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Proceedings Paper

The CHARA light pipe and vacuum system
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Paper Abstract

The CHARA Array employs vacuum light pipes between the telescopes and the beam combination area. The complex terrain of the Mt. Wilson site poses interesting problems, with light pipes both underground and suspended up to 10 meters above ground. Telescope to beam-combination distances are up to about 180 meters. The support scheme and alignment strategy will be described.

Paper Details

Date Published: 5 July 2000
PDF: 12 pages
Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); doi: 10.1117/12.390271
Show Author Affiliations
Stephen T. Ridgway, National Optical Astronomy Observatories (United States)
William G. Bagnuolo, CHARA/Georgia State Univ. (United States)
Rick Blakely, M3 Engineering (United States)
Theo Armand ten Brummelaar, CHARA (United States)
Douglas R. Ferrell, Patrell Engineering Group, Inc. (United States)
Harold A. McAlister, CHARA/Georgia State Univ. (United States)
Mark A. Shure, CHARA/Georgia State Univ. (United States)
Eric J. Simison, Sea West Enterprises, Inc. (United States)
Laszlo Sturmann, CHARA (United States)
Nils Henning Turner, CHARA (United States)


Published in SPIE Proceedings Vol. 4006:
Interferometry in Optical Astronomy
Pierre J. Lena; Andreas Quirrenbach, Editor(s)

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