quick reference for heat transfer analysis jason valentine...
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Quick Reference for Heat Transfer Analysiscompiled by Jason Valentine and Greg WalkerPlease contact [email protected] with corrections and suggestions
copyleft 2018: You may copy, distribute, and modify and redistribute as long as you attribute the originalauthor and distribute with an equivalent license.
Version: October 9, 2018
Nomenclature:
symbol name unitsq heat transfer Wq′′ heat flux W/m2
q′′′ = g generation W/m3
k thermal conductivity W/m KE energy rate WR thermal resistance K/WG conductance W/KR′′ thermal resistance m2 K/Wh convection coefficient W/m2KU overall heat transfer coefficient W/m2Kθ temperature difference K (or ◦C)C = mcp thermal capacitance W/Kω periodic frequency rad/s
Conversions:
1 R-value = 1h ft2 ◦F
btu= 0.176
m2 K
W1 kW = 0.284 tons of refrigeration
Physical Constants:
name parameterStefan-Boltzmann σ = 5.670× 10−8 W/m2K4
Boltzmann kB = 1.381× 10−23 J/Kblackbody C1 = 2πhc20 = 3.742× 108 Wµm4/m2
blackbody C2 = hc0/kB = 1.439× 104 µm KWien’s C3 = 2898µm Kspeed of light c0 = 2.998× 108 m/sPlanck’s constant h = 6.626× 10−34 J s
Assumed values:
name parametersolar constant q′′solar = 1370 W/m2
solar temperature Tsolar = 5780 Kgravity g = 9.81 m/s2
critical Reynolds for flat plate Recr = 5× 105
critical Reynolds for inside tube Recr = 2300critical Rayleigh for vertical plate Racr = 109
radius of the Sun RSun = 6.957× 105 kmaverage distance to the Sun LSun = 150× 106 km
1 Conduction
1.1 Equivalent resistance
Assumptions:
1. steady state
2. constant properties
3. one-dimensional transport
4. no generation
expression cartesian cylindrical spherical
heat equationd2T
dx2= 0
1
r
d
dr
(rdT
dr
)= 0
1
r2d
dr
(r2dT
dr
)= 0
temperaturedistribution
T1 −∆Tx
LT2 + ∆T
ln(r/r2)
ln(r1/r2)T1 −∆T
1− (r1/r)
1− (r1/r2)
heat flux k∆T
L
k∆T
r ln(r2/r1)
k∆T
r2(1/r1 − 1/r2)
heat transfer kA∆T
L
2πLk∆T
ln(r2/r1)
4πk∆T
1/r1 − 1/r2
resistanceL
kA
ln(r2/r1)
2πkL
1/r1 − 1/r24πk
criticalradius
–k
h
2k
hr1 < r2; ∆T = T1 − T2
1.2 Shape Factors
Description schematic restrictions shape factor
isothermal sphere in asemi-infinite medium
T1
T2
z
D
z > D/22πD
1−D/4z
horizontal isothermalcylinder buried in asemi-infinite medium
T1
T2
z
L
D L� D2πL
cosh−1(2z/D)
2
vertical cylinder in asemi-infinite medium
T1
T2
L
D
L� D2πL
ln(4L/D)
two parallel cylinders oflength L in infinitemedium
D1
w
T2
D2T
1
L� D1, D2L� w
2πL
cosh−1(
4w2−D21−D2
2
2D1D2
)
circular cylinder of lengthL midway between twoparallel plates of equallength and infinite width
T2
T2
z
z
T1
D
z � D/2L� z
2πL
ln(8z/πD)
cylinder of length Lcentered in a square solidof equal length
T2
T1
D
ww > DL� w
2πL
ln(1.08w/D)
eccentric circular cylinderof length L in a cylinderof equal length
T2
T1
d
D
z
D > dL� D
2πL
cosh−1(D2+d2−4z2
2Dd
)
conduction through theedge of adjoining walls
T2
T1
D
L
D > 5L 0.54D
3
conduction through thecorner of three walls witha temperature difference∆T1−2 across the walls L
L� length and width 0.15L
disk of diameter D andtemperature T1 on asemi-infinite medium oftemperature T2
