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  • 8/10/2019 Unit IV Radiation

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    Spectrum of Electromagnetic Radiation

    104 103

    102

    101

    100

    10-1

    10-2

    10-3

    1011 1012 1013 1014 1015 1016 1017

    m)

    Thermal Radiation(100m to 0.1m)

    Solar (3-0.1m)Radiation

    Visible Light(0.78-0.38)

    (freq) Infrared(1000-0.7m)

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    Radiation

    Radiation emissions propagate in the form ofwaves. Since waves propagate through somemedium, this theory assumes that Universe

    is filled with a hypothetical medium ETHER.

    Waves travel with the speed of light

    1. Wave Theory or Maxwells Classical Theory

    Every wave possesses certain amount ofenergy, a part of which is transferred onbeing impinged by some object in its routeof travel

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    Radiation

    Radiation emissions are in the form of seriesof entities known as quanta.

    Each quanta possesses certain amount ofenergy, which is proportional to its frequencyof emission.

    2. Quantum Theory or Plancks Theory

    Quanta moves with the speed of light andreleases its energy on being impinged bysome object in its route of travel

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    Some Definitions

    Black Body:

    A body which absorbs all incident energy anddoes not transmit and reflects at all, is called

    Black Body. It is also the highest emitter ofradiation

    1;1;0;0

    Examples:Surface coated with lamp black,milk, ice, water, white paper etc

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    Some Definitions

    White Body:A body which reflects the entire radiationfalling on it, is called White Body

    1;0;0;0

    Gray Body:

    The body having same value of emissivity atall wavelengths , which is equal to average

    emissivity, is known as Grey body.

    Generally, all engg metals are grey bodies,for which , when in thermal equilibrium

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    Some Definitions

    Monochromatic Emissive Power (q):

    It is the rate, at which radiant flux is emitted

    with a specific wave length at certain temp; itis dependent emissive power

    It is the rate, at which the radiant flux isemitted from the surface at certain temp

    Emissive Power (q):

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    Some Definitions

    Monochromatic Emissivity ( ):

    It is the ratio of monochromatic emissivepower of a surface to that of black bodywhen both are at same temp for same givenwavelength

    bq

    q

    bq

    q

    Emissivity ():

    It is the ratio of emissive power of a surfaceto that of black body when both at same temp

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    Some Definitions

    Irradiation (G):

    It is the net energy incident/falling on thesurface (need not necessarily be absorbed)

    Radiosity (J):

    It is the net energy leaving the surface.It consists of the radiant energy emitted andenergy reflected out of the incident radiation

    from the surface.J= 1qb + (1-1)G

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    Plancks Law

    Plancks law is based on Quantum theory andit gives the relationship among monochromaticEmissive powerof black body, the absoluteTempof the surface and corresponding

    Wavelengthand is given as:

    014387.0

    &10596.0

    ;/

    1.

    2

    2

    16

    1

    2

    5

    1

    2

    C

    xCwhere

    mW

    e

    Cq

    TCb

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    Plancks LawPlot shows the following:

    qat certain temp firstincreases with , attainssome max value andthen decreases

    For specific wavelength,qof black surfaceincreases with temp

    Most of the thermal radiations lie in wavelengthregion from 0.3 to 10 m

    Wavelength m), at which peak qobtained,decreases with increase in temp

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    Wiens Displacement Law

    Wiens Law gives therelationship betweenthe wavelengths (m) ,at which peak (q)monochromatic emissive

    power is obtained and theabsolute temp andgiven as:

    m.T=0.0029 mK

    Plot and above relation show that the value ofwavelength, at which peak/max monochromaticemissive power is obtained, decreases (displaces/shifts)with increase in surface temperature of the black body.

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    Derivation of Wiens Law

    As per Plancks law,

    1

    2

    25

    1

    TCb

    e

    Cq

    xT

    Cx

    T

    CPutting 22

    1

    2

    55

    5

    2

    1

    x

    b

    eTx

    C

    CqngSubstituti

    5

    2

    155

    1 1...2

    C

    eTxCqOr

    x

    b

    This eqn expressesqof black body asa function of x

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    Derivation of Wiens Law

    For obtaining the wavelength (m) for specified temp,

    at which max qoccurs, we have to differentiatethis equation wrt xand equate it to zero.

