Heat Conduction

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Fluids Review
TRN-1998-004
Heat Transfer
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Outline
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Introduction
Modes of heat transfer
Typical design problems
Coupling of fluid flow and heat transfer
Conduction
Convection
Radiation
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Introduction
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Heat transfer is the study of thermal energy (heat) flows
Heat always flows from “hot” to “cold”
Examples are ubiquitous:
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heat flows in the body
home heating/cooling systems
refrigerators, ovens, other appliances
automobiles, power plants, the sun, etc.
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Modes of Heat Transfer
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Conduction - diffusion of heat due to temperature gradient
Convection - when heat is carried away by moving fluid
Radiation - emission of energy by electromagnetic waves
qconvection
qradiation
qconduction
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Fluids Review
TRN-1998-004
Typical Design Problems
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To determine:
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overall heat transfer coefficient - e.g., for a car radiator
highest (or lowest) temperature in a system - e.g., in a gas turbine
temperature distribution (related to thermal stress) - e.g., in the walls of a
spacecraft
temperature response in time dependent heating/cooling problems - e.g.,
how long does it take to cool down a case of soda?
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Fluids Review
TRN-1998-004
Heat Transfer and Fluid Flow
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As a fluid moves, it carries heat with it -- this is called convection
Thus, heat transfer can be tightly coupled to the fluid flow solution
Additionally:
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The rate of heat transfer is a strong function of fluid velocity
Fluid properties may be strong functions of temperature (e.g., air)
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Fluids Review
TRN-1998-004
Conduction Heat Transfer
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Conduction is the transfer of heat by molecular interaction
In a gas, molecular velocity depends on temperature
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hot, energetic molecules collide with neighbors, increasing their speed
In solids, the molecules and the lattice structure vibrate
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Fourier’s Law
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“heat flux is proportional to temperature gradient”
 T T 
Q
 q  kT  k 


A
 x y 


units for q
are W/m2
where k = thermal conductivity
in general, k = k(x,y,z,T,…)
temperature profile
heat conduction in a slab
dT
dx
1
hot wall
cold wall
x
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Generalized Heat Diffusion Equation
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If we perform a heat balance on a small volume of material…
heat conduction
in

T
q
… we get:
heat conduction
out
heat generation
T
2
c
 k T  q
t
rate of change
of temperature

heat cond. heat
in/out
generation
k
 thermal diffusivity
c
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Fluids Review
TRN-1998-004
Boundary Conditions
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Heat transfer boundary conditions generally come in three types:
q = 20 W/m2
specified heat flux
Neumann condition
T = 300K
specified temperature
Dirichlet condition
Tbody
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q = h(Tamb-Tbody)
external heat transfer
coefficient
Robin condition
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Conduction Example
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Compute the heat transfer through the wall of a home:
Tout = 20° F
Tout = 68° F
Although slight, you
can see the “thermal
bridging” effect
through the studs
2x6 stud
k=0.15 W/m2-K
sheetrock
k=0.4 W/m2-K
shingles
k=0.15 W/m2-K
fiberglas insulation
sheathing
k=0.004 W/m2-K
k=0.15 W/m2-K
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Convection Heat Transfer
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Convection is movement of heat with a fluid
E.g., when cold air sweeps past a warm body, it draws away warm air
near the body and replaces it with cold air
flow over a
heated block

often, we want to know the heat transfer coefficient, h (next page)
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Fluids Review
TRN-1998-004
Newton’s Law of Cooling
T
q
Tbody
q  h (Tbody  T )  h T
h  average heat transfer coefficient (W/m2-K)
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Heat Transfer Coefficient
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h is not a constant, but h = h(T)
Three types of convection:
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Natural convection
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1
4
h  T , h  T
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Typical values of h:
fluid moves due to buoyancy
1
3
Thot
4 - 4,000 W/m2-K
Forced convection
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flow is induced by external means
h  const

