Dependence of seeing correlation on image separation at the CFH telescope on Mauna Kea

Astronomy and Astrophysics – Astronomy

Scientific paper

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Astronomical Observatories, Astronomical Photography, Atmospheric Effects, Fluctuation Theory, Image Analysis, Telescopes, Binary Stars, Camera Shutters, Correlation, Hawaii, High Resolution

Scientific paper

Trailed images of optical pairs of stars obtained with the Canada-France-Hawaii 3.6-m telescope on Mauna Kea were analyzed to study seeing fluctuations. The data show that seeing fluctuations, evaluated from the 'macroscopic' properties of a guide star image, i.e., image centroid and image width, are correlated for separations as large as 1 arc min. Seeing fluctuations as frequencies less than 5 Hz were correlated for most image pairs in this particular data set. Higher frequency variations were correlated only for pairs with separations less than 8 arc sec. In a simulation of very high resolution imagery using an offset guide star, the quality of detected program images were improved by as much as 70 percent. Guide decision times ranged from 10 to 50 msec, depending on the observational circumstances.

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