光电工程, 2018, 45 (11): 180058, 网络出版: 2018-12-16
1.8 m 太阳望远镜偏振标定单元设计
Polarization calibration unit design of 1.8 m Chinese large solar telescope
摘要
中国1.8 m太阳望远镜(Chinese large solar telescope,CLST)致力于对太阳偏振的高精度及高灵敏度测量。然而其系统本身会引入仪器偏振,并且在望远镜运行的过程中,仪器偏振会随其指向的变化而变化。这就降低了系统的测量精度。因此,需要一个偏振标定单元对其仪器偏振进行标定。为此,本文对偏振标定的原理和方法进行了研究,并且给出了针对CLST 的偏振标定单元设计方案。
Abstract
It is the main task for the Chinese large solar telescope (CLST) with a 1.8 m aperture to measure the solar polarization with a high accuracy and sensitivity. However, the telescope system itself will introduce instrumental polarization. It also will change constantly with the rotating of the telescope and will reduce the accuracy. Therefore, a calibration unit is necessary to calibrate it. In this paper, we introduced the polarization calibration method and proposed a calibration unit structure.
姚本溪, 饶长辉, 顾乃庭. 1.8 m 太阳望远镜偏振标定单元设计[J]. 光电工程, 2018, 45(11): 180058. Yao Benxi, Rao Changhui, Gu Naiting. Polarization calibration unit design of 1.8 m Chinese large solar telescope[J]. Opto-Electronic Engineering, 2018, 45(11): 180058.