Paper
28 June 2006 MROI's automated alignment system
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Abstract
We present an outline of the automated alignment system for the 350m baseline Magdalena Ridge Observatory Interferometer (MROI) which will manage the simultaneous alignment of its six principal optical subsystems (telescopes, beam relay trains, delay lines, beam reducing telescopes, switchyards, and beam combiners). Many of these components will be held under vacuum, will be subject to varying thermal loads and will use different coatings (optimized for either optical or near-IR wavelengths). We review the proposed architecture of our scheme and discuss the procedures, tools, and optical analyses we have used to design it.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
C. A. Jurgenson, D. F. Buscher, M. J. Creech-Eakman, C. A. Haniff, J. S. Young, T. A Coleman, C. B. Parameswariah, E. Seneta, and E. J. Bakker "MROI's automated alignment system", Proc. SPIE 6268, Advances in Stellar Interferometry, 62683Y (28 June 2006); https://doi.org/10.1117/12.672531
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KEYWORDS
Mirrors

Relays

Telescopes

Interferometers

Optical alignment

Beam shaping

Magdalena Ridge Observatory

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