詹姆斯·韦伯太空望远镜
干涉测量
主镜像
天文干涉仪
望远镜
光学
曲率
度量(数据仓库)
光路
振动
过程(计算)
计算机科学
工程类
物理
声学
数学
数据库
操作系统
几何学
作者
David Chaney,Babak N. Saif,P. Greenfield,Kyle Van Gorkom,Keira Brooks,W. Hack,Marcel Bluth,Josh Bluth,James A. Sanders,Koby Smith,Larkin Carey,Sze Chaung,Severine C. Tournois,Lee Feinberg,W. S. Smith,Vladimir Kradinov,Ritva Keski-Kuha
摘要
The James Webb Space Telescope (JWST) recently saw the completion of the assembly process for the Optical Telescope Element and Integrated Science Instrument Module (OTIS). This integration effort was performed at Goddard Space Flight Center (GSFC) in Greenbelt, Maryland. In conjunction with this assembly process a series of vibration and acoustic tests were performed. To help assure the telescope's primary mirror was not adversely impacted by this environmental testing an optical center of curvature (CoC) test was performed to measure changes in the mirror's optical performance. The primary is a 6.5 meter diameter mirror consisting of 18 individual hexagonal segments. Each segment is an off-axis asphere. There are a total of three prescriptions repeated six times each. As part of the CoC test each segment was individually measured using a high-speed interferometer (HSI) designed and built specifically for this test. This interferometer is capable of characterizing both static and dynamic characteristics of the mirrors. The latter capability was used, with the aid of a vibration stinger applying a low-level input force, to measure the dynamic characteristic changes of the PM backplane structure. This paper describes the CoC test setup, an innovative alignment method, and both static and dynamic test results.
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