Fundamentals of Heat Transfer
The following is a brief overview of some
fundamental heat transfer concepts. To learn more, the reader is encouraged to
review the source publications and Web sites.
1st and 2nd Laws of Thermodynamics
The 1st Law of Thermodynamics
involves the conservation of energy. It states that - within a closed system
where no other energy material can enter or leave - energy can neither be
created nor destroyed.1, 2 Although energy cannot be created or
destroyed, it can be transferred to work other forms of energy.
Transferring heat energy is subject to the 2nd Law
of Thermodynamics.3 The 2nd Law (again applying
to a closed system) says that - for a spontaneous process - there is a net
increase in entropy4 (i.e., a measure of the disorder that
exists in a system5).
Three alternate but equivalent ways to
describe the 2nd Law are:
1.
Heat flows
spontaneously from a hot body to a cool one. (Example: A hot
microprocessor or laser diode is cooled by flow of heat into heat sink or cold
plate.)
2.
It is impossible to
convert heat completely into useful work. (Example: In a combustion
engine, a certain heat component must always be exhausted without performing
work.)
3.
Every isolated system
becomes disordered in time. (Example: In conduction when hot and cold
bodies first contact each other, the system is somewhat ordered. Hotter
molecules move faster than cooler molecules. But, once the entire system
attains a uniform temperature, this order is lost.)
Expressed in mathematical terms, any of the above
statements imply the other two.6
The 1st and 2nd Laws
of Thermodynamics govern the various modes of heat transfer: conduction,
convection and radiation.
Modes of Heat Transfer
Conduction
In conduction, heat flows from a higher
temperature region to regions of lower temperature. This occurs within solid,
liquid, or gaseous mediums or between different mediums that make direct
physical contact with each other.7 "The transfer of the
energy of motion between adjacent molecules conducts the heat. In a gas, the
'hotter' molecules, have greater energy and motions, and impart energy to
adjacent molecules at lower energy levels. This type of transfer occurs to some
extent in all solids, gases or liquids in which a temperature gradient exists.
In conduction, energy can also be transferred by "free" electrons,
which is important in metallic solids." 8 Examples of
conduction are heat transfer through the surfaces of a cold plate or
through the walls of a refrigerator.
Convection
In convection, the combined action of heat
conduction, energy storage, and mixing motion serve to transport energy.
"Convection is most important as the mechanism of energy transfer between
a solid surface and a liquid or a gas." 9 "In
forced-convection heat transfer, a pump, fan, or other mechanism forces a fluid to flow past a solid
surface. In natural or free convection, warmer or cooler fluid next to the
solid surface causes a circulation because of density differences resulting
from the temperature differences in the fluid." 10 An
example of free convection is the loss of heat into ambient air via the fins of
a heat exchanger. If a fan is used to circulate the air over
the heat exchanger fins, this becomes an example of forced
convection.
Radiation
In radiation, heat flows from a higher
temperature body to a lower temperature body when the bodies are separated in
space, even across a vacuum. 11 "The same laws that
govern the transfer of light, also govern the transfer of heat. Solids and
liquids tend to absorb the radiation being transferred through it, hence
radiation is important mainly in transfer through space or gases."12
Examples of radiation include the transfer of
heat from the sun to the earth, and from a quartz lamp to a cool object that
requires warming.
Fourier's Equation
"The basic relation for heat transfer by
conduction, proposed by the French scientist J.B.J. Fourier in 1822, states:
The rate of heat flow by conduction in a
material, qk , equals the product of the following three quantities:
k
|
thermal conductivity
of the material.
|
A
|
area of the section
through which heat flows by conduction as measured perpendicularly to the
direction of heat flow.
|
dT/dx
|
temperature gradient
at the section, i.e., the rate of change of temperature T with respect to the
difference in the direction of the heat flow x.
|
Writing the heat conduction equation in
mathematical form requires a sign convention; i.e., the direction of increasing
distance x is the direction of positive heat flow. According to the second law
of thermodynamics, heat will automatically flow from points of higher
temperature to points of lower temperature. Thus, heat flow will be positive
when the temperature gradient is negative. The basic equation for
one-dimensional conduction in the steady state is: qk =
-kA (dT/dx)"13
Thermal Conductivity
Thermal conductivity is a measurement of the
rate at which a given material will transfer heat.14 "The
thermal conductivity of a substance is the quantity of heat in cal/sec passing
through a body 1 cm thick with a cross section of 1 sq. cm when the temperature
difference between the hot and cold sides of the body is 1 deg. C."15 This
intrinsic property is independent of the materials size, shape, or orientation.
Thermal Resistance
Thermal resistance is the inverse of thermal
conductivity and indicates how a material inhibits the conduction of
heat. 16 Materials with a high thermal conductivity have a
low thermal resistance and have poor heat insulation qualities (e.g., copper
and aluminum). Conversely, materials with a low thermal conductivity have a
high thermal resistance, and have good heat insulation qualities (e.g., fiberglass
insulation and corkboard).17
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