0. In the early days of aviation, this steepincrease in drag gave rise to the popular false notionof an unbreakable sound barrier, because it seemedthat no aircraft technology in the foreseeable futurewould have enough propulsive force or control

    authority to overcome it. Indeed, one of the popularanalytical methods for calculating drag at highspeeds, the Prandtl-Glauert rule, predicts an infiniteamount of drag at Mach 1.0.

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    Two of the important technological advancements thatarose out of attempts to conquer the sound barrierwere the Whitcomb area rule and the supercriticalairfoil. A supercritical airfoil is shaped specifically tomake the drag divergence Mach number as high aspossible, allowing aircraft to fly with relatively lowerdrag at high subsonic and low transonic speeds.These, along with other advancements including

    computational fluid dynamics, have been able toreduce the factor of increase in drag to two or threefor modern aircraft designs

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    swept wing

    A swept wing is a wing platform with a wing

    root to wingtip direction angled beyond

    (usually aft ward) the span wise axis,

    generally used to delay the drag rise caused

    by fluid compressibility.

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    swept wing

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    Unusual variants of this design feature areforward sweep, variable sweep wings , and

    pivoting wings. Swept wings as a means ofreducing wave drag were first used on jetfighter aircraft. Today, they have becomealmost universal on all but the slowest jets

    (such as the A-10), and most faster airlinersand business jets. The four-engine propeller-driven TU-95 aircraft has swept wings.

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    The angle of sweep which characterizes a

    swept wing is conventionally measured along

    the 25% chord line. If the 25% chord line

    varies in sweep angle, the leading edge is

    used; if that varies, the sweep is expressed

    in sections (e.g., 25 degrees from 0 to 50%span, 15 degrees from 50% to wingtip).

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    Transonic Area Rule

    Within the limitations of small perturbation theory, at a given transonicMach number, aircraft with the same longitudinal distribution of cross-sectional area, including fuselage, wings and all appendages will, atzero lift, have the same wave drag.

    Why: Mach waves under transonic conditions are perpendicular toflow.

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    Implication:

    Keep area distribution smooth, constant if possible.

    Else, strong shocks and hence drag result.

    Wing-body interaction leading to shock formation:

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    Observed: cp distributions are such that

    maximum velocity is reached far aft at root

    and far forward at tip.

    Hence, streamlines curves in at the root,

    compress, shock propagates out.

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    Transonic Area Rule

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    Transonic Area Rule

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    In fluid dynamics, potential flow describes

    the velocity field as the gradient of a scalar

    function: the velocity potential..

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    As a result, a potential flow is characterized

    by an irrotational velocity field, which is a

    valid approximation for several applications.

    The irrotationality of a potential flow is due to

    the curl of a gradient always being equal to

    zero

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    In the case of an incompressible flow the velocitypotential satisfies Laplace's equation. However,potential flows also have been used to describecompressible flows. The potential flow approachoccurs in the modeling of both stationary as well asnonstationary flows.

    Applications of potential flow are for instance: theouter flow field for aerofoils, water waves, and

    groundwater flow. For flows (or parts thereof) withstrong vorticity effects, the potential flowapproximation is not applicable.

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    Mach wave

    In fluid dynamics, a Mach wave is a pressure

    wave traveling with the speed of sound

    caused by a slight change of pressure added

    to a compressible flow.

    http://en.wikipedia.org/wiki/File:Schlierenfoto_Mach_1-2_Pfeilfl%C3%BCgel_-_NASA.jpg
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    Mach stem orMach front

    These weak waves can combine in

    supersonic flow to become a shock wave if

    sufficient Mach waves are present at any

    location. Such a shock wave is called a

    Mach stem orMach front.

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    Mach angle

    Thus it is possible to have shock lesscompression or expansion in a supersonic

    flow by having the production of Mach wavessufficiently spaced (cf. isentropiccompression in supersonic flows). A Machwave is the weak limit of an oblique shock

    wave (a normal shock is the other limit). Theypropagate across the flow at the Mach angle

    .

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    where Mis the Mach number. Mach waves can be used in schlieren or

    shadowgraph observations to determine the localMach number of the flow. Early observations by ErnstMach used grooves in the wall of a duct to produceMach waves in a duct, which were then photographedby the schlieren method, to obtain data about the flowin nozzles and ducts. Mach angles may also

    occasionally be visualized out of their condensation inair, as in the jet photograph below.

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    U.S. Navy F/A-18 breaking the sound barrier.

    The white halo is formed by condensed water

    droplets which are thought to result from an

    increase in air pressure behind the shock

    wave(see Prandtl-Glauert Singularity). The

    Mach angle of the weak attached shockmade visible by the halo, is seen to be close

    to arcsine (1) = 90 degrees.