    0

    1...2

    52

    155

    1

    C

    eTxC

    dx

    d x

    01..2 155

    2

    5

    1 x

    ex

    dx

    d

    C

    TCOr

    01 15 xexdx

    dOr

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    Derivation of Wiens Law

    01 15

    x

    exdx

    d

    0.1.1.5.1 2541 xxx eexxe

    0

    1.

    15 2

    54

    x

    x

    xe

    exe

    x

    0

    1

    .5

    1

    4

    x

    x

    x

    e

    ex

    e

    x

    05501

    .55

    xe

    e

    exeOr x

    x

    xx

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    Derivation of Wiens Law

    055 xehavenowWe x

    This eqn is satisfied by putting x=4.96

    TCxHence

    296.4,

    0029.0

    96.4

    014387.0 Tm

    mKTTherefore m 0029.0,

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    Stefan Boltzmanns Law

    Kirchhofs Law

    Emissive power of a black body is directlyproportional to fourth power of its absolutetemperature:

    428

    44

    /1067.5

    ;

    KmWxwhere

    TqorTq bb

    When a surface is in thermal equilibrium withits surroundings, the emissivity of the surfaceis equal to its absoptivity

    isThat

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    Solid Angle

    Solid angle subtended bysurface A2at surface dA1(elementary surface)is numerically equal to thearea on a surface of sphere

    with unit radius and centreat elementary area, whichis cut by conical surfacehaving its base as perimeterof A2and vertex at dA1

    Solid angle is measured in Steradians (Sr) anddenoted by symbol

    2

    2

    r

    Ad

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    Solid Angle Between Two Elementary Areas

    Solid Angle subtendedby elementary area dA2at dA1 can be given as:

    222

    r

    CosdAd

    Similarly, solid anglesubtended by area dA1at dA2can be given as:

    2

    11

    r

    CosdAd

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    Intensity of RadiationIntensity of radiation emitted by

    a surface is equal to the radiantenergy passing in a specifieddirection per unit solid angle

    Intensity of radiation varies in different directionsand is max in the direction normal to the surface

    Lambert Cosine Law:Intensity of radiation in any direction is proportionalto the Cosine of the angle made by that directionwith the normal.

    That is, I=InCos; where Inis the intensity (max) inthe normal direction and is the angle made by thatdirection with the normal

    4T

    IIqpoweremissiveTotal nn

    II

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    Shape Factor/Geometric Factor

    Shape factor is defined as the fraction ofenergy emitted by one surface and directlyintercepted by the other.

    1 2

    22121

    1

    121:

    A A r

    dAdACosCosA

    FFactorShape

    Shape Factor depends upon:1. Shape and size of surfaces2. Orientation of surfaces wrt each other3. Distance between the surfaces

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    Relations/ Theorems of Shape Factors

    1. Reciprocal Relation: F12.A1=F21.A2

    2. Enclosure Relation: If nno of surfaces form anenclosure, then: F11+F12+F13+..+F1n=1

    F21+F22+F23+..+F2n=1

    Fn1+Fn2+Fn3+..+Fnn=13. Summation Relation:

    Shape Factor F12between twosurfaces A1and A2is equal

    to the sum of shape factorsF13& F14, if the two areas A3& A4together make up area A2

    413121141312 ,; FFFHoweverFFF

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    Relations/ Theorems of Shape Factors

    4. Shape factor depends on geometry andorientation of surfaces and it does notchange with temp.

    5. Shape Factor wrt itself (F11, F22, F33)means radiation emitted by a portion of asurface falling on the other portion of itselfdirectly

    Example : Shape Factor for concave surface

    Shape factor for convex or Flat surface wrtitself is zero.

