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Response Curve

 

The case of whirling motions subject to a planar excitation is described by the equation

  equation3375

where the phase space is four-dimensional: tex2html_wrap_inline14038 . The extended phase space, when we add the forcing variable, is five-dimen-sional: tex2html_wrap_inline14040 .

Equation (3.56) can be analyzed for periodic motions by a combination of averaging and algebraic techniques not unlike the harmonic balance method. Because our text is an experimental introduction to nonlinear dynamics, we present here a qualitative description of the results of this analysis. For further details see references [19], [20], and [21].

As mentioned in the introduction to this section, an experimental frequency scan that passes through a main resonance can result in the following sequence of motions:

eqnarray3385

The basic features of these experimental observations agree with those predicted by equation (3.56), and are summarized in the response curve shown in Figure 3.17.

  
Figure 3.17: Response curve for planar and nonplanar motion. (Adapted from Johnson and Bajaj [19].)

In the parameter range tex2html_wrap_inline13836 , the response curve indicates the coexistence of three planar periodic motions and one nonplanar periodic orbit. In this parameter regime, the planar periodic orbit becomes unstable; the string ``pops out of the plane'' and begins to execute a whirling motion. At some parameter value tex2html_wrap_inline14044 , the nonplanar periodic motion itself becomes unstable and the system may do any number of things depending on the exact system parameters and initial conditions. For instance, it may hop to the small-amplitude planar periodic orbit. Or the ballooning orbit itself may become unstable and begin to precess (quasiperiodic motion). In addition, chaotic motions can sometimes be observed in this parameter range. These various dynamical possibilities are illustrated schematically in Figure 3.17. We repeat, the motion observed depends on the exact system parameters and the initial conditions, because there can be many coexisting attractors with complicated basins of attraction in this region. In particular, the chaotic motions are difficult to isolate (and observe experimentally) without a thorough understanding of the system.


next up previous contents
Next: Torus Attractor Up: Nonplanar Motions Previous: Free Whirling

Nicholas B. Tufillaro
Mon Mar 3 01:58:02 PST 1997