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HEAT AND MASS TRANSFER
HEAT AND MASS TRANSFER
SCOPE OF THE COURSE
ሢ
𝐐
Q
THERMODYNAMIC
ANALYSIS
HEAT TRANSFER
ANALYSIS
Deals with system in equilibrium.
That is to bring a system from one
equilibrium state to another, how
much amount of heat is required.
Evaluates at what rate the change
of state occurs by calculating rate
of heat transfer in Joule/Sec =
Watt.
HEAT AND MASS TRANSFER
SCOPE OF THE COURSE
SN Section/Units Contents
1. Introduction Modes of heat transfer and Governing laws of heat transfer
2. Conduction
Thermal conductivity, Heat conduction in gases, Intepretation Of Fourier's law,
Electrical analogy of heat transfer, Critical radius of insulation, Heat generation in a
slab and cylinder, Fins, Unsteady/Transient conduction
3. Convection
Forced convection heat transfer, Reynold’s Number, Prandtl Number, Nusselt
Number, Incompressible flow over flat surface, HBL, TBL, Forced convection in flow
through pipes and ducts, Free/Natural convection
4. Radiation
Absorbtivity, Reflectivity, Transmitivity, Laws of thermal radiation, Shape factor,
Radiation heat exchange
5. Heat Exchangers
Types of heat exchangers, First law of thermodynamics, Classification of heat
exchangers, LMTD for parallel and counter flow, NTU, Fouling factor.
HEAT AND MASS TRANSFER
MODES OF HEAT TRANSFER
MODES
Conduction Convection Radiation
HEAT AND MASS TRANSFER
MODES OF HEAT TRANSFER
Conduction – The mode of heat transfer which generally (mark the word) occurs in a solid
body due to temperature difference associated with molecular lattice’s vibrational energy
as well by transfer of free electrons.
This is the reason behind why all electrically good conductors are also in general a good
conductor of heat as well. Viz the presence of abundant FREE electrons. EXCEPTION = Diamond
HT
LT
HEAT AND MASS TRANSFER
MODES OF HEAT TRANSFER
HEAT AND MASS TRANSFER
MODES OF HEAT TRANSFER
Convection – The mode of heat transfer which generally occurs between solid surface and
the surrounding fluid due to temperature difference associated with macroscopic bulk
motion of the fluid transporting thermal energy.
Natural Convection Forced Convection
HEAT AND MASS TRANSFER
MODES OF HEAT TRANSFER
Radiation – All matter with a temperature greater than absolute zero (viz 0 K)emits
thermal radiation. The rate of emission occurs in form of electromagnetic waves which
can propagate even through the vacuum !
Radiation is the mode of heat transfer which does not require any material medium and
occurs at electromagnetic wave propagation travelling with speed of light.
HEAT AND MASS TRANSFER
GOVERNING LAWS OF HEAT TRANSFER
1. Fourier’s law of conduction – The law states that the rate of heat transfer by
conduction along a direction (given) is directly proportional to the temperature gradient
along that direction and is also proportional to the area of heat transfer lying
perpendicular to the direction of heat transfer.
Qx ο‚΅ -
𝑑𝑇
𝑑π‘₯
Qx ο‚΅ A
Qx = K A (
𝑑𝑇
𝑑π‘₯
)
HEAT AND MASS TRANSFER
K = Thermal conductivity
GOVERNING LAWS OF HEAT TRANSFER
2. Newton’s law of cooling (For Convection) – The law states that the rate of heat transfer
by convection between a solid body and surrounding fluid is directly proportional to the
temperature difference between them and is also directly proportional to the area of
contact or area of exposure between them.
Qconv ο‚΅ (Tw - Tο‚₯)
Qconv ο‚΅ A
Qconv = h A (Tw - Tο‚₯ )
HEAT AND MASS TRANSFER
h = Heat transfer coefficient
of convection.
GOVERNING LAWS OF HEAT TRANSFER
HEAT AND MASS TRANSFER
K = Thermal conductivity = Property of
the material
h = Heat coefficient for convection
ο‚Ή Property of the material
In forced convection h = f (v,D,,,Cp,k)
In free convection h = f (g,,,L,,,Cp,k)
GOVERNING LAWS OF HEAT TRANSFER
HEAT AND MASS TRANSFER
Ranges of β€œh”
SN Convection Value (Watt/m2K)
1 Free convection in gases. 3 - 25
2 Forced convection in gases. 25 – 400
3 Free convection in liquids. 250 – 600
4 Forced convection in liquids. 600 – 4000
5 Condensation heat transfer. 3000 – 25000
6 Boiling heat transfer. 5000 - 50000
GOVERNING LAWS OF HEAT TRANSFER
3.Stefan-Boltzman’s law of Radiation – The law states that the radiation energy emitted
from the surface of a black body (per unit time, per unit area) is directly proportional to
the 4th power of the absolute temperature of the black body.
Eb ο‚΅ T4
β€œT” is in Kelvin
Eb =  T4
HEAT AND MASS TRANSFER
 = Stefan-Boltzman constant
= 5.67 X 10-8 Watt/m2K
THERMAL CONDUCTIVITY (K)
HEAT AND MASS TRANSFER
It is a thermo-physical property of a material which tells about the ability of material to
allow heat energy to get conducted through the material more rapidly/quickly.
Insulators (a substance which does not readily allow the passage of heat) have very low
thermal conductivity and hence prevents the conduction heat transfer rate.
SN Material (Insulators) K (Watt/mK)
1. Asbestos 0.2
2. Refractory bricks 0.9
3. Glass wool 0.075
4. Polyurethane foam 0.02
HEAT CONDUCTION IN GASES
HEAT AND MASS TRANSFER
Heat conduction occurs in gases by molecular momentum transfer when high velocity and
high temperature molecules collides with the low velocity low temperature molecules.
However, in general gases are bad conductor of heat.
Kair =0.026 w/mK
HEAT CONDUCTION IN GASES
HEAT AND MASS TRANSFER
As the temperature of gases increase, their thermal conductivity also increases. This is
because at high temperature of gases, increased molecular activity may result in more no
of collisions per unit time and hence more momentum transfer rate & hence more
thermal heat conductivity.
K
T (Celsius)
HEAT AND MASS TRANSFER
K = 8.43 w/mK
HIGHEST
A Thermometric
Fluid.
Low vapour
Pressure
HEAT CONDUCTION IN GASES
FOURIER’S LAW INTEPRETATION
HEAT AND MASS TRANSFER
ASSUMPTIONS :-
❖ Steady state heat
transfer conditions.
T ο‚Ή f (Time)
❖ One dimensional
heat conduction.
T = f (x)
❖ Uniform/Constant
value of β€œK”
BOUNDARY CONDITIONS
At x = 0, T = T1
At x = b, T = T2
FOURIER’S LAW INTEPRETATION
HEAT AND MASS TRANSFER
ΰΆ±
π‘₯=0
π‘₯=𝑏
π‘žπ‘₯ 𝑑π‘₯ = ΰΆ±
𝑇1
𝑇2
βˆ’πΎπ΄ 𝑑𝑇
To satisfy steady state conditions,
qx ο‚Ή f (x)
Viz qx = qx+dx
qx X b = KA (T1-T2)
qx =
𝑲𝑨 (π‘»πŸ
βˆ’π‘»πŸ
)
𝒃
&
qx
𝑨
=
𝑲 (π‘»πŸ
βˆ’π‘»πŸ
)
𝒃
ELECTRICAL ANALOGY OF HEAT TRANSFER
HEAT AND MASS TRANSFER
Electrical Thermal
i (Ampere) q (Watt)
V (Volts) T (Celsius/Kelvin)
Relectrical RThermal
i q
Relectrical RThermal
V T
Relectrical =
V
𝑖
Ohms RThermal=
𝑇
π‘ž
K/Watt
ELECTRICAL ANALOGY OF HEAT TRANSFER
HEAT AND MASS TRANSFER
(RTh)Conduction =
𝑇1
βˆ’π‘‡2
π‘ž
=
𝑏
𝐾𝐴
CONDUCTION HEAT TRANSFER THROUGH A COMPOSITE SLAB
HEAT AND MASS TRANSFER
T1 T2 T3
q
RTh(1-2) =
𝑏1
𝐾1
𝐴
RTh(2-3) =
𝑏2
𝐾2
𝐴
RTh(1-3) =
𝑏1
𝐾1
𝐴
+
𝑏2
𝐾2
𝐴
RTh(1-3) =
𝑇
π‘ž
=
𝑇1
βˆ’π‘‡3
π‘ž
Rate of conduction heat
Transfer β€œq” is given by -
q =
𝑇
RTh(1βˆ’3)
=
𝑇1
βˆ’π‘‡3
𝑏1
𝐾1
𝐴
+
𝑏2
𝐾2
𝐴
π‘ž
𝐴
= π»π‘’π‘Žπ‘‘ 𝑓𝑙𝑒π‘₯ =
𝑇1 βˆ’ 𝑇3
𝑏1
𝐾1
+
𝑏2
𝐾2
NUMERICAL
HEAT AND MASS TRANSFER
Calculate the value of thermal conductivity of insulator in the composite slab as shown in the
adjoining figure.
500 K 360 K
q = 10,000 w/m2
20
1000𝑋10𝑋𝐴
1
1000𝑋𝐾𝑋𝐴
20
1000𝑋10𝑋𝐴
NUMERICAL
HEAT AND MASS TRANSFER
500 K 360 K
q/A = 10,000 w/m2
20
1000𝑋10𝑋𝐴
1
1000𝑋𝐾𝑋𝐴
20
1000𝑋10𝑋𝐴
Heat flux = q/A =
𝑇
π‘…π‘‡β„Ž
q/A =
500βˆ’360
20
10000
+
1
1000𝐾
+
20
10000
10000 =
500βˆ’360
20
10000
+
1
1000𝐾
+
20
10000
K = 0.1 w/mK
CONVECTION THERMAL RESISTANCE
HEAT AND MASS TRANSFER
qconv = h A (Tw - Tο‚₯)
(RTh)Covection =
Tw βˆ’ Tο‚₯
π‘ž
=
1
β„Žπ΄
CONDUCTION - CONVECTION HEAT TRANSFER THROUGH A COMPOSITE SLAB
HEAT AND MASS TRANSFER
CONDUCTION - CONVECTION HEAT TRANSFER THROUGH A COMPOSITE SLAB
HEAT AND MASS TRANSFER
TG Tο‚₯
T1 T2
T3
1
β„Ž1𝐴
𝑏1
𝐾1𝐴
𝑏2
𝐾2𝐴
1
β„Ž2𝐴
q
q =
𝑇𝐺
βˆ’π‘‡βˆž
1
β„Ž1
𝐴
+
𝑏1
𝐾1
𝐴
+
𝑏2
𝐾2
𝐴
+
1
β„Ž2
𝐴
= Rate of heat transfer.
q/A =
𝑇𝐺
βˆ’π‘‡βˆž
1
β„Ž1
+
𝑏1
𝐾1
+
𝑏2
𝐾2
+
1
β„Ž2
= Heat flux (w/m2)
q = UA (𝑇𝐺 βˆ’ π‘‡βˆž)
Remember
Resistance =
𝑻
𝒒
𝟏
𝑼
=
𝟏
π’‰πŸ
+
π’ƒπŸ
π‘²πŸ
+
π’ƒπŸ
π‘²πŸ
+
𝟏
π’‰πŸ
RADIAL CONDUCTION THROUGH HOLLOW CYLINDER
HEAT AND MASS TRANSFER
RADIAL CONDUCTION THROUGH HOLLOW CYLINDER
HEAT AND MASS TRANSFER
Area of conduction heat transfer = 2rL
q = - K A (
𝑑𝑇
π‘‘π‘Ÿ
) = - K 2rL (
𝑑𝑇
π‘‘π‘Ÿ
)
At r = r1, T = T1
At r = r2, T = T2
‫׬‬
π‘Ÿ1
π‘Ÿ2
π‘ž
π‘‘π‘Ÿ
π‘Ÿ = - ‫׬‬
𝑇1
𝑇2
2 𝐾𝐿 𝑑𝑇
q ln (
π‘Ÿ2
π‘Ÿ1
) = 2𝐾𝐿 (T1-T2)
q =
2𝑲𝑳 (T1βˆ’T2)
ln (π’“πŸ
π’“πŸ
)
& RTh =
𝑻
𝒒
=
ln (π’“πŸ
π’“πŸ
)
2𝐾𝐿
RADIAL CONDUCTION THROUGH COMPOSITE CYLINDER
HEAT AND MASS TRANSFER
RADIAL CONDUCTION THROUGH COMPOSITE CYLINDER
HEAT AND MASS TRANSFER
T1 T2 T3
q
𝑙𝑛
π‘Ÿ2
π‘Ÿ1
2πœ‹πΎ1𝐿
𝑙𝑛
π‘Ÿ3
π‘Ÿ2
2πœ‹πΎ2𝐿
q =
𝑇1 βˆ’π‘‡3
𝑙𝑛
π‘Ÿ2
π‘Ÿ1
2πœ‹πΎ1
𝐿
+
𝑙𝑛
π‘Ÿ3
π‘Ÿ2
2πœ‹πΎ2
𝐿
RADIAL CONDUCTION-CONVECTION HEAT TRANSFER THROUGH COMPOSITE CYLINDER
HEAT AND MASS TRANSFER
h1 = Heat transfer coefficient of convection (inside)
h2 = Heat transfer coefficient of convection (outside)
TG Tο‚₯
T1 T2 T3
q
(Convection)inner Conduction (Convection)Outer
Conduction
1
β„Ž1(2πœ‹π‘Ÿ1𝐿)
𝑙𝑛
π‘Ÿ2
π‘Ÿ1
(2πœ‹πΎ1𝐿)
𝑙𝑛
π‘Ÿ3
π‘Ÿ2
(2πœ‹πΎ2𝐿)
1
β„Ž2(2πœ‹π‘Ÿ3𝐿)
q =
2πœ‹π‘Ÿ1𝐿 (𝑇𝐺
βˆ’π‘‡βˆž
)
1
β„Ž1
(2πœ‹π‘Ÿ1
𝐿)
+
𝑙𝑛
π‘Ÿ2
π‘Ÿ1
(2πœ‹πΎ1
𝐿)
+
𝑙𝑛
π‘Ÿ3
π‘Ÿ2
(2πœ‹πΎ2
𝐿)
+ 1
β„Ž2
(2πœ‹π‘Ÿ3
𝐿)
q = UiAiT = U0A0T
= Ui (2πœ‹π‘Ÿ1𝐿)(𝑇𝐺 βˆ’ π‘‡βˆž) = U0 (2πœ‹π‘Ÿ3𝐿)(𝑇𝐺 βˆ’ π‘‡βˆž)
A
B
Also,
RADIAL CONDUCTION-CONVECTION HEAT TRANSFER THROUGH COMPOSITE CYLINDER
HEAT AND MASS TRANSFER
1
π‘ˆπ‘–
=
1
β„Ž1
+
π‘Ÿ1
𝐾1
ln
π‘Ÿ2
π‘Ÿ1
+
π‘Ÿ1
𝐾2
ln
π‘Ÿ3
π‘Ÿ2
+
π‘Ÿ1
π‘Ÿ3
1
β„Ž2
Comparing equation A and B
1
π‘ˆπ‘œ
=
1
β„Ž2
+
π‘Ÿ3
𝐾1
ln
π‘Ÿ2
π‘Ÿ1
+
π‘Ÿ3
𝐾2
ln
π‘Ÿ3
π‘Ÿ2
+
π‘Ÿ3
π‘Ÿ1
1
β„Ž1
𝟏
𝐔
=
𝟏
𝐑𝟏
+
𝟏
𝐑𝟐
Thermal resistance of conduction
gets neglected since ri = ro (approx)
CRITICAL RADIUS OF INSULATION
HEAT AND MASS TRANSFER
HEAT AND MASS TRANSFER
CRITICAL RADIUS OF INSULATION Conduction Convection
𝑙𝑛
π‘Ÿπ‘œ
π‘Ÿπ‘–
2πœ‹πΎπΏ
1
β„Ž (2πœ‹π‘Ÿ0𝐿)
q
Ti Tο‚₯
q =
𝑇𝑖
βˆ’π‘‡ο‚₯
𝑙𝑛
π‘Ÿπ‘œ
π‘Ÿπ‘–
2πœ‹πΎπΏ
+
1
β„Ž (2πœ‹π‘Ÿ0
𝐿)
q = f(ro) & dq/dr = 0 (For maximum heat transfer)
𝑑
π‘‘π‘Ÿπ‘œ
𝑇𝑖
βˆ’π‘‡ο‚₯
𝑙𝑛
π‘Ÿπ‘œ
π‘Ÿπ‘–
2πœ‹πΎπΏ
+
1
β„Ž (2πœ‹π‘Ÿ0
𝐿)
= 0 GIVES ro =
πΎπΌπ‘›π‘ π‘’π‘™π‘Žπ‘‘π‘–π‘œπ‘›
β„Ž
Critical radius of insulation
CRITICAL RADIUS OF INSULATION
HEAT AND MASS TRANSFER
Electric power transmission cables Semiconductor devices
Practical application of critical radius of insulation
rcritical = K/h rcritical = 2K/h
RADIAL CONDUCTION THROUGH HOLLOW SPHERE
HEAT AND MASS TRANSFER
A = 42
RADIUS CONDUCTION THROUGH HOLLOW SPHERE
HEAT AND MASS TRANSFER
q = - K A
𝑑𝑇
π‘‘π‘Ÿ
(From Fourier’s law of conduction)
= - K 4r2 (
𝑑𝑇
π‘‘π‘Ÿ
) π‘ž β‰  𝑓 π‘Ÿ 𝑣𝑖𝑧 π‘žπ‘Ÿ = π‘žπ‘Ÿ + π‘‘π‘Ÿ
β€«Χ¬β€¬π‘Ÿ1
π‘Ÿ2
π‘ž
π‘‘π‘Ÿ
π‘Ÿ2 = ‫׬‬𝑇1
𝑇2
βˆ’ 4πœ‹πΎπ‘‘π‘‡
q =
4πœ‹πΎ 𝑇1
βˆ’π‘‡2
π‘Ÿ1
π‘Ÿ2
π‘Ÿ2
βˆ’π‘Ÿ1
RTh
q
T1 T2
RTh =
βˆ†π‘‡
π‘ž
=
π‘Ÿ2
βˆ’π‘Ÿ1
4πœ‹πΎπ‘Ÿ1
π‘Ÿ2
DERIVATION OF GENERALIZED HEAT CONDUCTION EQUATION
HEAT AND MASS TRANSFER
qx = heat conducted into
the element in X-direction
= - K A (
𝑑𝑇
𝑑π‘₯
) watt
qx+dx = Heat conducted
out of the element along
X – direction.
= qx +
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯
qgenerated = ሢ
π‘ž A dx watt
GENERALIZED HEAT CONDUCTION EQUATION DERIVATION
HEAT AND MASS TRANSFER
Writing energy balance equation of X-direction conduction
qx + qgenerated = qx+dx + Rate of change of internal energy
qx + ሢ
π‘ž A dx = qx +
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯ +
πœ•
πœ•π‘‘
( mcpT)
t = sec, m = element’s mass =  X (A dx)
ሢ
π‘ž A dx =
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯ +
πœ•
πœ•π‘‘
( X (Adx) cp T)
K
πœ•2
𝑇
πœ•π‘₯2 + ሢ
π‘ž =  cp
πœ•π‘‡
πœ•π‘‘
Writing energy balance equation for all 3 dimensions.
K
πœ•2
𝑇
πœ•π‘₯2 + K
πœ•2
𝑇
πœ•π‘¦2 + K
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž =  cp
πœ•π‘‡
πœ•π‘‘
GENERALIZED HEAT CONDUCTION EQUATION DERIVATION
HEAT AND MASS TRANSFER
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž/K =  cp X
1
𝐾
πœ•π‘‡
πœ•π‘‘
Here
𝐾
 cp
=  = Thermal diffusivity, A thermophysical property
of material (The ratio between thermal conductivity of the material and its thermal capacity.)
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž/K =
1

