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29 May 2013 Adaptive optics for fiber-fed interferometers
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Optical interferometry is a cost-effective means to extend the resolving power of astronomical instruments. Typically, the light from separate small and movable telescopes is brought through vacuum pipes to a central beam combiner. We are developing a new generation of AO systems to enhance the performance of interferometers in which the vacuum lines are replaced with optical fibers. The AO, included on each of the telescopes, concentrates light on the fiber inputs to achieve the greatest optical throughput. We describe the design approach to the AO systems, how their requirements differ from those of a traditional system, and how the addition of AO enables further enhancements to the design of optical interferometers.
© (2013) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Michael Hart, Thomas Stalcup, Olivier Durney, Nicholas Emerson, Keith Powell, Michael Ward, Greg Feller, Rick Kendrick, James Mason, Matthew Bold, Larry Dewell, and Tracy Kubo "Adaptive optics for fiber-fed interferometers", Proc. SPIE 8725, Micro- and Nanotechnology Sensors, Systems, and Applications V, 87250U (29 May 2013); doi: 10.1117/12.2018046;

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