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    Radiation Heat Exchange BetweenTwo Parallel Plates

    T11

    T22

    Consider two grey opaque parallel platesmaintained at temperatures T1& T2havingemissivities 1& 2respectively

    For grey bodies, absoptivity = emissivity

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    Radiation Heat Exchange Between Two Parallel Plates

    T11

    T22 q2

    1q2

    2(1-1)q2

    (1-1)q2

    (1-1)(1-2)q2

    Consider radiant flux q2emitted by surface 2.

    Out of q2, a fraction 1q2will be absorbed by surface 1and rest (q21q2) will be reflected towards surface 2

    Out of this, 2(1-1)q2will be absorbed by surface 2

    and balance (1-1)(1-2)q2will be reflected to 1

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    Radiation Heat Exchange Between Two Parallel Plates

    T11

    T22 q2

    1q2

    2(1-1)q2

    (1-1)q2

    (1-1)(1-2)q2

    1(1-1)(1-2)q2

    (1-1)2(1-2)q2

    2(1-1)2(1-2)q2

    (1-1)2(1-2)

    2q2

    1(1-1)2(1-2)

    2q2

    (1-1)3(1-2)

    2q2

    2(1-1)3(1-2)

    2q2

    (1-1)3(1-2)

    3q2

    1(1-1)3(1-2)

    3q2

    This process of absorption and reflection goes onindefinitely, the quantities involved being

    successively smaller.

    Out of this, 1(1-1)(1-2)q2will be absorbed by

    surface 1 and balance (1-1)2(1-2)q2will be reflectedback to 2

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    Radiation Heat Exchange Between Two Parallel Plates

    Thus, total radiant flux absorbed by surface 1out of

    q2emitted by surface 2will be:

    .............11

    1111

    2

    3

    2

    3

    11

    2

    2

    2

    2

    11221121

    q

    qqq

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    Radiation Heat Exchange Between TwoParallel Plates

    2112

    111

    q

    2121

    12

    q

    .....1111111 323

    1

    2

    2

    2

    12112 q

    Similarly, considering radiation flux q1emitted by

    surface 1and fraction out of which absorbed bysurface 2can be given as:

    2121

    21

    q

    2121

    12

    11

    q

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    Radiation Heat Exchange Between Two Parallel Plates

    Assuming T1> T2, net radiant flux absorbed by 2:

    2121

    12

    2121

    2112

    qqq

    4

    222

    4

    111 & TqTqSince

    2121

    4

    221

    4

    11212

    TTq

    111

    21

    42

    41

    12

    TTq

    111

    21

    42

    41

    12

    TTAQOr

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    Electrical Analogy of RadiationShape/Space Resistance:

    Heat flow between two black surfaces at temps T1&T2can be written as:

    121

    4

    2

    4

    14

    2

    4

    111212 1

    FA

    TTTTAFQ

    212121

    4

    2

    4

    1

    11tanRe

    ,

    FAFAcesisEquivalentAnd

    TTDiffPotentialEquivalentHere

    Due to finite dimensions of the surfaces, 100%ofemitted radiation from surface 1does not fall on

    surface 2, hence some part of emitted energy go tosurroundings, thus lost. This loss is conceptuallyexplained to be caused due to resistance offered byfiniteness of dimensions of surfaces and theirorientation. Hence, it is called Shape/Space Resistance

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    Electrical Analogy of Radiation

    Surface Resistance:

    Black body emits max possible radiation and itsemissivity is taken as 1( the datum). However,Grey bodies emit less due to surface properties;and hence their emissivities are taken as less than 1

    (in comparison).Therefore, emission of radiation from grey bodies isalways less than that of black body. This lesseremission is conceptually assumed to be caused dueto a resistance offered by surface of the body as it

    depends on surface property; the emissivity. Thisresistance is called Surface Resistance and given as:

    )2(1

    &)1(1

    22

    2

    11

    1 surfaceofA

    surfacetheofA

    Rsurface

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    Radiation Heat Exchange Between TwoParallel Plates (By Other Method)