πœ•π‘‡
πœ•π‘‘
πœ•π‘‡
πœ•π‘‘
= 0, T ο‚Ή f(t) (Steady conditions)
ሢ
π‘ž = 0 (No heat generation)
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 = 0
gases > liquid
𝛻2 T = 0 Laplace’s equation in T
HEAT GENERATION IN A SLAB
HEAT AND MASS TRANSFER
Assumptions
(1) Steady state heat transfer conditions.
T ο‚Ή f(t)
(2) One dimensional heat transfer
T = f(x)
(3) Uniform heat generation rate.
(4) Constant value of β€œK”
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž/K =
1

πœ•π‘‡
πœ•π‘‘
HEAT GENERATION IN A SLAB
HEAT AND MASS TRANSFER
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž/K =
1

πœ•π‘‡
πœ•π‘‘
𝑑2
𝑇
𝑑π‘₯2+ ሢ
π‘ž/K = 0
𝑑2
𝑇
𝑑π‘₯2 = - ሢ
π‘ž/K
𝑑𝑇
𝑑π‘₯
= - ሢ
π‘ž/K x + C1
T = - ሢ
π‘ž/K
π‘₯2
2
+ C1x + C2
Boundary conditions
At x = +L and x = -L Gives T = Tw (Also renders C1 = 0)
HEAT GENERATION IN A SLAB
HEAT AND MASS TRANSFER
Temperature of the slab is max when
𝑑𝑇
𝑑π‘₯
= 0 which gives x = 0
Viz max temperature of slab would be at centerline
Now in case both sides of the slab are at different
temperature then C1 would not be zero and hence max
temp will not be at midplane (centerline)
For such case, Let max temperature of slab as To
At x = 0, T = T0 Viz C2 = 0 Which gives;
T = - ሢ
π‘ž/K
π‘₯2
2
+ T0
T – T0 = - ሢ
π‘ž/K
π‘₯2
2
T = - ሢ
π‘ž/K
π‘₯2
2
+ C1x + C2
Parabolic temperature distribution A
HEAT GENERATION IN A SLAB
HEAT AND MASS TRANSFER
At x = +L Or x = -L ; T = Tw
T0 – Tw =
π‘ž 𝐿2
2𝐾
Dividing equation A & B we have;
𝐴
𝐡
=
T – T0
T0 – Tw
= (
π‘₯
𝐿
)2
B
Non-dimensional temperature
distribution
Heat generated in slab = Heat out through convection
ሢ
π‘ž X (2L X A) = 2h A (Tw – Tο‚₯)
Tw =
ሢ
π‘žπΏ
β„Ž
+ Tο‚₯
HEAT GENERATION IN A SLAB
HEAT AND MASS TRANSFER
Also from equation B we have
T0 or Tmax =
π‘ž 𝐿2
2𝐾
+
ሢ
π‘žπΏ
β„Ž
+ Tο‚₯
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
r = 0
Tw
Tw i
R
qconvection Tο‚₯
h
L
ሢ
π‘ž = Heat generation rate
=
𝑖2
π‘…π‘’π‘™π‘’π‘π‘‘π‘Ÿπ‘–π‘
𝑅2
𝐿
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
πœ•2
𝑇
πœ•π‘₯2 +
πœ•2
𝑇
πœ•π‘¦2 +
πœ•2
𝑇
πœ•π‘§2 + ሢ
π‘ž/K =
1

πœ•π‘‡
πœ•π‘‘
1
π‘Ÿ
πœ•
πœ•π‘Ÿ
(π‘Ÿ
πœ•π‘‡
πœ•π‘Ÿ
) +
ሢ
π‘ž
𝐾
=
1
𝛼
πœ•π‘‡
πœ•π‘‘
1
π‘Ÿ2
πœ•
πœ•π‘Ÿ
(π‘Ÿ2 πœ•π‘‡
πœ•π‘Ÿ
) +
ሢ
π‘ž
𝐾
=
1
𝛼
πœ•π‘‡
πœ•π‘‘
Generalized heat
conduction coordinate
systems.
Rectilinear coordinate system
Cylindrical coordinate system
Spherical coordinate system
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
1
π‘Ÿ
πœ•
πœ•π‘Ÿ
(π‘Ÿ
πœ•π‘‡
πœ•π‘Ÿ
) +
ሢ
π‘ž
𝐾
=
1
𝛼
πœ•π‘‡
πœ•π‘‘
𝑑2𝑇
π‘‘π‘Ÿ2
+
1
π‘Ÿ
𝑑𝑇
π‘‘π‘Ÿ
= βˆ’
ሢ
π‘ž
𝐾
r
𝑑2
𝑇
π‘‘π‘Ÿ2 +
𝑑𝑇
π‘‘π‘Ÿ
= βˆ’
ሢ
π‘žπ‘Ÿ
𝐾
𝑑
π‘‘π‘Ÿ
(π‘Ÿ
𝑑𝑇
π‘‘π‘Ÿ
) = βˆ’
ሢ
π‘žπ‘Ÿ
𝐾
Integrating w.r.t β€œr”
π‘Ÿ
𝑑𝑇
π‘‘π‘Ÿ
= βˆ’
ሢ
π‘žπ‘Ÿ2
2𝐾
+ C1
𝑑𝑇
π‘‘π‘Ÿ
= βˆ’
ሢ
π‘žπ‘Ÿ
2𝐾
+
𝐢1
π‘Ÿ
𝑑𝑇
π‘‘π‘Ÿ At r = R = βˆ’
ሢ
π‘žπ‘…
2𝐾
+
𝐢1
𝑅
Equation 1
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
Again integrating
T = βˆ’
ሢ
π‘žπ‘Ÿ2
4𝐾
+ C1 log r + C2
From boundary condition (2)
Heat generated in the rod = Heat conducted radially at the surface
= Heat convected from the surface to the fluid.
ሢ
π‘ž X R2L = - K (2RL)
𝑑𝑇
π‘‘π‘Ÿ At r = R
𝑑𝑇
π‘‘π‘Ÿ At r = R = βˆ’
ሢ
π‘žπ‘Ÿ
2𝐾
From equation 1 and 2
C1 = 0
Boundary conditions
(1) AT r = R, T = Tw
(2) Steady state of rod
Equation 2
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
Temperature of the rod will be maximum at
𝑑𝑇
π‘‘π‘Ÿ
= 0
Gives r = 0 (viz at the axis of the rod/cylinder)
Let max temp = T0 (At axis)
i.e. At r = 0, T = T0 Gives T0 = C2
T = βˆ’
ሢ
π‘žπ‘Ÿ2
4𝐾
+ T0 Or T0 – T =
ሢ
π‘žπ‘Ÿ2
4𝐾
AT r = R, T = Tw Or T0 – Tw =
ሢ
π‘žπ‘…2
4𝐾
Dividing equation 3 by 4 we have
T0 – T
T0 – Tw
=
π‘Ÿ
𝑅
2
Equation 3 (Parabolic temp distribution)
Equation 4
Temperature distribution in non-dimensional format
HEAT GENERATION IN A CYLINDER
HEAT AND MASS TRANSFER
The surface temperature Tw can also be obtained from
energy balance equation for steady state condition of rod.
ሢ
π‘ž X R2L = h 2RL (Tw - Tο‚₯)
Tw =
ሢ
π‘žπ‘…
2β„Ž
+ Tο‚₯
Similarly, Maximum temperature T0 can also be found out.
T0 Or Tmax =
ሢ
π‘žπ‘…2
4𝐾
+
ሢ
π‘žπ‘…
2β„Ž
+ Tο‚₯
Surface temperature
Maximum temperature
FINS
HEAT AND MASS TRANSFER
Fins are the projections protruding from a hot surface into ambient fluid. They are meant
for increasing heat transfer rate by increasing surface area.
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
A = Profile area = zt
L = Length of fin
z = Width of fin
t = Thickness of fin
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
Objectives
(1) T = f(x)
(2) qfin = ?
qx = Heat conducted into the element
= - KA (
𝑑𝑇
𝑑π‘₯
)
qx+dx = Heat conducted out of the element
= qx +
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯
Heat convected from the surface of fin
= hP dx (T - Tο‚₯),
P = Perimeter of fin = (2z + 2t)
qx = qx+dx + qconvected (Energy balance equation)
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
qx = qx +
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯ + hP dx (T - Tο‚₯)
0 =
πœ•
πœ•π‘₯
π‘žπ‘₯ 𝑑π‘₯ + hP dx (T - Tο‚₯)
0 =
πœ•
πœ•π‘₯
βˆ’ KA (
𝑑𝑇
𝑑π‘₯
) 𝑑π‘₯ + hP dx (T - Tο‚₯)
𝑑2
𝑇
𝑑π‘₯2 -
β„Žπ‘ƒ
𝐾𝐴
(T βˆ’ Tο‚₯) = 0
Let (T - Tο‚₯) =  = f(x)
viz.
𝑑𝑇
𝑑π‘₯
=
𝑑
𝑑π‘₯
𝑑2
𝑇
𝑑π‘₯2 =
𝑑
𝑑π‘₯
and put m2 =
β„Žπ‘ƒ
𝐾𝐴
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
𝑑2

