Can a solar pulsation event be characterized by a low-dimensional chaotic attractor?

Details Can a solar pulsation event be characterized by a low-dimensional chaotic attractor? Can a solar pulsation event be characterized by a low-dimensional chaotic attractor?

Jan 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987soph..107...39k&link_type=abstract

Solar Physics (ISSN 0038-0938), vol. 107, no. 1, 1987, p. 39-45.

Physics

8

Fractals, Power Spectra, Solar Oscillations, Solar Radio Bursts, Strange Attractors, Kolmogoroff Theory, Liapunov Functions, Maximum Entropy Method, Modal Response

Scientific paper

Using the theory of nonlinear dynamical systems a time-series analysis of a pulsation event in solar radio emission suggests that there exists a low-dimensional attractor. The power spectrum cannot be interpreted as a superposition of periodic components. Estimates of the maximum Liapunov exponent and the Kolmogorov entropy give some hints to deterministic chaos. Consequences for the physical modeling of the event are discussed.

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