Design of athermalized mounting structure for the sub-aperture primary mirror of a synthetic aperture telescope

Author:

Li Yunfeng123,Li Zongxuan13ORCID,Yong Qiang13,Wang Tiancong13,Zhang Defu13

Affiliation:

1. Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun, China

2. University of Chinese Academy of Sciences, Beijing, China

3. Key Laboratory of Space-based Dynamic and Rapid Optical Imaging Technology, Chinese Academy of Sciences, Changchun, China

Abstract

The imaging quality of the synthetic aperture system is sensitive to the positioning accuracy of the sub-aperture primary mirror. A novel flexible mounting structure of bimetallic material is proposed for the athermalization of the sub-aperture primary mirror of the Fizeau Synthetic Aperture Telescope – which is composed of seven sub-aperture. The axial position accuracy of the sub-aperture primary mirror must be less than 5 µm under 10°C temperature rise to meet the requirements of the optical system. Firstly, a single mounting unit is analyzed theoretically, and the initial parameters are determined. The conceptual design of the mounting structure is carried out by using initial parameters. The orthogonal optimization algorithm and range analysis are used to optimize the structural parameters. The finite element model of the flexible mounting structure is established and the coupled thermal-mechanical simulation analysis is performed. Then the thermal sensitivity test of the sub-aperture primary mirror mounting structure was carried out. Under the effect of a temperature rise of 10°C, the axial displacement of the sub-aperture primary mirror mounting surface is less than 3 µm. Finally, the synthetic aperture system is assembled, and the optical test verifies that the synthetic aperture system has good imaging capabilities.

Funder

Youth Innovation Promotion Association of the Chinese Academy of Sciences

Publisher

SAGE Publications

Subject

Mechanical Engineering

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