Adaptive optical system based on deformable secondary mirror on 1.8-meter telescope
文献类型：会议论文
| 作者 | Rao, Changhui1,2; Zhang, Ang1,2; Fan, Xinlong1,2,3; Guo, Youming1,2,3; Wei, Kai1,2; Guan, Chunlin1,2; Zhang, Xuejun1,2; Li, Cheng1,2,3; Zhou, Luchun1,2; Chen, Shanqiu1,2 |
| 出版日期 | 2012 |
| 会议名称 | Proceedings of SPIE: Adaptive Optics Systems III |
| 会议日期 | 2012 |
| 卷号 | 8447 |
| 页码 | 84473H |
| 通讯作者 | Rao, C. |
| 中文摘要 | In 2009, A 127-element adaptive system had been manufactured and installed at the Coude room of the 1.8-meter telescope at the Gaomeigu site of Yunnan Astronomical Observatory, Chinese Academy of Sciences. A set of new adaptive optical system based on a 73-element deformable secondary mirror is being developed and will be integrated into the 1.8-meter telescope. The 73-element deformable secondary mirror with convex reflecting surface is designed to be compatible with the Cassegrain focus of the 1.8-meter telescope. Comparing with the AO system of Coude focus, the AO system on the deformable secondary mirror adopts much less reflections and consequently restrains the thermal noise and increases the energy transmitting to the system. The design and simulation results of this system will be described in this paper. Furthermore, the preliminary test result of the deformable secondary mirror in the lab is also presented. © 2012 SPIE. |
| 英文摘要 | In 2009, A 127-element adaptive system had been manufactured and installed at the Coude room of the 1.8-meter telescope at the Gaomeigu site of Yunnan Astronomical Observatory, Chinese Academy of Sciences. A set of new adaptive optical system based on a 73-element deformable secondary mirror is being developed and will be integrated into the 1.8-meter telescope. The 73-element deformable secondary mirror with convex reflecting surface is designed to be compatible with the Cassegrain focus of the 1.8-meter telescope. Comparing with the AO system of Coude focus, the AO system on the deformable secondary mirror adopts much less reflections and consequently restrains the thermal noise and increases the energy transmitting to the system. The design and simulation results of this system will be described in this paper. Furthermore, the preliminary test result of the deformable secondary mirror in the lab is also presented. © 2012 SPIE. |
| 收录类别 | EI |
| 语种 | 英语 |
| ISSN号 | 0277786X |
| 源URL | [http://ir.ioe.ac.cn/handle/181551/7790]  |
| 专题 | 光电技术研究所_自适应光学技术研究室（八室） |
| 作者单位 | 1.Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu 610209, China 2.Key Laboratory on Adaptive Optics Chinese Academy of Sciences, Chengdu 610209, China 3.Graduate University of Chinese Academy of Sciences, Beijing 100039, China |
| 推荐引用方式 GB/T 7714 | Rao, Changhui,Zhang, Ang,Fan, Xinlong,et al. Adaptive optical system based on deformable secondary mirror on 1.8-meter telescope[C]. 见:Proceedings of SPIE: Adaptive Optics Systems III. 2012. |
入库方式： OAI收割
来源：光电技术研究所
浏览0
下载0
收藏0
其他版本
除非特别说明，本系统中所有内容都受版权保护，并保留所有权利。