New website getting online, testing
    • 摘要: 针对空间引力波探测对望远镜系统提出的皮米级稳定性和λ/30波前误差的应用需求,提出了一种光机集成分析与优化方法。首先开展了主镜侧支撑点位置分析和支撑结构拓扑优化;然后基于并联Bipod连杆支撑的柔度矩阵,建立了各结构参数的评价函数,并通过Matlab分析初步确定柔性支撑尺寸参数取值范围;最后,搭建了光机集成仿真平台对结构进一步优化。结果表明,系统一阶频率为392.43 Hz,重力和温度载荷下主镜面形变化优于λ/60;在10 μK/Hz1/2的空间热扰动下,主镜组件尺寸稳定性在10 pm/Hz1/2水平。

       

      Abstract: In order to meet the application requirements of pimi-level stability and λ/30 wavefront error in space gravitational wave detection, an optical and mechanical integrated analysis and optimization method is proposed. Firstly, the position analysis of the support points on the main mirror side and the topology optimization of the support structure were carried out. Then, based on the flexibility matrix of parallel Bipod linkage support, the evaluation function of each structure parameter is established, and the value range of flexible support size parameters was preliminarily determined by Matlab analysis. Finally, an integrated optical and mechanical simulation platform was built to further optimize the structure.The results show that the first-order frequency of the system is 392.23 Hz, and the deformation of the primary mirror surface deformation under gravity and temperature loads is better than λ/60. Under thermal disturbances in a space environment of 10 μK/Hz1/2, the dimensional stability of the primary mirror component is at a level of 10 pm/Hz1/2.