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Successful production of the Engineering Development Unit (EDU) Primary Mirror segment and flight unit Tertiary Mirror for JWST

机译:成功开发了用于JWST的工程开发部(EDU)主镜部分和飞行单元第三镜

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During 2009, Tinsley finished most of the Configuration 1 pre-cryo test Computer Controlled Optical Surfacing (CCOS) operations on the James Webb Space Telescope primary mirror segments and in mid-2009 we began the Configuration 2 post-cryo test CCOS operations. After completing the grinding and polishing operations, including final figuring to a cryo-null target, we delivered the finished Engineering Development Unit (EDU) to Ball Aerospace Technology Corporation on 4 December 2009. Achieving fabrication and metrology conditions to meet the specifications for this off-axis ~1.5 m hexagonal point-to-point segmented mirror required special methods. Achieving repeatable and accurate interferometric alignment of the off-axis aspherical mirror surface and stable thermal gradient control of the beryllium substructure during tests required rigorous component and system-level validation. Final optical wavefront measurements over the various spatial frequency ranges have demonstrated that all of the requirements are met. This success has validated our processes of fabrication and metrology and allows us to proceed with the production of the 18 flight mirror segments. The first finished flight mirror, the Tertiary Mirror, was shipped to BATC on 24 February, 2010. Performance of that mirror is reported here also.
机译:在2009年期间,Tinsley在James Webb太空望远镜主镜段上完成了Configuration 1低温测试之前的大多数计算机控制光学表面(CCOS)操作,并且在2009年中期,我们开始了Configuration 2 Cryo测试之后的CCOS操作。在完成了研磨和抛光操作(包括最终加工成低温零靶)之后,我们于2009年12月4日将完成的工程开发单元(EDU)交付给Ball Aerospace Technology Corporation。轴〜1.5 m的六边形点对点分段镜需要特殊方法。为了在测试期间实现离轴非球面镜表面的可重复且精确的干涉对准以及对铍子结构的稳定热梯度控制,需要进行严格的组件和系统级验证。在各种空间频率范围内的最终光波阵面测量结果表明,已满足所有要求。这一成功验证了我们的制造和计量流程,使我们能够继续生产18个飞行镜分段。第一个完成的飞行镜,即第三级镜,已于2010年2月24日运至BATC。该镜的性能也在此处报告。

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