引力参考传感器耦合噪声的CNN-BiLSTM逐层自适应剥离OA
Layer-by-layer adaptive stripping of coupling noise in gravitational reference sensors using CNN-BiLSTM
以 LISA、太极计划和天琴计划为代表的空间探测计划面临的核心挑战之一是如何处理测试质量块复杂的噪声背景.引力参考传感器(GRS)的噪声包含布朗噪声、温度场耦合、磁场噪声、静电场噪声、驱动电压不稳定性及难以解释的 1/f超额噪声等多种物理起源.本文提出一种"物理机理→噪声分类→双向时序建模→自适应剔除"的完整算法链条:基于 LISA Pathfinder任务实测数据校准的物理噪声模型将出气效应等最新结果定量嵌入噪声合成管道;卷积神经网络(CNN)与双向长短期记忆网络(BiLSTM)在物理分类引导下互补捕获局部瞬态模式与双向长程依赖(链条第二环);按物理类别依次执行自适应谱减法实现噪声的逐层物理剥离(链条第三环).仿真结果表明,在输入信噪比为 10.2 dB的条件下,该算法链条对注入信号的恢复保真度达 0.97(归一化相关系数),优于传统匹配滤波及纯 CNN或纯 BiLSTM基线方法.本研究可为空间引力波探测中的噪声建模、数据管道设计提供有价值的参考.
This study addresses the difficulty of interpreting and separating multi-source coupling noise in gravitational reference sensors(GRSs)for spaceborne gravitational-wave detection.A unified acceleration-noise spectrum model is established for Brownian noise,thermal-field coupling,magnetic noise,electrostatic noise,drive-voltage noise,and residual low-frequency noise,with key parameters calibrated against LISA Pathfinder measurements.CNN layers are used to extract local transient features,BiLSTM layers are used to capture long-range temporal dependence,and adaptive spectral subtraction is then applied sequentially by physical noise category.At an input SNR of 10.2 dB,the proposed method achieves a recovery fidelity of 0.969 4 and a waveform overlap of 0.969 5,outperforming matched filtering,pure CNN,and pure BiLSTM baselines.Across an SNR range from −15 dB to+25 dB,the method shows a slower performance degrada-tion in the negative-SNR regime.Combining physics-guided noise classification with CNN-BiLSTM tempor-al modeling improves signal recovery under complex GRS noise backgrounds and provides a useful refer-ence for noise budgeting,simulation pipelines,and onboard denoising algorithms in spaceborne gravitational-wave missions.
李岚滨;董鹏
国科大杭州高等研究院 基础物理与数学科学学院,浙江 杭州 310024||中国科学院国家授时中心,陕西 西安 710600||中国科学院大学,北京 100049国科大杭州高等研究院 基础物理与数学科学学院,浙江 杭州 310024
数理科学
引力参考传感器卷积神经网络双向长短期记忆网络噪声分离LISA Pathfinder
gravitational reference sensorCNN-BiLSTMnoise strippingphysical noise modelingLISA Pathfinder
《中国光学(中英文)》 2026 (5)
1166-1179,14
国家重点研发计划资助项目(No.2024YFC2207203) Supported by the National Key Research and Development Program(No.2024YFC2207203)
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