摘要
在研究全息技术校正望远镜主镜像差原理的基础上,设计了全息校正望远镜主镜像差的实验系统,确立了系统像差校正结果的评价方法。分析表明:利用激光全息技术能有效的补偿和校正大口径反射镜的大面形误差和系统像差。
Based on the principle of holography, an experimental system for holographic correction of aberrated primary mirror has been described and analyzed. Besides, some methods are proposed for the evaluation of aberration correction results. The analysis shows the feasibility of holographic technology for the aberration correction of the primary mirror of a telescope.
出处
《苏州科技学院学报（自然科学版）》
CAS
2008年第4期28-30,共3页
Journal of Suzhou University of Science and Technology （Natural Science Edition）
基金
苏州科技学院科研基金资助项目(Z1094)
关键词
全息技术
望远镜主镜
面形误差
像差校正
holography
spherical mirror
surface error
aberration correction
