天文光学望远镜的调校与检测  

Alignment and testing of astronomical optical telescope

作　　者：李德培[1] 

机构地区：[1]中科院南京天文仪器研制中心

出　　处：《光学技术》1998年第3期26-30,共5页Optical Technique

摘　　要：本文扼要叙述了天文光学望远镜的通用调校步骤与方法，适用于诸如卡氏（Ｃａｓｓｅｇｒａｉｎ）、葛氏（Ｇｒｅｇｏｒｙ）、奈氏（Ｎａｓｍｙｔｈ）、折轴（Ｃｏｕｄé）、施密特（Ｓｃｈｍｉｄｔ）、牛顿（Ｎｅｗｔｏｎ）望远镜、…等的光学元件及系统的调校。对极轴的高度与方位的调整，也给以简要介绍。本文还概述了对成像质量的检测。文中以通光口径２．１６ｍ天文望远镜为例，给出了光路调整图。In this paper, the usual alignment procedure and method of the astronomical optical telescopes are described. It applies to the optical element and optical systems as Cassegrain, Gregory, Nasmyth, Coudé, Schmidt, Newton, etc.. The alignment of the polar axis and the testing of image quality are also described. Finally, as an example, the alignment diagram of the clear aperture 2.16m astronomical telescope is given.

关 键 词：光学望远镜 光学系统 光轴 调整 天文望远镜 

分 类 号：TH751.06[机械工程—仪器科学与技术]