5 July 2000 The CHARA light pipe and vacuum system
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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.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Stephen T. Ridgway, Stephen T. Ridgway, William G. Bagnuolo, William G. Bagnuolo, Rick Blakely, Rick Blakely, Theo Armand ten Brummelaar, Theo Armand ten Brummelaar, Douglas R. Ferrell, Douglas R. Ferrell, Harold A. McAlister, Harold A. McAlister, Mark A. Shure, Mark A. Shure, Eric J. Simison, Eric J. Simison, Laszlo Sturmann, Laszlo Sturmann, Nils Henning Turner, Nils Henning Turner, } "The CHARA light pipe and vacuum system", Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); doi: 10.1117/12.390271; https://doi.org/10.1117/12.390271
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