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Overview of LAMOST control system
Xinqi Xu; Lingzhe Xu; Gangping Jin
2003-02-01
会议录名称Large Ground-based Telescopes
卷号4837
期号4837
页码Vol.4837 484-493
会议日期2002-8-22
会议地点Hawaii USA
会议主办者The International Society for Optical Engineering
出版者SPIE
摘要
Based on an unconventional design concept the LAMOST telescope will become the world’s most powerful meter-class level ground astronomical optical survey telescope when it is completed. From technical perspective the goal with such a high profile has brought an extraordinary challenge to its control system. For better image quality the telescope’s segmented reflecting Schmidt mirror has to be actively controlled by nanometer technique. At the same time the mirror is driven on both azimuth and altitude axes in subarcsecond accuracy for tracking the star. Vigorous study has been done and a number of cutting edge techniques are applied to meet the tough requirements.

This paper gives the overview of LAMOST control system, outlines its distributed, real time, reliable and expansible configuration and the simulation approach. The current status of the control system is briefly reported in this paper too.
关键词Lamost Telescope Control System Overview Lan
学科领域郭守敬望远镜(lamost) ; 自动控制
文献类型会议论文
条目标识符http://ir.niaot.ac.cn/handle/114a32/360
专题会议论文
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Xinqi Xu,Lingzhe Xu,Gangping Jin. Overview of LAMOST control system[C]:SPIE,2003:Vol.4837 484-493.
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