    1 2

    1

    T1

    2

    T2

    22

    2

    12111

    1

    4

    2

    4

    112 111

    AFAA

    TTQ

    Since F12=1& A1=A2=A;

    11

    111

    21

    4

    2

    4

    112

    TT

    A

    Q

    111

    21

    4

    2

    4

    112

    TTq

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    R1R2

    T11

    Radiation Heat Exchange Between TwoConcentric Infinitely Long Grey Cylinders

    22

    2

    12111

    1

    4

    2

    4

    112

    111

    AFAA

    TTQ

    F12=1as inner cylinder is completely enclosed by 2

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    Radiation Heat Exchange Between TwoConcentric Infinitely Long Grey Cylinders

    22

    2

    12111

    1

    4

    2

    4

    112 111

    AFAA

    TTQ

    Putting F12=1,

    We have:

    11

    1111

    22

    1

    11

    4

    2

    4

    112

    A

    A

    A

    TTQ

    111

    22

    1

    1

    42

    411

    12

    A

    A

    TTAQ

    A1=2R1L

    A2=2R2L

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    Radiation Heat Exchange Between Two Surfaces

    1

    11

    22

    1

    1

    4

    2

    4

    1112

    A

    A

    TTA

    Q

    This expression is very

    useful as it can be appliedto so many situations:

    1. For heat exchange between two concentric spheres;Only diff will be : A

    1=4R

    1

    2& A2=4R

    2

    2

    2. For eccentric cylinders and spheres

    4. For convex/Flat surface completely enclosed byother body as F12=1and F21=A1/A2

    If enclosure (A2) is very large, A1/A20;Hence, Q = 1A1(T1

    4 - T24)

    3. For heat exchange between two parallel platesas A1 = A2 = A

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    Radiation ShieldIn order to reduce the radiation heat transfer

    rate between two surfaces, a third surface isinserted between them. This surface isknown as Radiation Shield.

    Requirements of Shield (Surface):- Highly reflecting- Lowest emissivity (also absorptivity)- Lowest thickness (thinnest)

    Applications in more effective thermos flasks,for reducing error in temp measurement bythermocouples etc

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    Radiation Shield 1T11

    2T22

    3T33

    Heat Flow Rate

    assuming T1>T2:

    111

    21

    4

    2

    4

    112

    TTq

    Now, a shield having both side emissivity 3isplaced between the surfaces 1& 2.

    On achieving steady state, the shield will

    attain steady temp T3between T1& T2.Since T3remains steady, that means whateverradiation, the shield is receiving from surface 1,the same it is giving out to surface 2.

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    Radiation Shield

    111

    111,

    23

    4

    2

    4

    3

    31

    4

    3

    4

    13213

    TTTTqqHence

    yandxngSubstituti 111

    1

    11

    2331

    y

    T

    x

    T

    x

    T

    y

    T

    y

    TT

    x

    TThaveWe

    4

    2

    4

    1

    4

    3

    4

    3

    4

    2

    4

    3

    4

    3

    4

    1,

    yx

    xTyTTxTyTyTxTOr

    4

    2

    4

    14

    3

    4

    2

    4

    1

    4

    3

    4

    3

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    Radiation Shield

    yxx

    xTyTyTxT

    x

    yx

    xTyTT

    q

    ressionqinTngSubstituti

    4

    2

    4

    1

    4

    1

    4

    1

    4

    2

    4

    14

    1

    13

    13

    4

    3 ;exp

    yxTT

    yxx

    TTxq

    4

    2

    4

    1

    4

    2

    4

    113

    ..

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    Radiation Shield

    On simplification:

    12

    111

    321

    42

    41

    13

    TTq

    Since 3will be very small, hence denominatorof q13will be very large, therefore, there shallbe large reduction of q12to q13.

