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8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Heat Transfer ME 3345
Introduction
Chapter 1
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Conduction
HEAT FLUX q
Where k is THERMAL CONDUCTIVITY (W/mK)
Two cases will be considered:
(1) Transient response, initial temperature T1 > T2, then heat conduction occursto spread the vibration (Thermal Energy) uniformly throughout solid so a new
temperature is reached at some time:
(2) Steady-state where T1 and T2 are a constant in time.
Gradient is therefore: and heat flux is:
Units of heat flux are W/m2 Units of heat conduction W/mK
For a rod of area A, the heat conducted is qA, units Watts = Joules/second
2
21 TT+
dx
dTkqx =
"
L
TT
dx
dT 12 =
L
TTkqx
12" =
1T
2T
L
time
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Convection
Forced Convection imposed flow of fluid
Natural Convection due to boyancy forces
Flat Plate:
BOUNDARY LAYER region over which temperature and the velocity change.
Convection Heat Transfer occurs through both random molecular motion & bulk
fluid motion within the boundary layer.
qCONV = hA(TS Tinfinity)
where h is the HEAT TRANSFER COEFFICIENT
NUSSELT # Nu = hL/k a dimensionless parameter
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Radiation - 1
Radiation is emitted by any material at a finite temperature,T, this includessolids, liquids, and gases.
Temperature T is above absolute zero -273oC or 0oKelvin
A Black Body is a perfect source of radiant emission.
Emissive Power PLANCKS LAW
is STEFAN-BOLTZMANN CONSTANT = 5.67x10-8 W/m2/K4
A real surface emits less energy by the amount
where is the EMISSIVITY of the real surface
4TEb =
4
TE=
10
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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G IRRADIATION of a surface is sum of radiant energy
arriving at a surface from all sources.ABSORPTIVITY is fraction of irradiation that is adsorbed
GADS = G and E = T4
Conservation of energy yields:
qnett = GADS E
A GRAY surface has a emissivity that is independent ofdirection and wavelength.
Hence and GADS =
T
4
10
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Radiation Exchange - 1
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Nett qRAD = q/A = heat loss heat gain
qRAD = T4S G and because =
Then: qRAD =
(T4
s T4
sur)
If we include convection to gas then:
q = qCONV + qRAD= hA(Ts Tinfinity) + A(T
4s T
4sur)
Radiation Exchange - 2
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Modes of Heat Transfer
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Conservation of Energy 1st Law
Consider a control volume
The rate at which thermal and mechanical energy enters acontrol volume, plus the rate at which thermal energy isgenerated within the control volume, minus the rate at which
thermal energy and mechanical energy leave the controlvolume must equal the rate of increase of energy stored withinthe control volume.
i.e. If inflow of energy greater than outflow, difference must be
stored internally.
V
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Conservation of Energy over time t
The amount of thermal and mechanical energy that enters a control volume,
plus the amount of thermal energy that is generated within a control volume,
minus the amount of thermal and mechanical energy that leaves the control
volume must equal the increase in the amount of energy stored in the
control volume.
dtdEEEE stoutgin =+ &&&
is the volumetric energy generation rate
is the volumetric energy stored
Conservation of Energy:
gE&
stE&
t
dt
dEEEE stoutgin =+
V
gE&
stE&in
E& outE&
8/6/2019 Lecture 1 Chapt 1 Fundamentals
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Control Volume
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Surface Control Volume