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Topology optimization design of a space mirror

机译:空间镜的拓扑优化设计

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As key components of the optical system of the space optical remote sensor, Space mirrors' surface accuracy had a direct impact that could't be ignored of the imaging quality of the remote sensor. In the future, large-diameter mirror would become an important trend in the development of space optical technology. However, a sharp increase in the mirror diameter would cause the deformation of the mirror and increase the thermal deformation caused by temperature variations. A reasonable lightweight structure designed to ensure the optical performance of the system to meet the requirements was required. As a new type of lightweight approach, topology optimization technology was an important direction of the current space optical remote sensing technology research. The lightweight design of rectangular mirror was studied, the variable density method of topology optimization was used. The mirror type precision of the mirror assemblies was obtained in different conditions. PV value was less than λ/10 and RMS value was less than λ/50(λ = 632.8nm). The results show that the entire The mirror assemblies can achieve a sufficiently high static rigidity, dynamic stiffness and thermal stability and has the capability of sufficient resistance to external environmental interference.
机译:作为空间光学遥感器光学系统的关键组成部分,空间镜的表面精度直接影响着遥感器的成像质量。未来,大口径镜将成为空间光学技术发展的重要趋势。然而,反射镜直径的急剧增加将引起反射镜的变形并增加由温度变化引起的热变形。需要一种合理的轻质结构,以确保系统的光学性能满足要求。作为一种新型的轻量级方法,拓扑优化技术是当前空间光学遥感技术研究的重要方向。研究了矩形镜的轻量化设计,并采用了变密度拓扑优化方法。在不同条件下获得了镜组件的镜类型精度。 PV值小于λ/ 10,RMS值小于λ/ 50(λ= 632.8nm)。结果表明,整个后视镜组件可以实现足够高的静态刚度,动态刚度和热稳定性,并具有足够的抵抗外部环境干扰的能力。

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