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Variances of Optical Transfer Functions of the Turbulent Atmosphere

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Abstract

The variances of optical transfer functions of the optical system “Turbulent Atmosphere - Telescope” are investigated theoretically by two methods of posteriory processing (Labeyrie and Knox-Tompson) of the astronomical images. This characteristics are approximated the phase variances of intensity spectrum of the images.

© 1996 Optical Society of America

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