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Relative rotation rates: Fingerprints for strange attractors

N. B. Tufillaro, Hernán G. Solari, and R. Gilmore
Phys. Rev. A 41, 5717(R) – Published 1 May 1990
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Abstract

Chaotic dynamics on a strange attractor of low dimensionality can be characterized by a set of recently proposed topological invariants. These are the relative rotation rates of the unstable periodic orbits embedded in the strange attractor. We demonstrate the efficiency of this characterization by extracting the topological invariants from chaotic time-series data for the Duffing oscillator.

  • Received 16 March 1990

DOI:https://doi.org/10.1103/PhysRevA.41.5717

©1990 American Physical Society

Authors & Affiliations

N. B. Tufillaro

  • Department of Physics, Bryn Mawr College, Bryn Mawr, Pennsylvania 19010-2899

Hernán G. Solari and R. Gilmore

  • Department of Physics and Atmospheric Science, Drexel University, Philadelphia, Pennsylvania 19104-9984

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Vol. 41, Iss. 10 — May 1990

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