Page 75 - Bird R.B. Transport phenomena
P. 75

60  Chapter 2  Shell Momentum Balances and Velocity  Distributions in Laminar Flow


                             is  — (p  +  r )| r=R (cos  в).  We  now  multiply  this  by  a  differential  element  of  surface
                                        rr
                             R 2  sin  в  dO йф to  get  the  force  on  the  surface  element  (see  Fig.  A.8-2).  Then  we  inte-
                             grate  over  the surface  of  the sphere  to get  the resultant normal force  in the z direction:
                                                      77
                                                n)  f-  Г _     ^|
                                                   =      (  (  +  T  r=R  e)R2  s i n
                                                    Jo  Jo
                                                                       5
                             According  to Eq. 2.6-5, the normal stress  r  is zero  at r  = R and can be omitted in the in-
                                                                rr
                             tegral  in  Eq. 2.6-7.  The pressure  distribution  at the surface  of  the sphere  is, according  to
                             Eq.  2.6-4,
                                                   V \г-к  = Po ~ PgR cos в  -  |  ^  cos в         (2.6-8)

                             When  this  is  substituted  into Eq. 2.6-7  and  the integration performed,  the term contain-
                             ing p  gives  zero, the term containing the gravitational  acceleration g  gives  the buoyant
                                  0
                             force, and  the term containing the approach velocity  v  gives the "form  drag"  as  shown
                                                                           x
                             below:
                                                                 3
                                                        F {n)  = $irR pg  +  2TTHRV               (2.6-9)
                                                                           X
                                                                          3
                             The  buoyant  force  is the mass  of  displaced  fluid  (f тгК р) times the gravitational  accelera-
                             tion (g).
        Integration of  the Tangential Force

                             At  each  point  on  the  solid  surface  there  is  also  a  shear  stress  acting  tangentially.  The
                             force  per  unit  area  exerted  in  the  —0 direction by  the  fluid  (region  of  greater  r) on  the
                             solid  (region  of  lesser  r) is  +т \ . The z-component of  this  force  per unit area  is  (r \ )
                                                                                                    re r=R
                                                       гв г=к
                             sin  0. We  now  multiply  this by  the surface  element R 2  sin  в dвdф and  integrate  over  the
                             entire spherical  surface.  This gives the resultant force  in the z direction:
                                                                          2
                                                        7
                                                  f(»  =  Г "  Г  ( Tr0 \ r=R  sin 0)R  sin в dd dф  (2.6-10)
                                                       Jo  Jo
                             The  shear stress  distribution on the sphere surface,  from  Eq. 2.6-6, is
                                                          T e\r=R  = \^Y~  S i n  в                (2.6-11)
                                                           r
                             Substitution  of this expression  into the integral  in Eq. 2.6-10 gives the "friction  drag"

                                                             F U)  =  ATTLJLRV,»                  (2.6-12)
                             Hence  the total  force  F  of  the fluid  on  the sphere  is  given  by  the sum  of  Eqs.  2.6-9  and
                             2.6-12:
                                                            3
                                                     F  = \TrR pg + infiRVoo  + A7rfiRv x        (2.6-13)
                                                        buoyant   form     friction
                                                         force    drag      drag
                             or
                                                                     3
                                                                 i<rrR pg +  бтг/LtRi;»           (2.6-14)
                                                                 buoyant  kinetic
                                                                  force    force



                                 5
                                  In Example 3.1-1 we show  that, for incompressible, Newtonian fluids,  all three of the normal
                             stresses  are zero at fixed  solid  surfaces  in all flows.
   70   71   72   73   74   75   76   77   78   79   80