T2
T1
D
none 2D
square channel of lengthL
L
W
w
T1
2T
W/w < 1.42πL
0.785 ln(W/w)
W/w > 1.4 2πL
0.930 ln(W/w)− 0.050L�W
1.3 Temperature distribution for fins of uniform cross section
tip boundary θ(x)/θb heat transfer
θ(L) = θL(θL/θb) sinhβx+ sinhβ(L− x)
sinhβLkAcβθb
coshβL− θL/θbsinhβL
dθ
dx
∣∣∣∣x=L
= 0coshβ(L− x)
coshβLkAcβθb tanhβL
θ(L→∞) = 0 e−βx kAcβθb
dθ
dx
∣∣∣∣x=L
= −hkθ(L)
coshβ(L− x) + (h/βk) sinhβ(L− x)
coshβL+ (h/βk) sinhβLkAcβθb
sinhβL+ (h/βk) coshβL
coshβL+ (h/βk) sinhβL
β =√hP/kAc
θ ≡ T − T∞θb = θ(0) = T (0)− T∞θL = θ(L) = T (L)− T∞
4
1.4 Fin charts
1.4.1 Plate fins (or straight fins)
rectangle
w
2t
ηf =tanh ξ
ξ
triangle
w
2t
ηf =1
ξ
I1(2ξ)
I0(2ξ)
parabola
w
2t
ηf =2
1 +√
1 + 4ξ2
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
η
ξ = w√h/kt
rectangular fintriangular finparabolic fin
5
1.4.2 Spines (or pin fins)
rectangle
w
2t ηf =tanh
√2ξ√
2ξ
triangle
w
2t
ηf =2√2ξ
I2(2√
2ξ)
I1(2√
2ξ)
parabola
w
2t
ηf =2
1 +√
1 + 89ξ
2
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
η
ξ = w√h/kt
rectanglar fintrianglar fin
parabolic fin
6
1.4.3 Annular fins (or circular fins)
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
0 0.5 1 1.5 2 2.5 3 3.5 4 4.5 5
η
ξ = w√h/kt
re/r
b = 1
re/r
b = 2
re/r
b = 3
re/r
b = 5
2t
rb
re
w
1.5 Semi-infinite slab solutions
penetration depth (90%): δp = 2.3√αt
1.5.1 Constant surface temperature T (0, t) = Ts
T (x, t)− TsTi − Ts
= erf
(x√4αt
)q′′s (t) =
k(Ts − Ti)√παt
1.5.2 Constant surface heat flux q′′(0, t) = q′′o
T (x, t)− Ti =q′′ok
[√4αt
πexp
(− x2
4αt
)− x erfc
(x√4αt
)]
1.5.3 Surface convection −k dT/dx|x=0 = h[T∞ − T (0, t)]
T (x, t)− TiT∞ − Ti
= erfc
(x√4αt
)− exp
(hx
k+h2αt
k2
)erfc
(x√4αt
+h√αt
k
)
7
1.5.4 Surface pulse of energy E
T (x, t)− Ti =E
ρc√παt
exp
(− x2
4αt
)
1.5.5 Steady-periodic
T (x, t)− Ti∆T
= exp(−x√ω/2α
)sin(ωt− x
√ω/2α
)penetration depth (90%): δp = 4
√α/ω
NB: ω has units of rad/s, not Hz.
1.5.6 Two semi-infinite slabs in contact
Ts =(√ρck)ATA,i + (
√ρck)BTB,i
(√ρck)A + (
√ρck)B
8
2 Convection
2.1 Forced/external: plate and sphere
Geometry Correlation Conditions
flat plate Nux = 0.332 Re1/2x Pr1/3 laminar, local, Tf , Pr > 0.6
flat plate NuL = 0.664 Re1/2L Pr1/3 laminar, average, Tf , Pr > 0.6
flat plate Nux = 0.0296 Re4/5x Pr1/3 turbulent, local, Tf , Rex < 108, 0.6 < Pr < 60
flat plate NuL = (0.037 Re4/5L − 871) Pr1/3
mixed, average, Tf , Recr = 5× 105,ReL < 108, 0.6 < Pr < 60
sphere NuD = 2 + (0.4 Re1/2D + 0.06 Re
2/3D ) Pr1/3
average, T∞, 3.5 < Re < 7.6× 104,0.71 < Pr < 380
falling drop NuD = 2 + 0.6 Re1/2D Pr1/3 average, T∞
Rex = U∞xν Nux = hx
kf
2.2 Forced/external: cylinder in a cross-flow
NuD =hD
k= C RemD Pr1/3 ReD =
U∞D
ν
ReD C m0.4–4 0.989 0.3304–40 0.911 0.385
40–4000 0.683 0.4664000–40,000 0.193 0.618
40,000–400,000 0.027 0.805 10-1
100
101
102
103
104
105
100
101
102
103
104
105
Nu
––
D
ReD
air
water
oil
2.3 Forced/external: non-circular bars
NuD =hD
k= C RemD Pr1/3
Geometry ReD C msquare
V 6000–60,000 0.304 0.59
V 5000–60,000 0.158 0.66thin plate
Vfront
back10,000–50,000 0.667 0.5007000–80,000 0.191 0.667
