Page 102 - Bird R.B. Transport phenomena
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§3.6  Use of the Equations of Change to Solve  Flow Problems  87

                     In Chapter  1 we  gave the components  of  the stress  tensor  in Cartesian coordinates,
                 and  in this chapter we  have  derived  the equations  of continuity and motion in Cartesian
                 coordinates.  In  Tables  B.I,  4,  5,  6,  and  7  we  summarize  these  key  equations  in  three
                 much-used coordinate systems:  Cartesian  {x, y, z), cylindrical  (г, 0, z), and spherical  (r, 0,
                 ф). Beginning  students should  not concern themselves  with  the derivation  of  these equa-
                 tions, but they should  be very  familiar  with  the tables  in Appendix  В and be able  to use
                 them  for  setting  up  fluid  dynamics  problems.  Advanced  students  will  want  to  go
                 through the details  of Appendix  A and learn how  to develop  the expressions  for  the var-
                 ious V-operations, as  is done in §§A.6 and  A.7.
                     In  this  section  we  illustrate  how  to  set  up  and  solve  some  problems  involving  the
                 steady,  isothermal,  laminar  flow  of  Newtonian  fluids.  The  relatively  simple  analytical
                 solutions  given  here are not to be regarded  as ends in themselves, but rather as  a prepa-
                 ration  for  moving  on to the analytical  or numerical solution  of  more complex  problems,
                 the use  of various  approximate methods, or the use  of dimensional  analysis.
                     The complete solution  of  viscous  flow  problems, including  proofs  of  uniqueness  and
                 criteria  for  stability,  is  a formidable  task.  Indeed, the attention of  some  of  the world's  best
                 applied mathematicians has been devoted  to the challenge  of solving the equations  of con-
                 tinuity  and  motion. The beginner  may  well  feel  inadequate when  faced  with  these  equa-
                 tions  for  the first time. All  we  attempt to do in the illustrative  examples  in this section is to
                 solve  a  few  problems  for  stable  flows  that are  known  to exist.  In each  case  we  begin  by
                 making  some postulates about the form  for  the pressure  and velocity  distributions:  that is,
                 we guess how  p and v  should  depend  on position  in the problem being  studied.  Then  we
                 discard  all  the terms  in  the equations  of  continuity and  motion that are  unnecessary  ac-
                 cording  to the postulates  made.  For example,  if  one postulates  that  v x  is  a  function  of  у
                                           2
                 alone, terms  like  dvjdx  and  d v /dz 2  can be  discarded.  When  all  the unnecessary  terms
                                            x
                 have been eliminated, one is frequently  left  with  a small number of relatively  simple  equa-
                 tions; and  if the problem is sufficiently  simple, an analytical solution can be obtained.
                     It must be emphasized  that in listing  the postulates, one makes  use  of  intuition.  The
                 latter  is based  on our daily  experience  with flow phenomena. Our intuition often  tells  us
                 that  a flow will be  symmetrical  about  an axis,  or that some component of  the velocity  is
                 zero.  Having  used  our  intuition  to  make  such  postulates,  we  must  remember  that  the
                 final  solution  is  correspondingly  restricted.  However,  by  starting  with  the equations  of
                 change, when  we  have  finished  the "discarding  process"  we  do at least  have  a complete
                 listing  of  all  the assumptions  used  in the solution.  In some  instances  it  is  possible  to  go
                 back and remove some  of the assumptions and get  a better solution.
                     In several  examples  to be  discussed,  we  will  find  one solution  to the  fluid  dynamical
                 equations. However, because the full  equations are nonlinear, there may be other solutions
                 to the problem. Thus a complete solution to a fluid dynamics problem requires the  specifi-
                 cation  of  the limits  on the stable  flow  regimes  as well as  any  ranges  of  unstable  behavior.
                 That  is, we  have  to develop  a "map" showing  the various  flow  regimes  that are  possible.
                 Usually  analytical  solutions  can  be  obtained  for  only  the  simplest  flow  regimes;  the re-
                 mainder  of  the  information  is  generally  obtained  by  experiment  or by  very  detailed  nu-
                 merical solutions. In other words, although we know the differential  equations that govern
                 the fluid motion, much is yet unknown about how  to solve them. This is a challenging  area
                 of applied mathematics, well above  the level  of an introductory  textbook.
                     When  difficult  problems  are encountered, a search should  be made through some  of
                 the advanced  treatises  on  fluid  dynamics. 1


                     1
                      R. Berker, Handbuch der Physik, Volume  VIII-2, Springer, Berlin  (1963), pp. 1-384; G. K. Batchelor,
                 An  Introduction  to Fluid Mechanics, Cambridge University  Press  (1967); L. Landau and  E. M. Lifshitz, Fluid
                 Mechanics, Pergamon Press, Oxford, 2nd edition (1987); J. A. Schetz and A.  E. Fuhs (eds.), Handbook of Fluid
                 Dynamics  and Fluid Machinery,  Wiley-Interscience, New York  (1996); R. W. Johnson (ed.), The Handbook of
                 Fluid Dynamics,  CRC Press, Boca Raton, Fla. (1998); С  Y. Wang,  Ann.  Revs. Fluid Mech., 23,159-177  (1991).
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