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Optimized design for the supporting structure of a large aperture mirror

机译:大孔径镜支柱结构的优化设计

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With the continuous development of optical technology in recent years, the pace of human exploration of space has further accelerated. Space remote sensing technology is widely used in surveying and mapping, environmental monitoring and other fields. Therefore, the requirements for space optics technology are gradually increasing. In order to reduce the launch cost and the deformation of the supporting member and the main mirror base under its own gravity, a lightweight design must be carried out. Therefore, under the premise of ensuring the rigid body displacement of the mirror body and the error of the mirror shape, lightweight has become a key requirement for the development of remote sensing technology. By comparing various supporting structures, the spatial freedom of the mirror is calculated. Choose a combination of 9-point post-support and 3-point peripheral support. Compare and select the materials commonly used in the structure of the supporting part and the main mirror base. Although the support structure adopts topology optimization, a very effective support method can be obtained, but the final result cannot be universally applied to the support structure of mirrors with different apertures. Therefore, this paper determines the design structure of the relationship between the mirror support position, the fundamental frequency and the surface shape accuracy and the support structure parameters based on the flexibility matrix. For the rigid parts of the supporting structure and the main mirror base, simulation software was used to optimize the design of the initial design structure to remove excess materials. The final main mirror base lightweight rate was 36.6%, and the triangular plate lightweight rate was 65.9%. The static analysis and modal analysis of the supporting scheme are carried out by analysis software. After optimization, the shape accuracy of the primary mirror under its own weight is better than λ/50. Structural resonance will seriously affect the use and life of the equipment. Therefore, the modal analysis is performed, and the fundamental frequency is within a reasonable range during the optimization process. The simulation results show that the first-order fundamental frequency is 836.55 Hz. The analysis results show that while ensuring the shape accuracy of the primary mirror, the lightweight design of the mirror support assembly is realized.
机译:随着近年来光学技术的不断发展,人类对空间的探索的步伐进一步加速了。空间遥感技术广泛用于测量和映射,环境监测和其他领域。因此,空间光学技术的要求逐渐增加。为了降低支撑构件的发射成本和支撑构件的变形,并且在其自身的重力下,必须进行轻质设计。因此,在确保镜子体刚体位移和镜子形状的误差的前提下,重量级已成为遥感技术开发的关键要求。通过比较各种支撑结构,计算镜子的空间自由度。选择9点后支撑后和3点外围支持的组合。比较并选择常用于支撑部件和主镜底座的结构中的材料。尽管支持结构采用拓扑优化,但是可以获得非常有效的支持方法,但是最终结果不能普遍地应用于具有不同孔的镜子的支撑结构。因此,本文基于柔性矩阵确定了镜子支撑位与表面形状精度和支持结构参数之间的关系的设计结构。对于支撑结构的刚性部件和主镜基部,使用仿真软件用于优化初始设计结构的设计,以除去多余的材料。最终主镜基体积轻速率为36.6%,三角形板轻量级率为65.9%。支持方案的静态分析和模态分析由分析软件进行。优化后,其自身重量下的主镜的形状精度优于λ/ 50。结构共振将严重影响设备的使用和寿命。因此,执行模态分析,并且在优化过程期间,基本频率在合理范围内。仿真结果表明,一阶基频率为836.55 Hz。分析结果表明,在确保主镜的形状精度的同时,实现了镜子支撑组件的轻质设计。

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