1 January 1987 High-Resolution Astronomical Imaging By Photon-Counting Triple Correlation Techniques
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Proceedings Volume 0813, Optics and the Information Age; (1987) https://doi.org/10.1117/12.967163
Event: 14th Congress of the International Commission for Optics, 1987, Quebec, Canada
Speckle masking1-4 is a triple correlation method that can overcome image degradation caused by the atmosphere, by telescope aberrations and by image motion of the speckle interferograms (guiding errors etc.). True images are obtained since it is possible to reconstruct both the modulus and the phase of the object Fourier transform. In other words, speckle masking is a solution of the phase problem in speckle interferometry.5 Other speckle methods are described in Ref. 6.
© (1987) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
G. Baier, G. Baier, K. H. Hofmann, K. H. Hofmann, D. Schertl, D. Schertl, G. Weigelt, G. Weigelt, } "High-Resolution Astronomical Imaging By Photon-Counting Triple Correlation Techniques", Proc. SPIE 0813, Optics and the Information Age, (1 January 1987); doi: 10.1117/12.967163; https://doi.org/10.1117/12.967163


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