六足动物
詹姆斯·韦伯太空望远镜
执行机构
变形镜
有源光学
主镜像
望远镜
计算机科学
容错
波前
自适应光学
职位(财务)
光学
物理
机器人
人工智能
分布式计算
经济
财务
作者
Allison Barto,D. Scott Acton,Paul T. Finley,Benjamin Gallagher,Bruce Hardy,J. Scott Knight,Paul A. Lightsey
摘要
The James Webb Space Telescope (JWST) telescope's secondary mirror and eighteen primary mirror segments are each actively controlled in rigid body position via six hexapod actuators. The mirrors are stowed to the mirror support structure to survive the launch environment and then must be deployed 12.5 mm to reach the nominally deployed position before the Wavefront Sensing and Control (WFSandC) alignment and phasing process begins. The actuation system is electrically, but not mechanically redundant. Therefore, with the large number of hexapod actuators, the fault tolerance of the OTE architecture and WFSandC alignment process has been carefully considered. The details of the fault tolerance will be discussed, including motor life budgeting, failure signatures, and motor life.
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