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Manufacturing and testing of a convex aspherical mirror for ASSIST

机译:ASSIST凸面非球面镜的制造和测试

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ASSIST is the testbed for the ESO Adaptive Optics Facility. The main objective of ASSIST is the characterization of the1.2 meter deformable mirror which will replace the existing secondary of one of the 8 meter VLT telescopes. A largeconcave 1.65 meter diameter aspherical primary mirror combined with a 140 mm diameter convex aspherical secondaryforms the main optical system of ASSIST. Two additional optical units provide the light sources and the wave frontanalyzing optics. Without having the possibility for checking the entire optical system as a whole, each individual mirrorhad to be manufactured and tested using reliable techniques. The secondary mirror for ASSIST (AM2) is made of anoptically transparent material (BK7) with a specific and accurate backside radius in order to achieve a null test intransmission. Furthermore, not only the overall RMS surface error of AM2 is important, but due to the fact that it will beused in a setup that measures specific spatial frequencies, also the spatial frequencies of the surface error of AM2 isimportant. The aspherical surface is tested in double pass using an optical flat and an interferometer with a transmissionsphere. Manufacturing of this asphere is mainly done by hand at the optical lab of NOVA-ASTRON. The final accuracyof the reflecting surface is within the required 50 nm RMS with a surface roughness of less than 2 nm RMS. This paperreports in more detail on manufacturing and testing of the a-spherical convex mirror.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:ASSIST是ESO自适应光学设备的测试平台。 ASSIST的主要目的是表征1.2米可变形镜,它将取代8米VLT望远镜之一的现有辅助镜。大凹面直径1.65米的非球面主镜与140毫米直径的凸面非球面副镜相结合,构成了ASSIST的主要光学系统。另外两个光学单元提供了光源和波前分析光学器件。在没有可能检查整个光学系统整体的情况下,必须使用可靠的技术来制造和测试每个单独的反射镜。 ASSIST的辅助反射镜(AM2)由具有特定且精确的背面半径的光学透明材料(BK7)制成,以实现零测试透射。此外,不仅AM2的整体RMS表面误差很重要,而且由于它将用于测量特定空间频率的设置中,因此AM2的表面误差的空间频率也很重要。使用光学平面和具有透射球的干涉仪对非球面进行两次通过测试。该非球面材料的制造主要由NOVA-ASTRON的光学实验室手工完成。反射表面的最终精度在要求的50 nm RMS以内,且表面粗糙度小于2 nm RMS。本文更详细地报告了非球面凸面镜的制造和测试。©(2012)COPYRIGHT光电仪器工程师协会(SPIE)。摘要的下载仅允许个人使用。

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