天文台
望远镜
计量学
主镜像
光学
次镜
光圈(计算机存储器)
物理
计算机科学
遥感
天文
地质学
声学
作者
Breann N. Sitarski,Andrew Rakich,Hugo Chiquito,Wylie Rosenthal,Antonin H. Bouchez,W. Schoenell,B. Xin,Priscila Pires,J. A. Nissen,Patricio Schurter,Richard Demers,Peter L. Thompson,B. A. McLeod,B. Nemati,Glenn Brossus,Brian Walls,Heejoo Choi,Guillermo González,David Nemati
摘要
The Giant Magellan Telescope will be a 25.4-m visible and infrared telescope at Las Campanas Observatory. The optical design consists of 7 8.4-m primary mirror segments that reflect light to 7 secondary mirror segments in a doubly segmented direct Gregorian configuration. GMT is developing a Telescope Metrology System (TMS) to decrease the complexity of alignment and increase observatory efficiency. The TMS has been developed to Preliminary Design Review level. A prototyping, modelling, and analysis effort has been completed. All components of the system were matured, and the edge-sensing strategy was significantly revised. This paper describes the current TMS design.
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