𝑑π‘₯2 - m2 = 0
T - Tο‚₯ =  = C1e-mx + C2emx
Where, m =
β„Žπ‘ƒ
𝐾𝐴
C1 and C2 are constant of integration
Boundary condition 1
At x = 0, T = T0
 = 0 = T0 - Tο‚₯
Boundary condition 2 (Has 3 unique cases)
Standard format of 2nd order differential equation
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
Case 1 – Fin is infinitely long (A very long fin)
At x = ο‚₯, T = Tο‚₯ viz  = 00
i.e.
𝑇 βˆ’π‘‡ο‚₯
𝑇0
βˆ’π‘‡ο‚₯
= e-mx
qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯)
Case 2 – Fin is finite in length but tip is insulated (A adiabatic tip)
qconvected from tip = h A (Tx=L - Tο‚₯) = Very small (negligible value)
Heat conducted into the tip of fin = 0
βˆ’ KA (
𝑑𝑇
𝑑π‘₯
)At x=L = 0 (viz. insulated tip)
Temperature distribution
Heat transfer
ANALYSIS OF RECTANGULAR FINS
HEAT AND MASS TRANSFER
(
𝑑𝑇
𝑑π‘₯
)At x=L = 0
𝑑
𝑑π‘₯ At x = L = 0
𝑇 βˆ’π‘‡ο‚₯
𝑇0
βˆ’π‘‡ο‚₯
=
cos β„Ž π‘š (πΏβˆ’π‘₯)
cos β„Ž π‘šπΏ
qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mL
Case 3 – Fin is finite and tip is not insulated (Uninsulated tip)
𝑇 βˆ’π‘‡ο‚₯
𝑇0
βˆ’π‘‡ο‚₯
=
cos β„Ž π‘š (πΏπ‘βˆ’π‘₯)
cos β„Ž π‘šπΏπ‘
qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mLc
m =
𝒉𝑷
𝑲𝑨
Temperature distribution
Heat transfer
Temperature distribution
Heat transfer
Lc = Corrected length of fin
= L + t/4 (Rectangular)
= L + d/4 (Pin)
NUMERICAL
HEAT AND MASS TRANSFER
An uninsulated fin of 0.3 mm length is shown in the adjoining figure. Calculate
the heat convected from the tip of the fin.
NUMERICAL
HEAT AND MASS TRANSFER
Lc = L + t/4 = 0.30
P = 2z + 2t = 2 (0.3 + 2/1000) = 0.604
A = z X t = 0.3 X 2 = 0.6 m2
m =
𝒉𝑷
𝑲𝑨
= 8.603 m-1
𝑇 βˆ’π‘‡ο‚₯
𝑇0
βˆ’π‘‡ο‚₯
=
cos β„Ž π‘š (πΏπ‘βˆ’π‘₯)
cos β„Ž π‘šπΏπ‘
Putting x = 0.3 m
T At x = 0.3 = 70.30C
qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mLc = 281.1 Watt
FIN EFFICIENCY & FIN EFFECTIVENESS
HEAT AND MASS TRANSFER
Fin efficiency is defined as the ratio between actual heat transfer rate taking place
through the fin and the maximum possible heat transfer that can occur through the fin.
fin =
π‘žπ‘Žπ‘π‘‘π‘’π‘Žπ‘™
π‘žπ‘šπ‘Žπ‘₯
Fin effectiveness is defined as the ratio between heat transfer with fins and heat transfer
without fins.
ο₯fin =
π‘žπ‘€π‘–π‘‘β„Ž 𝑓𝑖𝑛𝑠
π‘žπ‘€π‘–π‘‘β„Žπ‘œπ‘’π‘‘ 𝑓𝑖𝑛𝑠
ο₯fin ο‚΅ 1/ β„Ž
ο₯fin ο‚΅
𝑃
𝐴
ο₯fin ο‚΅ 𝐾
FIN EFFICIENCY & FIN EFFECTIVENESS
HEAT AND MASS TRANSFER
Moderately short
Number of fins
Closely spaced fins
Thin
High conductivity material
As such Al
Number of fins regulated = n
=
π‘‡π‘œπ‘‘π‘Žπ‘™ β„Žπ‘’π‘Žπ‘‘ π‘‘π‘œ 𝑏𝑒 π‘‘π‘–π‘ π‘ π‘–π‘π‘Žπ‘‘π‘’π‘‘
π»π‘’π‘Žπ‘‘ π‘Ÿπ‘Žπ‘‘π‘’ π‘‘β„Žπ‘Ÿπ‘œπ‘’π‘”β„Ž π‘’π‘Žπ‘β„Ž 𝑓𝑖𝑛
UNSTEADY STATE/TRANSIENT CONDUCTION HEAT TRANSFER
HEAT AND MASS TRANSFER
T = f(t)
Ti = Initial temperature of the body at the moment at which
t=0 seconds. Viz when the body is just exposed to fluid.
T = Temperature of body at any time β€œt sec” later
The rate of convection heat transfer between body and fluid =
The rate of decrease of internal energy of body w.r.t time
hA (T - Tο‚₯) = - m Cp (
𝑑𝑇
𝑑𝑑
) Joules/Sec
= -  vCp (
𝑑𝑇
𝑑𝑑
) J/S
Treating all the parameters including β€œh” as constant and
separating the variable T and t and then integrating, we have;
UNSTEADY STATE/TRANSIENT CONDUCTION HEAT TRANSFER
HEAT AND MASS TRANSFER
ΰΆ±
𝑑=0
𝑑
(
β„Žπ΄
 vCp
) 𝑑𝑑 = ΰΆ±
𝑇𝑖
𝑇
βˆ’ 𝑑𝑇
𝑇 βˆ’ 𝑇ο‚₯
(
β„Žπ΄
 vCp) t = ln 𝑇 βˆ’ 𝑇ο‚₯ = ln
𝑇𝑖
βˆ’π‘‡ο‚₯
𝑇 βˆ’π‘‡ο‚₯
e
(
β„Žπ΄
 vCp
) t =
𝑇𝑖
βˆ’π‘‡ο‚₯
𝑇 βˆ’π‘‡ο‚₯
dT
dt
dT
dt
dT/dt
t (Time) t (Time)
T T
-dT/dt = Rate of cooling
= f(t)
- Ve + Ve
CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
q = h A T
Convection
Forced convection
heat transfer
Free convection
heat transfer
Velocity is evident Velocity is not evident
r
X
R
Y
X
u
u
u = f(r)
u = f(x,y)
FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
h = f (v, D, , , Cp, K)
v = velocity of fluid = [LT-1]
D = characteristics dimensions of the body = [L]
 = Density = [ML-3]
 = Dynamic viscosity (Pascal-Sec) = [ML-1T-1]
Cp = Specific heat at constant pressure = [L2T-2-1]
K = Thermal conductivity = [MLT-3-1]
h = Convective heat transfer coefficient = [MT-3 -1]
FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
Buckingham  theorem of dimensional analysis states that if there are β€œn” number of
variables in any functional relationship both dependent and independent. And if all the
variables put together contains β€˜β€m” number of fundamental dimensions, then the
functional relationship among the variables can be expressed in term of β€œn-m” number of
dimensionless  terms.
h = f (v, D, , , Cp, K)
Here n = 7
m = 4 [M,L,T,]
According to Buckingham  theorem
n – m = Number of dimensionless  terms = 7 – 4 = 3
Let 1, 2, 3 be these dimensionless terms.
FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
1 = ( ha1 , vb1, Dc1 , d1 ) 
2 = ( ha2 , vb2, Dc2 , d2 ) Cp
3 = ( ha2 , vb2, Dc2 , d2 ) K
Now 1 = [M0L0T00] = [MT-3-1]a1 [LT-1]b1 [L]c1 [ML-3]d1 [ML-1T-1]
For mass β€œM”, 0 = a1 + d1 + 1
For length β€œL”, 0 = b1 + c1 + - 3d1 – 1
For time β€œT”, 0 = -3a1 – b1 – 1
For temperature β€œο±β€, 0 = -a1
h = f (v, D, , , Cp, K)
1 =

𝒗𝑫
FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
h = f (v, D, , , Cp, K) Similarly 2 =
𝑣Cp
β„Ž
3 =
𝐾
β„Žπ·
Now,
1
1
= Reynold’s Number = Re =
𝒗𝑫

1
2
= Stanton’s Number = Sn =
β„Ž
𝑣Cp
1
3
= Nusselt Number = Nu =
β„Žπ·
𝑲
12
3
= Prandtl’s Number = Pr =
Cp
𝑲
PHYSICAL SIGNIFICANCE OF Re IN FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
1.Reynold’s Number Re – Defined as the ratio between inertia forces and viscous forces
to which a flowing fluid is subjected to.
Re =
πΌπ‘›π‘’π‘Ÿπ‘‘π‘–π‘Ž πΉπ‘œπ‘Ÿπ‘π‘’π‘ 
π‘‰π‘–π‘ π‘π‘œπ‘’π‘  π‘“π‘œπ‘Ÿπ‘π‘’π‘ 
=
𝒗𝑫

=
𝒗𝑫
/
=
𝒗𝑫
  = Kinematic viscosity
Re is the criteria to tell whether the fluid flow is laminar or turbulent for incompresible
flow through pipes as well ducts.
Re < 2000 (Lower critical) – Flow is laminar
Re > 4000 (Upper critical) – Flow is turbulent
HEAT AND MASS TRANSFER
Axi-symmetric parabolic
distribution of velocity. u = f(r)
Logarithmic distribution
of velocity. u = f(r)
LAMINAR
TURBULENT
PHYSICAL SIGNIFICANCE OF Re IN FORCED CONVECTION HEAT TRANSFER
INCOMPRESSIBLE FLOW OVER FLAT SURFACE
HEAT AND MASS TRANSFER
INCOMPRESSIBLE FLOW OVER FLAT SURFACE
HEAT AND MASS TRANSFER
Hydrodynamic boundary layer (HBL) is defined as a thin region formed over a flat surface
(plate) inside which velocity gradient are seen in the normal direction to the plate.
These velocity gradient are formed due to viscos nature or more precisely due to
momentum diffusion through the fluid layer in the normal direction to the plate.
Outside the HBL, free stream velocity exists in which no viscos influence can be seen
At any given β€œx”
At y = 0, u = 0
At y = ,
πœ•π’–
πœ•π’š
= 0
At y = 0,
πœ•πŸ
𝒖
πœ•π’šπŸ = 0
At any given β€œx”
πœ•π’–
πœ•π’š
= f(y) so for
πœ•π’–
πœ•π’š
At y = 0
 = f(x)
INCOMPRESSIBLE FLOW OVER FLAT SURFACE
HEAT AND MASS TRANSFER
Rex < 5 X 105 (Flow over plate is laminar)
Rex > 6.7-7 X 105 (Flow over plate is turbulent)
PHYSICAL SIGNIFICANCE OF Nu & PrIN FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
2. Nusselt number Nu - Nusselt number is the ratio of convective to conductive heat
transfer at a boundary in a fluid. Sometimes also known as dimensionless heat transfer
coefficient.
The Biot number is the ratio of the
internal resistance of a body to heat
conduction to its external resistance to
heat convection. Therefore, a small Biot
number represents small resistance to
heat conduction, and thus small
temperature gradients within the body.
Nu =
β„Žπ·
𝐾𝑓𝑙𝑒𝑖𝑑
=
𝐷
𝐾𝐴
1
β„Žπ΄
=
πΆπ‘œπ‘›π‘‘π‘’π‘π‘‘π‘–π‘œπ‘› π‘Ÿπ‘’π‘ π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’ π‘œπ‘“π‘“π‘’π‘Ÿπ‘’π‘‘ 𝑏𝑦 𝑓𝑙𝑒𝑖𝑑 (π‘ π‘‘π‘Žπ‘‘π‘–π‘œπ‘›π‘Žπ‘Ÿπ‘¦)
π‘†π‘’π‘Ÿπ‘“π‘Žπ‘π‘’ π‘π‘œπ‘›π‘£π‘’π‘π‘‘π‘–π‘£π‘’ π‘Ÿπ‘’π‘ π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’
But fluids are bad conductor of heat
Numerator > Denominator
Nu is always greater than 1
Bi =
β„Žπ·
πΎπ‘†π‘œπ‘™π‘–π‘‘
PHYSICAL SIGNIFICANCE OF Nu & PrIN FORCED CONVECTION HEAT TRANSFER
HEAT AND MASS TRANSFER
3. Prandtl Number (Pr) – The only dimensionless number which is a property of the fluid.
Defined as the ratio between kinematic viscosity and thermal diffusivity of fluid.
Pr =
πΎπ‘–π‘›π‘’π‘šπ‘Žπ‘‘π‘–π‘ π‘£π‘–π‘ π‘π‘œπ‘ π‘–π‘‘π‘¦
π‘‡β„Žπ‘’π‘Ÿπ‘šπ‘Žπ‘™ 𝑑𝑖𝑓𝑓𝑒𝑠𝑖𝑣𝑖𝑑𝑦
=


𝐢𝑝
𝐾
=


𝐾
𝐢𝑝
Pr for air = 0.65 to 0.73
Pr for water = 2 to 6
For engine oils = up to 100 !
Very low Pr
THERMAL BOUNDARY LAYER (TBL)
HEAT AND MASS TRANSFER
THERMAL BOUNDARY LAYER (TBL)
HEAT AND MASS TRANSFER
Thermal Boundary Layer (TBL) is similar to HBL inside which velocity gradient are seen in
the normal direction to the plate. Thermal boundary layer is also a thin region in which
temperature gradients are present in the normal direction to the flat surface (Plate). These
temperature gradient are formed due to heat transfer between plate and flowing fluid.
At any given β€œx”
measured from leading
edge.
At y = 0, T = Tw
At y = t, T = Tο‚₯ ,
πœ•π‘»
πœ•π’š
= 0
At y = 0,
πœ•πŸ
𝑻
πœ•π’šπŸ = 0
At any given β€œx”
πœ•π‘»
πœ•π’š
= f(y) with maximum
value of
πœ•π‘»
πœ•π’š
At y = 0
ENERGY BALANCE FOR DIFFERENTIAL CONTROL VOLUME OF TBL
HEAT AND MASS TRANSFER
Heat conducted into the control volume = Heat convected from
the hot plate at Tw to free stream fluid at Tο‚₯
- K dA (
πœ•π‘‡
πœ•π‘¦
) AT y = 0 = hx dA (Tw - Tο‚₯)
hx =
βˆ’ 𝐾(πœ•π‘‡
πœ•π‘¦
) AT y = 0
(Tw βˆ’ Tο‚₯)
Local convective heat transfer coefficient.
hx
x
hx ο‚΅ 𝒙
Fourier’s law Newton’s law
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER  = f (x,y) &  = f (x,y),  = c
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER
CONTROL VOLUME
Viscos force =  [
πœ•π‘’
πœ•π‘¦
+
πœ•
πœ•π‘¦
(
πœ•π‘’
πœ•π‘¦
) 𝑑𝑦 ] (𝑑π‘₯ 𝑋 1)
dx
dy
Pressure force = p X dy X 1
Pressure force = (p
+
πœ•π‘
πœ•π‘₯
𝑑π‘₯) 𝑑𝑦 X 1
Viscos force
Gravity force
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER
Applying Newton’s II law of motion
Οƒ 𝐹π‘₯ = max (Conservation of linear momentum)
Resulting momentum equation of HBL is ;
u
πœ•π‘’
πœ•π‘₯
+ v
πœ•π‘’
πœ•π‘¦
= (


