Physics – Optics
Scientific paper
Jan 1991
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991optl...16...64j&link_type=abstract
Optics Letters (ISSN 0146-9592), vol. 16, Jan. 15, 1991, p. 64-66. Research supported by NSERC.
Physics
Optics
9
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.
Aitken George J. M.
Hege Keith E.
Jorgenson Mark B.
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