Page 67 - Modelling in Transport Phenomena A Conceptual Approach
P. 67

48                             CHAPTER 3.  EVTER.F'PHASE  TRANSPORT


                The entire resistance to heat transfer is assumed to be due to a stagnant film
             in the fluid next to the wall.  The thickness of  the film, &, is such that it provides
             the same resistance to heat  transfer  as the resistance that exists for  the actual
             convection process.  The temperature gradient in the film is constant and is equal
             to
                                                                             (3.2- 10)


             Substitution of  Eq.  (3.2-10) into Eq. (3.2-9) gives

                                             (h=$(                           (3.2- 1 1)

             Equation (3.211) indicates that the thickness of the film, at, determines the value
             of  h.  For  this reason the term h is frequently referred to as the film heat  transfer
             coefficient.

             Example 3.2  Energy generation rate per unit volume as a result of  fission within
             a spherical reactor of  radius R is given as a finction of  position as
                                        ?I? [1- (:,"I
                                            R0
                                          =
             where r is the radial distance measured from the center of the sphere.  Cooling fluid
             at  a temperature  of Tw Bows ouer the reactor.  If the  average heat  transfer coefi-
             cient  (h) at the surface  of  the reactor is known,  determine the surface tempemture
             of  the reactor ut steady-state.

             Solution
             System:  Reactor
             Analysis

             The inventory  rate  equation for energy becomes
                            Rate of  energy out = Rate of  energy generation      (1)
             The rate at which energy leaves the sphere by convection is given by Newton's  law
             of  cooling  as
                              Rate  of  energy out = (47rR2)(h) (T, - T,)         (2)
             where T,,,  is the surface  temperature of the sphere.
                The rate of energy generation  can be  determined  by integrating  W over the vol-
             ume of  the sphere.  The result is
                                                                 '1
                 Rate of  energy generation = Jd2T Jdr Jd"  Ro [1- (G) r2 sin 8 drd8d4


                                           8lr
                                         =                                        (3)
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