High-Resolution Astronomical Imaging: Auto- And Cross-Triple Correlation Processing And Triple Shearing Interferometry

K. H. Hofmann; G. Weigelt

doi:10.1117/12.967165

1 January 1987 High-Resolution Astronomical Imaging: Auto- And Cross-Triple Correlation Processing And Triple Shearing Interferometry

K. H. Hofmann, G. Weigelt

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Proceedings Volume 0813, Optics and the Information Age; (1987) https://doi.org/10.1117/12.967165
Event: 14th Congress of the International Commission for Optics, 1987, Quebec, Canada

Abstract

The atmosphere of the earth restricts the resolution of conventional astrophotography to about 1 arcsec. Much higher resolution can be obtained by interferometric techniques (see review article Ref.

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K. H. Hofmann and G. Weigelt "High-Resolution Astronomical Imaging: Auto- And Cross-Triple Correlation Processing And Triple Shearing Interferometry", Proc. SPIE 0813, Optics and the Information Age, (1 January 1987); https://doi.org/10.1117/12.967165

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