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CHAPTER 43
HEAT TRANSFER FUNDAMENTALS
G. P. "Bud" Peterson
Executive Associate Dean and Associate Vice Chancellor of Engineering
Texas A&M University
College Station, Texas
43.1 SYMBOLS AND UNITS 13 67
43.3.4 The Log Mean
Temperature Difference 1400
43.2 CONDUCTION HEAT
TRANSFER 13 69
43.2.1 Thermal Conductivity 13 70
43.2.2 One-Dimensional Steady-
State Heat Conduction 1375
43.2.3 Two-Dimensional Steady-
State Heat Conduction 1377
43.2.4 Heat Conduction with
Convection Heat Transfer
on the Boundaries 1381
43.2.5 Transient Heat Conduction 1383
43.4 RADIATION HEAT
TRANSFER 1400
43.4.1 Black-Body Radiation 1400
43.4.2 Radiation Properties 1404
43.4.3 Configuration Factor 1407
43 A A Radiative Exchange
among Diffuse-Gray
Surfaces in
an Enclosure
1410
43.4.5 Thermal Radiation
Properties of Gases 1415
43.3 CONVECTION HEAT
TRANSFER
13 85
43.5 BOILING AND
CONDENSATION HEAT
TRANSFER 1417
43.5.1 Boiling 1420
43.5.2 Condensation 1423
43.5.3 Heat Pipes
43.3.1 Forced Convection —
Internal Flow
1385
43.3.2 Forced Convection —
External Flow 13 93
43.3.3 Free Convection 13 97
1424
43.1 SYMBOLS AND UNITS
A area of heat transfer
Bi Biot number, hL/k, dimensionless
C circumference, m, constant defined in text
Cp specific heat under constant pressure, J/kg • K
D diameter, m
e emissive power, W/m2
/ drag coefficient, dimensionless
F cross flow correction factor, dimensionless
Ff_j configuration factor from surface i to surface j, dimensionless
Fo Fourier number, atA2/V2, dimensionless
FO-\T radiation function, dimensionless
G irradiation, W/m2; mass velocity, kg/m2 • sec
g local gravitational acceleration, 9.8 m/sec2
gc proportionality constant, 1 kg • m/N • sec2
Gr Grashof number, gL3/3Ar/f2, dimensionless
h convection heat transfer coefficient, equals q/AAT, W/m2 • K
hfg heat of vaporization, J/kg
J radiocity, W/m2
k thermal conductivity, W/m • K
Mechanical Engineers' Handbook, 2nd ed., Edited by Myer Kutz.
ISBN 0-471-13007-9 © 1998 John Wiley & Sons, Inc.
815044281.003.png 815044281.004.png
K wick permeability, m2
L length, m
Ma Mach number, dimensionless
N screen mesh number, m"1
Nu Nusselt number, NuL = hL/k, NuD = hDlk, dimensionless
Nu Nusselt number averaged over length, dimensionless
P pressure, N/m2, perimeter, m
Pe Peclet number, RePr, dimensionless
Pr Prandtl number, Cpjjilk, dimensionless
q rate of heat transfer, W
cf' rate of heat transfer per unit area, W/m2
R distance, m; thermal resistance, K/W
r radial coordinate, m; recovery factor, dimensionless
Ra Rayleigh number, GrPr; RaL = GrLPr, dimensionless
Re Reynolds number, ReL = pVLI /n, Re^, = pVDI /a, dimensionless
S conduction shape factor, m
T temperature, K or °C
t time, sec
Tas adiabatic surface temperature, K
Tsat saturation temperature, K
Tb fluid bulk temperature or base temperature of fins, K
Te excessive temperature, Ts — Tsan K or °C
Tf film temperature, (Tx + Ts)/2, K
T. initial temperature; at t = 0, K
T0 stagnation temperature, K
Ts surface temperature, K
^ free stream fluid temperature, K
U overall heat transfer coefficient, W/m2 • K
V fluid velocity, m/sec; volume, m3
w groove width, m; or wire spacing, m
We Weber number, dimensionless
x one of the axes of Cartesian reference frame, m
Greek Symbols
a thermal diffusivity, kl pCp, m2/sec; absorptivity, dimensionless
(3 coefficient of volume expansion, 1/K
r mass flow rate of condensate per unit width, kg/m • sec
y specific heat ratio, dimensionless
A7 temperature difference, K
8 thickness of cavity space, groove depth, m
e emissivity, dimensionless
e wick porosity, dimensionless
A wavelength, /nm
T]f fin efficiency, dimensionless
jji viscosity, kg/m • sec
v kinematic viscosity, m2/sec
p reflectivity, dimensionless; density, kg/m3
or surface tension, N/m; Stefan-Boltzmann constant, 5.729 X 10~8 W/m2 • K4
T transmissivity, dimensionless, shear stress, N/m2
M* angle of inclination, degrees or radians
Subscripts
a adiabatic section, air
b boiling, black body
c convection, capillary, capillary limitation, condenser
e entrainment, evaporator section
eff effective
/ fin
/ inner
/ liquid
m mean, maximum
n nucleation
o outer
0 stagnation condition
P PiPe
r radiation
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s surface, sonic or sphere
w wire spacing, wick
v vapor
A spectral
oo free stream
— axial hydrostatic pressure
+ normal hydrostatic pressure
The science or study of heat transfer is that subset of the larger field of transport phenomena that
focuses on the energy transfer occurring as a result of a temperature gradient. This energy transfer
can manifest itself in several forms, including conduction, which focuses on the transfer of energy
through the direct impact of molecules; convection, which results from the energy transferred through
the motion of a fluid; and radiation, which focuses on the transmission of energy through electro-
magnetic waves. In the following review, as is the case with most texts on heat transfer, phase change
heat transfer, that is, boiling and condensation, will be treated as a subset of convection heat transfer.
