Abstract
Lens-atmosphere modulation transfer function measurements are presented for speckle interferometry using the 193 cm telescope of the Observatoire de Haute Provence, France. A single photoelectric scanning detector is used to record the speckle pattern, and real-time data processing is achieved using a power spectrum analyser. Normal and log-normal models are used to compare theory with experiment. The results are in substantial agreement with Korff's log-normal assumptions.
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