Issue |
A&A
Volume 691, November 2024
|
|
---|---|---|
Article Number | A246 | |
Number of page(s) | 9 | |
Section | Astronomical instrumentation | |
DOI | https://doi.org/10.1051/0004-6361/202451919 | |
Published online | 15 November 2024 |
An optimization method for deformable mirror configuration in multi-conjugate adaptive optics systems
1
National Laboratory on Adaptive Optics,
Chengdu
610209,
Sichuan,
China
2
Institute of Optics and Electronics, Chinese Academy of Sciences,
Chengdu
610209,
Sichuan,
China
3
University of Chinese Academy of Sciences,
Beijing
100049,
China
4
School of Electronic, Electrical and Communication Engineering, University of Chinese Academy of Sciences,
Beijing
100049,
China
★ Corresponding author; lqzhang@ioe.ac.cn
Received:
19
August
2024
Accepted:
10
October
2024
Context. Multi-conjugate adaptive optics (MCAO) is a crucial technology for achieving high-resolution imaging over a wide field of view with modern ground-based optical telescopes. The configuration of deformable mirrors (DMs) is a key component in the analysis and optimization of MCAO performance. Currently, the search for the optimal DM configuration often relies on iterative and time-consuming Monte Carlo simulations. This issue arises from the lack of an appropriate optimization method for DM configurations.
Aims. The primary objective of this paper is to establish an optimization method for DM configurations in MCAO systems. We established a quantitative criterion for evaluating DM configurations by analyzing their correction capabilities for turbulence aberrations at different altitudes. Then, we optimized the DM configurations based on this criterion. This method provides a new theoretical foundation and practical tool for the design and performance optimization of MCAO systems.
Methods. Based on the pupil phase structure function, we established a DM configuration evaluation criterion, namely the non-conjugate correction index (NCCI). Using NCCI as the optimal criterion, combined with the particle swarm optimization algorithm, we searched for the optimal solution across different DM configuration spaces.
Results. We conducted simulations based on the turbulence profiles of typical telescope sites. We validated our proposed theoretical model against Monte Carlo simulation models and find that the NCCI error ranges from 0.05 to 0.1. For optimizing DM conjugate heights, the results of our optimization algorithm differ by less than 1 km from those obtained via Monte Carlo simulations. Regarding the performance of the DM optimization algorithm, the average convergence accuracy error is less than 0.1 km, and the average convergence speed is approximately ten iterations. Additionally, our optimization method runs in just a few minutes; Monte Carlo simulations, in comparison, require several dozen hours.
Key words: instrumentation: adaptive optics / methods: analytical / techniques: high angular resolution / telescopes
© The Authors 2024
Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.
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