Dynamic analysis of the active control system for the CGST
文献类型:会议论文
作者 | Dai YC(戴懿纯); Yang, DH; Zago, L; Liu Z(刘忠); Dai YC(戴懿纯)![]() ![]() |
出版日期 | 2012 |
会议名称 | Conference on Modeling, Systems Engineering, and Project Management for Astronomy V |
会议日期 | 2012-07-01 |
会议地点 | Amsterdam, NETHERLANDS |
关键词 | Solar Telescope Segmented Mirror Active Control Structural Model Dynamic Analysis |
卷号 | 8449 |
通讯作者 | Dai, YC (reprint author), Chinese Acad Sci, Yunnan Astron Observ, POB 110, Kunming 650011, Peoples R China. |
英文摘要 | The Chinese Giant Solar Telescope (CGST) is the China's next generation solar telescope with an aperture of 8 m in diameter. The unique feature of the CGST is its ring primary, which facilitates the polarization detection and thermal control. The CGST is now in its design and development phase. A mosaic mirror with 24 trapezoidal segments is a candidate for its primary mirror, which highly relies on a segment active control system to achieve competitive optical quality of a monolithic mirror. The CGST is designed to operate in open-air observation mode, its active control system thus faces new challenges. As the CGST has an aperture larger than that of current solar telescopes, and as the magnitude of wind load in open air is greater than that of a stellar telescope with a similar aperture yet under the protection of a dome and/or an enclosure. Furthermore, as a mosaic mirror, high precision real-time tip sensing is required to serve the feedback of its control system. The accuracy depends on integration time (or working bandwidth) when an optical metrology is adopted, which should match the bandwidth of the segment control system. In this paper, a dynamic analysis of the segment control system of the CGST is presented. We demonstrate how the dynamic interaction between the segment control system and the telescope structure impacts the telescope's optical performance under wind disturbances. The dynamic analysis helps to understand the bandwidth limit for the segment control system, and further to clarify technical requirements for tip sensing implementation, telescope structure design and wind shielding design. |
收录类别 | EI ; CPCI |
产权排序 | 第一完成单位 |
会议网址 | http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1363198 |
会议录 | Proceedings of SPIE - MODELING, SYSTEMS ENGINEERING, AND PROJECT MANAGEMENT FOR ASTRONOMY V
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会议录出版者 | SPIE-INT SOC OPTICAL ENGINEERING |
学科主题 | Astronomy & Astrophysics; Computer Science; Optics |
会议录出版地 | 1000 20TH ST, PO BOX 10, BELLINGHAM, WA 98227-0010 USA |
语种 | 英语 |
ISSN号 | 0277-786X |
ISBN号 | 978-0-8194-9150-3 |
源URL | [http://ir.ynao.ac.cn/handle/114a53/4857] ![]() |
专题 | 云南天文台_抚仙湖太阳观测站 |
通讯作者 | Dai YC(戴懿纯) |
推荐引用方式 GB/T 7714 | Dai YC,Yang, DH,Zago, L,et al. Dynamic analysis of the active control system for the CGST[C]. 见:Conference on Modeling, Systems Engineering, and Project Management for Astronomy V. Amsterdam, NETHERLANDS. 2012-07-01.http://proceedings.spiedigitallibrary.org/proceeding.aspx?articleid=1363198. |
入库方式: OAI收割
来源:云南天文台
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