CHAOTIC PULSE TRAINS

N.J. Balmforth, Astronomy Department, Columbia University, New York, NY 10027

G.R. Ierley, Scripps Institute of Oceanography, University of California, San Diego, CA 92093-0225

E.A. Spiegel, Astronomy Department, Columbia University, New York, NY 10027

We study a third-order nonlinear ordinary differential equation whose solutions, under certain specific conditions, are individual pulses. These correspond to homoclinic orbits in the phase space of the equation and we study the possible pulse types in some detail. Sufficiently close to the conditions under which a homoclinic orbit exists, the solutions take the form of trains of well-separated pulses. A measure of closeness to homoclinic conditions provides a small parameter for the development of an asymptotic solution consisting of superposed, isolated pulses. The solvability condition in the resulting singular perturbation theory is a timing map relating successive pulse spacings. This map of the real line onto itself, together with the known form of the homoclinic orbit, provides a concise and accurate solution of the equation.

Last Revised: 23 Apr 1996