    1

    111

    11;&

    2331

    4

    2

    4

    113

    TTqyxngSubstituti

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    Radiation Shield

    If 1=

    2

    3= ;

    12

    12

    12

    111

    4

    2

    4

    1

    4

    2

    4

    113

    TTTTq

    shieldonewithtwiceusedismeansThis

    1

    2,

    shieldsnwith

    n

    TTqHence

    1

    21

    ,

    4

    2

    4

    113

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    Radiation Shield

    shieldsnwith

    n

    TTqHence

    12

    1

    ,

    4

    2

    4

    113

    21112

    ;

    12

    4

    2

    4

    113

    qTTq

    shieldONEWith

    Hence, q13now becomes half of q12

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    Radiation Shield

    Home Assignment:

    .&

    &int&

    2&1/

    ,

    1

    2

    1

    11Pr

    21

    2121

    3

    33

    1

    22

    1

    1

    4

    2

    4

    1113

    AAareashaving

    TTtempsatainedmaesemissiviti

    havingSphheresCylindersTWObetween

    placedisemissivityhavingshieldawhen

    A

    A

    A

    A

    TTAQthatveo

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    Q1:Effective temp of a body having an areaof 0.12m2is 527C. Calculate the following:

    a) Rate of radiation energy emissionb) Intensity of normal radiationc) Wavelength of max monochromatic

    emissive power

    Solution:

    a) Total emission of radiation Q=A T4

    WxxxQ 9.278627352712.01067.5 48

    srmWxxTq

    I

    RadiationNormalofIntensityb

    bn ./5.73922735271067.5

    )

    2484

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    c) Wavelength of max monochromatic

    emissive power:

    From Wiens Displacement Law;

    mmx

    T

    mKT

    m

    m

    m

    625.310625.3

    273527

    0029.00029.00029.0

    6

    Answer

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    Q2: A sphere of radius 5cmis concentric with anothersphere. Find the radius of the outer sphere so that

    shape factor of outer sphere wrt inner sphere is 0.6.

    1

    2

    R1

    R2

    Solution:

    A1=4r12

    A2=4r22 F21=0.6

    Since sphere 1is completely enclosedby sphere 2, hence F12=1

    We know that F12.A1=F21.A2

    222

    46.005.041;,

    RxxhavewevaluesngSubstituti

    AnswercmR 45.62

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    Q3: Find F12.

    5

    8

    4 3

    1

    3

    4 2

    5

    6141612 FFF 41

    1

    461

    1

    6 FA

    AF

    A

    A

    43451

    46365

    1

    6 FFA

    AFF

    A

    A

    L1=y/x

    L2=z/x

    65.0

    20

    13&35.0

    20

    7: 2165

    W

    L

    W

    LF

    From graph: F65=0.32

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    Solution (Contd):

    4.020

    8&35.0

    20

    7: 2163 W

    L

    W

    LF

    From graph: F63=0.26

    65.02013&2.0

    204: 2145

    WL

    WLF

    From graph: F45=0.36

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    Solution (Contd):

    4.020

    8

    &2.020

    4

    : 21

    43 W

    L

    W

    L

    F

    From graph: F43=0.33

    43451

    46365

    1

    6

    12 FF

    A

    AFF

    A

    AF

    06.033.036.0205

    20426.032.0

    205

    20712

    x

    x

    x

    xF

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    Q 3: Find out heat transfer rate due to radiationbetween two infinitely long parallel planes. One plane

    has emissivity of 0.4and is maintained at 200C.Other plane has emissivity of 0.2and is maintained at30C. If a radiation shield ( =0.5) is introducedbetween the two planes, find percentage reduction inheat transfer rate and steady state temp of the shield.

    Solution:

    111

    21

    42

    41

    12

    TTq

    2

    448

    12

    /363

    12.0

    1

    4.0

    1273302732001067.5

    mW

    xq

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    Solution (Contd):

    ;insertedisshieldWhen

    12111

    321

    4

    2

    4

    113

    TTq

    2448

    13 /4.248

    15.0

    21

    2.0

    1

    4.0

    1273302732001067.5 mWxq

    %57.31100363

    4.248363

    10012

    1312

    x

    xq

    qq

    reductionPercentage

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    Solution (Contd):

    111

    111

    23

    4

    2

    4

    3

    31

    4

    3

    4

    13213

    TTTTqq

    Under Steady StateConditions, we have:

    12.0

    1

    5.0

    1

    27330

    15.0

    1

    4.0

    1

    273200 44

    3

    4

    3

    4TT

    or

    KT 67.4313

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    Q4: Cryogenic fluid flows through annular space ofinner tube dia of 30mm and outer tube of 90mm dia.

