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 |
推荐引用方式 GB/T 7714 | Xinqi Xu,Lingzhe Xu,Gangping Jin. Overview of LAMOST control system[C]:SPIE,2003:Vol.4837 484-493. |
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文件名称/大小 | 文献类型 | 版本类型 | 开放类型 | 使用许可 | ||
Overview of LAMOST c(140KB) | 开放获取 | CC BY-NC-ND | 浏览 下载 |
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