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    One-Dimensional Flow

    Modern Compressible Flow, Chap 39/30/02; 10/2/02; 10/7/02; 10/9/02

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    One-Dimensional and Quasi-One-

    Dimensional Flow By one-dimensional flow, we mean a flow

    whose properties are functions of only one spatial

    coordinate, typically the streamwise coordinate.Strictly, this requires constant streamtube area.

    But when the variation of area A = A(x) is

    gradual, we often assume the flow is one-

    dimensional. We call it a quasi-one-dimensionalflow.

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    One-Dimensional Flow Equations

    For a steady 1-D flow with constant cross-

    sectional area, no body force, and no shaft

    work,

    2211 uu

    2

    222

    2

    111

    upup

    22

    2

    2

    2

    2

    1

    1

    uhq

    uh

    (3.2)

    (3.5)

    (3.9)

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    Sound Wave

    A sound wave, by definition, is a weak pressure wave with

    negligible friction and thermal conduction effects. In other

    words, the thermodynamic process inside the sound wave

    is isentropic.

    The sound speed, a, can be expressed as

    So the sound speed is a direct measure of compressibility.

    ss

    vp

    a

    (3.18)

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    Sound Speed and Mach Number

    For thermally perfect gas and calorically perfect

    gas,

    At sea level, a = 340.0 m/s = 1117 ft/s

    The Mach number is defined as M=V/a.

    M 1, supersonic flow

    RTp

    a

    (3.19-20)

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    Total (Stagnation) Conditions - 1

    For a steady, inviscid, adiabatic flow with

    negligible body force, we can prove that

    or

    along the streamline.

    0)2/( 2

    Dt

    VhD

    .2/2 constVh

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    Total (Stagnation) Conditions2

    Total Temperature

    Imagine a fluid element in a flow is brought to zero speed

    adiabatically, the resulting temperature is defined as the

    total temperature To, and the corresponding enthalpy as the

    total enthalpy ho.

    For a steady, inviscid, adiabatic flow with negligible body

    force, ho = const. along a streamline. For a calorically

    perfect gas, this implies To = const. along the streamline.

    If all streamlines are from a common freestream, then both

    To and ho are constant throughout the entire flow.

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    Total (Stagnation) Conditions - 3

    Stagnation speed of sound:

    where the subscript o denotes the Mach

    zero condition arrived via an isentropic

    process.

    Total (stagnation) density:

    RTa

    RTp

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    Total (Stagnation) Conditions4

    Total Pressure and Density

    Imagine that a fluid element is brought to

    zero speed isentropically, the resulting

    pressure and density are defined as the totalpressure po and total density o,

    respectively.

    Since an isentropic process is adiabatic, theresulting total temperature is the same as

    that defined before.

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    Characteristic Conditions - 1

    T* If a fluid element is brought to sonic speed

    adiabatically, the resulting temperature is defined

    as T*. The speed of sound at this hypothetical Mach 1 is

    defined as a*, which for thermally perfect gas and

    calorically perfect gas is

    ** RTa

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    Characteristic Conditions - 2

    Characteristic Mach number: V/a*,

    where * denotes the reference Mach 1

    condition arrived via an adiabatic

    process.

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    Energy Equations - 1

    Without Heat Addition

    For 1-D flow without heat addition, the energy

    equation for calorically perfect gas can be

    expressed in alternative forms as follows:

    22

    2

    2

    2

    1 uTcu

    Tc pp

    2121

    2

    2

    2

    2

    2

    1

    2

    1uaua

    2121

    2

    2

    21

    2

    2

    1

    1

    1upup

    (3.22)

    (3.24)

    (3.25)

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    Energy Equations - 2

    Without Heat Addition

    From the previous page, we have

    So for each point in the flow, there is anassociated a*. For an adiabatic flow, a* is

    constant in the flow.

    2*22

    )1(2

    1

    21a

    ua

    (3.26)

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    Energy Equations - 3

    Without Heat Addition

    Similarly, for the stagnation condition, we

    can prove

    opp Tcu

    Tc 2

    2

    2

    211 M

    TTo

    (3.27)

    (3.28)

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    Energy Equations - 4

    Without Heat Addition

    For isentropic, calorically perfect gas,

    12)

    2

    11(

    M

    p

    po

    1

    1

    2)2

    11(

    Mo

    (3.30)

    (3.31)

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    Energy Equations - 5

    Without Heat Addition

    The earlier equations yields,

    1

    2*

    2*

    oo TT

    aa

    1*

    1

    2

    o

    p

    p

    11

    *

    12

    o

    112

    2*

    2

    M

    M

    (3.34)

    (3.36)

    (3.35)

    (3.37)

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    1-D Flow Energy Equations

    (Continued)

    4.1833.012*

    atTT

    o

    )4.1528.0()1

    2(

    1

    *

    atp

    p

    o

    )4.1634.0()1

    2( 1

    1*

    at

    o

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    M*

    )1()1(

    2

    2*

    2

    M

    M

    From the above equation,

    M* = 1 if M =1M* < 1 if M < 1

    M* > 1 if M > 1

    ifMM

    1

    1*

    (3.37)

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    Normal Shock

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    Normal Shocks

    The normal shock wave (and the shock waves ingeneral) is a sudden discontinuity for flow

    properties.

    By definition, a normal shock wave is a shockwave that isperpendicular to the flow. The flowvelocity decreases across the normal shock wave;the flow is supersonic ahead ofthe normal shockwave and subsonic afterthe shock wave.

