Page 67 - Basics of Fluid Mechanics and Introduction to Computational Fluid Dynamics
P. 67

52       BASICS  OF  FLUID  MECHANICS  AND  INTRODUCTION  TO  CFD




                      Dw                                                   gradp        1...
                    ——  = (w-  grad) v  —w(divv  + rot  (—                           +  Zaiv{a)
                                                                                              [o]
                                                                                        ,
                                                                               ,
                       pi  ~  |            )         (div    v)
             we  set  [ao]  =  O,  then  we  get

                            Dw  |                              ;                  grad  p
                                                                                     5
                             Det  (w+  grad)  v  —  w(divv)  +  rot  (                    }  ,


                 For  a  barotropic  fluid  (obviously  for  an  incompressible  fluid  too)  be-
              cause  grad  {       =  gredp  and  taking  into  account  the  equation  of  conti-

             nuity,  it  turns  out  that  div  v  =  —178,  so  that  we  obtain


                                   D     [w         Gs                              GJ
                                  —       {—]= |  —-grad}v  =              (gradv)  —
                                  ni  ()           (5  4        )      (9         MS

                 Similarly,  from


                                     DI                gradp       1...
                                                          D
                                     Di  =  / (-                +  “div(ol)     -  or
                                             C


             we  get  a  =  —  f  meee  -  dr  such  that,  for  a  barotropic  fluid,  we  fi-

             nally  have  oes =  0.  This  result,  also  known  as  the  Thompson  (Lord
             Kelvin)  theorem,  states  that  the  circulation  along  a  simple  closed  curve,

              observed  during  its  motion,  is  constant  whenever  the  fluid  is  inviscid
              (ideal),  barotropic  (or  incompressible)  and  the  mass  (external)  forces
              are  potential.'    Correspondingly,  in  the  above  conditions,  the  strength
              of  a  vortex  tube  is  a  constant  too  (Helmholtz).
                 In  the  case  of  the  ideal  incompressible  or  barotropic  compressible  fluid

             flows,  the  vorticity  (rotation)  equation  (obtained  by  taking  the  curl  of
             each  term  of  the  Euler  equation)  could  be  written  as  oe  +  rot  (wxv)  =0.
              On  the  other  hand,  if  we  consider  the  flux  of  rotation  (vorticity)  across
             a  fluid  surface  %,  that  is  ®  =  J {  w-ndo,  as  divw  =  0  and  the  formula


              [153],
                                      a= //  Se  +  rot  (woxv)|  -ndo




             holds,  we  can  state  the  following  theorem:




              '  The  Thompson  theorem  requires,  basically,  the  existence  of a  uniform  potential  of  accelera-
             tions.  Somne  recent  results,  which  have  also  taken  into  consideration  the  case  of  nonuniform
             potential  of  accelerations,  should  be  mentioned  [122].
   62   63   64   65   66   67   68   69   70   71   72