Tilted-component telescopes. Part I: theory.
Tilted-component telescopes. Part I: theory.
复制标题
倾斜组件望远镜。
DOI：
10.1364/ao.9.002169
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发表时间：
1970
期刊：
影响因子：
1.9
通讯作者：
R. Buchroeder
中科院分区：
文献类型：
--
作者：
R. Buchroeder
三级像差理论的一种简单但非正统的应用使人们能够设计出一种简单形式的高度修正的离轴望远镜。被称为倾斜分量望远镜，有(A)SchiefSpiegler、(B)Yolo和(C)折反射Herschelian(CHT)子类，它的特点是轴对称分量，通常只需要球面曲率。
A simple but unorthodox application of third-order aberration theory enables one to design a simple form of highly corrected off-axis telescope. Known as the tilted component telescope, with subclasses (a) Schiefspiegler, (b) Yolo, and (c) catadioptric herschelian (CHT), is it distinguished by axially symmetric components that frequently require only spherical curvature.