编码孔径成像光谱仪光学系统设计  

Optical system design of the coded aperture imaging spectrometer

作　　者：裴琳琳[1] 吕群波[1] 王建威[1] 刘扬阳[1] 

机构地区：[1]中国科学院光电研究院,北京100094

出　　处：《物理学报》2014年第21期61-67,共7页Acta Physica Sinica

基　　金：国家高技术研究发展计划(863计划)(批准号:2012AA0055)资助的课题~~

摘　　要：本文设计了一种以双Amici棱镜为分光元件的成像光谱系统,该系统主要包括前置望远物镜、编码板、双Amici棱镜、准直镜和成像镜.此类光学系统可以获得很高的衍射效率,相比于狭缝结构的成像光谱系统,该光谱仪为两维空间扩展的视场,无疑增加了设计难度.后期的数据反演算法对一次像面编码板的成像效果过于依赖,基于此,对光学系统的像差校正提出了更高的要求.本文设计、分析了基于双Amici棱镜的成像光谱仪的原理及特点,设计了一套完整的成像光谱系统.前置望远物镜的设计为像方远心,MTF在39线对处,达到0.8,成像质量良好.创新性的将前置望远物镜倒置用做准直系统.全系统各个波长在39线对处的MTF值均在0.65以上.对室外目标景物进行推扫成像,从获得的成像数据判断,本文设计的编码孔径成像光谱仪原理可行,衍射效率高,全视场成像质量良好,全谱段光谱数据可信.The coded aperture imaging spectrometer system based on the double-Amici-prism is designed in this paper, which includes the telescope objective, the coded template, the double-Amici-prism, the collimator lens and the imaging lens.This optical system can obtain a high diffraction efficiency. Compared to the imaging spectrometer system with a slit for this kind of system, the field of view is a two-dimensional spatial expansion, increasing the difficulty of design. For the subsequent data inversion algorithm, perfect imaging is needed, and based on this, the optical aberration of the system should be corrected carefully wildly. In this paper, we design and analyse the features of the imaging spectrometer system based on the double-Amici-prism, then the comple imaging spectrometer system. Telescope objective is designed to be telecentric, its MTF at 39 line pairs is 0.8, implying that good images can be obtained. Innovatively, an inverted telescope objective is used as a collimation system.The imaging spectrometer system＇s MTF at 39 line pairs is higher than 0.65. The imaging of the outdoor target scene, obtained by the coded aperture imaging spectrometer, proves that the design principle is feasible,the system is of high diffraction efficiency, the full-field imaging is of good quality, and the full spectrum of data is creditabe.

关 键 词：成像光谱仪 光学设计 双Amici棱镜 

分 类 号：O433.1[机械工程—光学工程]