    Surface emissivitiesof inner and outer tubes are 0.2and 0.5, while respective temps are 100and 300K.Find Heat gain rate by the fluid per meter length.Also, percentage reduction in heat gain, if a radiationshield of tubular shape having 45mm diameter and

    emissivitiesof 0.1on inner surface and 0.05on outersurface is introduced between the two tubes.

    Solution:

    1

    23

    111

    22

    1

    1

    4

    2

    4

    1112

    A

    A

    TTAQ

    W

    xx

    xx

    xxxx8

    15.0

    1

    109.0

    103.0

    2.0

    1

    300100103.01067.5 448

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    Solution (Contd):

    With shield:

    11111132313

    1

    22

    1

    1

    4

    2

    4

    1113

    AA

    AA

    TTAQ

    W

    xxxx

    xxxx

    xxxx

    732.1

    105.01

    1.01

    1045.0103.01

    5.01

    109.0103.0

    2.01

    300100103.01067.5 448

    10012

    1312

    xQ

    QQreductionPercentage

    ANSWERx %38.781008

    732.18

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    Q5: A pipe carrying steam having an outside dia of20cmpasses through a large room and is exposed to

    air at temp of 30C. Pipe surface temp is 200C. Findthe heat loss per meter length of pipe both byconvection and radiation taking emissivity of the pipesurface as 0.8.

    Use following relations:Nu=0.53(Gr.Pr)0.25for horizontal pipe

    Air properties:

    Temp C K (W/mK) x106

    (m2/s)

    Pr

    30 0.0267 18.60 0.701

    115 0.0330 24.93 0.687

    200 0.0393 26.00 0.680

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    Solution:

    For Radiation:

    11122

    1

    1

    4

    2

    4

    11

    AA

    TTAQr

    0)()(

    2

    112

    A

    APipeARoomASince

    4

    2

    4

    111 TTAQr

    mW

    xxxxx

    /6.1185

    2733027320012.01067.58.0 448

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    Solution (Contd):

    For Convection:CTmean

    115

    2

    30200

    7

    26

    3

    2

    3

    1053.51093.24273115

    2.030200181.9x

    x

    xxxTLgG r

    67 1038687.01053.5Pr. xxxGr

    k

    hDGrNuselectingHence

    25.0Pr.53.0,

    KmW

    xxh

    2

    25.06

    /87.62.0

    103853.0033.0

    mWxxxTTAhQ wc /8.7333020012.087.6

    mWQQQTotal rc /4.19196.11858.733

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    Q7: Find shape factor for the following wrt itself:a) Cylindrical cavity of dia Dand depth H

    b) Conical hole of dia Dand depth Hc) Hemispherical hole of dia D

    Solution: a) We know F21=1

    As F12A1= F21A2 F12 = A2/A1

    We know that F11 + F12= 1as surfaces 1and 2form enclosure

    1

    21211 11

    A

    AFFHence

    2

    2

    2

    1

    4

    4

    DAAnd

    DDHANow

    DH

    H

    DDH

    DF

    4

    4

    4

    412

    2

    11

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    Solution:

    c) F11+F12=1as surfaces 1& 2

    form enclosureHence F11=1- F12

    221112 AFAFthatknowalsoWe

    1211

    221

    1

    212 FasA

    AFA

    AFHence

    1

    211 1

    A

    AF 2

    2

    2

    2

    14

    &22

    24

    DAD

    D

    ANow

    5.05.015.0

    2

    4112

    2

    1

    2 FHenceD

    D

    A

    A

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    Q7: Two concentric spheres 210mmand 300mmdiameters with the space between evacuated are to

    be used to store liquid air (-153C) in a room at 27C.The surfaces of the spheres are flushed with aluminum=0.03) and latent heat of vaporization of liquid airis 209.35 kJ/kg. Calculate the rate of evaporation ofliquid air per hour. ( Ans. 0.0217 kg/h)