D is the height of the object
102
104
105
Nu
––
D/P
r1/3
ReD
diamondsquare
plate frontplate back
9
2.4 Forced/internal: turbulent flow in circular tubes
Geometry Correlation Conditions
circular tube NuD = 0.023 Re4/5D Prn
turbulent, fully developed, 0.6 < Pr < 160,n = 0.4 for Ts > Tm, n = 0.3 for Ts < Tm
ReD = 4mπDµ Dh = 4Ac
P Recr = 2300
2.5 Forced/internal: fully developed laminar flow in tubes
section uniform qs uniform Tscircular 4.36 3.66rectangular see chart belowinfinite plates (b→∞) 8.23 7.54infinite plates (one sided) 5.39 4.86
2
3
4
5
6
7
1 2 3 4 5 6 7 8
Nusselt n
um
ber
(Nu
D)
aspect ratio (b/a)
uniform qsuniform Ts
b
a
10
2.6 Natural/external
Geometry Correlation Conditions
vertical plate NuL = 0.59Ra1/4L laminar (104 < RaL < 109)
vertical plate NuL = 0.10Ra1/3L turbulent (109 < RaL < 1013)
horizontal plate NuL = 0.54Ra1/4L
upper surface of hot plate orlower surface of cold plate;104 < RaL < 107; Pr > 0.7
horizontal plate NuL = 0.15Ra1/3L
upper surface of hot plate orlower surface of cold plate;107 < RaL < 1011
horizontal plate NuL = 0.52Ra1/5L
lower surface of hot plate orupper surface of cold plate;104 < RaL < 109, Pr > 0.7
horizontal cylinder NuD =
{0.60 +
0.387Ra1/6D
[1 + (0.559/Pr)9/16]8/27
}2
RaD < 1012
sphere NuD = 2 +0.589Ra
1/4D
[1 + (0.469/Pr)9/16]4/9RaD < 1011; Pr > 0.7
Rax = gβ(Ts−T∞)x3
να
For 0 < θ < 60◦, where θ is the angle measured from vertical, use the vertical plate expression with greplaced by g cos θ.
2.7 Natural/internal
Geometry Correlation Conditions
horizontal cavity NuL = 0.069Ra1/3L Pr0.074
heated from below;3× 105 < RaL < 7× 109
horizontal cavity NuL = 1 heated from above
vertical cavity NuL = 0.22
(Pr
0.2 + PrRaL
)0.28(H
L
)−1/4 2 < H/L < 10; Pr < 105;103 < RaL < 1010
vertical cavity NuL = 0.18
(Pr
0.2 + PrRaL
)0.29 1 < H/L < 2; 10−3 < Pr < 105;103 < RaLPr
0.2+Pr
vertical cavity NuL = 0.42Ra1/4L Pr0.012(H/L)−0.3
10 < H/L < 40; 1 < Pr < 2× 104;104 < RaL < 107
H is cavity height; L is distance between heated sides.
11
3 Radiation
3.1 Blackbody Emissive Power (band emission)
nλT F0→nλT nλT F0→nλT(µm K) (µm K)
200 0.0000 6200 0.7541400 0.0000 6400 0.7692600 0.0000 6600 0.7832800 0.0000 6800 0.7961
1000 0.0003 7000 0.80811200 0.0021 7200 0.81921400 0.0078 7400 0.82951600 0.0197 7600 0.83911800 0.0393 7800 0.84802000 0.0667 8000 0.85632200 0.1009 8500 0.87462400 0.1403 9000 0.89002600 0.1831 9500 0.90302800 0.2279 10000 0.91422898 0.2501 10500 0.92373000 0.2732 11000 0.93183200 0.3181 11500 0.93893400 0.3617 12000 0.94513600 0.4036 13000 0.95513800 0.4434 14000 0.96294000 0.4809 15000 0.96894200 0.5160 16000 0.97384400 0.5488 17000 0.97774600 0.5793 18000 0.98084800 0.6075 20000 0.98565000 0.6337 25000 0.99225200 0.6579 30000 0.99535400 0.6803 40000 0.99795600 0.7010 50000 0.99895800 0.7201 75000 0.99976000 0.7378 100000 0.9999
0
0.1
0.2
0.3
0.4
0.5
0.6
0.7
0.8
0.9
1
1000 10000 100000
F0
-nλ
T
nλT (µm K)
10-10
10-5
100
105
1010
0.01 0.1 1 10 100 1000 10000
Draper point
0.0936
em
issiv
e p
ow
er
(W/m
2 µ
m)
wavelength (µm)
3 K77 K
303 K798 K
5780 KWien’s law
12
3.2 View factors
