Quantitative analysis of backscattering contamination sources in the TianQin telescope.

IF 3.3 2区 物理与天体物理 Q2 OPTICS
Optics express Pub Date : 2025-09-08 DOI:10.1364/OE.570389
Xinxin Liu, Zizheng Li, Yiping Wang, Tianxiang Lv, Jingxiao Peng, Shanxiang Liang, Xin Zhang
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引用次数: 0

Abstract

The utilization of smooth optical surfaces represents a critical approach for suppressing backscattering in spaceborne gravitational wave telescopes, such as those employed in the TianQin project. The bidirectional reflectance distribution function (BRDF) serves as an effective physical parameter for characterizing light scattering properties and has been extensively applied in stray light suppression research. This study employs surface scattering theory to quantitatively analyze the impact of three major stray light sources - surface roughness, defects, and contamination-on telescope system backscattering. Based on this analysis, we establish specific performance requirements for single mirror surface roughness, defect tolerance, and cleanliness levels.

天琴望远镜后向散射污染源的定量分析。
平滑光学表面的利用是抑制星载引力波望远镜后向散射的关键方法,例如天琴项目中使用的望远镜。双向反射分布函数(BRDF)作为表征光散射特性的有效物理参数,在杂散光抑制研究中得到了广泛应用。本研究运用表面散射理论定量分析了三种主要杂散光源——表面粗糙度、缺陷和污染对望远镜系统后向散射的影响。基于这一分析,我们建立了对单镜表面粗糙度、缺陷容忍度和清洁度的具体性能要求。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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来源期刊
Optics express
Optics express 物理-光学
CiteScore
6.60
自引率
15.80%
发文量
5182
审稿时长
2.1 months
期刊介绍: Optics Express is the all-electronic, open access journal for optics providing rapid publication for peer-reviewed articles that emphasize scientific and technology innovations in all aspects of optics and photonics.
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