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?

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986soph..107...39k&link_type=abstract

Solar Physics, Volume 107, Issue 1, pp.39-45

Physics

1

Pulsations:Solar Radio Radiation, Solar Radio Radiation:Pulsations

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 Lyapunov exponent and the Kolmogorov entropy give some hints to deterministic chaos. Consequences for the physical modelling of the event are discussed.

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