Internal auto-parametric instabilities in the free non-linear vibrations of
a cylindrical shell are studied numerically, focusing on two modes (a conc
ertina mode and a chequerboard mode) whose non-linear interaction breaks th
e in-out symmetry of the linear vibration theory. The two-mode interaction
leads to preferred vibration patterns with larger deflection inwards than o
utwards, and at internal resonance, significant energy transfer occurs betw
een the modes. This has regular and chaotic features. Here, direct numerica
l integration is employed to examine chaotic motions. Using a set of 2-D Po
incare sections, each valid for a fixed level of the Hamiltonian, H, the in
stability under increasing H appears, as a supercritical period-doubling pi
tchfork bifurcation. Chaotic motions near a homoclinic separatrix appear im
mediately after the bifurcation, giving an irregular exchange of energy. Th
is chaos occurs at arbitrarily low amplitude as perfect tuning is approache
d. The instability manifests itself as repeating excursions around the sepa
ratrix, and a number of practical predictions can be made. These include th
e magnitude of the excursion, the time taken to reach this magnitude and th
e degree of chaos and unpredictability in the outcome. The effect of small
damping is to pull the motion away from what was the chaotic separatrix, gi
ving a response that resembles, for a while, the lower-energy quasi-periodi
c orbits of the underlying Hamiltonian system. (C) 2001 Academic Press.