    Solution:

    1

    2

    Liquid O2:21 asgivenissurfaceouterto

    surfaceinnerfromFlowHeat

    111

    22

    1

    1

    42

    411

    12

    A

    A

    TTAQ

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    Solution (Contd):

    WQ

    xx

    Q

    26.1

    103.0

    1

    150.04

    105.04

    03.0

    1

    273272731531067.5105.04

    12

    2

    2

    4482

    12

    )(1 Oxygensurfacebyreceived

    beingheatindicatessignNegative

    hkgx

    xQm

    nevaporatioofRate

    /0217.0100035.209

    360026.1:

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    Q8: The filament of a 75Wlight bulb may beconsidered a black body radiating in to black enclosureat 70C. The filament dia is 0.1mm and length is 5cm.Considering radiation, determine the filament temp.(Ans. 2756C)

    Solution:

    111

    .

    22

    1

    1

    4

    2

    4

    1112

    A

    A

    TTAQ

    Since small A1is enclosed in large A2, hence A1/A2 0

    441834

    2

    4

    11112

    273701067.5105.0101.075

    Txxxxxx

    TTAQ

    )2756(30291 CKT

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    Q9: Determine the heat loss rate by radiation from asteel tube of outside dia 70mmand 3mlong at a tempof 227C, if the tube is located within a square brickconduit of 0.3mside and at 27C. Take emissivity ofsteel=0.79and that for brick=0.93. (Ans. 1589.7W)

    Solution:

    111

    22

    1

    1

    4

    2

    4

    1112

    AA

    TTAQ

    AnswerW

    xx

    xx

    xxxxQ

    7.1589

    193.0

    1

    33.04

    )307.0(

    79.0

    1

    273272732271067.5)307.0( 448

    12

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    Q10: Three hollow thin walled cylinders having dia10cm, 20cmand 30cmare arranged concentrically.

    The temps of the innermost and outermost cylindricalsurfaces are 100Kand 300Krespectively. Assumingvacuum in annular spaces, find the steady state tempattained by the surface having dia of 20cm. Takeemissivities of all surfaces as 0.05.

    (Ans. 269K)

    Solution:

    111

    111

    33

    2

    2

    43

    422

    23

    22

    1

    1

    42

    411

    12

    A

    A

    TTAQ

    A

    A

    TTAQ

    Under steady state:

    12

    3

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    Solution (Contd):

    A1DL=3.14x0.1x1=0.314

    A2=3.14x0.2x1=0.628 A3=3.14x0.3x1=0.942

    1

    11

    1

    11:

    33

    2

    2

    4

    3

    4

    22

    22

    1

    1

    4

    2

    4

    11

    A

    A

    TTA

    A

    A

    TTAhaveWe

    105.0

    1

    942.0

    628.0

    05.0

    1

    300628.0

    105.0

    1

    628.0

    314.0

    05.0

    1

    100314.0 44

    2

    4

    2

    4TT

    nsweKT 2692

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    Gas RadiationGases in many cases are transparent to radiation

    When they absorb and emit radiation, they usuallydo so only in certain narrow wavelength bands.

    Some gases such as N2, O2and other non-polargases are essentially transparent to radiation and

    they do not emit radiation

    While polar gases like CO2, H2O and varioushydrocarbon gases absorb and emit radiation toan appreciable extent in narrow wavelength bands.

    For solids and liquids, radiation occurs from thinlayer (1m to 1mm) of surface, hence it is surfacephenomenon. However, for gases it is not surfacebut volumetric phenomenon.

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    Volumetric Absorption:

    Let a monochromatic beam of radiation having an

    Intensity Iiimpinges on the gas layer of thicknessdxas shown in Fig.