)
πœ•2
𝑒
πœ•π‘¦2 -
1

(
𝑑𝑃
𝑑π‘₯
)
u
v V = u Τ¦
π’Š + v Τ¦
𝒋
dp/dx = 0 for flow
over plates & (

) = 
u
𝝏𝒖
𝝏𝒙
+ v
𝝏𝒖
ππ’š
= 
𝝏𝟐
𝒖
ππ’šπŸ
Momentum equation of HBL
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER  = f (x,y) &  = f (x,y), T = f(x,y),  = c
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER
Consider negligible
heat conduction in
x-direction.
Thermal heat energy
convected by fluid =
mCpT J/Sec
Viscos heat is
neglected
CONTROL VOLUME
Heat convected =  (dx X 1) (v +
πœ•π‘£
πœ•π‘¦
dy) Cp (T +
πœ•π‘‡
πœ•π‘¦
dy) Heat conducted = - K (dx X 1) (
πœ•π‘‡
πœ•π‘¦
+
πœ•
πœ•π‘¦
πœ•π‘‡
πœ•π‘¦
dy)
Heat conducted = - K (dx X 1)
πœ•π‘‡
πœ•π‘¦
Heat convected =  (dx X 1) v Cp T
Heat convected =
 (dy X 1) u Cp T
Heat convected =  (dx X 1)
(u +
πœ•π‘’
πœ•π‘₯
du) Cp (T +
πœ•π‘‡
πœ•π‘₯
dx)
MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL
HEAT AND MASS TRANSFER
Heat conducted through bottom face
+
Heat convected through left face
+
Heat convected through bottom face
Heat conducted through top face
+
Heat convected through right face
+
Heat convected through top face
6 energies
u
𝝏𝑻
𝝏𝒙
+ v
𝝏𝑻
ππ’š
= 
𝝏𝟐
𝑻
ππ’šπŸ Energy equation for TBL
u
𝝏𝒖
𝝏𝒙
+ v
𝝏𝒖
ππ’š
= 
𝝏𝟐
𝒖
ππ’šπŸ Momentum equation of HBL
FORCED CONVECTION IN FLOW THROUGH PIPES AND DUCTS
HEAT AND MASS TRANSFER
ሢ
π‘š =  X R2 X Vmean Kg/s
FORCED CONVECTION IN FLOW THROUGH PIPES AND DUCTS
HEAT AND MASS TRANSFER
Tb (Bulk mean temperature) – Defined as {At a given cross section of pipe} the
temperature which takes into account the variation of temperature of fluid layers with
respect to β€œr” at the cross section of the pipe and thus indicates the total thermal
energy transported by the fluid through the cross section.
Thermal energy/enthalpy transported by fluid through the
cross section of pipe = ሢ
π‘š CpTb =  X R2 X Vmean CpTb
And the Bulk mean temperature is given by.
Tb =
2 ‫׬‬0
𝑅
π‘Ÿ 𝑒 𝑇 π‘‘π‘Ÿ
R2 X Vmean
NUMERICAL
HEAT AND MASS TRANSFER
Find out the bulk mean temperature at exit.
dq = qw X Area = qw 𝐷 𝑑π‘₯
Differential heat rate through differential heat transfer area of
length β€œdx” = dq = ሢ
π‘š Cp dTb
‫׬‬0
3
2500 π‘₯ 𝐷 𝑑π‘₯ = ‫׬‬𝑖𝑛𝑙𝑒𝑑
𝑒π‘₯𝑖𝑑
ሢ
π‘š Cp dTb
(Tb)Exit = 620C
FREE/NATURAL CONVECTION
HEAT AND MASS TRANSFER
FREE/NATURAL CONVECTION
HEAT AND MASS TRANSFER
h = f ( g, , , L, , , Cp, K )
g = acceleration due to gravity
 = Isobaric volume expansion coefficient
RADIATION
HEAT AND MASS TRANSFER
Any body at a given temperature emit thermal radiation at all probable wavelength on
electromagnetic spectrum and in all possible hemispherical direction.
Total hemispherical emissive power (E) – Defined as radiation energy emitted from the
surface of a body per unit time per unit area in all possible hemispherical directions
integrated over all the wavelengths.
RADIATION
HEAT AND MASS TRANSFER
Total emissivity (ο₯) – Defined as the ratio between total hemispherical emissive power of
a non-black body to that of a black body at same temperature.
Non-black Black body
E Eb
ο₯ =
𝑬
𝑬𝒃
ο₯ ο‚£ 1 ο₯b = 1
RADIATION
HEAT AND MASS TRANSFER
Black body is a body which
absorbs all the thermal
radiation incident or falling
upon the body.
Perfect absorber Ideal emitter Diffusive in nature
RADIATION
HEAT AND MASS TRANSFER
Monochromatic/Spectral hemispherical emissive power (E) - E at a particular
wavelength β€œο¬β€ is defined as the quantity which when multiplied by β€œd” (Differentially
small increment in wavelength) shall give the radiation energy emitted from the surface of
a body per unit time per unit area in the wavelength range  -  + d
d
  + d
E = f()
RADIATION
HEAT AND MASS TRANSFER
Monochromatic/Spectral emissivity (ο₯) – Ratio of monochromatic hemispherical emissive
power of a non-black body to that of a black body at same temperature & wavelength.
ο₯ b

ο₯ 

For grey body
ο₯  = Constant
ABSORBTIVITY (), REFLECTIVITY (), TRANSMITIVITY ()
HEAT AND MASS TRANSFER
 = Fraction of radiation energy incident upon a surface which
is absorbed by it.
 = Fraction of radiation energy incident upon a surface which
is reflected by it.
 = Fraction of radiation energy incident upon a surface which
is transmitted through it.
For any surface,  +  +  = 1
For opaque surface,  +  = 1 (  = 0 )
For black body,  = b = 1
ABSORBTIVITY (), REFLECTIVITY (), TRANSMITIVITY ()
HEAT AND MASS TRANSFER
Sun
Earth
Short wavelength Long wavelength
Co2
LAWS OF THERMAL RADIATION
HEAT AND MASS TRANSFER
1.Kirchhoff's law of thermal radiation – States that whenever a body is in thermal
equilibrium with its surroundings, its emissivity is equal to its absorptivity.
ο₯ = 
β€œA good absorber is always a good emitter”
For black body
b = 1
ο₯b = 1
LAWS OF THERMAL RADIATION
HEAT AND MASS TRANSFER
2.Plank’s law of thermal radiation – The law states that the monochromatic emissive
power of a black body is dependent both upon the absolute temperature of the body and
the wavelength of radiation energy emitted.
Eb = f (,T)
LAWS OF THERMAL RADIATION
HEAT AND MASS TRANSFER
3.Stefan-Boltzman’s law – The law states that the total hemispherical emissive power of a
black body is directly proportional to the fourth power of the absolute temperature of the
black body.
Eb ο‚΅ T4
Eb =  T4 watt/m2
 = Stefan-Boltzman’s constant
= 5.67 X 10-8 w/m2K4
LAWS OF THERMAL RADIATION
HEAT AND MASS TRANSFER
4.Weins displacement law – For a non black body, whose emissivity is ο₯ , The total
hemispherical emissive power of non-black body E = ο₯Eb
E = ο₯  T4
If β€œA” is the total surface area of non-black body, The total radiation energy emitted from
entire non-black body = EA watt
= ο₯  T4A
SHAPE FACTOR
HEAT AND MASS TRANSFER
1 2
Radiation energy leaving 1
Radiation energy leaving 2
F12 = Fraction of radiation
energy leaving surface 1
and that of reaching
surface 2.
F21 = Fraction of radiation
energy leaving surface 2
and that of reaching
surface 1.
0 ο‚£ Fmn ο‚£ 1
SHAPE FACTOR
HEAT AND MASS TRANSFER
Shapes with size difference Flat surface
Concave surface Convex surface
Reciprocity relationship
A1 F12 = A2 F21
F21 > F12
F11 = 0
F11 = 0
F11 > 0
RADIATION HEAT EXCHANGE
HEAT AND MASS TRANSFER
CASE 1 Two infinitely large parallel plates
Assumptions – 1. Steady state heat transfer conditions Tο‚Ή f(t)
2. Surfaces are diffuse and grey. ο₯ = f ()
Net radiation heat exchange between 1 and 2 per unit area is
(q/A)1-2 =
 ( 𝑇1
4
βˆ’π‘‡2
4
)
1
ο₯1
+
1
ο₯2
βˆ’1
Watt/m2 = Radiation flux
In case both the surfaces are black, ο₯1 = ο₯2 = 1
(q/A)1-2 =  ( 𝑇1
4 βˆ’ 𝑇2
4) w/m2
RADIATION HEAT EXCHANGE
HEAT AND MASS TRANSFER
CASE 2 Two infinitely long concentric cylindrical surfaces
RADIATION HEAT EXCHANGE
HEAT AND MASS TRANSFER
CASE 2 Two infinitely long concentric cylindrical surfaces
Assumptions – 1. Steady state heat transfer conditions Tο‚Ή f(t)
2. Surfaces are diffuse and grey. ο₯ = f ()
3. Let T1 > T2
Net radiation heat exchange between 1 and 2 is
(q)1-2 =
 𝑇1
4
βˆ’π‘‡2
4
𝐴1
1
ο₯1
+
𝐴1
𝐴2
(
1
ο₯2
βˆ’1)
Watt
F12 = 1
F21 < 1
𝐴1
𝐴2
=
𝑅1
𝑅2
TYPES OF HEAT EXCHANGERS
HEAT AND MASS TRANSFER
Heat exchanger is a steady flow adiabatic open system device
in which two flowing fluids exchange or transfer heat without
loosing or gaining any heat from the ambient.
TYPES OF HEAT EXCHANGERS
HEAT AND MASS TRANSFER
Surface (steam) condenser
Steam to cold water
Economizer
Hot flue gas to cold water
Superheater
Hot flue gas to dry saturated steam
Air preheater
Hot flue gas to combustion air Cooling tower
Hot water to atmospheric air
Oil cooler
Hot oil to cool water/air
FIRST LAW OF THERMODYNAMICS
HEAT AND MASS TRANSFER
Q – W = H + KE + PE
Q = 0 (adiabatic),W = 0 , KE = 0, PE = 0 (no datum change)
(H)HE = 0
(H)Hot fluid + (H)Cold fluid = 0
- (H)Hot fluid = +(H)Cold fluid
β€œ Rate of enthalpy decrease of hot fluid = Rate of enthalpy increase of cold fluid β€œ
ሢ
π‘šh Cph (Thi – The) = ሢ
π‘šc Cpc (Tce – Tci)
CLASSIFICATION OF HEAT EXCHANGER
HEAT AND MASS TRANSFER
HE
Direct
transfer
Parallel
Counter
Cross
Direct
contact
Regenerative/
storage
CLASSIFICATION OF HEAT EXCHANGER
HEAT AND MASS TRANSFER
Direct
transfer
Parallel Counter Cross
Parallel flow HE – An automobile radiator
1
π‘ˆ
=
1
β„Ž1
+
1
β„Ž2
T = Th – Tc
= f (x)
dq = U T dA
Tce > The
CLASSIFICATION OF HEAT EXCHANGER
HEAT AND MASS TRANSFER
(S)Parallel flow HE > (S)Counter flow HE
Counter flow HE is thermodynamically more
efficient than parallel flow HE.
Mean Temperature Difference MTD (Tm)
HEAT AND MASS TRANSFER
A parameter which takes into account the variation of temperature with respect to direction
of flow of hot fluid by taking average all along the length of HE from inlet to exit.
Q = U A Tm
Q = Total heat transfer rate.
U = Overall heat transfer coefficient.
A = Total heat transfer area of HE.
Tm = Mean Temperature Difference.
Equation - 1
Mean Temperature Difference MTD (Tm)
HEAT AND MASS TRANSFER
dq = U T dA
‫׬‬𝐼𝑛𝑙𝑒𝑑
𝐸π‘₯𝑖𝑑
π‘‘π‘ž = ‫׬‬𝐼𝑛𝑙𝑒𝑑
𝐸π‘₯𝑖𝑑
π‘ˆο„T dA
Q = U ‫׬‬𝐼𝑛𝑙𝑒𝑑
𝐸π‘₯𝑖𝑑
T dA
From equation 1 and 2, we have
Tm =
𝟏
𝑨
‫׬‬𝐼𝑛𝑙𝑒𝑑
𝐸π‘₯𝑖𝑑
T dA
Equation - 2
Logarithmic Mean Temperature Difference LMTD (Tm)
HEAT AND MASS TRANSFER
Parallel flow HE
Logarithmic Mean Temperature Difference LMTD (Tm)
HEAT AND MASS TRANSFER
Parallel flow HE
dq = U T dA
dA = B dx
T = Th – Tc = f (x)
At x = 0, T = Ti = Thi – Tci
At x = L, T = Te = The – Tce
Also dq = - ሢ
π‘š h Cph dT = + ሢ
π‘š h Cpc dT
Now T = Th – Tc
d(T) = dTh – dTc
d(T) = -
π‘‘π‘ž
ሢ
π‘šβ„Ž
πΆπ‘β„Ž
-
π‘‘π‘ž
ሢ
π‘šπ‘
𝐢𝑝𝑐
Logarithmic Mean Temperature Difference LMTD (Tm)
HEAT AND MASS TRANSFER
Parallel flow HE
d(T) = - dq
1
ሢ
π‘šβ„Ž
πΆπ‘β„Ž
+
1
ሢ
π‘šπ‘
𝐢𝑝𝑐
d(T) = - U T dA
1
ሢ
π‘šβ„Ž
πΆπ‘β„Ž
+
1
ሢ
π‘šπ‘
𝐢𝑝𝑐
Separating the variables, we have
ΰΆ±
βˆ†π‘‡π‘–
βˆ†π‘‡π‘’
βˆ’
d(T)
T
= ΰΆ±
0
𝐿
π‘ˆ 𝐡
1
ሢ
π‘šβ„Ž πΆπ‘β„Ž
+
1
ሢ
π‘šπ‘ 𝐢𝑝𝑐
ln
βˆ†π‘‡π‘–
βˆ†π‘‡π‘’
= U B L
1
ሢ
π‘šβ„Ž
πΆπ‘β„Ž
+
1
ሢ
π‘šπ‘
𝐢𝑝𝑐
Q = Total heat rate of entire HE = ሢ
π‘šβ„Ž πΆπ‘β„Ž (Thi – The)
= ሢ
π‘šπ‘ 𝐢𝑝𝑐 (Tce – Tci)
Logarithmic Mean Temperature Difference LMTD
HEAT AND MASS TRANSFER
Parallel flow HE
ln
βˆ†π‘‡π‘–
βˆ†π‘‡π‘’
= U A
π‘‡β„Žπ‘– βˆ’π‘‡β„Žπ‘’
𝑄
+
𝑇𝑐𝑒 βˆ’π‘‡π‘π‘–
𝑄
=
π‘ˆπ΄
𝑄
( Ti - Te )
Q = U A
Ti βˆ’ Te
ln βˆ†π‘‡π‘–
βˆ†π‘‡π‘’
, Comparing this with Q = U A Tm , We have
Tm = (T)LMTD =
Ti βˆ’ Te
ln βˆ†π‘»π’Š
βˆ†π‘»π’†
Logarithmic mean temperature
difference for parallel flow HE
Logarithmic Mean Temperature Difference LMTD
HEAT AND MASS TRANSFER
Counter flow HE
Logarithmic Mean Temperature Difference LMTD
HEAT AND MASS TRANSFER
Counter flow HE
(T)LMTD =
Ti βˆ’ Te
ln βˆ†π‘»π’Š
βˆ†π‘»π’†
SPECIAL CASES
HEAT AND MASS TRANSFER
When one of the fluids in the HE is undergoing phase change like a steam
condenser or evaporator or steam generator.
Steam Condenser
LMTD Parallel = LMTD Counter
SPECIAL CASES
HEAT AND MASS TRANSFER
Steam Generator
LMTD Parallel = LMTD Counter
SPECIAL CASES
HEAT AND MASS TRANSFER
When both hot and cold fluids have equal capacity rates in a counter flow
heat exchanger.
ሢ
π‘šβ„Ž πΆπ‘β„Ž = ሢ
π‘šπ‘ 𝐢𝑝𝑐
Then from energy balance equation,
ሢ
π‘šβ„Ž πΆπ‘β„Ž ( Thi –The ) = ሢ
π‘šπ‘ 𝐢𝑝𝑐 ( Tce – Tci )
( Thi –The ) = ( Tce – Tci )
Thi – Tce = The – Tci
Ti = Te
(T)LMTD =
Ti βˆ’ Te
ln βˆ†π‘»π’Š
βˆ†π‘»π’†
=
𝟎
𝟎
= Undefined = Ti Or Te
ሢ
π‘š 𝐢𝑝 = Heat capacity rate
L’Hospital’s rule
Effectiveness of HE (ο₯)
HEAT AND MASS TRANSFER
It is defined as the ratio between actual heat transfer rate taking place between hot and
cold fluids and the maximum possible heat transfer rate between them.
ο₯HE =
𝒒 𝒂𝒄𝒕𝒖𝒂𝒍
𝒒 π’Žπ’‚π’™
𝒒 𝒂𝒄𝒕𝒖𝒂𝒍 = Rate of enthalpy change of either fluid
= ሢ
π‘šβ„Ž πΆπ‘β„Ž ( Thi –The ) = ሢ
π‘šπ‘ 𝐢𝑝𝑐 ( Tce – Tci )
𝒒 π’Žπ’‚π’™ = ሢ
π‘š 𝐢𝑝 ( Thi –Tci )
ሢ
π‘š 𝐢𝑝 = Heat capacity rate
NUMBER OF TRANSFER UNITS NTU
HEAT AND MASS TRANSFER
The number of transfer units (NTU = UA/(mcp)) itself is a combination of overall
heat transfer coefficients, transfer area, fluid flow rate and heat capacity.
It summarizes these dimensional parameters into one dimensionless parameter. The
performance becomes a monotone function of this dimensionless parameter.
It indicates overall size of HE.
NTU =
𝑼𝑨
ሢ
π’Ž π‘ͺ𝒑 π‘Ίπ’Žπ’‚π’π’
FOULING FACTOR (F)
HEAT AND MASS TRANSFER
It takes into account the thermal resistance offered by any chemical scaling or deposits that
are formed on the heat transfer surface on both hot side and cold side.
Generally ranges from 0.0004 – 0.0006
𝟏
𝑼
=
𝟏
π’‰πŸ
+ F1 +
𝟏
π’‰πŸ
+ F2
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Heat and Mass Transfer - HMT

