Wu Cong-Jun, Yan Chang-Xiang, Liu Wei, Dai Hu
Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Guang Pu Xue Yu Guang Pu Fen Xi. 2013 Aug;33(8):2272-6.
To satisfy imaging spectrometers's miniaturization, lightweight and large field requirements in space application, the current optical design of imaging spectrometer with Offner structure was analyzed, and an simple method to design imaging spectrometer with concave grating based on current ways was given. Using the method offered, the sub-field imaging spectrometer with 400 km altitude, 0.4-1.0 microm wavelength range, 5 F-number of 720 mm focal length and 4.3 degrees total field was designed. Optical fiber was used to transfer the image in telescope's focal plane to three slits arranged in the same plane so as to achieve subfield. The CCD detector with 1 024 x 1 024 and 18 microm x 18 microm was used to receive the image of the three slits after dispersing. Using ZEMAX software optimization and tolerance analysis, the system can satisfy 5 nm spectrum resolution and 5 m field resolution, and the MTF is over 0.62 with 28 lp x mm(-1). The field of the system is almost 3 times that of similar instruments used in space probe.
为满足成像光谱仪在空间应用中的小型化、轻量化和大视场要求,分析了当前具有Offner结构的成像光谱仪的光学设计,并基于现有方法给出了一种设计凹面光栅成像光谱仪的简单方法。利用所提供的方法,设计了一种用于亚视场成像光谱仪,其高度为400 km,波长范围为0.4 - 1.0微米,焦距720 mm的F数为5,总视场为4.3度。采用光纤将望远镜焦平面上的图像传输到排列在同一平面上的三个狭缝,以实现亚视场。使用1024×1024且像素为18微米×18微米的CCD探测器接收经色散后的三个狭缝的图像。通过ZEMAX软件优化和公差分析,该系统可满足5 nm的光谱分辨率和5 m的视场分辨率,并且在28 lp×mm⁻¹时调制传递函数(MTF)超过0.62。该系统的视场几乎是用于空间探测器的类似仪器的3倍。