Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory
文献类型：期刊论文
| 作者 | Rao, Changhui1,2; Zhu, Lei1,2; Rao, Xuejun1,2; Zhang, Lanqiang1,2; Bao, Hua1,2; Kong, Lin1,2,3; Guo, Youming1,2; Ma, Xue'an1,2; Li, Mei1,2; Wang, Cheng1,2 |
| 刊名 | Chinese Optics Letters
 |
| 出版日期 | 2015 |
| 卷号 | 13期号:12页码:120101 |
| ISSN号 | 1671-7694 |
| 通讯作者 | Zhu, Lei (zhulei_cas@aliyun.com) |
| 中文摘要 | A second generation solar adaptive optics (AO) system is built and installed at the 1-m New Vacuum Solar Telescope (NVST) of the Fuxian Solar Observatory (FSO) in 2015. The AO high-order correction system consists of a 151-element deformable mirror (DM), a correlating Shack-Hartmann (SH) wavefront sensor (WFS) with a 3500 Hz frame rate, and a real-time controller. The system saw first light on Mar. 16, 2015. The simultaneous high-resolution photosphere and chromosphere images with AO are obtained. The on-sky observational results show that the contrast and resolution of the images are apparently improved after the wavefront correction by AO. © 2015 Chinese Optics Letters. |
| 英文摘要 | A second generation solar adaptive optics (AO) system is built and installed at the 1-m New Vacuum Solar Telescope (NVST) of the Fuxian Solar Observatory (FSO) in 2015. The AO high-order correction system consists of a 151-element deformable mirror (DM), a correlating Shack-Hartmann (SH) wavefront sensor (WFS) with a 3500 Hz frame rate, and a real-time controller. The system saw first light on Mar. 16, 2015. The simultaneous high-resolution photosphere and chromosphere images with AO are obtained. The on-sky observational results show that the contrast and resolution of the images are apparently improved after the wavefront correction by AO. © 2015 Chinese Optics Letters. |
| 学科主题 | Electric appliances - Observatories - Telescopes - Wavefronts |
| 收录类别 | SCI ; EI |
| 语种 | 英语 |
| WOS记录号 | WOS:000366603400001 |
| 源URL | [http://ir.ioe.ac.cn/handle/181551/6417]  |
| 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.The Key Laboratory on Adaptive Optics, Chinese Academy of Sciences, Chengdu, China 2.The Laboratory on Adaptive Optics, Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, China 3.University of Chinese Academy of Sciences, Beijing, China |
| 推荐引用方式 GB/T 7714 | Rao, Changhui,Zhu, Lei,Rao, Xuejun,et al. Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory[J]. Chinese Optics Letters,2015,13(12):120101. |
| APA | Rao, Changhui.,Zhu, Lei.,Rao, Xuejun.,Zhang, Lanqiang.,Bao, Hua.,...&Wang, Zhiyong.(2015).Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory.Chinese Optics Letters,13(12),120101. |
| MLA | Rao, Changhui,et al."Second generation solar adaptive optics for 1-m New Vacuum Solar Telescope at the Fuxian Solar Observatory".Chinese Optics Letters 13.12(2015):120101. |
入库方式： OAI收割
来源：光电技术研究所
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