20 August 1986 Segment Alignment For The Keck Telescope Primary Mirror
Author Affiliations +
We propose to use a Shack-Hartmann camera to align and phase the thirty-six segments of the ten meter primary mirror of the Keck Telescope. Tilt errors are determined by employing the Shack-Hartmann device in a manner exactly analogous to that used in mirror testing and in adaptive optics. Piston errors are determined (with the same device) by exploiting diffraction effects near the intersegment edges. These two tests are shown to have sensitivities that are comparable to each other and that are sufficient to achieve the design goals of the telescope. We describe how the tilt test can be extended to give information both about the individual segment figures and about the global mirror parameters. Some of the complications and potential systematic effects associated with these tests are discussed.
© (1986) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Gary A. Chanan, Gary A. Chanan, Jerry E. Nelson, Jerry E. Nelson, Terry S. Mast, Terry S. Mast, } "Segment Alignment For The Keck Telescope Primary Mirror", Proc. SPIE 0628, Advanced Technology Optical Telescopes III, (20 August 1986); doi: 10.1117/12.963566; https://doi.org/10.1117/12.963566


Non-redundant masking ideas on JWST
Proceedings of SPIE (August 27 2014)
Wavefront sensing on 100-m scale
Proceedings of SPIE (October 24 2004)
Cophasing techniques for extremely large telescopes
Proceedings of SPIE (July 06 2004)
BATC multipurpose wavefront error sensing assembly
Proceedings of SPIE (October 28 1999)

Back to Top