- •Solution to integral momentum and energy equations with trial velocity and temperature profiles
- •Flow over a cylinder
- •Flow over a sphere
- •Heat transfer in flows across a bank of tubes
- •Reynolds analogy
- •Noncircular ducts
- •Thermal considerations
- •The mean temperature
- •Newton’s law of cooling
- •Fully developed conditions
- •Analytical solution for Nusselt number for a fully developed flow
- •Correlation for turbulent flow inside tubes and ducts
- •Problems
- •References
5.4 Approximate solution to the boundary layer equations 137
N uL = 0.662Re1/2 Pr1/3
N uL = 0.662 × (2.66 ×105 )1/2 (0.711)1/3
N uL = 304.77
N uL = hL = 304.77 kf
h = 304.77 × 0.027
1
h = 8.23 W/m2 K
The rate of heat transfer is given by
q = hA T
q = 494.1 W/m2
Flow over a cylinder
Flow over a cylinder is commonly encountered in several heat transfer applications like evaporator, condenser, recuperator, automative radiator, and so on. The special difficulty associated with flow over a cylinder is the curvature and its effect on the boundary layer development. Consider a flow over a cylinder, as shown in Fig. 5.3.
The key difference between the flat plate and this flow is that U∞ is no longer a constant and varies with x, as indicated in the figure. For θ = 0 to 90 , u∞ (x) increases
FIGURE 5.3
Development and separation of boundary layer over a cylinder.
138 CHAPTER 5 Forced convection
with x and this results in a favorable pressure gradient, whereas for 90 ≤ θ ≤ 180 , the fluid decelerates consequent upon which there is an adverse pressure gradient, and separation of the boundary layer occurs from the wall the condition for which is mathematically given by ∂u/∂y = 0. When the boundary layer detaches at the surface, a wake is formed in the downstream. Please refer to Incropera et al. (2013) for a more comprehensive discussion on this special flow. If ReD ≤ 2 ×105 , the flow stays laminar and separation occurs at θ = 80 . However, beyond a ReD of 2 ×105 , transition to turbulence (more on this in Section 5.5) occurs and separation takes place at θ = 140 .
For flow over a cylinder, the correlation for Nusselt number (NuD ) proposed by Zukauskas (1972) is of the form
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Pr 0.25 |
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The constants C, m are reported in Table 5.1.
This correlation is valid for 0.7 ≤ Pr ≤ 500 and 1 ≤ ReD ≤ 106. If Pr ≤ 10 then n = 0.37 and if Pr >10, then n = 0.36. Churchill and Bernstein (1977) have proposed a single comprehensive equation as follows
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+ |
0.62 Re1/2D Pr1/3 |
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5/8 4/5 |
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0.4 |
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28200 |
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0.25 1 |
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The above equation is recommended for all the values of ReD Pr ≥ 0.2
Flow over a sphere
Whitaker (1972) proposed a correlation for the average Nusselt number for flow over a sphere as follows.
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1/2 |
2/3 |
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1/2 |
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NuD = 2 + (0.4 ReD |
+ 0.06 ReD |
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s |
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This |
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is valid for 0.71 ≤ Pr ≤ 380,3.5 ≤ ReD ≤ 7.6 ×106 , and |
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1 ≤ / s |
≤ 3.2. All properties are to be evaluated at T |
except for s, which alone is to |
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be evaluated at the surface (or wall temperature) Ts (∞or Tw ). |
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Table 5.1 Constants in Eq. (5.135). |
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m |
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0.4–4 |
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0.989 |
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0.330 |
4−40 |
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0.911 |
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0.385 |
40–4000 |
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0.683 |
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0.466 |
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4000–40000 |
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0.193 |
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0.618 |
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40000–400000 |
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0.027 |
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0.805 |
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5.4 Approximate solution to the boundary layer equations 139
Heat transfer in flows across a bank of tubes
Flow and heat transfer over a bank of tubes or rod bundles frequently occur in industrial practice, as, for example, in heat exchangers, regenerators (for example, in an application where exhaust gases preheat the incoming fluid, say air or water), and in nuclear fuel rods. A variety of configurations are possible. Two frequently encountered ones are shown below in Figs. 5.4A and 5.4B.
In the above two figures, there are three rows of tubes. The difference between the two is that in (a) the arrangement is aligned and is frequently referred to as “in-line arrangement” while in (b) the arrangement of the tubes is staggered. There are two key geometrical parameters that enter the problem. These are the transverse pitch ST and the longitudinal pitch SL. For such flows, it is intuitive to expect that the average Nusselt number is a function of the pertinent parameters as follows.
