Performance of the 37-element solar adaptive optics for the 26 cm solar fine structure telescope at Yunnan Astronomical Observatory
文献类型：期刊论文
| 作者 | Rao, CH1,2; Zhu, L1,2; Rao, XJ1,2; Guan, CL1,2; Chen, DH1,2; Chen, SQ1,2; Lin J(林隽)3 ; Liu ZZ(刘子忠)3
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| 刊名 | APPLIED OPTICS
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| 出版日期 | 2010-11 |
| 卷号 | 49期号:31页码:G129-G135 |
| ISSN号 | 1559-128X |
| 产权排序 | 第三完成单位 |
| 通讯作者 | Zhu, L (reprint author), Chinese Acad Sci, Key Lab Adapt Opt, POB 350, Chengdu 610209, Sichuan, Peoples R China. |
| 英文摘要 | A 37-element solar adaptive optics system, which consists of a fine tracking loop with a tip/tilt mirror and a correlation tracker, and a high-order correction loop with a 37-element deformable mirror, a correlating Shack-Hartmann wavefront sensor, and a real-time controller, was built and installed at the 26 cm solar fine structure telescope of the Yunnan Astronomical Observatory in 2009. In this system, the absolute difference algorithm is used. A new architecture with field-programmable gate array (FPGA) and digital signal processor (DSP) for the real-time controller based on systolic array and pipeline was developed. The computational latencies of the fine tracking loop and high-order correction loop are about 35 and 100 mu s, respectively. The tracking residual root-mean-square error is less than 0.1 arcsec, and the wavefront residual root-mean-square error is about 0.05 wavelengths (lambda = 550 nm) after correction. The observational results show that the contrast and resolution of the solar images are improved after the correction by this adaptive optics system. (C) 2010 Optical Society of America |
| WOS标题词 | Science & Technology ; Physical Sciences |
| 学科主题 | Optics |
| 类目[WOS] | Optics |
| 研究领域[WOS] | Optics |
| 关键词[WOS] | SYSTEM |
| 收录类别 | SCI ; EI |
| 原文出处 | https://www.osapublishing.org/ao/abstract.cfm?uri=ao-49-31-G129 |
| 语种 | 英语 |
| WOS记录号 | WOS:000283653000014 |
| 源URL | [http://ir.ynao.ac.cn/handle/114a53/6157]  |
| 专题 | 云南天文台_太阳物理研究组 |
| 作者单位 | 1.The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, P.O. Box 350, Shuangliu, Chengdu 610209, Sichuan, China 2.The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, P.O. Box 350, Shuangliu, Chengdu 610209, Sichuan, China 3.Yunnan Astronomical Observatory, National Astronomical Observatories, Chinese Academy of Sciences, Phoenix Hill, Kunming 650011, Yunnan, China |
| 推荐引用方式 GB/T 7714 | Rao, CH,Zhu, L,Rao, XJ,et al. Performance of the 37-element solar adaptive optics for the 26 cm solar fine structure telescope at Yunnan Astronomical Observatory[J]. APPLIED OPTICS,2010,49(31):G129-G135. |
| APA | Rao, CH.,Zhu, L.,Rao, XJ.,Guan, CL.,Chen, DH.,...&Liu ZZ.(2010).Performance of the 37-element solar adaptive optics for the 26 cm solar fine structure telescope at Yunnan Astronomical Observatory.APPLIED OPTICS,49(31),G129-G135. |
| MLA | Rao, CH,et al."Performance of the 37-element solar adaptive optics for the 26 cm solar fine structure telescope at Yunnan Astronomical Observatory".APPLIED OPTICS 49.31(2010):G129-G135. |
入库方式： OAI收割
来源：云南天文台
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