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Testing of the Gemini secondary mirrors

机译:双子座辅助镜的测试

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Abstract: The first 1-m secondary mirror for the Gemini 8-m telescopes project was delivered by Zeiss in 1998, and 2nd mirror will be delivered in the summer of 1999. For first use during commissioning we produced an extreme lightweight Zerodur solution prefabricated at Schott. To reach the 85 percent weight reduction a novel etching technique was used. INterferometric testing was done performing full aperture measurements using a concave matrix. In progress with the fabrication process of the matrix we applied 3D-mechanical measurements, IR-interferometry, and VIS-interferometry using null lenses to reach the final intrinsic quality of 6 nm rms. For interferometric testing of the secondaries phase shifting interferometry with a tunable laser diode was applied. The optical test results of the secondaries show, that the mirrors are well within specification. The finally achieved intrinsic surface quality is 17 nm rms for Unit 1 and 13 nm rms for Unit 2, dominated by cutting effects which were introduced by removing the oversize at the inner and outer edge of the mirror after the final polishing step. !5
机译:摘要:蔡司于1998年交付了用于双子星8米望远镜项目的第一块1-m辅助镜,第二块镜子将在1999年夏季交付。在调试期间的首次使用,我们生产了一种超轻型Zerodur解决方案,该解决方案预制于肖特。为了达到重量减轻85%的目的,使用了一种新颖的蚀刻技术。干涉仪测试是使用凹矩阵进行全孔径测量的。在矩阵的制造过程中,我们使用零透镜应用了3D机械测量,IR干涉测量和VIS干涉测量,以达到6 nm rms的最终固有质量。为了对二次光束进行干涉测量,使用了可调激光二极管进行了相移干涉测量。二次透镜的光学测试结果表明,这些反射镜完全在规格范围内。最终达到的固有表面质量对于单元1来说是17 nm rms,对于单元2来说是13 nm rms,主要由切割效果决定,在最后的抛光步骤之后,通过去除镜面内外边缘的过大尺寸引入了切割效果。 !5

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