FIGURE 5.4
Arrangement of (A) aligned and (B) staggered rows of tubes in tube/rod bundle.
140 CHAPTER 5 Forced convection
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= f (Re,Pr,ST , SL ) |
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NuD |
(5.138) |
Following the development presented in the earlier portions of this chapter, the Nusselt number should vary as
Nu |
D |
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= aReb Pr1/3Sc Sd , or |
(5.139) |
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L |
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Professor Zukauskas from Lithuania did extensive work and has presented reviews of heat transfer in these geometries. In fact, he synthesized the work of all the investigators before him and proposed a generic expression for NuD as
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= Pr0.36 (Pr/Prw )n Z (ReD ) |
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NuD |
(5.141) |
where n = 0 for gases and 0.25 for liquids. All properties need to be evaluated at the bulk fluid temperature, while Prw is evaluated at the wall temperature Tw .
For 102 ≤ ReD ≤ 103
Aligned rows : Z = 0.52ReD0.5
Staggered rows : Z = 0.71ReD0.5
For 103 ≤ ReD ≤ 2 ×105
Aligned rows : Z = 0.27 ReD0.63 , ST /SL ≥ 0.7
Staggered rows : Z = 0.35(ST /SL )0.2 ReD0.6 , ST /SL ≤ 2
For even higher Reynolds numbers and for liquid metals, please refer to Lienhard and Lienhard (2020), who have presented a comprehensive account of heat transfer across tube bundles.
Example 5.2: Consider a long pin fin of diameter 8 mm. The fin is made of aluminum (k = 205 W /mK ) and is maintained at a base temperature of 100 °C. Air at 30 °C flows over the fin with a velocity of 8 m/s.
a.Determine the heat transfer coefficient from the fin.
b.Determine the net heat transfer from the fin.
c.If the diameter of the fin is changed to 14 mm, with all other conditions being the same, determine the heat transfer coefficient and the heat transfer from the fin.
Solution: |
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u∞ D |
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The Reynolds number, ReD = |
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Air properties at T = |
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= 100 + 30 = 65 C = 338 K. |
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Now, we obtain the air properties at 338 K from Table 5.2 given on the next page.
5.4 Approximate solution to the boundary layer equations 141
Table 5.2 Thermophysical properties of air at atmospheric pressure (Kadoya et al., 1985; Jacobsen, R. T., et al., 1992).
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µ (kg/m.s) |
α (m2/s) |
ν (m2/s) |
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T(K) |
ρ (kg/m3) |
cp (J/kg.K) |
k (W/m.K) |
× 106 |
× 105 |
× 106 |
Pr |
100 |
3.605 |
1039 |
0.00941 |
7.11 |
0.251 |
1.97 |
0.784 |
135 |
2.739 |
1020 |
0.01267 |
9.38 |
0.486 |
3.65 |
0.757 |
150 |
2.368 |
1012 |
0.01406 |
10.35 |
0.587 |
4.37 |
0.745 |
170 |
2.128 |
1010 |
0.01578 |
11.54 |
0.764 |
5.63 |
0.739 |
200 |
1.769 |
1007 |
0.01836 |
13.33 |
1.031 |
7.54 |
0.731 |
225 |
1.591 |
1007 |
0.02038 |
14.69 |
1.305 |
9.46 |
0.726 |
250 |
1.412 |
1006 |
0.02241 |
16.06 |
1.578 |
11.37 |
0.721 |
260 |
1.358 |
1006 |
0.02329 |
16.49 |
1.705 |
12.14 |
0.712 |
270 |
1.308 |
1006 |
0.02400 |
16.99 |
1.824 |
12.99 |
0.712 |
273 |
1.294 |
1006 |
0.02400 |
17.13 |
1.841 |
13.25 |
0.712 |
280 |
1.261 |
1006 |
0.02473 |
17.47 |
1.879 |
13.85 |
0.711 |
290 |
1.217 |
1006 |
0.02544 |
17.95 |
2.078 |
14.75 |
0.710 |
300 |
1.177 |
1007 |
0.02623 |
18.57 |
2.213 |
15.78 |
0.713 |
310 |
1.139 |
1007 |
0.02684 |
18.89 |
2.340 |
16.59 |
0.709 |
320 |
1.103 |
1008 |
0.02753 |
19.35 |
2.476 |
17.54 |
0.708 |
330 |
1.070 |
1008 |
0.02821 |
19.81 |
2.616 |
18.51 |
0.708 |
340 |
1.038 |
