Page 349 - Bird R.B. Transport phenomena
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Nonisothermal                     Systems




                            §11.1  The energy equation
                            §11.2  Special forms  of the energy equation

                            §11.3  The Boussinesq equation  of motion for forced  and free  convection
                            §11.4  Use of the equations  of change to solve steady-state  problems
                            §11.5  Dimensional analysis  of the equations  of change for nonisothermal  systems




                            In Chapter  10 we introduced  the shell energy balance method  for solving relatively  sim-
                            ple,  steady-state  heat  flow  problems.  We  obtained  the  temperature  profiles,  as  well  as
                            some derived  properties  such  as average temperature and  energy fluxes.  In this  chapter
                            we generalize the shell energy balance and  obtain  the equation of energy, a partial  differ-
                            ential equation that describes the transport  of energy in a homogeneous  fluid  or solid.
                               This chapter  is also closely related  to Chapter  3, where we introduced  the  equation
                            of  continuity  (conservation  of  mass)  and  the  equation  of  motion  (conservation  of  mo-
                            mentum). The addition  of  the equation  of  energy  (conservation  of  energy)  allows us  to
                            extend our problem-solving  ability to include nonisothermal  systems.
                               We  begin  in  §11.1  by  deriving  the  equation  of  change  for  the  total energy. As  in
                            Chapter  10, we use the combined  energy  flux  vector  e in applying  the law  of  conserva-
                            tion  of  energy.  In  §11.2 we  subtract  the  mechanical  energy equation  (given  in  §3.3)  from
                            the  total  energy  equation  to  get  an  equation  of  change  for  the  internal energy. From  the
                            latter we can get an equation  of change  for  the  temperature, and  it is this kind  of  energy
                            equation that is most commonly used.
                               Although  our  main  concern  in  this  chapter  will  be  with  the  various  energy  equa-
                            tions  just  mentioned,  we  find  it  useful  to  discuss  in  §11.3 an  approximate  equation  of
                            motion that is convenient  for solving problems involving free  convection.
                               In  §11.4 we summarize  the equations  of change encountered  up  to this point.  Then
                            we proceed  to illustrate  the use  of these equations  in  a series  of examples, in which  we
                            begin  with  the general equations and  discard  terms that are not needed.  In this way  we
                            have a standard procedure  for setting up and solving problems.
                               Finally,  in  §11.5 we  extend  the  dimensional  analysis  discussion  of  §3.7 and  show
                            how additional dimensionless groups arise in heat transfer  problems.


       111.1  THE ENERGY EQUATION
                            The equation  of change for energy is obtained by applying the law  of conservation  of en-
                            ergy to a small element  of volume  Ax Ay Az (see Fig. 3.1-1) and  then allowing the dimen-
                            sions  of  the  volume  element  to  become  vanishingly  small.  The  law  of  conservation  of

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