  • 1. Workshop Technology OR Machine Shop Theory Heat And Mass Transfer – HMT Production planning and control – PPC Applied Mechanics Or Engineering Mechanics Engineering Materials or Material Science Engineering Thermodynamics Or Applied Thermodynamics IC Engines Engineering Mathematics - Numerical Analysis & more Strength of material OR Mechanics of solid @thelearninghub2019 @essentialamalgame @jaatishrao
  • 2. HEAT AND MASS TRANSFER HEAT AND MASS TRANSFER
  • 3. SCOPE OF THE COURSE ሢ 𝐐 Q THERMODYNAMIC ANALYSIS HEAT TRANSFER ANALYSIS Deals with system in equilibrium. That is to bring a system from one equilibrium state to another, how much amount of heat is required. Evaluates at what rate the change of state occurs by calculating rate of heat transfer in Joule/Sec = Watt. HEAT AND MASS TRANSFER
  • 4. SCOPE OF THE COURSE SN Section/Units Contents 1. Introduction Modes of heat transfer and Governing laws of heat transfer 2. Conduction Thermal conductivity, Heat conduction in gases, Intepretation Of Fourier's law, Electrical analogy of heat transfer, Critical radius of insulation, Heat generation in a slab and cylinder, Fins, Unsteady/Transient conduction 3. Convection Forced convection heat transfer, Reynold’s Number, Prandtl Number, Nusselt Number, Incompressible flow over flat surface, HBL, TBL, Forced convection in flow through pipes and ducts, Free/Natural convection 4. Radiation Absorbtivity, Reflectivity, Transmitivity, Laws of thermal radiation, Shape factor, Radiation heat exchange 5. Heat Exchangers Types of heat exchangers, First law of thermodynamics, Classification of heat exchangers, LMTD for parallel and counter flow, NTU, Fouling factor. HEAT AND MASS TRANSFER
  • 5. MODES OF HEAT TRANSFER MODES Conduction Convection Radiation HEAT AND MASS TRANSFER
  • 6. MODES OF HEAT TRANSFER Conduction – The mode of heat transfer which generally (mark the word) occurs in a solid body due to temperature difference associated with molecular lattice’s vibrational energy as well by transfer of free electrons. This is the reason behind why all electrically good conductors are also in general a good conductor of heat as well. Viz the presence of abundant FREE electrons. EXCEPTION = Diamond HT LT HEAT AND MASS TRANSFER
  • 7. MODES OF HEAT TRANSFER HEAT AND MASS TRANSFER
  • 8. MODES OF HEAT TRANSFER Convection – The mode of heat transfer which generally occurs between solid surface and the surrounding fluid due to temperature difference associated with macroscopic bulk motion of the fluid transporting thermal energy. Natural Convection Forced Convection HEAT AND MASS TRANSFER
  • 9. MODES OF HEAT TRANSFER Radiation – All matter with a temperature greater than absolute zero (viz 0 K)emits thermal radiation. The rate of emission occurs in form of electromagnetic waves which can propagate even through the vacuum ! Radiation is the mode of heat transfer which does not require any material medium and occurs at electromagnetic wave propagation travelling with speed of light. HEAT AND MASS TRANSFER
  • 10. GOVERNING LAWS OF HEAT TRANSFER 1. Fourier’s law of conduction – The law states that the rate of heat transfer by conduction along a direction (given) is directly proportional to the temperature gradient along that direction and is also proportional to the area of heat transfer lying perpendicular to the direction of heat transfer. Qx ο‚΅ - 𝑑𝑇 𝑑π‘₯ Qx ο‚΅ A Qx = K A ( 𝑑𝑇 𝑑π‘₯ ) HEAT AND MASS TRANSFER K = Thermal conductivity
  • 11. GOVERNING LAWS OF HEAT TRANSFER 2. Newton’s law of cooling (For Convection) – The law states that the rate of heat transfer by convection between a solid body and surrounding fluid is directly proportional to the temperature difference between them and is also directly proportional to the area of contact or area of exposure between them. Qconv ο‚΅ (Tw - Tο‚₯) Qconv ο‚΅ A Qconv = h A (Tw - Tο‚₯ ) HEAT AND MASS TRANSFER h = Heat transfer coefficient of convection.
  • 12. GOVERNING LAWS OF HEAT TRANSFER HEAT AND MASS TRANSFER K = Thermal conductivity = Property of the material h = Heat coefficient for convection ο‚Ή Property of the material In forced convection h = f (v,D,,,Cp,k) In free convection h = f (g,,,L,,,Cp,k)
  • 13. GOVERNING LAWS OF HEAT TRANSFER HEAT AND MASS TRANSFER Ranges of β€œh” SN Convection Value (Watt/m2K) 1 Free convection in gases. 3 - 25 2 Forced convection in gases. 25 – 400 3 Free convection in liquids. 250 – 600 4 Forced convection in liquids. 600 – 4000 5 Condensation heat transfer. 3000 – 25000 6 Boiling heat transfer. 5000 - 50000
  • 14. GOVERNING LAWS OF HEAT TRANSFER 3.Stefan-Boltzman’s law of Radiation – The law states that the radiation energy emitted from the surface of a black body (per unit time, per unit area) is directly proportional to the 4th power of the absolute temperature of the black body. Eb ο‚΅ T4 β€œT” is in Kelvin Eb =  T4 HEAT AND MASS TRANSFER  = Stefan-Boltzman constant = 5.67 X 10-8 Watt/m2K
  • 15. THERMAL CONDUCTIVITY (K) HEAT AND MASS TRANSFER It is a thermo-physical property of a material which tells about the ability of material to allow heat energy to get conducted through the material more rapidly/quickly. Insulators (a substance which does not readily allow the passage of heat) have very low thermal conductivity and hence prevents the conduction heat transfer rate. SN Material (Insulators) K (Watt/mK) 1. Asbestos 0.2 2. Refractory bricks 0.9 3. Glass wool 0.075 4. Polyurethane foam 0.02
  • 16. HEAT CONDUCTION IN GASES HEAT AND MASS TRANSFER Heat conduction occurs in gases by molecular momentum transfer when high velocity and high temperature molecules collides with the low velocity low temperature molecules. However, in general gases are bad conductor of heat. Kair =0.026 w/mK
  • 17. HEAT CONDUCTION IN GASES HEAT AND MASS TRANSFER As the temperature of gases increase, their thermal conductivity also increases. This is because at high temperature of gases, increased molecular activity may result in more no of collisions per unit time and hence more momentum transfer rate & hence more thermal heat conductivity. K T (Celsius)
  • 18. HEAT AND MASS TRANSFER K = 8.43 w/mK HIGHEST A Thermometric Fluid. Low vapour Pressure HEAT CONDUCTION IN GASES
  • 19. FOURIER’S LAW INTEPRETATION HEAT AND MASS TRANSFER ASSUMPTIONS :- ❖ Steady state heat transfer conditions. T ο‚Ή f (Time) ❖ One dimensional heat conduction. T = f (x) ❖ Uniform/Constant value of β€œK” BOUNDARY CONDITIONS At x = 0, T = T1 At x = b, T = T2
  • 20. FOURIER’S LAW INTEPRETATION HEAT AND MASS TRANSFER ΰΆ± π‘₯=0 π‘₯=𝑏 π‘žπ‘₯ 𝑑π‘₯ = ΰΆ± 𝑇1 𝑇2 βˆ’πΎπ΄ 𝑑𝑇 To satisfy steady state conditions, qx ο‚Ή f (x) Viz qx = qx+dx qx X b = KA (T1-T2) qx = 𝑲𝑨 (π‘»πŸ βˆ’π‘»πŸ ) 𝒃 & qx 𝑨 = 𝑲 (π‘»πŸ βˆ’π‘»πŸ ) 𝒃
  • 21. ELECTRICAL ANALOGY OF HEAT TRANSFER HEAT AND MASS TRANSFER Electrical Thermal i (Ampere) q (Watt) V (Volts) T (Celsius/Kelvin) Relectrical RThermal i q Relectrical RThermal V T Relectrical = V 𝑖 Ohms RThermal= 𝑇 π‘ž K/Watt
  • 22. ELECTRICAL ANALOGY OF HEAT TRANSFER HEAT AND MASS TRANSFER (RTh)Conduction = 𝑇1 βˆ’π‘‡2 π‘ž = 𝑏 𝐾𝐴
  • 23. CONDUCTION HEAT TRANSFER THROUGH A COMPOSITE SLAB HEAT AND MASS TRANSFER T1 T2 T3 q RTh(1-2) = 𝑏1 𝐾1 𝐴 RTh(2-3) = 𝑏2 𝐾2 𝐴 RTh(1-3) = 𝑏1 𝐾1 𝐴 + 𝑏2 𝐾2 𝐴 RTh(1-3) = 𝑇 π‘ž = 𝑇1 βˆ’π‘‡3 π‘ž Rate of conduction heat Transfer β€œq” is given by - q = 𝑇 RTh(1βˆ’3) = 𝑇1 βˆ’π‘‡3 𝑏1 𝐾1 𝐴 + 𝑏2 𝐾2 𝐴 π‘ž 𝐴 = π»π‘’π‘Žπ‘‘ 𝑓𝑙𝑒π‘₯ = 𝑇1 βˆ’ 𝑇3 𝑏1 𝐾1 + 𝑏2 𝐾2
  • 24. NUMERICAL HEAT AND MASS TRANSFER Calculate the value of thermal conductivity of insulator in the composite slab as shown in the adjoining figure. 500 K 360 K q = 10,000 w/m2 20 1000𝑋10𝑋𝐴 1 1000𝑋𝐾𝑋𝐴 20 1000𝑋10𝑋𝐴
  • 25. NUMERICAL HEAT AND MASS TRANSFER 500 K 360 K q/A = 10,000 w/m2 20 1000𝑋10𝑋𝐴 1 1000𝑋𝐾𝑋𝐴 20 1000𝑋10𝑋𝐴 Heat flux = q/A = 𝑇 π‘…π‘‡β„Ž q/A = 500βˆ’360 20 10000 + 1 1000𝐾 + 20 10000 10000 = 500βˆ’360 20 10000 + 1 1000𝐾 + 20 10000 K = 0.1 w/mK
  • 26. CONVECTION THERMAL RESISTANCE HEAT AND MASS TRANSFER qconv = h A (Tw - Tο‚₯) (RTh)Covection = Tw βˆ’ Tο‚₯ π‘ž = 1 β„Žπ΄
  • 27. CONDUCTION - CONVECTION HEAT TRANSFER THROUGH A COMPOSITE SLAB HEAT AND MASS TRANSFER
  • 28. CONDUCTION - CONVECTION HEAT TRANSFER THROUGH A COMPOSITE SLAB HEAT AND MASS TRANSFER TG Tο‚₯ T1 T2 T3 1 β„Ž1𝐴 𝑏1 𝐾1𝐴 𝑏2 𝐾2𝐴 1 β„Ž2𝐴 q q = 𝑇𝐺 βˆ’π‘‡βˆž 1 β„Ž1 𝐴 + 𝑏1 𝐾1 𝐴 + 𝑏2 𝐾2 𝐴 + 1 β„Ž2 𝐴 = Rate of heat transfer. q/A = 𝑇𝐺 βˆ’π‘‡βˆž 1 β„Ž1 + 𝑏1 𝐾1 + 𝑏2 𝐾2 + 1 β„Ž2 = Heat flux (w/m2) q = UA (𝑇𝐺 βˆ’ π‘‡βˆž) Remember Resistance = 𝑻 𝒒 𝟏 𝑼 = 𝟏 π’‰πŸ + π’ƒπŸ π‘²πŸ + π’ƒπŸ π‘²πŸ + 𝟏 π’‰πŸ
  • 29. RADIAL CONDUCTION THROUGH HOLLOW CYLINDER HEAT AND MASS TRANSFER
  • 30. RADIAL CONDUCTION THROUGH HOLLOW CYLINDER HEAT AND MASS TRANSFER Area of conduction heat transfer = 2rL q = - K A ( 𝑑𝑇 π‘‘π‘Ÿ ) = - K 2rL ( 𝑑𝑇 π‘‘π‘Ÿ ) At r = r1, T = T1 At r = r2, T = T2 ‫׬‬ π‘Ÿ1 π‘Ÿ2 π‘ž π‘‘π‘Ÿ π‘Ÿ = - ‫׬‬ 𝑇1 𝑇2 2 𝐾𝐿 𝑑𝑇 q ln ( π‘Ÿ2 π‘Ÿ1 ) = 2𝐾𝐿 (T1-T2) q = 2𝑲𝑳 (T1βˆ’T2) ln (π’“πŸ π’“πŸ ) & RTh = 𝑻 𝒒 = ln (π’“πŸ π’“πŸ ) 2𝐾𝐿
  • 31. RADIAL CONDUCTION THROUGH COMPOSITE CYLINDER HEAT AND MASS TRANSFER
  • 32. RADIAL CONDUCTION THROUGH COMPOSITE CYLINDER HEAT AND MASS TRANSFER T1 T2 T3 q 𝑙𝑛 π‘Ÿ2 π‘Ÿ1 2πœ‹πΎ1𝐿 𝑙𝑛 π‘Ÿ3 π‘Ÿ2 2πœ‹πΎ2𝐿 q = 𝑇1 βˆ’π‘‡3 𝑙𝑛 π‘Ÿ2 π‘Ÿ1 2πœ‹πΎ1 𝐿 + 𝑙𝑛 π‘Ÿ3 π‘Ÿ2 2πœ‹πΎ2 𝐿
  • 33. RADIAL CONDUCTION-CONVECTION HEAT TRANSFER THROUGH COMPOSITE CYLINDER HEAT AND MASS TRANSFER h1 = Heat transfer coefficient of convection (inside) h2 = Heat transfer coefficient of convection (outside) TG Tο‚₯ T1 T2 T3 q (Convection)inner Conduction (Convection)Outer Conduction 1 β„Ž1(2πœ‹π‘Ÿ1𝐿) 𝑙𝑛 π‘Ÿ2 π‘Ÿ1 (2πœ‹πΎ1𝐿) 𝑙𝑛 π‘Ÿ3 π‘Ÿ2 (2πœ‹πΎ2𝐿) 1 β„Ž2(2πœ‹π‘Ÿ3𝐿) q = 2πœ‹π‘Ÿ1𝐿 (𝑇𝐺 βˆ’π‘‡βˆž ) 1 β„Ž1 (2πœ‹π‘Ÿ1 𝐿) + 𝑙𝑛 π‘Ÿ2 π‘Ÿ1 (2πœ‹πΎ1 𝐿) + 𝑙𝑛 π‘Ÿ3 π‘Ÿ2 (2πœ‹πΎ2 𝐿) + 1 β„Ž2 (2πœ‹π‘Ÿ3 𝐿) q = UiAiT = U0A0T = Ui (2πœ‹π‘Ÿ1𝐿)(𝑇𝐺 βˆ’ π‘‡βˆž) = U0 (2πœ‹π‘Ÿ3𝐿)(𝑇𝐺 βˆ’ π‘‡βˆž) A B Also,
  • 34. RADIAL CONDUCTION-CONVECTION HEAT TRANSFER THROUGH COMPOSITE CYLINDER HEAT AND MASS TRANSFER 1 π‘ˆπ‘– = 1 β„Ž1 + π‘Ÿ1 𝐾1 ln π‘Ÿ2 π‘Ÿ1 + π‘Ÿ1 𝐾2 ln π‘Ÿ3 π‘Ÿ2 + π‘Ÿ1 π‘Ÿ3 1 β„Ž2 Comparing equation A and B 1 π‘ˆπ‘œ = 1 β„Ž2 + π‘Ÿ3 𝐾1 ln π‘Ÿ2 π‘Ÿ1 + π‘Ÿ3 𝐾2 ln π‘Ÿ3 π‘Ÿ2 + π‘Ÿ3 π‘Ÿ1 1 β„Ž1 𝟏 𝐔 = 𝟏 𝐑𝟏 + 𝟏 𝐑𝟐 Thermal resistance of conduction gets neglected since ri = ro (approx)
