Schock M, Spillar EJ
Centre de Recherche Astronomique de Lyon, Observatoire de Lyon, St. Genis Laval, France.
J Opt Soc Am A Opt Image Sci Vis. 2000 Sep;17(9):1650-8. doi: 10.1364/josaa.17.001650.
We present a technique to test the frozen flow hypothesis quantitatively, using data from wave-front sensors such as those found in adaptive optics systems. Detailed treatments of the theoretical background of the method and of the error analysis are presented. Analyzing data from the 1.5-m and 3.5-m telescopes at the Starfire Optical Range, we find that the frozen flow hypothesis is an accurate description of the temporal development of atmospheric turbulence on time scales of the order of 1-10 ms but that significant deviations from the frozen flow behavior are present for longer time scales.
