Paper
1 January 1987 Optical Long-Baseline Interferometry And Aperture Synthesis On Earth And In Space
G. Weigelt, K. H. Hofmann, T. Reinheimer
Author Affiliations +
Proceedings Volume 0813, Optics and the Information Age; (1987) https://doi.org/10.1117/12.967152
Event: 14th Congress of the International Commission for Optics, 1987, Quebec, Canada
Abstract
During the last few years it has been shown that speckle masking observations with large telescopes can yield diffraction-limited images in spite of image degradation by the atmosphere and by telescope aberrations1-4. Much higher resolution can be obtained if the Coude beams of many telescopes are combined coherently in a central station and if the obtained long-baseline speckle interferograms are evaluated by speckle masking5,6. For example, a 10-km array on earth can yield images with the fasci-nating resolution of 10-5 arcsec. Labeyrie has for the first time shown that it is possible to combine the Coude beams of two telescopes coherently.
© (1987) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
G. Weigelt, K. H. Hofmann, and T. Reinheimer "Optical Long-Baseline Interferometry And Aperture Synthesis On Earth And In Space", Proc. SPIE 0813, Optics and the Information Age, (1 January 1987); https://doi.org/10.1117/12.967152
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KEYWORDS
Space telescopes

Speckle

Telescopes

Signal to noise ratio

Interferometers

Phase measurement

Synthetic apertures

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