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136  Aerodynamics for Engineering Students

                  respectively, occurring on the horizontal axis. As r is increased positively a small
                  amount the stagnation points move down below the horizontal axis.
                    Since from the equation for the velocity anywhere on the surface
                                                r
                                  qt = 2U sin 0 + - 0 at the stagnation points
                                                   =
                                               27ra
                                             8 = arc sin(-r/47raU)

                  which  is  negative.  As  r  is  further  increased  a  limiting  condition  occurs  when
                  0 = -42, i.e. I' = 47raU, the stagnation points merge at the bottom of the cylinder.
                  When I' is greater than 47raU the stagnation point (S) leaves the cylinder. The cylinder
                  continues to rotate  within  the  closed loop  of  the  stagnation  streamline, carrying
                  round with it a region of fluid confined within the loop.

                  3.3.1 1  Bernoulli's equation for rotational flow

                  Consider fluid moving in a circular path. Higher pressure must be exerted from the
                  outside, towards the centre of rotation, in order to provide the centripetal force. That
                  is, some outside pressure force must be available to prevent the particles moving in a
                  straight line. This suggests that the pressure is growing in magnitude as the radius
                  increases, and a corollary is that the velocity of flow must fall as the distance from the
                  centre increases.
                    With a segmental element at P(r, 0) where the velocity is qt only and the pressurep,
                  the pressures on the sides will be shown as in Fig. 3.26  and the resultant pressure
                  thrust inwards is

                             (.  + % g) (. + $) se - (.  - % $) (r - $) se -p sr se

                  which reduces to


                                                                                     (3.53)
                  This must provide the centripetal force = mass x centripetal acceleration
                                                = pr sr se &Ip                       (3.54)




















                  Fig. 3.26
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