Paper
20 October 2004 Adaptive optics performance model for optical interferometry
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Abstract
We argue that adding large apertures with adaptive optics to an optical interferometer improves the performance of the interferometer in two ways: it improves the signal to noise of bright, low-visibility fringes and it also improves the sensitivity of the interferometer. A simple model is presented to support this conclusion.
© (2004) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David Mozurkewich, Sergio Raffaele Restaino, and G. Charmaine Gilbreath "Adaptive optics performance model for optical interferometry", Proc. SPIE 5491, New Frontiers in Stellar Interferometry, (20 October 2004); https://doi.org/10.1117/12.552361
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KEYWORDS
Adaptive optics

Wavefronts

Interferometers

Signal to noise ratio

Interferometry

Performance modeling

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