43.2 CONDUCTION HEAT TRANSFER
The exchange of energy or heat resulting from the kinetic energy transferred through the direct impact
of molecules is referred to as conduction and takes place from a region of high energy (or temper-
ature) to a region of lower energy (or temperature). The fundamental relationship that governs this
form of heat transfer is Fourier's law of heat conduction, which states that in a one-dimensional
system with no fluid motion, the rate of heat flow in a given direction is proportional to the product
of the temperature gradient in that direction and the area normal to the direction of heat flow. For
conduction heat transfer in the ^-direction this expression takes the form
,A dT
qx = -kA —
**
dx
where qx is the heat transfer in the ^-direction, A is the area normal to the heat flow, dT/dx is the
temperature gradient, and k is the thermal conductivity of the substance.
Writing an energy balance for a three-dimensional body, and utilizing Fourier's law of heat con-
duction, yields an expression for the transient diffusion occurring within a body or substance.
d / dT\ d / dT\ d / df\
d dT
—Ik —} + —[k — \ +—\k — } + q = pcv
dx\ dx/ dy\ dy/ dz\ dz/
p dx dt
This expression, usually referred to as the heat diffusion equation or heat equation, provides a basis
for most types of heat conduction analysis. Specialized cases of this equation, such as the case where
the thermal conductivity is a constant
tfT <PT #T q = pCpdT
dx2 + dy2 + dz2 + k ~ k dt
steady-state with heat generation
d (, dT\ d /, dT\ d f, dT\
—Ik — + —Ik — + —\k — + q = 0
dx\ dx/ dy\ dy/ dz\ dz/
steady-state, one-dimensional heat transfer with heat transfer to a heat sink (i.e., a fin)
-iprW'-o
dx\dx/ k
or one-dimensional heat transfer with no internal heat generation
Ji(?I\ = №p?L
dx\dx) k dt
can be utilized to solve many steady-state or transient problems. In the following sections, this
equation will be utilized for several specific cases. However, in general, for a three-dimensional body
of constant thermal properties without heat generation under steady-state heat conduction, the tem-
perature field satisfies the expression
v2r= o
815044281.006.png
43.2.1 Thermal Conductivity
The ability of a substance to transfer heat through conduction can be represented by the constant of
proportionality k, referred to as the thermal conductivity. Figures 43.la, b, and c illustrate the char-
acteristics of the thermal conductivity as a function of temperature for several solids, liquids and
gases, respectively. As shown, the thermal conductivity of solids is higher than liquids, and liquids
higher than gases. Metals typically have higher thermal conductivities than nonmetals, with pure
metals having thermal conductivities that decrease with increasing temperature, while the thermal
conductivities of nonmetallic solids generally increase with increasing temperature and density. The
addition of other metals to create alloys, or the presence of impurities, usually decreases the thermal
conductivity of a pure metal.
In general, the thermal conductivities of liquids decrease with increasing temperature. Alterna-
tively, the thermal conductivities of gases and vapors, while lower, increase with increasing temper-
ature and decrease with increasing molecular weight. The thermal conductivities of a number of
commonly used metals and nonmetals are tabulated in Tables 43.1 and 43.2, respectively. Insulating
materials, which are used to prevent or reduce the transfer of heat between two substances or a
substance and the surroundings are listed in Tables 43.3 and 43.4, along with the thermal properties.
The thermal conductivities for liquids, molten metals, and gases are given in Tables 43.5, 43.6 and
43.7, respectively.
Fig. 43.1 a Temperature dependence of the thermal conductivity of selected solids.
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Fig. 43.1 b Selected nonmetallic liquids under saturated conditions.
Fig. 43.1 c Selected gases at normal pressures.1
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