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PIPES CONVEYING FLUID: NONLINEAR AND CHAOTIC DYNAMICS          389

               The system can also be perturbed by adding a small oscillatory component to the flow,
             so that u = u, + u sin wt - cf. Sections 4.5 and 5.9. Prior to doing this, Li & Paldoussis
             (1994) conducted a Melnikov analysis on a reduced subsystem, the details of  which are
             not given here; for nonautonomous systems, this can give an indication of the parameters
             near which chaos can arise. The central idea is to construct a scalar function which gives a
             measure of the distance between the stable and unstable manifolds when the unperturbed
             heteroclinic (or homoclinic) orbit is broken by  perturbations. If  and  when this distance
             vanishes  as  a  system parameter  varies,  the  two  manifolds intersect  transversally; one
             such intersection implies infinitely many, yielding horsehoes and chaos (Guckenheimer
             & Holmes  1983). The  analysis in  this  case gives  u > d(w) for  this  to  occur,  where
             (T  = 0.1 is the viscous damping coefficient [equation (3.71)], viscous damping being the
             only dissipation included, and R(w) is a function of  the forcing frequency of the system,
             which has a minimum at w = wo  = 2.45, 00  being the frequency of oscillation at the Hopf
             point. Simulations for a forcing frequency of  o = 2.50  while varying v show that chaotic
             oscillations arise for  v  > 1.22; this  value of  u  is  very  much  higher than  the  minimum
             required  according to  the  Melnikov calculation. The  sequence of  oscillatory states for
             increasing  u  is  (a) quasiperiodic,  (b) periodic  and  (c) chaotic motions.  The  results  are
             similar to those discussed next, and hence no further details are given here.
               The next case to be considered is that of the pipe-spring  system, discussed in relatively
             great detail in Section 5.7.3(a). In this case, heteroclinic orbits arise along one of the lines
             shown  in  Figure 5.27(a).  Here,  simulations are  conducted  exclusively with  a  periodic
             flow-velocity perturbation of  the system, with parameters as given in Figure 5.55, where
             a bifurcation diagram and a few phase-plane plots are shown; a fuller set, consisting of
             several power spectra, time traces, phase-plane plots and Lyapunov exponent calculations
             are given in Paldoussis & Sender (1993b). The sequence of oscillatory states for increasing
             u  is (i) periodic oscillations around one or the other of  the two buckled states (both are
             shown, obtained via different initial conditions), (ii) quasiperiodic oscillations around both
             buckled states, (iii) periodic motions with sub-, combination, and super-harmonic content
             (3 < u  < 8 approximately), and (iv) chaotic oscillations. It is of interest that quasiperiodic
             and chaotic oscillations in Figure 5.55(a) look not too dissimilar, but the difference in the
             Lyapunov exponents is quite clear: zero in the former case and positive in the latter.
               Three-dimensional motions of  the  same system are considered by  Steindl & Troger
             (1996), who determine in  a map of  j3 versus the location of  the  spring support, tS, the
             regions of existence and stability of heteroclinic cycles. Physically, the heteroclinic cycle
             involves the  following set  of  transitions, as  shown in  Figure 5.56(a): (i) the  system  is
             buckled in one of  the two mutually perpendicular planes; (ii) oscillations develop in that
             plane about the buckled state; (iii) the amplitude of these oscillations increases, while the
             static deformation due to buckling diminishes, eventually leading to oscillations about the
             straight equilibrium state (about the origin); (iv) oscillations develop in the perpendicular
             plane,  with  decreasing amplitude as the  amplitude of  buckling increases in  that  plane;
             (v) eventually buckling in that plane results, with no oscillation. By symmetry, this state is
             fundamentally identical to the initial one, and so the sequence just described begins anew.
               Steindl (1996) considers another type of heteroclinic cycles for the same system, this
             time associated with Hopf-Hopf  bifurcations, rather than Hopf-pitchfork  ones as in the
             foregoing, again obtaining a map of stable heteroclinic cycles in the {B, &}  plane, as shown
             in Figure 5.56(b). In this case, the oscillations in one plane develop a secondary bifurcation
             at the TB boundary (corresponding to a simultaneous occurrence of a Hopf bifurcation and
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