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Research on Micro-Vibration Analysis of Segmented Telescope Based on Opto-Mechanical Integration
Kangmin Wen1,2,3, Lingjie Wang1,3, Xuefeng Zeng1,3
1Changchun Institute of Optics, Fine Mechanics and Physics, Chinese Academy of Sciences, Changchun 130033, China.
Sensors (Basel, Switzerland)
|April 28, 2025
Summary
A new dynamic opto-mechanical analysis method evaluates how in-orbit micro-vibrations affect segmented telescope imaging. This method ensures wavefront error remains below 0.071λ, crucial for maintaining high imaging quality during long exposures.
Area of Science:
- Optics and Space Engineering
- Mechanical Engineering
- Vibration Analysis
Background:
- In-orbit micro-vibrations significantly impact the imaging quality of segmented telescopes.
- Complex interactions between optical and mechanical systems under vibration are challenging to model.
Purpose of the Study:
- To propose a dynamic full-link opto-mechanical integration analysis method.
- To quantify the effect of micro-vibration on imaging quality for segmented telescopes with long exposure times.
Main Methods:
- Utilized measured micro-vibration signals from an infrared refrigerator.
- Performed transient response analysis using the finite element method in Patran/Nastran.
- Developed a Matlab interface for rigid body displacement calculation and real-time data interaction with Zemax.
Main Results:
- Achieved a wavefront error Root-Mean-Square (RMS) value below 0.071λ at a 1 μm wavelength over 4 seconds.
- Evaluated imaging quality using the point spread function peak ratio.
- Observed maximum peak ratio values of 0.4628 (X-axis) and 0.6207 (Y-axis) with a 2-second exposure time.
Conclusions:
- The developed method effectively analyzes the impact of micro-vibrations on segmented telescope imaging quality.
- Provides a crucial reference for evaluating optical system performance in micro-vibration environments, especially for long exposures.