    Decrease in intensity resultingfrom absorption in the layers is

    proportional to the thickness oflayer and intensity of radiation atthat point

    Thus;

    Ii Io

    X=0x dx

    Ix

    tcoefficienabsorptionticmonochromacallediskwhere

    dxIkdI

    ;

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    Volumetric Absorption:

    Integrating this equation gives;

    This is Beers Law and representsexponential decay of radiationintensity

    Ii Io

    X=0x dx

    Ix

    xxI

    iI

    dxkI

    dI

    0

    .

    xk

    i

    x eI

    Ior

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    Gas Radiation

    If gas is non-reflecting, then;

    we know that monochromatic transmissivity;

    1

    1

    henceand

    xke

    xketyAbsorptiviTherefore

    .1

    xkeEmissivitysurfacegreyforAnd

    .1,,

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    Emissivity of CO2, H2O Vapor & Gas

    Emissivity of a gas mixture is a function of total

    pressure (P), partial pressure of a gas(p), gastemperature (T) and characteristic dimension of thesystem; also known as beam length

    LTpPf ,,,

    When the gas mixture is at 1 atm total pressure,the emissivity of CO2 and H2O vapors are given byfollowing empirical relations;

    3

    6.08.0

    5.3

    33.0

    1005.3

    100).(5.3

    TLp

    TLp

    w

    c

    enclosureofareaSurface

    mixtureGasofVolumexL

    astakenisLengthBeamMean

    casespracticalmostFor

    6.3

    ,

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    Heat Exchange between Gas Volume & its Enclosure

    If the enclosure surface is grey, the net heat transfer

    to grey enclosure having emissivity greyis given by:

    2

    1

    grey

    black

    grey

    Q

    Q

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    Error In Temp Measurement By Thermocouple

    For measurement of temp of a hot gas flowing

    through a duct, a thermocouple (TC) is placed indirect contact with gas.

    Tg

    Tw

    h

    Tt Att

    AwThermocouple receives heatfrom gas by convection andtries to attain gas temp.

    As the temp of thermocouplejunction rises, it starts loosingenergy by radiation to ductwall , which is at a lower temp.

    Thus, temp of thermocouple (TC) reduces. Hence,temp recorded by thermocouple (Tt) is always lessthan gas temp (Tg)

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    Error In Temp Measurement By Thermocouple

    When TC attains steady state

    temp Tt, this means heatenergy being received by it byconvection from hot gas attemp Tgis equal to heat beinglost by it by radiation to duct

    which is at Tw

    111

    ..

    44

    ww

    t

    t

    wtt

    tgt

    A

    A

    TTATTAh

    tmeasuremeninerrorisTTwhere

    TTTThhenceA

    ASince

    tg

    wtttg

    w

    t

    44

    .,0

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    Error In Temp Measurement By Thermocouple

    Error (Tg - Tt) inmeasurement can be

    reduced by;

    1) Providing radiationshield around Thermocouple

    2) Reducing emissivity of thermocouplejunction. For this, junction may be coatedwith some material having low emissivitylike Aluminum, Zinc, Chromium, etc

    44

    . wtttg TTTTh

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    Solution (Contd):

    1

    11

    .

    .

    44

    ww

    t

    t

    wtt

    tgt

    A

    A

    TTA

    TTAh

    Since At/Aw0,

    We have; 44.. wttttgt TTATTAh

    448

    27320273500

    200

    1067.56.0

    xx

    TT tg

    KTT

    tmeasurementempinErrorHence

    tg 60

    ,

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    Solution (Contd):

    Assuming At

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    Solution (Contd):

    Now taking up heat transfer from hot gases to TC byConvection and from TC to shield by radiation:

    h.At.(Tg Tt) = .t.At.(Tt4 Ts

    4)

    Substituting:200 (833 Tt) = 5.67x10

    -8x0.6x(Tt4 8154)

    Tt=829K

    Hence, error with shield now becomes:Tg Tt= 833 829 = 4 K