Paper
1 February 1994 Fabrication and testing of the 3.5-m, f/1.75, WIYN primary mirror
David S. Anderson, James H. Burge, Dean A. Ketelsen, Hubert M. Martin, Steve C. West, Gary A. Poczulp, John H. Richardson, Woon-Yin Wong
Author Affiliations +
Abstract
The continuing development of rapid fabrication methods for large optics at the Steward Observatory Mirror Lab has resulted in the completion of the WIYN 3.5 m primary mirror in only five months. The use of these methods, though rapid, also resulted in one of the best surface figures we have produced (16 nm rms), excellent microroughness (8 angstroms rms), and very smooth small-scale figure error as determined by the structure function of the surface errors. In this paper, we review the important techniques in the grinding, polishing, and testing of the mirror used to achieve these results.
© (1994) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
David S. Anderson, James H. Burge, Dean A. Ketelsen, Hubert M. Martin, Steve C. West, Gary A. Poczulp, John H. Richardson, and Woon-Yin Wong "Fabrication and testing of the 3.5-m, f/1.75, WIYN primary mirror", Proc. SPIE 1994, Advanced Optical Manufacturing and Testing IV, (1 February 1994); https://doi.org/10.1117/12.167968
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Cited by 4 scholarly publications.
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KEYWORDS
Mirrors

Polishing

Computer generated holography

Aspheric lenses

Holograms

Monochromatic aberrations

Surface finishing

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