1009 |
0.02888 |
20.25 |
2.821 |
19.51 |
0.707 |
350 |
1.008 |
1009 |
0.02984 |
20.90 |
2.931 |
20.73 |
0.707 |
360 |
0.983 |
1010 |
0.03052 |
21.34 |
3.089 |
21.82 |
0.706 |
380 |
0.932 |
1012 |
0.03191 |
22.22 |
3.405 |
24.01 |
0.705 |
400 |
0.882 |
1014 |
0.03328 |
23.10 |
3.721 |
26.19 |
0.704 |
420 |
0.843 |
1017 |
0.03459 |
23.93 |
4.059 |
28.55 |
0.704 |
440 |
0.803 |
1020 |
0.03590 |
24.76 |
4.397 |
30.92 |
0.703 |
450 |
0.784 |
1021 |
0.03656 |
25.17 |
4.567 |
32.10 |
0.703 |
460 |
0.768 |
1023 |
0.03719 |
25.56 |
4.746 |
33.37 |
0.703 |
480 |
0.737 |
1027 |
0.03845 |
26.35 |
5.105 |
35.91 |
0.704 |
500 |
0.706 |
1030 |
0.03971 |
27.13 |
5.464 |
38.45 |
0.704 |
550 |
0.642 |
1040 |
0.04277 |
29.02 |
6.412 |
45.24 |
0.706 |
600 |
0.588 |
1051 |
0.04573 |
30.82 |
7.400 |
52.42 |
0.708 |
650 |
0.543 |
1063 |
0.04863 |
32.57 |
8.430 |
60.01 |
0.712 |
700 |
0.504 |
1075 |
0.05146 |
34.25 |
9.498 |
67.96 |
0.715 |
750 |
0.471 |
1087 |
0.05425 |
35.88 |
10.612 |
76.23 |
0.719 |
800 |
0.441 |
1099 |
0.05699 |
37.47 |
11.761 |
84.97 |
0.723 |
900 |
0.392 |
1121 |
0.06237 |
40.52 |
14.193 |
103.42 |
0.728 |
1000 |
0.353 |
1142 |
0.06763 |
43.43 |
16.792 |
123.13 |
0.733 |
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142CHAPTER 5 Forced convection
ρ= 1.038 kg/m3 cp = 1009 J/kg.K
ν= 1.951 × 10−5
k = 0.0289 W/mK Pr = 0.707
(For convenience, all properties were taken at 340 K.)
ReD = |
u |
∞ |
D |
= |
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× 8 |
×10−3 |
= 3280 |
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19.51×10−6 |
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The constants C and m from Table 5.1 corresponding to this Reynolds number are
C = 0.683 and m = 0.466.
Nu = 0.683Re0.466 Pr0.37 Pr 0.25
D
Prs
Prs = 0.706
(It is to be noted that for air, unless the temperature difference between the surface and the surrounding is very high (100 to 150 °C), the Prandtl number correction parameter will have a negligible role in the determination of the Nusselt number.)
a. For the problem under consideration,
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b. |
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94.43 × π × 8 × 10−3 × π × |
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× 205 |
× 70 |
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Q= 10.94 W
c.When the fin diameter is increased to 14 mm
ReD = 3280 × 148 = 5740
Now, the constants C and m change to 0.193 and 0.618, respectively.
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0.25 |
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NuD = 35.72
5.4 Approximate solution to the boundary layer equations 143
h = |
NuD |
.k |
= |
35.72 × 0.0289 |
= 73.75 W/m2K |
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π × 14 × 10−3 × |
π × |
(14 |
× 10−3 )2 |
× 205 × 70 |
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The key takeaway from this problem is that if we had tried to solve this problem with knowledge of only fin heat transfer but without any idea of how the heat transfer coefficient will change for a change in diameter, our solution would have been
Q |
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.k θ |
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1.5 |
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Q2 = 2.311
Q1
The actual ratio of Q2 /Q1 We obtained is 2.04 (i.e., 22.37 W/10.94 W), which leads to a significantly different result by about 15%.
Example 5.3: A heated sphere made of aluminum (k = 205 W/mK) of 8 mm diameter at 100 °C cools in a current of air at 30 °C, with a free stream velocity of 8 m/s. The density and specific heat of aluminum are 2700 kg/m3 and 900 J /kgK respectively.
a.Determine the heat transfer coefficient from the sphere.
b.Determine the time constant of the sphere.
c.How much time will it take for the sphere to cool to 50 °C.
