Demonstrates improved noise suppression in gravitational wave detection systems, suggesting increased measurement accuracy.
空间引力波探测中,超前指向机构(PAAM)是实现星间激光链路高精度指向的关键部件,但其转动引入的抖动耦合(TTL)噪声严重制约干涉测量精度。为抑制PAAM角抖动引起的局部TTL噪声,本文提出一种成像系统方案,通过将探测器光学成像至PAAM等效旋转中心,从几何光路主动抑制噪声。基于激光外差干涉原理构建高对称等臂干涉仪测试平台,利用IFOCAD软件系统分析非理想条件(角抖动、旋转中心偏移、安装误差、热致形变)下成像系统的抑制性能。实现表明:理想对准时,成像系统可抑制98.9%的杠杆光程变化和98.2%的活塞光程变化;安装误差下TTL噪声抑制在<tex-math id="M2">{document}1\;pm/√Hz{document}</tex-math><alternatives></alternatives>以内,引入热噪声后仍稳定在<tex-math id="M4">{document}10\;pm/√Hz{document}</tex-math><alternatives></alternatives>以内。仿真验证了杠杆噪声与角抖动呈二阶相关、活塞噪声呈一阶相关,与理论吻合。本研究为高稳定度光束指向控制系统设计及噪声评估提供了理论依据与仿真实现。
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ZHANG et al. (2026) studied this question.
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