  • 35. CRITICAL RADIUS OF INSULATION HEAT AND MASS TRANSFER
  • 36. HEAT AND MASS TRANSFER CRITICAL RADIUS OF INSULATION Conduction Convection 𝑙𝑛 π‘Ÿπ‘œ π‘Ÿπ‘– 2πœ‹πΎπΏ 1 β„Ž (2πœ‹π‘Ÿ0𝐿) q Ti Tο‚₯ q = 𝑇𝑖 βˆ’π‘‡ο‚₯ 𝑙𝑛 π‘Ÿπ‘œ π‘Ÿπ‘– 2πœ‹πΎπΏ + 1 β„Ž (2πœ‹π‘Ÿ0 𝐿) q = f(ro) & dq/dr = 0 (For maximum heat transfer) 𝑑 π‘‘π‘Ÿπ‘œ 𝑇𝑖 βˆ’π‘‡ο‚₯ 𝑙𝑛 π‘Ÿπ‘œ π‘Ÿπ‘– 2πœ‹πΎπΏ + 1 β„Ž (2πœ‹π‘Ÿ0 𝐿) = 0 GIVES ro = πΎπΌπ‘›π‘ π‘’π‘™π‘Žπ‘‘π‘–π‘œπ‘› β„Ž Critical radius of insulation
  • 37. CRITICAL RADIUS OF INSULATION HEAT AND MASS TRANSFER Electric power transmission cables Semiconductor devices Practical application of critical radius of insulation rcritical = K/h rcritical = 2K/h
  • 38. RADIAL CONDUCTION THROUGH HOLLOW SPHERE HEAT AND MASS TRANSFER A = 42
  • 39. RADIUS CONDUCTION THROUGH HOLLOW SPHERE HEAT AND MASS TRANSFER q = - K A 𝑑𝑇 π‘‘π‘Ÿ (From Fourier’s law of conduction) = - K 4r2 ( 𝑑𝑇 π‘‘π‘Ÿ ) π‘ž β‰  𝑓 π‘Ÿ 𝑣𝑖𝑧 π‘žπ‘Ÿ = π‘žπ‘Ÿ + π‘‘π‘Ÿ β€«Χ¬β€¬π‘Ÿ1 π‘Ÿ2 π‘ž π‘‘π‘Ÿ π‘Ÿ2 = ‫׬‬𝑇1 𝑇2 βˆ’ 4πœ‹πΎπ‘‘π‘‡ q = 4πœ‹πΎ 𝑇1 βˆ’π‘‡2 π‘Ÿ1 π‘Ÿ2 π‘Ÿ2 βˆ’π‘Ÿ1 RTh q T1 T2 RTh = βˆ†π‘‡ π‘ž = π‘Ÿ2 βˆ’π‘Ÿ1 4πœ‹πΎπ‘Ÿ1 π‘Ÿ2
  • 40. DERIVATION OF GENERALIZED HEAT CONDUCTION EQUATION HEAT AND MASS TRANSFER qx = heat conducted into the element in X-direction = - K A ( 𝑑𝑇 𝑑π‘₯ ) watt qx+dx = Heat conducted out of the element along X – direction. = qx + πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ qgenerated = ሢ π‘ž A dx watt
  • 41. GENERALIZED HEAT CONDUCTION EQUATION DERIVATION HEAT AND MASS TRANSFER Writing energy balance equation of X-direction conduction qx + qgenerated = qx+dx + Rate of change of internal energy qx + ሢ π‘ž A dx = qx + πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ + πœ• πœ•π‘‘ ( mcpT) t = sec, m = element’s mass =  X (A dx) ሢ π‘ž A dx = πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ + πœ• πœ•π‘‘ ( X (Adx) cp T) K πœ•2 𝑇 πœ•π‘₯2 + ሢ π‘ž =  cp πœ•π‘‡ πœ•π‘‘ Writing energy balance equation for all 3 dimensions. K πœ•2 𝑇 πœ•π‘₯2 + K πœ•2 𝑇 πœ•π‘¦2 + K πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž =  cp πœ•π‘‡ πœ•π‘‘
  • 42. GENERALIZED HEAT CONDUCTION EQUATION DERIVATION HEAT AND MASS TRANSFER πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž/K =  cp X 1 𝐾 πœ•π‘‡ πœ•π‘‘ Here 𝐾  cp =  = Thermal diffusivity, A thermophysical property of material (The ratio between thermal conductivity of the material and its thermal capacity.) πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž/K = 1  πœ•π‘‡ πœ•π‘‘ πœ•π‘‡ πœ•π‘‘ = 0, T ο‚Ή f(t) (Steady conditions) ሢ π‘ž = 0 (No heat generation) πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 = 0 gases > liquid 𝛻2 T = 0 Laplace’s equation in T
  • 43. HEAT GENERATION IN A SLAB HEAT AND MASS TRANSFER Assumptions (1) Steady state heat transfer conditions. T ο‚Ή f(t) (2) One dimensional heat transfer T = f(x) (3) Uniform heat generation rate. (4) Constant value of β€œK” πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž/K = 1  πœ•π‘‡ πœ•π‘‘
  • 44. HEAT GENERATION IN A SLAB HEAT AND MASS TRANSFER πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž/K = 1  πœ•π‘‡ πœ•π‘‘ 𝑑2 𝑇 𝑑π‘₯2+ ሢ π‘ž/K = 0 𝑑2 𝑇 𝑑π‘₯2 = - ሢ π‘ž/K 𝑑𝑇 𝑑π‘₯ = - ሢ π‘ž/K x + C1 T = - ሢ π‘ž/K π‘₯2 2 + C1x + C2 Boundary conditions At x = +L and x = -L Gives T = Tw (Also renders C1 = 0)
  • 45. HEAT GENERATION IN A SLAB HEAT AND MASS TRANSFER Temperature of the slab is max when 𝑑𝑇 𝑑π‘₯ = 0 which gives x = 0 Viz max temperature of slab would be at centerline Now in case both sides of the slab are at different temperature then C1 would not be zero and hence max temp will not be at midplane (centerline) For such case, Let max temperature of slab as To At x = 0, T = T0 Viz C2 = 0 Which gives; T = - ሢ π‘ž/K π‘₯2 2 + T0 T – T0 = - ሢ π‘ž/K π‘₯2 2 T = - ሢ π‘ž/K π‘₯2 2 + C1x + C2 Parabolic temperature distribution A
  • 46. HEAT GENERATION IN A SLAB HEAT AND MASS TRANSFER At x = +L Or x = -L ; T = Tw T0 – Tw = π‘ž 𝐿2 2𝐾 Dividing equation A & B we have; 𝐴 𝐡 = T – T0 T0 – Tw = ( π‘₯ 𝐿 )2 B Non-dimensional temperature distribution Heat generated in slab = Heat out through convection ሢ π‘ž X (2L X A) = 2h A (Tw – Tο‚₯) Tw = ሢ π‘žπΏ β„Ž + Tο‚₯
  • 47. HEAT GENERATION IN A SLAB HEAT AND MASS TRANSFER Also from equation B we have T0 or Tmax = π‘ž 𝐿2 2𝐾 + ሢ π‘žπΏ β„Ž + Tο‚₯
  • 48. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER r = 0 Tw Tw i R qconvection Tο‚₯ h L ሢ π‘ž = Heat generation rate = 𝑖2 π‘…π‘’π‘™π‘’π‘π‘‘π‘Ÿπ‘–π‘ 𝑅2 𝐿
  • 49. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER πœ•2 𝑇 πœ•π‘₯2 + πœ•2 𝑇 πœ•π‘¦2 + πœ•2 𝑇 πœ•π‘§2 + ሢ π‘ž/K = 1  πœ•π‘‡ πœ•π‘‘ 1 π‘Ÿ πœ• πœ•π‘Ÿ (π‘Ÿ πœ•π‘‡ πœ•π‘Ÿ ) + ሢ π‘ž 𝐾 = 1 𝛼 πœ•π‘‡ πœ•π‘‘ 1 π‘Ÿ2 πœ• πœ•π‘Ÿ (π‘Ÿ2 πœ•π‘‡ πœ•π‘Ÿ ) + ሢ π‘ž 𝐾 = 1 𝛼 πœ•π‘‡ πœ•π‘‘ Generalized heat conduction coordinate systems. Rectilinear coordinate system Cylindrical coordinate system Spherical coordinate system
  • 50. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER 1 π‘Ÿ πœ• πœ•π‘Ÿ (π‘Ÿ πœ•π‘‡ πœ•π‘Ÿ ) + ሢ π‘ž 𝐾 = 1 𝛼 πœ•π‘‡ πœ•π‘‘ 𝑑2𝑇 π‘‘π‘Ÿ2 + 1 π‘Ÿ 𝑑𝑇 π‘‘π‘Ÿ = βˆ’ ሢ π‘ž 𝐾 r 𝑑2 𝑇 π‘‘π‘Ÿ2 + 𝑑𝑇 π‘‘π‘Ÿ = βˆ’ ሢ π‘žπ‘Ÿ 𝐾 𝑑 π‘‘π‘Ÿ (π‘Ÿ 𝑑𝑇 π‘‘π‘Ÿ ) = βˆ’ ሢ π‘žπ‘Ÿ 𝐾 Integrating w.r.t β€œr” π‘Ÿ 𝑑𝑇 π‘‘π‘Ÿ = βˆ’ ሢ π‘žπ‘Ÿ2 2𝐾 + C1 𝑑𝑇 π‘‘π‘Ÿ = βˆ’ ሢ π‘žπ‘Ÿ 2𝐾 + 𝐢1 π‘Ÿ 𝑑𝑇 π‘‘π‘Ÿ At r = R = βˆ’ ሢ π‘žπ‘… 2𝐾 + 𝐢1 𝑅 Equation 1
  • 51. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER Again integrating T = βˆ’ ሢ π‘žπ‘Ÿ2 4𝐾 + C1 log r + C2 From boundary condition (2) Heat generated in the rod = Heat conducted radially at the surface = Heat convected from the surface to the fluid. ሢ π‘ž X R2L = - K (2RL) 𝑑𝑇 π‘‘π‘Ÿ At r = R 𝑑𝑇 π‘‘π‘Ÿ At r = R = βˆ’ ሢ π‘žπ‘Ÿ 2𝐾 From equation 1 and 2 C1 = 0 Boundary conditions (1) AT r = R, T = Tw (2) Steady state of rod Equation 2
  • 52. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER Temperature of the rod will be maximum at 𝑑𝑇 π‘‘π‘Ÿ = 0 Gives r = 0 (viz at the axis of the rod/cylinder) Let max temp = T0 (At axis) i.e. At r = 0, T = T0 Gives T0 = C2 T = βˆ’ ሢ π‘žπ‘Ÿ2 4𝐾 + T0 Or T0 – T = ሢ π‘žπ‘Ÿ2 4𝐾 AT r = R, T = Tw Or T0 – Tw = ሢ π‘žπ‘…2 4𝐾 Dividing equation 3 by 4 we have T0 – T T0 – Tw = π‘Ÿ 𝑅 2 Equation 3 (Parabolic temp distribution) Equation 4 Temperature distribution in non-dimensional format
  • 53. HEAT GENERATION IN A CYLINDER HEAT AND MASS TRANSFER The surface temperature Tw can also be obtained from energy balance equation for steady state condition of rod. ሢ π‘ž X R2L = h 2RL (Tw - Tο‚₯) Tw = ሢ π‘žπ‘… 2β„Ž + Tο‚₯ Similarly, Maximum temperature T0 can also be found out. T0 Or Tmax = ሢ π‘žπ‘…2 4𝐾 + ሢ π‘žπ‘… 2β„Ž + Tο‚₯ Surface temperature Maximum temperature
  • 54. FINS HEAT AND MASS TRANSFER Fins are the projections protruding from a hot surface into ambient fluid. They are meant for increasing heat transfer rate by increasing surface area.
  • 55. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER A = Profile area = zt L = Length of fin z = Width of fin t = Thickness of fin
  • 56. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER Objectives (1) T = f(x) (2) qfin = ? qx = Heat conducted into the element = - KA ( 𝑑𝑇 𝑑π‘₯ ) qx+dx = Heat conducted out of the element = qx + πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ Heat convected from the surface of fin = hP dx (T - Tο‚₯), P = Perimeter of fin = (2z + 2t) qx = qx+dx + qconvected (Energy balance equation)
  • 57. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER qx = qx + πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ + hP dx (T - Tο‚₯) 0 = πœ• πœ•π‘₯ π‘žπ‘₯ 𝑑π‘₯ + hP dx (T - Tο‚₯) 0 = πœ• πœ•π‘₯ βˆ’ KA ( 𝑑𝑇 𝑑π‘₯ ) 𝑑π‘₯ + hP dx (T - Tο‚₯) 𝑑2 𝑇 𝑑π‘₯2 - β„Žπ‘ƒ 𝐾𝐴 (T βˆ’ Tο‚₯) = 0 Let (T - Tο‚₯) =  = f(x) viz. 𝑑𝑇 𝑑π‘₯ = 𝑑 𝑑π‘₯ 𝑑2 𝑇 𝑑π‘₯2 = 𝑑 𝑑π‘₯ and put m2 = β„Žπ‘ƒ 𝐾𝐴
  • 58. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER 𝑑2  𝑑π‘₯2 - m2 = 0 T - Tο‚₯ =  = C1e-mx + C2emx Where, m = β„Žπ‘ƒ 𝐾𝐴 C1 and C2 are constant of integration Boundary condition 1 At x = 0, T = T0  = 0 = T0 - Tο‚₯ Boundary condition 2 (Has 3 unique cases) Standard format of 2nd order differential equation
  • 59. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER Case 1 – Fin is infinitely long (A very long fin) At x = ο‚₯, T = Tο‚₯ viz  = 00 i.e. 𝑇 βˆ’π‘‡ο‚₯ 𝑇0 βˆ’π‘‡ο‚₯ = e-mx qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Case 2 – Fin is finite in length but tip is insulated (A adiabatic tip) qconvected from tip = h A (Tx=L - Tο‚₯) = Very small (negligible value) Heat conducted into the tip of fin = 0 βˆ’ KA ( 𝑑𝑇 𝑑π‘₯ )At x=L = 0 (viz. insulated tip) Temperature distribution Heat transfer
  • 60. ANALYSIS OF RECTANGULAR FINS HEAT AND MASS TRANSFER ( 𝑑𝑇 𝑑π‘₯ )At x=L = 0 𝑑 𝑑π‘₯ At x = L = 0 𝑇 βˆ’π‘‡ο‚₯ 𝑇0 βˆ’π‘‡ο‚₯ = cos β„Ž π‘š (πΏβˆ’π‘₯) cos β„Ž π‘šπΏ qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mL Case 3 – Fin is finite and tip is not insulated (Uninsulated tip) 𝑇 βˆ’π‘‡ο‚₯ 𝑇0 βˆ’π‘‡ο‚₯ = cos β„Ž π‘š (πΏπ‘βˆ’π‘₯) cos β„Ž π‘šπΏπ‘ qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mLc m = 𝒉𝑷 𝑲𝑨 Temperature distribution Heat transfer Temperature distribution Heat transfer Lc = Corrected length of fin = L + t/4 (Rectangular) = L + d/4 (Pin)
  • 61. NUMERICAL HEAT AND MASS TRANSFER An uninsulated fin of 0.3 mm length is shown in the adjoining figure. Calculate the heat convected from the tip of the fin.
  • 62. NUMERICAL HEAT AND MASS TRANSFER Lc = L + t/4 = 0.30 P = 2z + 2t = 2 (0.3 + 2/1000) = 0.604 A = z X t = 0.3 X 2 = 0.6 m2 m = 𝒉𝑷 𝑲𝑨 = 8.603 m-1 𝑇 βˆ’π‘‡ο‚₯ 𝑇0 βˆ’π‘‡ο‚₯ = cos β„Ž π‘š (πΏπ‘βˆ’π‘₯) cos β„Ž π‘šπΏπ‘ Putting x = 0.3 m T At x = 0.3 = 70.30C qfin = β„Žπ‘ƒπΎπ΄ (T0 - Tο‚₯) Tanh mLc = 281.1 Watt
  • 63. FIN EFFICIENCY & FIN EFFECTIVENESS HEAT AND MASS TRANSFER Fin efficiency is defined as the ratio between actual heat transfer rate taking place through the fin and the maximum possible heat transfer that can occur through the fin. fin = π‘žπ‘Žπ‘π‘‘π‘’π‘Žπ‘™ π‘žπ‘šπ‘Žπ‘₯ Fin effectiveness is defined as the ratio between heat transfer with fins and heat transfer without fins. ο₯fin = π‘žπ‘€π‘–π‘‘β„Ž 𝑓𝑖𝑛𝑠 π‘žπ‘€π‘–π‘‘β„Žπ‘œπ‘’π‘‘ 𝑓𝑖𝑛𝑠 ο₯fin ο‚΅ 1/ β„Ž ο₯fin ο‚΅ 𝑃 𝐴 ο₯fin ο‚΅ 𝐾
