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Optimization Design of Large-Aperture Primary Mirror for a Space Remote Camera
Xiaohan Liu1, Kaihui Gu1, Meixuan Li1
1Jilin Engineering Laboratory for Quantum Information Technology, Jilin Engineering Normal University, Changchun 130052, China.
Sensors (Basel, Switzerland)
|July 8, 2023
Summary
This study optimized a large-aperture primary mirror for space cameras, achieving high stability and accuracy using silicon carbide (SiC) and an innovative flange design. Experimental results confirm the mirror meets stringent space camera requirements for remote sensing applications.
Area of Science:
- Optical Engineering
- Materials Science
- Aerospace Engineering
Background:
- Designing primary mirrors for micro/nano satellite remote sensing cameras requires lightweight, high stability, and high-temperature adaptable materials.
- Traditional back plate support systems can be susceptible to shock, vibration, and temperature fluctuations, impacting mirror surface accuracy.
- Advancements in silicon carbide (SiC) material casting enable complex reflector structures.
Purpose of the Study:
- To optimize the design and experimentally verify a large-aperture (Φ610 mm) primary mirror for a space camera.
- To improve the primary mirror's long-term surface shape accuracy under dynamic and thermal loads.
- To ensure the primary mirror assembly meets the demanding performance requirements for space-based remote sensing.
Main Methods:
- Determined design performance index based on a coaxial tri-reflective optical imaging system.
- Selected silicon carbide (SiC) as the primary mirror material due to its excellent comprehensive properties.
- Improved initial design by integrating the flange with the mirror body for direct support force transmission.
- Employed a parametric optimization algorithm (compromise programming) for initial structural parameters and flexible hinge.
- Conducted finite element simulation to analyze performance under gravity, temperature rise, and assembly errors.
- Precision manufactured and assembled the primary mirror, followed by ZYGO interferometry and vibration testing.
Main Results:
- Optimized SiC primary mirror assembly achieved a mass of 8.66 kg.
- Finite element simulation showed RMS surface error < λ/50, maximum displacement < 10 μm, and maximum inclination < 5″.
- Fundamental frequency was simulated at 203.74 Hz and experimentally verified at 208.25 Hz.
- ZYGO interferometer testing confirmed a surface shape accuracy of 0.02 λ.
Conclusions:
- The optimized primary mirror design, utilizing an integrated flange and SiC material, successfully maintains high surface accuracy under various environmental conditions.
- The achieved performance metrics meet and exceed the design requirements for the space camera's primary mirror.
- This study demonstrates a viable approach for developing high-performance, lightweight primary mirrors for satellite remote sensing applications.