Neglect radiation from the sphere.
Solution:
a. The Reynolds number ReD , is given by
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∞ |
D |
= |
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8 × 8 ×10−3 |
= 3280 |
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19.51× |
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ReD , is the same as in part (a) of Example 5.2. |
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0.5 |
+ 0.06(3280) |
0.667 |
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144 CHAPTER 5 Forced convection
b. Time constant
τ = |
mcp |
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π (4 × 10−3 )3 × 900 |
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τ= 27.33 s
c.Let us now calculate the Biot number.
Bi = hr = 118.58 × 4 ×10−3 3k 3× 205
Bi = 0.00077
Since Bi < 0.1, the lumped capacitance method is valid. Recalling the solution for a spatially lumped object undergoing cooling (from Chapter 3),
((T − T∞ )) = e−t /T
Ti − T∞
(50 − 30) = e−t /27.33
(100 − 30)
0.2857 = e−t /27.33t = 34.24 s
5.5 Turbulent flow
Consider flow and heat transfer over a flat plate. Up to ReL = 5 ×105 , the flow stays laminar and beyond this there is transition to turbulence. The boundary layer grows thicker and eddies, and consequent mixing will be in the transition region and in the fully turbulent region beyond the transition. A depiction of the boundary layer flow over a flat plate is shown in Fig. 5.5.
FIGURE 5.5
Forced convection boundary layer development over a horizontal flat plate depicting the laminar, transition, and turbulent regions of flow.
5.5 Turbulent flow 145
FIGURE 5.6
Typical variation of velocity with time for a turbulent flow.
In the turbulent regions of flow, we encounter time-dependent velocities and temperatures, and these dependencies are characterized by fluctuations.
For example, the horizontal velocity u may be expressed as
u = |
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+ u′ |
(5.142) |
u |
In the above equation, u is the mean velocity and u′ is the fluctuating component. The velocity u typically varies with time, as shown in Fig. 5.6.
Similarly,
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+ v′ |
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and |
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T = |
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u |
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u = |
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1 |
∫ T0 u dt |
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T0 is the integrating time and must be larger than the slowest fluctuations associated with velocity u or any variable for that matter.
For two-dimensional, steady, incompressible flow with constant properties, using the expressions for u, v, and T , with the inclusion of fluctuating components, the governing equations after applying the boundary layer assumptions become
∂∂ux + ∂∂uy
ρu ∂u + v ∂u∂x ∂y
=0
=∂ µ ∂u
∂y ∂y
(5.146)
− ρu′v′ (5.147)
146CHAPTER 5 Forced convection
and
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∂ |
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∂ |
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∂ |
∂ |
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T |
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T |
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ρcp u |
∂x |
+ v |
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∂y |
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∂y |
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− ρcp v′T ′ (5.148)
The above equations are obtained after we perform time averaging of the governing equations. Let us demonstrate this for term uv.
Consider the term
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= |
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= |
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+ |
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+ u′ |
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+ |
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(u + u ')(v + v ') |
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uv |
u v |
u′v′ |
v |
uv′ |
(5.149) |
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However, as fluctuations have a zero mean |
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′ = 0 |
(5.150) |
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u |
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and |
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′ = 0 |
(5.151) |
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v |
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But, |
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≠ 0 |
(5.152) |
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u′v′ |
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uv = u v + |
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u′ |
v′ |
(5.153) |
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(with the understanding that u v = u v).
A similar procedure can be followed for other terms in the momentum and energy equations.
Now, we can define two new quantities, namely, total shear stress, τ total, and total heat flux, qtotal , as follows
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∂ |
u |
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(5.154) |
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τ total = µ ∂y − ρu′v′ |
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and |
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∂ |
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qtotal = − |
T |
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(5.155) |
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k |
∂y |
− ρcp v′T ′ |
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Now we introduce two new quantities, namely, eddy viscosity of momentum, εm , and eddy viscosity of heat, εH, as follows.
ρεm |
∂u |
= −ρ |
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u′v′ |
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∂y |
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(5.156) |
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and
ρcpεH |
∂ |
H |
= −ρcp |
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v′T′ |
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(5.157) |
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∂y |
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∂ |
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τ total |
= ρ (ν +εm ) |
u |
(5.158) |
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∂y |
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