摘要
传统的无遮拦三反射镜光学系统设计是先设计轴对称反射系统,然后通过偏光瞳、偏视场或者两者结合的方法来实现系统无遮拦设计,系统中不可避免地用到了离轴非球面反射镜。以矢量波像差理论的相关结论出发,将反射镜的倾斜作为系统的优化变量,利用轴对称非球面反射镜实现了无遮拦三反射系统的设计。分析了此种系统的设计思路及步骤,设计了焦距为1000mm、视场角为10°×20°、F数为10的三反射镜光学系统,系统结构紧凑,成像质量接近衍射极限。该系统与其他无遮拦三反光学系统相比,最大的优点是系统中的非球面均为轴对称反射面,极大地降低了系统成本。
The traditional unobscured three-mirror optical system is an intrinsically rotationally symmetric optical system with an offset aperture stop, a biased input field, or both of them, so off-axis sections of rotationally symmetric aspheric parent surface are ineluctable. Using the conclusion of vector wavefront aberration theory, a new unobscured three-mirror system by tilted the rotationally symmetric aspheric mirror was presented. The design reason and step of this system was analyzed, and then a system with effective focal length of 1 000 mm, field of view of 10° ×20° and F-number 10 was designed. The volume of system (Length×Wide×Height) less than 350 mm×350 mm×120 mm and image qualities of the example are near diffraction limit. Compared with other unobscured three-mirror system, the most prominent advantage of this system is that using tilted rotationally symmetric aspheric mirror to achieve unobscured style, thus reducing cost of the system.
出处
《红外与激光工程》
EI
CSCD
北大核心
2014年第2期569-573,共5页
Infrared and Laser Engineering
基金
国家"863"计划(Y112G81800)
青年科学与基金项目(Y111B6150Z)
关键词
光学设计
空间光学
反射系统
矢量波像差理论
无遮拦三反系统
optical design
space optical
reflective system
vector wavefront aberration theory
unobscured three-mirror optical system