    The static pressure, temperature and density allincrease across the normal shock wave.

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    Shock Waves

    If the flow is supersonic (relative to a moving

    vehicle), then Vinf> ainfso the sound waves can no

    longer propagate upstream ahead of the vehicle.Instead, they coalesce ahead of the vehicle,

    forming a thin shock wave. See Fig. 4.5.

    The shock wave is usually a few mean free path

    thick, say, 10-5 cm for air at standard conditions.

    The flow is adiabatic across the shock waves.

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    Normal Shock Relations - 1

    Prandtl Relation

    For calorically perfect gas,

    21

    2* uua

    1*

    2

    *

    1MM

    So the Mach number behind the normal shock

    wave is always subsonic.

    or(3.47)

    (3.48)

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    Normal Shock Relations - 2

    For calorically perfect gas with a given ,

    M2, 2/1,p2/p1, and T2/T1 are functions of M1 only:

    2/)1(

    ]2/)1[(12

    1

    2

    12

    2

    M

    MM

    )1(1

    21

    2

    1

    1

    2

    Mp

    p

    2

    1

    2

    1

    1

    2

    )1(2

    )1(

    M

    M

    (3.51) from (3.37) and (3.48)

    (3.57)

    (3.53)

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    Normal Shock Relations - 3

    Furthermore,

    2

    1

    2

    12

    1

    1

    2

    1

    2

    )1(

    )1(21

    1

    21

    M

    MM

    h

    h

    T

    T

    (3.59)

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    Normal Shock Relations - 4

    Substituting eqs. (3.57) and (3.59) into

    we have

    1

    2

    1

    2

    12 lnln p

    p

    RT

    T

    css p

    11

    21ln

    )1(

    )1(211

    21ln

    2

    1

    2

    1

    2

    12

    112

    MR

    M

    MMcss p

    (3.60)

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    Normal Shock Relations - 5

    From the 2nd law, s2>s1 only if M1>1. So the onlyphysically possible process is .

    For ,

    At M1 =1, M2 =2. Then we have Mach wave with no finiteproperty changes across the wave. Also,

    Note that for thermally perfect gas, the changes across thenormal shock wave depend on both M1 and T1. Forchemically reacting gases, they depend on M1, T1 and p1.

    11 M

    1,,,11

    2

    1

    2

    1

    2

    2

    T

    T

    p

    pM

    1

    1M

    6lim,378.0lim 12

    211

    MM M

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    Normal Shock Relations - 6

    For a stationary normal shock, the total

    enthalpy is constant across the shock wave.

    For calorically perfect gas, since h = cpT,the total temperature is constant across the

    normal shock wave:

    021TT

    o (3.61)

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    Normal Shock Relations - 7

    For calorically perfect gas, the total pressure

    decreases across the normal shock:

    If the shock wave is not stationary, neither thetotal enthalpy nor the total temperatures are

    constant across the shock wave.

    R

    ss

    o

    oe

    p

    p/12

    1

    2

    (3.64)

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    Normal Shock Relations - 8

    Hugoniot Equation The normal shock can be viewed as thermodynamic device

    that compresses gas following the Hugoniot equation:

    Since e1 is a function p1 and v1 and e2 a function of p2 and

    v2, for given p1 and v1 upstream of a normal shock, each

    point on the Hugoniot curve (the p2v2 curve represented bythe Hugoniot equation) represents a different shock with a

    different upstream M1. See Figure 3.11.

    )(2

    2121

    12 vvppee

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    1-D Flow with Heat Addition - 1

    Forsupersonic flow in region 1 when heat isadded

    a. Mach number decreases, M2p1d. Total pressure decreases, po2T1

    f. Total temperature increases, To2>To1For cooling, all trends are opposite.

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    1-D Flow With Heat Addition - 2

    Forsubsonic flow in region 1 when heat isadded

    a. Mach number increases, M2>M1b. Velocity increases, u2>u1c. Pressure decreases, p2

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    1-D Flow With Heat Addition - 3Rayleigh Curve (Fig. 3.13)

    The Rayleigh curve is a curve for a give set of upstream

    condition on the Mollier (h-s) diagram for 1-D heat

    addition flow. Each point on the curve corresponds to a

    different value of q added or taken away.

    For the 1-D flow, the effect of heat addition is always to

    drive the Mach number towards 1.

    The maximum entropy location corresponds to the sonic

    location. The flow is said to be choked at this conditionbecause of any further increase in q is not possible without

    a drastic revision of the upstream condition in region 1.

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    1-D Flow With Friction - 1

    Forsupersonic inlet flow, the effect of friction on

    the downstream flow is

    a. Mach number decreases, M2

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    1-D Flow With Friction - 2

    Forsubsonic flow, the effect of friction on

    downstream flow is

    a. Mach number increases, M2>M1b. Velocity increases, u2>u1

    c. Pressure decreases, p2

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    1-D Flow With Friction - 3Fanno Curve (3.15)

    The Fanno curve is a curve on the Mollier (h-s) diagramfor a given upstream condition for different amount offriction (different length of pipe).

    The maximum entropy condition corresponds to the soniccondition at which the flow is choked. Friction alwaysdrive the Mach number towards 1.

    Once the sonic condition is reached at the exit, anyincrease in pipe length is not possible without drastic

    revision of the inlet condition.

    Within the framework of 1-D theory, it is not possible tofirst slow a supersonic flow to the sonic condition and thento further slow it to subsonic speeds also by friction.