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Contamination control requirements implementation for the James Webb Space Telescope (JWST), Part 1: Optics, instruments and thermal vacuum testing

机译:詹姆斯·韦伯太空望远镜(JWST)的污染控制要求实施,第1部分:光学,仪器和热真空测试

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The derivation of contamination control (CC) requirements for the JWST Optical Telescope Element (OTE) was presented at the SPIE conference in 2008. Since then, much work has been done to allocate contamination at each phase of Integration and Test (I&T) and to plan for achieving the allocations. Because JWST is such a large and complicated observatory, plans for meeting the requirements are many and varied. There are primary mirror segments that must be cleaned early and maintained clean; there are four science instruments that each have tight contamination requirements but cannot be cleaned after they are integrated onto the Integrated Science Instrument Module (ISIM) structure; there is the composite ISIM structure that is fragile and must be minimally handled; there are numerous cryo-vacuum tests that must be controlled and monitored in order to minimize molecular contamination during return to ambient; …and more. An overview of plans developed to implement contamination control for JWST optics, instruments, and thermal vacuum testing for JWST will be presented.
机译:在2008年的SPIE会议上提出了JWST光学望远镜元件(OTE)的污染控制(CC)要求的推导。自那时以来,已经做了很多工作来在集成和测试(I&T)的每个阶段分配污染,并计划以实现分配。由于JWST是一个如此庞大而复杂的天文台,因此满足要求的计划是多种多样的。有主要的镜段必须尽早清洁并保持清洁。有四种科学仪器,每个仪器都有严格的污染要求,但是将它们集成到集成科学仪器模块(ISIM)结构中后无法清洗;有一个复合的ISIM结构,它很脆弱,必须进行最少的处理;为了控制回到室温时的分子污染,必须控制和监视许多低温真空测试。 …和更多。将概述为实施JWST光学器件,仪器的污染控制以及JWST的热真空测试而制定的计划。

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