Paper
11 October 2015 Advances in diamond generating for 8.4 meter telescope mirrors
Johnathan M. Davis, Hubert M. Martin, Dae Wook Kim, Adrian R. Loeff, Kurtis L. Kenagy, Raymond W. Sisk, Jeffery R. Hagen
Author Affiliations +
Proceedings Volume 9633, Optifab 2015; 96330Y (2015) https://doi.org/10.1117/12.2196060
Event: SPIE Optifab, 2015, Rochester, New York, United States
Abstract
The Richard F. Caris Mirror Lab is in the process of fabricating 8.4 meter mirror segments for the Giant Magellan Telescope. Seven of the segments are off-axis with 14 mm of aspheric departure. In order to successfully fabricate these mirrors we are constantly taking steps towards faster, more deterministic methods, from diamond generating to stressed lap polishing. The Large Optical Generator (LOG) is celebrating its 30-year anniversary at the University of Arizona with a complement of technological updates and enhancements. This paper shows how some of these upgrades will aid in the manufacture of the GMT segments.
© (2015) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Johnathan M. Davis, Hubert M. Martin, Dae Wook Kim, Adrian R. Loeff, Kurtis L. Kenagy, Raymond W. Sisk, and Jeffery R. Hagen "Advances in diamond generating for 8.4 meter telescope mirrors", Proc. SPIE 9633, Optifab 2015, 96330Y (11 October 2015); https://doi.org/10.1117/12.2196060
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Cited by 4 scholarly publications.
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KEYWORDS
Mirrors

Calibration

Diamond

Computer programming

Photovoltaics

Telescopes

Surface finishing

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