3.2.1 2D configurations (infinite into page)
Configuration Relation
w
w➋
➊
hH = h/w
F12 = F21 =√
1 +H2 −H
➋
➊
w
α
w
F12 = F21 = 1− sin(α
2
)
w
h
➋
➊
H = h/w
F12 =1
2
(1 +H −
√1 +H2
)
r r
➊➋s
X = 1 +s
2r
F12 = F21 =1
π
(√X2 − 1 + sin−1
1
X−X
)r➋
a
b
➊
c F12 =r
b− a
(tan−1
b
c− tan−1
a
c
)
13
3.2.2 3D configurations
Configuration Relation
h
y
x
➊
➋
0.01
0.1
1
0.1 1 10
y/h=0.1
0.2
0.4
1.0
2.0
10.0
F1
2
x/h
h
r2
r1
➋
➊
0
0.2
0.4
0.6
0.8
1
0.1 1 10
r2/h=0.3
0.5
0.7
1.0
1.5
2.0
3.04.0
6.010.0
F1
2
h/r1
l
h
w
➋
➊
0
0.1
0.2
0.3
0.4
0.5
0.1 1 10
w/l=10
4.0
2.0
1.0
0.6
0.4
0.2
0.1
0.05
F1
2
h/l
14
4 Heat exchanger relations
NTU =UA
Cmin; ε =
q
qmax; Cr =
Cmin
Cmax
Single stream (Cr = 0): ε = 1− exp(−NTU)
parallel counterflow
0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00 0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00
shell and tube 1-pass shell and tube 2-pass
0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00 0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00
crossflow (unmixed) crossflow (mixed)
0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00 0
0.2
0.4
0.6
0.8
1
0 1 2 3 4 5
mixedmixed
dashed Cmaxdashed Cmax
solid Cminsolid Cmin
ε
NTU
Cr = 0.00
Cr = 0.25
Cr = 0.50
Cr = 0.75
Cr = 1.00
15
5 Material Properties
5.1 Solids
substance k (W/m K) cp (J/kg K) ρ (kg/m3) α (m2/s)aluminum 237 903 2702 97.1× 10−6
brick 0.72 835 1920 0.45× 10−6
cork 0.039 1800 120 0.18× 10−6
copper 401 385 8933 117× 10−6
diamond 2300 509 3500 1290× 10−6
fiberglass 0.038 835 32.0 0.142× 10−6
germanium 59.9 322 5360 34.7× 10−6
glass 1.38 745 2220 0.834× 10−6
gold 317 129 19300 127× 10−6
silicon 148 712 2330 89.2× 10−6
stainless 13.4 468 8238 3.48× 10−6
steel 60.5 434 7850 17.8× 10−6
styrofoam 0.040 1210 16.0 2.07× 10−6
tungsten 174 132 19300 68.3× 10−6
5.2 Fluids
substance k (W/m K) cp (J/kg K) ρ (kg/m3) ν (m2/s) α (m2/s) Prair 0.0263 1010 1.16 15.9× 10−6 22.5× 10−6 0.707freon 0.0803 1430 1200 0.145× 10−6 0.0468× 10−6 3.40mercury 8.54 139 13500 0.113× 10−6 4.55× 10−6 0.0248oil 0.145 1910 884 550× 10−6 0.0859× 10−6 6400water 0.613 4180 1000 0.858× 10−6 0.146× 10−6 5.83
5.3 Phase change
heat of fusion for water: hsf = 333.7 kJ/kgheat of vaporization for water: hfg = 2257 kJ/kg
16
6 Non-dimensional quantities
name expression description
Biot Bi =hL
ks
ratio of internal thermal resistance to the externalthermal resistance
Fourier Fo =αt
L2dimensionless time
Grashof Gr =gβ(Ts − T∞)L3
ν2ratio of buoyancy forces to viscous forces whereβ = 1/T
Jakob Ja =cp(Ts − Tsat)
hfgratio of sensible heat to latent energy
Nusselt Nu =hL
kfratio of convection to conduction in a fluid
Prandtl Pr =ν
α
ratio of momentum b.l thickness to thermal b.l.thickness
Rayleigh Ra =gβ(Ts − T∞)L3
να
ratio of thermally derived buoyancy to thermaldissipation (Ra = GrPr, where β = 1/T )
Reynolds Re =UL
νratio of inertial and viscous forces
7 Math
7.1 Solutions to ODEs
ODE solution
dy
dx+ λy = α y = C1 exp(−λx) +
α
λ
d2y
dx2− λ2y = α y = C1 exp(−λx) + C2 exp(λx)− α
λ2
y = C3 cosh(λx) + C4 sinh(λx)− α
λ2
d2y
dx2+ λ2y = α y = C1 cos(λx) + C2 sin(λx) +
α
λ2
17