  • 64. FIN EFFICIENCY & FIN EFFECTIVENESS HEAT AND MASS TRANSFER Moderately short Number of fins Closely spaced fins Thin High conductivity material As such Al Number of fins regulated = n = π‘‡π‘œπ‘‘π‘Žπ‘™ β„Žπ‘’π‘Žπ‘‘ π‘‘π‘œ 𝑏𝑒 π‘‘π‘–π‘ π‘ π‘–π‘π‘Žπ‘‘π‘’π‘‘ π»π‘’π‘Žπ‘‘ π‘Ÿπ‘Žπ‘‘π‘’ π‘‘β„Žπ‘Ÿπ‘œπ‘’π‘”β„Ž π‘’π‘Žπ‘β„Ž 𝑓𝑖𝑛
  • 65. UNSTEADY STATE/TRANSIENT CONDUCTION HEAT TRANSFER HEAT AND MASS TRANSFER T = f(t) Ti = Initial temperature of the body at the moment at which t=0 seconds. Viz when the body is just exposed to fluid. T = Temperature of body at any time β€œt sec” later The rate of convection heat transfer between body and fluid = The rate of decrease of internal energy of body w.r.t time hA (T - Tο‚₯) = - m Cp ( 𝑑𝑇 𝑑𝑑 ) Joules/Sec = -  vCp ( 𝑑𝑇 𝑑𝑑 ) J/S Treating all the parameters including β€œh” as constant and separating the variable T and t and then integrating, we have;
  • 66. UNSTEADY STATE/TRANSIENT CONDUCTION HEAT TRANSFER HEAT AND MASS TRANSFER ΰΆ± 𝑑=0 𝑑 ( β„Žπ΄  vCp ) 𝑑𝑑 = ΰΆ± 𝑇𝑖 𝑇 βˆ’ 𝑑𝑇 𝑇 βˆ’ 𝑇ο‚₯ ( β„Žπ΄  vCp) t = ln 𝑇 βˆ’ 𝑇ο‚₯ = ln 𝑇𝑖 βˆ’π‘‡ο‚₯ 𝑇 βˆ’π‘‡ο‚₯ e ( β„Žπ΄  vCp ) t = 𝑇𝑖 βˆ’π‘‡ο‚₯ 𝑇 βˆ’π‘‡ο‚₯ dT dt dT dt dT/dt t (Time) t (Time) T T -dT/dt = Rate of cooling = f(t) - Ve + Ve
  • 67. CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER q = h A T Convection Forced convection heat transfer Free convection heat transfer Velocity is evident Velocity is not evident r X R Y X u u u = f(r) u = f(x,y)
  • 68. FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER h = f (v, D, , , Cp, K) v = velocity of fluid = [LT-1] D = characteristics dimensions of the body = [L]  = Density = [ML-3]  = Dynamic viscosity (Pascal-Sec) = [ML-1T-1] Cp = Specific heat at constant pressure = [L2T-2-1] K = Thermal conductivity = [MLT-3-1] h = Convective heat transfer coefficient = [MT-3 -1]
  • 69. FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER Buckingham  theorem of dimensional analysis states that if there are β€œn” number of variables in any functional relationship both dependent and independent. And if all the variables put together contains β€˜β€m” number of fundamental dimensions, then the functional relationship among the variables can be expressed in term of β€œn-m” number of dimensionless  terms. h = f (v, D, , , Cp, K) Here n = 7 m = 4 [M,L,T,] According to Buckingham  theorem n – m = Number of dimensionless  terms = 7 – 4 = 3 Let 1, 2, 3 be these dimensionless terms.
  • 70. FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER 1 = ( ha1 , vb1, Dc1 , d1 )  2 = ( ha2 , vb2, Dc2 , d2 ) Cp 3 = ( ha2 , vb2, Dc2 , d2 ) K Now 1 = [M0L0T00] = [MT-3-1]a1 [LT-1]b1 [L]c1 [ML-3]d1 [ML-1T-1] For mass β€œM”, 0 = a1 + d1 + 1 For length β€œL”, 0 = b1 + c1 + - 3d1 – 1 For time β€œT”, 0 = -3a1 – b1 – 1 For temperature β€œο±β€, 0 = -a1 h = f (v, D, , , Cp, K) 1 =  𝒗𝑫
  • 71. FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER h = f (v, D, , , Cp, K) Similarly 2 = 𝑣Cp β„Ž 3 = 𝐾 β„Žπ· Now, 1 1 = Reynold’s Number = Re = 𝒗𝑫  1 2 = Stanton’s Number = Sn = β„Ž 𝑣Cp 1 3 = Nusselt Number = Nu = β„Žπ· 𝑲 12 3 = Prandtl’s Number = Pr = Cp 𝑲
  • 72. PHYSICAL SIGNIFICANCE OF Re IN FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER 1.Reynold’s Number Re – Defined as the ratio between inertia forces and viscous forces to which a flowing fluid is subjected to. Re = πΌπ‘›π‘’π‘Ÿπ‘‘π‘–π‘Ž πΉπ‘œπ‘Ÿπ‘π‘’π‘  π‘‰π‘–π‘ π‘π‘œπ‘’π‘  π‘“π‘œπ‘Ÿπ‘π‘’π‘  = 𝒗𝑫  = 𝒗𝑫 / = 𝒗𝑫   = Kinematic viscosity Re is the criteria to tell whether the fluid flow is laminar or turbulent for incompresible flow through pipes as well ducts. Re < 2000 (Lower critical) – Flow is laminar Re > 4000 (Upper critical) – Flow is turbulent
  • 73. HEAT AND MASS TRANSFER Axi-symmetric parabolic distribution of velocity. u = f(r) Logarithmic distribution of velocity. u = f(r) LAMINAR TURBULENT PHYSICAL SIGNIFICANCE OF Re IN FORCED CONVECTION HEAT TRANSFER
  • 74. INCOMPRESSIBLE FLOW OVER FLAT SURFACE HEAT AND MASS TRANSFER
  • 75. INCOMPRESSIBLE FLOW OVER FLAT SURFACE HEAT AND MASS TRANSFER Hydrodynamic boundary layer (HBL) is defined as a thin region formed over a flat surface (plate) inside which velocity gradient are seen in the normal direction to the plate. These velocity gradient are formed due to viscos nature or more precisely due to momentum diffusion through the fluid layer in the normal direction to the plate. Outside the HBL, free stream velocity exists in which no viscos influence can be seen At any given β€œx” At y = 0, u = 0 At y = , πœ•π’– πœ•π’š = 0 At y = 0, πœ•πŸ 𝒖 πœ•π’šπŸ = 0 At any given β€œx” πœ•π’– πœ•π’š = f(y) so for πœ•π’– πœ•π’š At y = 0  = f(x)
  • 76. INCOMPRESSIBLE FLOW OVER FLAT SURFACE HEAT AND MASS TRANSFER Rex < 5 X 105 (Flow over plate is laminar) Rex > 6.7-7 X 105 (Flow over plate is turbulent)
  • 77. PHYSICAL SIGNIFICANCE OF Nu & PrIN FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER 2. Nusselt number Nu - Nusselt number is the ratio of convective to conductive heat transfer at a boundary in a fluid. Sometimes also known as dimensionless heat transfer coefficient. The Biot number is the ratio of the internal resistance of a body to heat conduction to its external resistance to heat convection. Therefore, a small Biot number represents small resistance to heat conduction, and thus small temperature gradients within the body. Nu = β„Žπ· 𝐾𝑓𝑙𝑒𝑖𝑑 = 𝐷 𝐾𝐴 1 β„Žπ΄ = πΆπ‘œπ‘›π‘‘π‘’π‘π‘‘π‘–π‘œπ‘› π‘Ÿπ‘’π‘ π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’ π‘œπ‘“π‘“π‘’π‘Ÿπ‘’π‘‘ 𝑏𝑦 𝑓𝑙𝑒𝑖𝑑 (π‘ π‘‘π‘Žπ‘‘π‘–π‘œπ‘›π‘Žπ‘Ÿπ‘¦) π‘†π‘’π‘Ÿπ‘“π‘Žπ‘π‘’ π‘π‘œπ‘›π‘£π‘’π‘π‘‘π‘–π‘£π‘’ π‘Ÿπ‘’π‘ π‘–π‘ π‘‘π‘Žπ‘›π‘π‘’ But fluids are bad conductor of heat Numerator > Denominator Nu is always greater than 1 Bi = β„Žπ· πΎπ‘†π‘œπ‘™π‘–π‘‘
  • 78. PHYSICAL SIGNIFICANCE OF Nu & PrIN FORCED CONVECTION HEAT TRANSFER HEAT AND MASS TRANSFER 3. Prandtl Number (Pr) – The only dimensionless number which is a property of the fluid. Defined as the ratio between kinematic viscosity and thermal diffusivity of fluid. Pr = πΎπ‘–π‘›π‘’π‘šπ‘Žπ‘‘π‘–π‘ π‘£π‘–π‘ π‘π‘œπ‘ π‘–π‘‘π‘¦ π‘‡β„Žπ‘’π‘Ÿπ‘šπ‘Žπ‘™ 𝑑𝑖𝑓𝑓𝑒𝑠𝑖𝑣𝑖𝑑𝑦 =   𝐢𝑝 𝐾 =   𝐾 𝐢𝑝 Pr for air = 0.65 to 0.73 Pr for water = 2 to 6 For engine oils = up to 100 ! Very low Pr
  • 79. THERMAL BOUNDARY LAYER (TBL) HEAT AND MASS TRANSFER
  • 80. THERMAL BOUNDARY LAYER (TBL) HEAT AND MASS TRANSFER Thermal Boundary Layer (TBL) is similar to HBL inside which velocity gradient are seen in the normal direction to the plate. Thermal boundary layer is also a thin region in which temperature gradients are present in the normal direction to the flat surface (Plate). These temperature gradient are formed due to heat transfer between plate and flowing fluid. At any given β€œx” measured from leading edge. At y = 0, T = Tw At y = t, T = Tο‚₯ , πœ•π‘» πœ•π’š = 0 At y = 0, πœ•πŸ 𝑻 πœ•π’šπŸ = 0 At any given β€œx” πœ•π‘» πœ•π’š = f(y) with maximum value of πœ•π‘» πœ•π’š At y = 0
  • 81. ENERGY BALANCE FOR DIFFERENTIAL CONTROL VOLUME OF TBL HEAT AND MASS TRANSFER Heat conducted into the control volume = Heat convected from the hot plate at Tw to free stream fluid at Tο‚₯ - K dA ( πœ•π‘‡ πœ•π‘¦ ) AT y = 0 = hx dA (Tw - Tο‚₯) hx = βˆ’ 𝐾(πœ•π‘‡ πœ•π‘¦ ) AT y = 0 (Tw βˆ’ Tο‚₯) Local convective heat transfer coefficient. hx x hx ο‚΅ 𝒙 Fourier’s law Newton’s law
  • 82. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER  = f (x,y) &  = f (x,y),  = c
  • 83. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER CONTROL VOLUME Viscos force =  [ πœ•π‘’ πœ•π‘¦ + πœ• πœ•π‘¦ ( πœ•π‘’ πœ•π‘¦ ) 𝑑𝑦 ] (𝑑π‘₯ 𝑋 1) dx dy Pressure force = p X dy X 1 Pressure force = (p + πœ•π‘ πœ•π‘₯ 𝑑π‘₯) 𝑑𝑦 X 1 Viscos force Gravity force
  • 84. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER Applying Newton’s II law of motion Οƒ 𝐹π‘₯ = max (Conservation of linear momentum) Resulting momentum equation of HBL is ; u πœ•π‘’ πœ•π‘₯ + v πœ•π‘’ πœ•π‘¦ = (   ) πœ•2 𝑒 πœ•π‘¦2 - 1  ( 𝑑𝑃 𝑑π‘₯ ) u v V = u Τ¦ π’Š + v Τ¦ 𝒋 dp/dx = 0 for flow over plates & (  ) =  u 𝝏𝒖 𝝏𝒙 + v 𝝏𝒖 ππ’š =  𝝏𝟐 𝒖 ππ’šπŸ Momentum equation of HBL
  • 85. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER  = f (x,y) &  = f (x,y), T = f(x,y),  = c
  • 86. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER Consider negligible heat conduction in x-direction. Thermal heat energy convected by fluid = mCpT J/Sec Viscos heat is neglected CONTROL VOLUME Heat convected =  (dx X 1) (v + πœ•π‘£ πœ•π‘¦ dy) Cp (T + πœ•π‘‡ πœ•π‘¦ dy) Heat conducted = - K (dx X 1) ( πœ•π‘‡ πœ•π‘¦ + πœ• πœ•π‘¦ πœ•π‘‡ πœ•π‘¦ dy) Heat conducted = - K (dx X 1) πœ•π‘‡ πœ•π‘¦ Heat convected =  (dx X 1) v Cp T Heat convected =  (dy X 1) u Cp T Heat convected =  (dx X 1) (u + πœ•π‘’ πœ•π‘₯ du) Cp (T + πœ•π‘‡ πœ•π‘₯ dx)
  • 87. MOMENTUM EQUATION OF HBL AND ENERGY EQUATION OF TBL HEAT AND MASS TRANSFER Heat conducted through bottom face + Heat convected through left face + Heat convected through bottom face Heat conducted through top face + Heat convected through right face + Heat convected through top face 6 energies u 𝝏𝑻 𝝏𝒙 + v 𝝏𝑻 ππ’š =  𝝏𝟐 𝑻 ππ’šπŸ Energy equation for TBL u 𝝏𝒖 𝝏𝒙 + v 𝝏𝒖 ππ’š =  𝝏𝟐 𝒖 ππ’šπŸ Momentum equation of HBL
  • 88. FORCED CONVECTION IN FLOW THROUGH PIPES AND DUCTS HEAT AND MASS TRANSFER ሢ π‘š =  X R2 X Vmean Kg/s
  • 89. FORCED CONVECTION IN FLOW THROUGH PIPES AND DUCTS HEAT AND MASS TRANSFER Tb (Bulk mean temperature) – Defined as {At a given cross section of pipe} the temperature which takes into account the variation of temperature of fluid layers with respect to β€œr” at the cross section of the pipe and thus indicates the total thermal energy transported by the fluid through the cross section. Thermal energy/enthalpy transported by fluid through the cross section of pipe = ሢ π‘š CpTb =  X R2 X Vmean CpTb And the Bulk mean temperature is given by. Tb = 2 ‫׬‬0 𝑅 π‘Ÿ 𝑒 𝑇 π‘‘π‘Ÿ R2 X Vmean
  • 90. NUMERICAL HEAT AND MASS TRANSFER Find out the bulk mean temperature at exit. dq = qw X Area = qw 𝐷 𝑑π‘₯ Differential heat rate through differential heat transfer area of length β€œdx” = dq = ሢ π‘š Cp dTb ‫׬‬0 3 2500 π‘₯ 𝐷 𝑑π‘₯ = ‫׬‬𝑖𝑛𝑙𝑒𝑑 𝑒π‘₯𝑖𝑑 ሢ π‘š Cp dTb (Tb)Exit = 620C
  • 92. FREE/NATURAL CONVECTION HEAT AND MASS TRANSFER h = f ( g, , , L, , , Cp, K ) g = acceleration due to gravity  = Isobaric volume expansion coefficient
