Affiliation:
1. Key Laboratory of Optical System Advanced Manufacturing Technology, Chinese Academy of Sciences, Changchun 130033, China
2. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China
Abstract
This paper introduces an optimization strategy for fabricating large aspheric mirrors. We polished a large SiC aspheric mirror, 4 m in diameter, achieving a surface error of 1/40λ RMS. To the best of our knowledge, this is the first instance of such a result for a mirror of this material and size combination. Due to the various performance settings of different tools, achieving optimal polishing results with a single setting is challenging. We evaluated the performance of various tool settings and developed an optimization strategy, dividing error maps to enhance efficiency in large-aperture aspheric mirror fabrication. We established the relationship between tool size and its error control capability. The residual error map of the mirror was divided into two parts using Zernike polynomial expansion based on the frequency order of the error map. Here, we used the first 36 terms of the Zernike polynomial fit to define a low-order error map, and the residual error was used to define a high-order error map. Large tools were used to correct the low-order frequency error map, whereas small tools were used to correct the high-order frequency error map. Therefore, the original residual error map could be corrected with significantly high efficiency. By employing this strategy, we fabricated a 4 m SiC aspheric mirror in 18 months, achieving a final surface error better than 0.024λ RMS.
Funder
Youth Innovation Promotion Association CAS
National Natural Science Foundation of China
National Key Research and Development Program
Reference30 articles.
1. James Webb Space Telescope;Daukantas;Proc. Int. Astron. Union,2007
2. The large binocular telescope;Hill;Appl. Opt.,2010
3. SUBARU Telescope;Kaifu;Proc. SPIE,1998
4. Interferometry with the ESO Very Large Telescope;Luehe;Proc. SPIE—Int. Soc. Opt. Eng.,1995
5. Production of primary mirror segments for the Giant Magellan Telescope;Martin;SPIE Astron. Telesc. Instrum.,2014