Study on the detecting ability of the adaptive astronomical telescopes
文献类型：会议论文
| 作者 | Bitao, Tan1,2,3,4; Myers, R.M.4; Hongbin, Chen1 |
| 出版日期 | 2015 |
| 会议名称 | Journal of Physics: Adapting to the Atmosphere Conference 2014 |
| 会议日期 | 2015 |
| 卷号 | 595 |
| 页码 | 012004 |
| 中文摘要 | Adaptive imaging systems have been developed to compensate for distortion introduced by atmospheric turbulence. The performance of its imaging quality can be evaluated by the Strehl ratio, but this does not directly quantify the detecting ability of an adaptively correcting telescope. Combining the normally detecting SNR and the telescope Strehl ratio, a new method evaluating the detecting ability of an adaptive astronomical telescope is put forward, which can give a quantified value. The new method is simulated on a computer, the simulation results indicated that the detecting ability of an adaptively correcting a 2-m telescopes improves 2 visual magnitudes. The effects of different atmospheric coherence length on detecting ability also can be quantitatively studied through the new method, which can give a scientific basis for the optimization of the design of the system and the development of implementations. |
| 英文摘要 | Adaptive imaging systems have been developed to compensate for distortion introduced by atmospheric turbulence. The performance of its imaging quality can be evaluated by the Strehl ratio, but this does not directly quantify the detecting ability of an adaptively correcting telescope. Combining the normally detecting SNR and the telescope Strehl ratio, a new method evaluating the detecting ability of an adaptive astronomical telescope is put forward, which can give a quantified value. The new method is simulated on a computer, the simulation results indicated that the detecting ability of an adaptively correcting a 2-m telescopes improves 2 visual magnitudes. The effects of different atmospheric coherence length on detecting ability also can be quantitatively studied through the new method, which can give a scientific basis for the optimization of the design of the system and the development of implementations. |
| 收录类别 | EI |
| 学科主题 | Atmospheric turbulence - Radio telescopes - Signal to noise ratio |
| 语种 | 英语 |
| ISSN号 | 1742-6588 |
| 源URL | [http://ir.ioe.ac.cn/handle/181551/7432]  |
| 专题 | 光电技术研究所_光电工程总体研究室（一室） |
| 作者单位 | 1.Institute of Optics and Electronics, Chinese Academy of Sciences, Chengdu, China 2.University of Chinese Academy of Sciences, Beijing, China 3.Northwest Institute of Nuclear Technology, Xi'an, China 4.University of Durham, Durham, United Kingdom |
| 推荐引用方式 GB/T 7714 | Bitao, Tan,Myers, R.M.,Hongbin, Chen. Study on the detecting ability of the adaptive astronomical telescopes[C]. 见:Journal of Physics: Adapting to the Atmosphere Conference 2014. 2015. |
入库方式： OAI收割
来源：光电技术研究所
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