  • 93. RADIATION HEAT AND MASS TRANSFER Any body at a given temperature emit thermal radiation at all probable wavelength on electromagnetic spectrum and in all possible hemispherical direction. Total hemispherical emissive power (E) – Defined as radiation energy emitted from the surface of a body per unit time per unit area in all possible hemispherical directions integrated over all the wavelengths.
  • 94. RADIATION HEAT AND MASS TRANSFER Total emissivity (ο₯) – Defined as the ratio between total hemispherical emissive power of a non-black body to that of a black body at same temperature. Non-black Black body E Eb ο₯ = 𝑬 𝑬𝒃 ο₯ ο‚£ 1 ο₯b = 1
  • 95. RADIATION HEAT AND MASS TRANSFER Black body is a body which absorbs all the thermal radiation incident or falling upon the body. Perfect absorber Ideal emitter Diffusive in nature
  • 96. RADIATION HEAT AND MASS TRANSFER Monochromatic/Spectral hemispherical emissive power (E) - E at a particular wavelength β€œο¬β€ is defined as the quantity which when multiplied by β€œd” (Differentially small increment in wavelength) shall give the radiation energy emitted from the surface of a body per unit time per unit area in the wavelength range  -  + d d   + d E = f()
  • 97. RADIATION HEAT AND MASS TRANSFER Monochromatic/Spectral emissivity (ο₯) – Ratio of monochromatic hemispherical emissive power of a non-black body to that of a black body at same temperature & wavelength. ο₯ b  ο₯   For grey body ο₯  = Constant
  • 98. ABSORBTIVITY (), REFLECTIVITY (), TRANSMITIVITY () HEAT AND MASS TRANSFER  = Fraction of radiation energy incident upon a surface which is absorbed by it.  = Fraction of radiation energy incident upon a surface which is reflected by it.  = Fraction of radiation energy incident upon a surface which is transmitted through it. For any surface,  +  +  = 1 For opaque surface,  +  = 1 (  = 0 ) For black body,  = b = 1
  • 99. ABSORBTIVITY (), REFLECTIVITY (), TRANSMITIVITY () HEAT AND MASS TRANSFER Sun Earth Short wavelength Long wavelength Co2
  • 100. LAWS OF THERMAL RADIATION HEAT AND MASS TRANSFER 1.Kirchhoff's law of thermal radiation – States that whenever a body is in thermal equilibrium with its surroundings, its emissivity is equal to its absorptivity. ο₯ =  β€œA good absorber is always a good emitter” For black body b = 1 ο₯b = 1
  • 101. LAWS OF THERMAL RADIATION HEAT AND MASS TRANSFER 2.Plank’s law of thermal radiation – The law states that the monochromatic emissive power of a black body is dependent both upon the absolute temperature of the body and the wavelength of radiation energy emitted. Eb = f (,T)
  • 102. LAWS OF THERMAL RADIATION HEAT AND MASS TRANSFER 3.Stefan-Boltzman’s law – The law states that the total hemispherical emissive power of a black body is directly proportional to the fourth power of the absolute temperature of the black body. Eb ο‚΅ T4 Eb =  T4 watt/m2  = Stefan-Boltzman’s constant = 5.67 X 10-8 w/m2K4
  • 103. LAWS OF THERMAL RADIATION HEAT AND MASS TRANSFER 4.Weins displacement law – For a non black body, whose emissivity is ο₯ , The total hemispherical emissive power of non-black body E = ο₯Eb E = ο₯  T4 If β€œA” is the total surface area of non-black body, The total radiation energy emitted from entire non-black body = EA watt = ο₯  T4A
  • 104. SHAPE FACTOR HEAT AND MASS TRANSFER 1 2 Radiation energy leaving 1 Radiation energy leaving 2 F12 = Fraction of radiation energy leaving surface 1 and that of reaching surface 2. F21 = Fraction of radiation energy leaving surface 2 and that of reaching surface 1. 0 ο‚£ Fmn ο‚£ 1
  • 105. SHAPE FACTOR HEAT AND MASS TRANSFER Shapes with size difference Flat surface Concave surface Convex surface Reciprocity relationship A1 F12 = A2 F21 F21 > F12 F11 = 0 F11 = 0 F11 > 0
  • 106. RADIATION HEAT EXCHANGE HEAT AND MASS TRANSFER CASE 1 Two infinitely large parallel plates Assumptions – 1. Steady state heat transfer conditions Tο‚Ή f(t) 2. Surfaces are diffuse and grey. ο₯ = f () Net radiation heat exchange between 1 and 2 per unit area is (q/A)1-2 =  ( 𝑇1 4 βˆ’π‘‡2 4 ) 1 ο₯1 + 1 ο₯2 βˆ’1 Watt/m2 = Radiation flux In case both the surfaces are black, ο₯1 = ο₯2 = 1 (q/A)1-2 =  ( 𝑇1 4 βˆ’ 𝑇2 4) w/m2
  • 107. RADIATION HEAT EXCHANGE HEAT AND MASS TRANSFER CASE 2 Two infinitely long concentric cylindrical surfaces
  • 108. RADIATION HEAT EXCHANGE HEAT AND MASS TRANSFER CASE 2 Two infinitely long concentric cylindrical surfaces Assumptions – 1. Steady state heat transfer conditions Tο‚Ή f(t) 2. Surfaces are diffuse and grey. ο₯ = f () 3. Let T1 > T2 Net radiation heat exchange between 1 and 2 is (q)1-2 =  𝑇1 4 βˆ’π‘‡2 4 𝐴1 1 ο₯1 + 𝐴1 𝐴2 ( 1 ο₯2 βˆ’1) Watt F12 = 1 F21 < 1 𝐴1 𝐴2 = 𝑅1 𝑅2
  • 109. TYPES OF HEAT EXCHANGERS HEAT AND MASS TRANSFER Heat exchanger is a steady flow adiabatic open system device in which two flowing fluids exchange or transfer heat without loosing or gaining any heat from the ambient.
  • 110. TYPES OF HEAT EXCHANGERS HEAT AND MASS TRANSFER Surface (steam) condenser Steam to cold water Economizer Hot flue gas to cold water Superheater Hot flue gas to dry saturated steam Air preheater Hot flue gas to combustion air Cooling tower Hot water to atmospheric air Oil cooler Hot oil to cool water/air
  • 111. FIRST LAW OF THERMODYNAMICS HEAT AND MASS TRANSFER Q – W = H + KE + PE Q = 0 (adiabatic),W = 0 , KE = 0, PE = 0 (no datum change) (H)HE = 0 (H)Hot fluid + (H)Cold fluid = 0 - (H)Hot fluid = +(H)Cold fluid β€œ Rate of enthalpy decrease of hot fluid = Rate of enthalpy increase of cold fluid β€œ ሢ π‘šh Cph (Thi – The) = ሢ π‘šc Cpc (Tce – Tci)
  • 112. CLASSIFICATION OF HEAT EXCHANGER HEAT AND MASS TRANSFER HE Direct transfer Parallel Counter Cross Direct contact Regenerative/ storage
  • 113. CLASSIFICATION OF HEAT EXCHANGER HEAT AND MASS TRANSFER Direct transfer Parallel Counter Cross Parallel flow HE – An automobile radiator 1 π‘ˆ = 1 β„Ž1 + 1 β„Ž2 T = Th – Tc = f (x) dq = U T dA Tce > The
  • 114. CLASSIFICATION OF HEAT EXCHANGER HEAT AND MASS TRANSFER (S)Parallel flow HE > (S)Counter flow HE Counter flow HE is thermodynamically more efficient than parallel flow HE.
  • 115. Mean Temperature Difference MTD (Tm) HEAT AND MASS TRANSFER A parameter which takes into account the variation of temperature with respect to direction of flow of hot fluid by taking average all along the length of HE from inlet to exit. Q = U A Tm Q = Total heat transfer rate. U = Overall heat transfer coefficient. A = Total heat transfer area of HE. Tm = Mean Temperature Difference. Equation - 1
  • 116. Mean Temperature Difference MTD (Tm) HEAT AND MASS TRANSFER dq = U T dA ‫׬‬𝐼𝑛𝑙𝑒𝑑 𝐸π‘₯𝑖𝑑 π‘‘π‘ž = ‫׬‬𝐼𝑛𝑙𝑒𝑑 𝐸π‘₯𝑖𝑑 π‘ˆο„T dA Q = U ‫׬‬𝐼𝑛𝑙𝑒𝑑 𝐸π‘₯𝑖𝑑 T dA From equation 1 and 2, we have Tm = 𝟏 𝑨 ‫׬‬𝐼𝑛𝑙𝑒𝑑 𝐸π‘₯𝑖𝑑 T dA Equation - 2
  • 117. Logarithmic Mean Temperature Difference LMTD (Tm) HEAT AND MASS TRANSFER Parallel flow HE
  • 118. Logarithmic Mean Temperature Difference LMTD (Tm) HEAT AND MASS TRANSFER Parallel flow HE dq = U T dA dA = B dx T = Th – Tc = f (x) At x = 0, T = Ti = Thi – Tci At x = L, T = Te = The – Tce Also dq = - ሢ π‘š h Cph dT = + ሢ π‘š h Cpc dT Now T = Th – Tc d(T) = dTh – dTc d(T) = - π‘‘π‘ž ሢ π‘šβ„Ž πΆπ‘β„Ž - π‘‘π‘ž ሢ π‘šπ‘ 𝐢𝑝𝑐
  • 119. Logarithmic Mean Temperature Difference LMTD (Tm) HEAT AND MASS TRANSFER Parallel flow HE d(T) = - dq 1 ሢ π‘šβ„Ž πΆπ‘β„Ž + 1 ሢ π‘šπ‘ 𝐢𝑝𝑐 d(T) = - U T dA 1 ሢ π‘šβ„Ž πΆπ‘β„Ž + 1 ሢ π‘šπ‘ 𝐢𝑝𝑐 Separating the variables, we have ΰΆ± βˆ†π‘‡π‘– βˆ†π‘‡π‘’ βˆ’ d(T) T = ΰΆ± 0 𝐿 π‘ˆ 𝐡 1 ሢ π‘šβ„Ž πΆπ‘β„Ž + 1 ሢ π‘šπ‘ 𝐢𝑝𝑐 ln βˆ†π‘‡π‘– βˆ†π‘‡π‘’ = U B L 1 ሢ π‘šβ„Ž πΆπ‘β„Ž + 1 ሢ π‘šπ‘ 𝐢𝑝𝑐 Q = Total heat rate of entire HE = ሢ π‘šβ„Ž πΆπ‘β„Ž (Thi – The) = ሢ π‘šπ‘ 𝐢𝑝𝑐 (Tce – Tci)
  • 120. Logarithmic Mean Temperature Difference LMTD HEAT AND MASS TRANSFER Parallel flow HE ln βˆ†π‘‡π‘– βˆ†π‘‡π‘’ = U A π‘‡β„Žπ‘– βˆ’π‘‡β„Žπ‘’ 𝑄 + 𝑇𝑐𝑒 βˆ’π‘‡π‘π‘– 𝑄 = π‘ˆπ΄ 𝑄 ( Ti - Te ) Q = U A Ti βˆ’ Te ln βˆ†π‘‡π‘– βˆ†π‘‡π‘’ , Comparing this with Q = U A Tm , We have Tm = (T)LMTD = Ti βˆ’ Te ln βˆ†π‘»π’Š βˆ†π‘»π’† Logarithmic mean temperature difference for parallel flow HE
  • 121. Logarithmic Mean Temperature Difference LMTD HEAT AND MASS TRANSFER Counter flow HE
  • 122. Logarithmic Mean Temperature Difference LMTD HEAT AND MASS TRANSFER Counter flow HE (T)LMTD = Ti βˆ’ Te ln βˆ†π‘»π’Š βˆ†π‘»π’†
  • 123. SPECIAL CASES HEAT AND MASS TRANSFER When one of the fluids in the HE is undergoing phase change like a steam condenser or evaporator or steam generator. Steam Condenser LMTD Parallel = LMTD Counter
  • 124. SPECIAL CASES HEAT AND MASS TRANSFER Steam Generator LMTD Parallel = LMTD Counter
  • 125. SPECIAL CASES HEAT AND MASS TRANSFER When both hot and cold fluids have equal capacity rates in a counter flow heat exchanger. ሢ π‘šβ„Ž πΆπ‘β„Ž = ሢ π‘šπ‘ 𝐢𝑝𝑐 Then from energy balance equation, ሢ π‘šβ„Ž πΆπ‘β„Ž ( Thi –The ) = ሢ π‘šπ‘ 𝐢𝑝𝑐 ( Tce – Tci ) ( Thi –The ) = ( Tce – Tci ) Thi – Tce = The – Tci Ti = Te (T)LMTD = Ti βˆ’ Te ln βˆ†π‘»π’Š βˆ†π‘»π’† = 𝟎 𝟎 = Undefined = Ti Or Te ሢ π‘š 𝐢𝑝 = Heat capacity rate L’Hospital’s rule
  • 126. Effectiveness of HE (ο₯) HEAT AND MASS TRANSFER It is defined as the ratio between actual heat transfer rate taking place between hot and cold fluids and the maximum possible heat transfer rate between them. ο₯HE = 𝒒 𝒂𝒄𝒕𝒖𝒂𝒍 𝒒 π’Žπ’‚π’™ 𝒒 𝒂𝒄𝒕𝒖𝒂𝒍 = Rate of enthalpy change of either fluid = ሢ π‘šβ„Ž πΆπ‘β„Ž ( Thi –The ) = ሢ π‘šπ‘ 𝐢𝑝𝑐 ( Tce – Tci ) 𝒒 π’Žπ’‚π’™ = ሢ π‘š 𝐢𝑝 ( Thi –Tci ) ሢ π‘š 𝐢𝑝 = Heat capacity rate
  • 127. NUMBER OF TRANSFER UNITS NTU HEAT AND MASS TRANSFER The number of transfer units (NTU = UA/(mcp)) itself is a combination of overall heat transfer coefficients, transfer area, fluid flow rate and heat capacity. It summarizes these dimensional parameters into one dimensionless parameter. The performance becomes a monotone function of this dimensionless parameter. It indicates overall size of HE. NTU = 𝑼𝑨 ሢ π’Ž π‘ͺ𝒑 π‘Ίπ’Žπ’‚π’π’
  • 128. FOULING FACTOR (F) HEAT AND MASS TRANSFER It takes into account the thermal resistance offered by any chemical scaling or deposits that are formed on the heat transfer surface on both hot side and cold side. Generally ranges from 0.0004 – 0.0006 𝟏 𝑼 = 𝟏 π’‰πŸ + F1 + 𝟏 π’‰πŸ + F2
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