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成像光谱仪宽视场离轴三反望远系统的光学设计
引用本文:李欢,周峰.成像光谱仪宽视场离轴三反望远系统的光学设计[J].航天返回与遥感,2012,33(2):28-33.
作者姓名:李欢  周峰
作者单位:北京空间机电研究所,北京,100076
摘    要:视场宽、结构紧凑、质量轻是空间光学系统设计研究的热点。文章从离轴三反望远系统的应用技术指标分析、设计思想、设计流程及光学系统优化4个方面,研究了成像光谱仪用宽视场、大相对孔径离轴三反消像散望远系统的设计问题,设计出一个光谱范围0.4~2.5μm、焦距f′=700mm、相对孔径f′/4、线视场角20°的离轴三反望远系统,次镜为球面,主镜和三镜非球面最高次数为4次,在Nyquist频率27.8对线/mm处,调制传递函数值均大于0.87。

关 键 词:望远系统  光学设计  宽视场  三反镜系统

Optical Design of Wide-field Off-axis Three-mirror Telescope Systems
LI Huan,ZHOU Feng.Optical Design of Wide-field Off-axis Three-mirror Telescope Systems[J].Spacecraft Recovery & Remote Sensing,2012,33(2):28-33.
Authors:LI Huan  ZHOU Feng
Institution:(Beijing Institute of Space Mechanics & Electricity,Beijing 100076,China)
Abstract:Wide field of view,compact configuration and light mass were study hotspots on the design of imaging systems in space optics.The paper describes the study of the design of off-axis three-mirror anastigmatic telescope systems with wide field of view and large relative aperture of imaging spectrometers,in terms of the four aspects of applied specifications analysis,design thinking,design flow,and design optimization of the off-axis three-mirror anastigmatic telescopes system.An off-axis three-mirror telescope system with 700 mm focal length,f′/4 relative aperture and 20° field angle is worked out.The highest degree is four of the off-axis three-mirror anastigmatic telescope system of the imaging spectrometer.Its spectral range is 0.4~2.5μm,and the module translate function is over 0.87 when Nyquist frequency is at 27.8 lp/mm.
Keywords:telescope system  optical design  wide-field  three-mirror system
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