24 July 1998 3D layout of the CHARA array on Mount Wilson
Author Affiliations +
Abstract
A brief description of the problems found and methods used to calculate the exact position of each mirror of the CHARA Array on Mount Wilson. The problem is highly constrained due to polarization and logistic considerations, yet many unusable solutions are still possible.
© (1998) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Theo Armand ten Brummelaar, "3D layout of the CHARA array on Mount Wilson", Proc. SPIE 3350, Astronomical Interferometry, (24 July 1998); doi: 10.1117/12.317109; https://doi.org/10.1117/12.317109
PROCEEDINGS
4 PAGES


SHARE
RELATED CONTENT

ALOHA @3,39 μm Implementation of the up conversion...
Proceedings of SPIE (August 19 2016)
Polarization fidelity in an optical interferometer
Proceedings of SPIE (July 28 2008)
345-GHz facility SIS receiver for the JCMT
Proceedings of SPIE (July 31 1998)
Integrated-optics 3-way beam combiner for IOTA
Proceedings of SPIE (February 21 2003)
Large stellar interferometer MIRA-ST
Proceedings of SPIE (February 21 2003)

Back to Top