unit iv radiation
TRANSCRIPT
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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