Page 109 - Bird R.B. Transport phenomena
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94  Chapter 3  The Equations  of Change for  Isothermal  Systems


                                                           Fig. 3.6-6.  Rotating liquid  with a free  surface, the
                                                           shape  of which  is a paraboloid  of  revolution.

                                       V  = Pati
                                       surface /





                                                p = p(r, z)
                           -и                   ~ within  fluid






     SOLUTION             Cylindrical  coordinates  are  appropriate  for  this  problem,  and  the  equations  of  change  are
                          given in Tables  B.2 and  B.6. At  steady  state we  postulate that v  and v  are both zero and that
                                                                            r     z
                          v  depends only on r. We  also postulate that p depends on z because  of the gravitational  force
                           0
                          and on r because  of the centrifugal  force but not on 0.
                              These postulates give 0 = 0 for the equation of continuity, and the equation of motion gives:
                                                             Vl    dp
                                                                                               (3.6-33)
                          r-component                      —p — = ——
                                                                                               (3.6-34)
                          0-component                   0 =  /x -
                                                                                               (3.6-35)
                          z-component                     0  =  —-^- — pg
                          The 0-component of the equation of motion can be integrated  to give

                                                                                               (3.6-36)
                          in which  C l  and C  are constants  of integration. Because v  cannot be infinite at r  = 0, the con-
                                                                        0
                                         2
                          stant C  must be zero. At r = R the velocity v  is RCl. Hence C }  = 2П and
                                2
                                                              0
                                                             v* =                              (3.6-37)
                          This states  that each element  of  the rotating  liquid  moves  as  an element  of  a rigid  body  (we
                          could have  actually  postulated  that the liquid  would  rotate as a rigid body  and written  down
                          Eq. 3.6-37 directly). When  the result  in Eq. 3.6-37 is  substituted  into Eq. 3.6-33, we  then  have
                          these two equations  for  the pressure  gradients:

                                                    dp             dp
                                                           2
                                                       =  pu r  and  = ~Pg                  (3.6-38,39)
                                                    dr             T z
                           Each of these equations can be integrated, as  follows:
                                             p = Iptfr 2  + / (0, z)  and  p  = -pgz  + / (r, в)  (3.6-40,41)
                                                        :
                                                                              2
                           where fa and /  are arbitrary  functions  of integration. Since we  have postulated  that p does not
                                      2
                                                                         2
                           depend  on в, we  can choose fa =  -pgz  + С and / 2  = \pCl rp  +  C, where  С is  a constant, and
                           satisfy  Eqs. 3.6-38 and 39. Thus the solution to those equations has the form
                                                                   2 2
                                                      p = -pgz  + \рп г  + С                   (3.6-42)
                           The constant С may  be  determined  by  requiring  that p  = p  at  r  = 0 and  z  = z , the latter
                                                                          atm               0
                           being the elevation  of the liquid  surface  at r = 0. When  С is obtained in this way,  we  get
                                                   V  ~  Patm  =  ~ Z 0 )                      (3.6-43)
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