Tcold
Tcold
Thot
80 - 75,000
Boiling convection
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body is hot enough to boil liquid
h  T
Tcold
Thot
2
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300 - 900,000
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Looking in more detail...
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Just as there is a viscous boundary layer in the velocity distribution,
there is also a thermal boundary layer
thermal boundary
layer edge
velocity boundary
layer edge
y
T , U
T ( y)
t

Tw
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Nusselt Number
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Equate the heat conducted from the wall to the same heat transfer in
convective terms:
conductivity
of the fluid

T
kf
 h(Tw  T )
y
Define dimensionless quantities:
Tw  T
T
Tw  T

y
y
L
Then rearrange to get:
 T T 

  w
 Tw  T   hL  Nu
kf
 y
 
 L
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Nusselt number
“dimensionless heat
transfer coefficient”
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Energy Equation
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Generalize the heat conduction equation to include effect of fluid
motion:
T
c
 u  T  k2T  q
t
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Assumes incompressible fluid, no shear heating, constant properties,
negligible changes in kinetic and potential energy
Can now solve for temperature distribution in boundary layer
Then calculate h using Fourier’s law:
From calculated
q
k
T
temperature
h

distribution
T T
T  T y
w

w
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
y 0
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Correlations for Heat Transfer Coefficient
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As an alternative, can use correlations to obtain h
E.g., heat transfer from a flat plate in laminar flow:
Nu x  0.332 Re 0x.5 Pr 0.333
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where the Prandtl number is defined as:
 c 
Pr 

 k 
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momentum diffusivit y
thermal diffusivit y
Typical values are:
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Pr = 0.01 for liquid metals
Pr = 0.7 for most gases
Pr = 6 for water at room temperature
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Convection Examples
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Developing flow in a pipe (constant wall temperature)
Tw
T
T
Tw
T
Tw
T
T
Tw
Tw
bulk fluid temperature
heat flux from wall
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x
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Convection Examples
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Natural convection (from a heated vertical plate)
T
   (T )
Tw
As the fluid is warmed by the plate,
its density decreases and a buoyant
force arises which induces flow in
the vertical direction. The force is
equal to:
(    ) g
u
gravity
The dimensionless group that
governs natural convection is the
Rayleigh number:
T , 
Ra 
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gTL3

© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Radiation Heat Transfer
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Thermal radiation is emission of energy as electromagnetic waves
Intensity depends on body temperature and surface characteristics
Important mode of heat transfer at high temperatures
Can also be important in natural convection problems
Examples:
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toaster, grill, broiler
fireplace
sunshine
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Surface Characteristics
q W/m2
(incident energy flux)
q (reflected)
q (absorbed)
translucent slab
q (transmitted)
1     
absorptance
transmittance
reflectance
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Black Body Radiation
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A “black body”:
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is a model of a perfect radiator
absorbs all energy that reaches it; reflects nothing
therefore  = 1,  =  = 0
The energy emitted by a black body is the theoretical maximum:
q s T4
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This is Stefan-Boltzmann law; s is the Stefan-Boltzmann constant
(5.6697e-8 W/m2-K4)
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
“Real” Bodies
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Real bodies will emit less radiation than a black body:
q  s T 4
emissivity (between 0 and 1)
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Example: radiation from a small body to its surroundings
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both the body and its surroundings emit thermal radiation
the net heat transfer will be from the hotter to the colder
Qnet   As (Tw4  T4 )
Qnet
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T
q
qw
Tw
A
© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
When is radiation important?
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Radiation exchange is significant in high temperature problems: e.g.,
combustion
Radiation properties can be strong functions of chemical composition,
especially CO2, H2O
Radiation heat exchange is difficult solve (except for simple
configurations) — we must rely on computational methods
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© Fluent Inc. 3/19/2016
Fluids Review
TRN-1998-004
Heat Transfer — Summary
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Heat transfer is the study of thermal energy (heat) flows:
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The fluid flow and heat transfer problems can be tightly coupled
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
conduction
convection
radiation
through the convection term in the energy equation
when properties (, ) are dependent on temperature
While analytical solutions exist for some simple problems, we must
rely on computational methods to solve most industrially relevant
applications
Can I go back to
sleep now?
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© Fluent Inc. 3/19/2016
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