摘要
本文以大气、望远镜和终端接收器组成的成像系统的分辨率的讨论为出发点,从傅里叶光学和统计光学观点阐明高分辨率天文像复原的确切含义,并按统一的思路讨论了几种典型的方法。最后对此领域的现状和发展进行了评论.
By starting from discussions on the resolution of an imaging system consisting of the earth atmosphere, a telescope and a terminal receiver, the exact meaning of the high-resolution image reconstruction for astronomy is expounded from the point of view of Fourier optics and statistical optics. Then, some typical methods are discussed according to a unitary train of thought. Finally, some comments are made on the status quo and developments of this field.
出处
《天文学进展》
CSCD
北大核心
1989年第4期328-336,共9页
Progress In Astronomy
