Evidence of a chaotic attractor in star-wander data

Physics – Optics

Scientific paper

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Adaptive Optics, Astronomical Photography, Atmospheric Turbulence, Chaos, Image Processing, Strange Attractors, Probability Density Functions, Stellar Motions, Stochastic Processes, Wave Fronts

Scientific paper

The observed motion of stellar-image centroids is shown to have a chaotic attractor with a correlation dimension of about 6. The existence of a chaotic attractor in star wander, or equivalently in wave-front tilts, indicates that the atmospheric processes that cause image degradation may be more accurately described as chaotic, and are not so random as is usually assumed. This new result has important implications for the accurate modeling of atmospheric processes, the operation of adaptive optics systems, and the processing of stellar images.

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