Wavefront sensing and control demo during the cryo-vacuum testing of JWST: exercising the science and operations center

詹姆斯·韦伯太空望远镜 望远镜 天文台 航空航天工程 波前 遥感 系统工程 计算机科学 一套 地面段 任务控制中心 研究中心 物理 工程类 光学 天文 卫星 地质学 病理 考古 历史 医学
作者
Charles-Philippe Lajoie,Marshall D. Perrin,D. Scott Acton,Erin M. Wolf,Mark Abernathy,Marsha Allen,Elizabeth A. Barker,Matthew Lallo,Laurent Pueyo,J. A. Stansberry,D. S. Zak,Carey R. Myers,Thomas Comeau,Bernard Kulp,Margaret Jordan,Heather Livingston,Christopher Hanley,John D. Scott,Christopher C. Stark,J. Scott Knight
出处
期刊:Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave 卷期号:: 132-132 被引量:2
标识
DOI:10.1117/12.2312145
摘要

Aligning and commissioning the James Webb Space Telescope's segmented mirrors after launch will last many months and involve the telescope itself, all science instruments, and all parts of the observatory ground system. In an effort to assess and demonstrate readiness of the complete end-to-end system - i.e. the flight optical telescope elements (OTE), the Integrated Science Instruments Module, the on-board operational scripts, and the ground processing infrastructure - we performed two operations tests during the JWST OTIS cryogenic campaign in 2017. They are the Wavefront Sensing and Control Demonstration activities at NASA Johnson Space Center (JSC), where we performed flight-like sensing and control using the flight software to command mirror moves and take measurements, and a "Shadow Mode test" at the Space Telescope Science Institute's Mission Operations Center (MOC), where we demonstrated processing of the JSC data through the entire ground system infrastructure. Overall, these tests demonstrated that the full system that will support OTE commissioning is soundly designed although still not fully mature. This paper focuses on the operations and systems testing aspects and some lessons learned. We also report on a series of Wavefront Rehearsals being held at the MOC that are providing additional opportunities to build team readiness in operating the ground system as a whole using high fidelity observatory simulators

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