Introduction of a 2.5m telescope mount and its performance
文献类型:会议论文
作者 | Shihai Yang![]() ![]() ![]() ![]() ![]() ![]() ![]() |
出版日期 | 2010-07-28 |
会议日期 | 2010-6-27 |
会议地点 | San Diego, California, USA |
关键词 | telescope mount structure |
卷号 | 7733 |
期号 | 7733 |
页码 | Vol.7733 3H-1-7 |
英文摘要 |
Telescope is a very important tool for astronomers to survey and study the stellar stars and astronomical phenomena. The performance of a telescope is its capability to track the observing objects and keep the image on the field of view during the observing period. All these functions will be achieved by telescope mount, including mount control system. The mount is to support the mirror cell and keep the mirror cell position stability. Meanwhile, with the help of control system, the mount acts as tracker of the observing objects. So, for a telescope, the mount and its control system play an important role during the telescope operation. This paper gives an introduction of a mount structure designed for a 2.5m optical/infrared telescope and the corresponding control system. Some of preliminary test results are also given in this paper. |
会议主办者 | The International Society for Optical Engineering |
会议录 | Ground-based and Airborne Telescopes III
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会议录出版者 | SPIE |
学科主题 | 光学/红外望远镜 ; 天文技术与方法 |
源URL | [http://ir.niaot.ac.cn/handle/114a32/584] ![]() |
专题 | 会议论文 |
推荐引用方式 GB/T 7714 | Shihai Yang,Guomin Wang,Bozhong Gu,et al. Introduction of a 2.5m telescope mount and its performance[C]. 见:. San Diego, California, USA. 2010-6-27. |
入库方式: OAI收割
来源:南京天文光学技术研究所
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