Page 55 - Fluid-Structure Interactions Slender Structure and Axial Flow (Volume 1)
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38                 SLENDER STRUCTURES AND AXIAL FLOW

                   The  vibration of  the  shells  induces oscillatory flow  in  the  fluid, and  the  task  is  to
                 determine the unsteady fluid loading on the shells, resulting thereby. By further assuming
                 that the amplitude of  shell vibrations is small, it follows that all fluid velocities are also
                 small and hence governed by equations (2.71)-(2.73a,b). Because the shells are very long,
                 end effects are negligible; also, because the mode of  deformation is such that motion is
                 essentially two-dimensional as outlined in the previous paragraph, motion-induced flow
                 variations in  the  direction of the  long  axis of  the  shells are  negligible. Hence,  in  this
                 case, ap/ax = 0 and 4 = 4(r, 8, t); the analysis is therefore carried out in  the plane of
                 Figure 2.7(a).
                   The solution to the fluid flow resulting from this motion may be obtained via equations
                 (2.73a,b), although (2.72) could be used equally well  (Gibert 1988). The eigenmodes of
                                             =
                 each shell are of the form (v, w)~ {v, sin ne, w,  cos   where the relation between
                 v,  and w,  is dependent on the shell equations used [e.g. Fliigge (1960)], which need not
                 concern us here; n  is the circumferential wavenumber. The cross-sectional deformation
                 for n = 1-4 is shown in Figure 2.7(c).
                   Consider first the case where the outer shell is replaced by  a rigid immobile cylinder
                 of inner radius R,,  and let v;  and wi be the displacement components of the inner shell.
                 Furthermore, consider oscillation in the nth mode, such that

                                vi(&  t) = vni(r) sin ne,   roi(8, t) = w,,;(t) cos ne,   (2.1 13)

                 in  which  it  is  understood  that  v,,;  and  W,Ii  are  harmonic  functions,  e.g.  w,;(t) =
                 -
                 w,; exp(if2t). The corresponding velocity potential is
                                                4 = $(r, e) eiRf.                    (2.114)
                 The boundary conditions for the fluid are


                                                                                    (2.1 15a)


                                                                                    (2.115b)

                   The solution of the Laplace equation for 5 = $(r, e), after separation of variables, gives

                    -        00
                    4(r, 6) =   {r"[A,, cos ne + B,  sin ne] + r-"[C,, cos ne + D,  sin ne]};   (2.1 16)
                            n=l
                 application of the boundary conditions yields





                   The pressure on the inner shell and the outer cylinder in the nth circumferential mode
                 may be determined through equation (2.73b), yielding
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