首页 | 本学科首页   官方微博 | 高级检索  
     

高分辨率光谱仪与极大望远镜耦合问题分析
引用本文:张弛,朱永田,张凯. 高分辨率光谱仪与极大望远镜耦合问题分析[J]. 应用光学, 2014, 35(5): 868-872
作者姓名:张弛  朱永田  张凯
作者单位:1.中国科学院 国家天文台 南京天文光学技术研究所,江苏 南京 210042;
基金项目:国家自然科学基金国际合作重大项目(10373015)
摘    要:介绍国际上地面极大光学/红外望远镜的研制概况,分析高分辨率光谱仪与极大口径望远镜耦合中的难题,结果表明极大口径望远镜需要超大面积阶梯光栅和超快焦比相机。根据光谱仪与望远镜的匹配关系,30 m级极大口径望远镜的高分辨率光谱仪的准直光束将大于70 cm,主色散阶梯光栅的面积大于2 m2,照相机的焦比F/0.5,按照目前的制造技术无法提供上述光栅和相机,因此,提出高分辨率光谱仪与极大望远镜进行耦合的技术。针对耦合问题给出了相应解决方案,即采用像切分器、拼接光栅以及白瞳设计等技术将是极大口径望远镜与高分辨率光谱仪耦合的主要解决方案。

关 键 词:天文望远镜   高分辨率光谱仪   阶梯光栅   光谱
收稿时间:2014-03-26

Technique challenges in coupling of high resolution spectrograph with extremely large telescope
Affiliation:1.National Astronomical Observatories/Nanjing Institute of Astronomical Optics &Technology,CAS,Nanjing 210042,China;2.Key Laboratory of Astronomical Optics &Technology,CAS,Nanjing 210042,China;3.University of Chinese Academy of Sciences,Beijing 100049,China
Abstract:We reviewed the designing of several international ground-based extremely large optical/infrared telescopes and introduced the problems faced in the coupling of high resolution spectrograph with telescopes of extremely large aperture. It is proposed that large area of echelle and ultrafast focal ratio camera can serve as a solution. According to the coupling rule of the spectrogragh and the telescope, the diameter of collimated beam for a 30 m telescope would be over 70 cm, and the size of the main dispersion echelle grating would be larger than 2 m2. To build such huge and costly equipment would be difficult with current techniques. And large aperture camera with focal ratio F/0.5 is also hard to design and manufacture. Image slicer, mosaic gratings and white pupil optic become major solutions in designing the high resolution spectrograph for an extremely large aperture telescope.
Keywords:astronomical telescope  high-resolution spectrograph  echelle grating  spectra
点击此处可从《应用光学》浏览原始摘要信息
点击此处可从《应用光学》下载免费的PDF全文
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号