Paper
11 July 2006 Precision, range, bandwidth, and other tradeoffs in hexapods with application to large ground-based telescopes
Eric H. Anderson, Michael F. Cash, Paul C Janzen, Gregory W. Pettit, Christian A. Smith
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Abstract
Hexapods can be an effective means of positioning optics of all sizes, including those within large ground-based telescopes. A hexapod is often a convenient geometry when multiple axes of positioning are required. The paper reviews several small and mid-sized hexapods built for different applications, and emphasizes experience with a three-meter- diameter unit built to position a large optical component. The discussion highlights design tradeoffs in precision, including repeatability, resolution and accuracy, range in multiple axes, and bandwidth of operation, and addresses test and verification of performance. The paper concludes with a discussion and presentation of hexapod concepts for secondary mirror positioning for Thirty Meter Telescope and Cornell Caltech Atacama Telescope.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Eric H. Anderson, Michael F. Cash, Paul C Janzen, Gregory W. Pettit, and Christian A. Smith "Precision, range, bandwidth, and other tradeoffs in hexapods with application to large ground-based telescopes", Proc. SPIE 6273, Optomechanical Technologies for Astronomy, 62731F (11 July 2006); https://doi.org/10.1117/12.672947
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Cited by 6 scholarly publications.
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KEYWORDS
Telescopes

Actuators

Mirrors

Thirty Meter Telescope

Optical instrument design

Motion measurement

Computer programming

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