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target="_blank" rel="nofollow" href="#ulink_62fdc32a-ad7a-5e74-b7c3-5227b352c76d">(1.117)equation

      (1.118)equation

      (b) The Cylinder

      Consider a long cylinder (Figure 1.18) with uniform heat generation. The heat conduction equation can be rewritten as

      (1.120)equation

      After combining terms, the dimensionless temperature equation results:

      (1.121)equation

      The approach mentioned previously can also be used for obtaining the temperature distributions in solid spheres and spherical shells for a wide range of boundary conditions.

      1.6.9 Natural Convection

      Heat transfer by natural (or free) convection involving motion in a fluid is due to differences in density and the action of gravity, which causes a natural circulation flow and leads to heat transfer. For many problems involving fluid flow across a surface, the superimposed effect of natural convection is negligibly small. The heat transfer coefficients for natural convection are generally much lower than that for forced convection. When there is no forced velocity of the fluid, heat is transferred entirely by natural convection (when there is negligible radiation). For some practical cases, it is necessary to consider the radiative effect on the total heat loss or gain. Radiation heat transfer may be of the same order of magnitude as natural convection in some circumstances even at room temperatures. Hence, wall temperatures in a room can affect the comfort of occupants.

      It is pointed out that in many systems, involving multimode heat transfer effects, natural convection provides the largest resistance to heat transfer, and therefore plays an important role in the design or performance of the system. Moreover, when it is desirable to minimize the heat transfer rates or to minimize operating costs, natural convection is often preferred to forced convection.

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      1.6.10 Forced Convection

      The study of forced convection is concerned with the heat transfer occurring between a forced moving fluid and a solid surface. To apply Newton's law of cooling as given in Eq. (1.85), it is necessary to determine the heat transfer coefficient. For this purpose, the Nusselt–Reynolds correlations may be used. The definitions of the Nusselt and Reynolds numbers have been given in Table 1.9. Forced air and water coolers, forced air and water evaporators and condensers, and heat exchangers are examples of equipments commonly involved in forced convection heat transfer.

      Source: Olson and Wright [8].

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Equation or correlation
General equations
Nu = hY/kf = cRan and Ra = Gr Pr = (TsTa)Y3/νa
where n is 1/4 for laminar flow and 1/3 for turbulent flow. Y denotes the height for vertical plates or pipes, diameter for horizontal pipes, and radius for spheres. Tfm ≡ (Ts + Ta)/2.
Correlations for vertical plates (or inclined plates, inclined up to 60°)
Nu = [0.825 + 0.387Ra1/6/(1 + (0.492/Pr)9/16)4/9]2 for an entire range of Ra
Nu = 0.68 + 0.67Ra1/4/(1 + (0.492/Pr)9/16)4/9 for 0 < Ra < 109
Correlations for horizontal plates (YAs/P)
For upper surface of heated plate or lower surface of cooled plate:
Nu = 0.54Ra1/4 for 104 ≤ Ra ≤ 107
Nu = 0.15Ra1/3 for 107 ≤ Ra ≤ 1011
For lower surface of heated plate or upper surface of cooled plate:
Nu = 0.27Ra1/4 for 105 ≤ Ra ≤ 1010