A multi-fidelity transfer learning strategy for surface deformation measurement of large reflector antennas

IF 2.7 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS
Zihan Zhang, Qian Ye, Na Wang, Guoxiang Meng
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引用次数: 0

Abstract

As the observation frequency of large-aperture antennas increases, the requirements for measuring main reflector deformation have become more stringent. Recently, the rapid development of deep learning has led to its application in antenna deformation prediction. However, achieving high accuracy requires a large number of high-fidelity deformation samples, which is often challenging to obtain. To address these problems, this paper establishes a high-accuracy antenna surface deformation measurement model based on a multi-fidelity transfer learning neural network (MF-TLNN). Firstly, a low-fidelity surrogate model is constructed using a large number of simulation deformation samples to ensure its robustness. Secondly, the MF-TLNN structure is designed and trained using a small number of high-fidelity samples obtained from actual measurements of the main reflector deformation via out-of-focus (OOF) holography method. Thirdly, a Zernike correction module is utilized to provide additional constraints and ensure the stability of the results. Experimental results show that the proposed method can closely approximate radio holography measurements in terms of accuracy and is almost real-time in terms of speed.

大型反射面天线表面变形测量的多保真度迁移学习策略
随着大口径天线观测频率的增加,对测量主反射面变形的要求也越来越严格。近年来,深度学习的快速发展使其在天线变形预测中得到了应用。然而,实现高精度需要大量高保真变形样本,这往往是具有挑战性的。针对这些问题,本文建立了一种基于多保真度迁移学习神经网络(MF-TLNN)的高精度天线表面变形测量模型。首先,利用大量模拟变形样本构建低保真代理模型,保证模型的鲁棒性;其次,利用离焦(OOF)全息法对主反射面变形进行实测得到的少量高保真样本,设计并训练了MF-TLNN结构;第三,利用Zernike校正模块提供额外约束,保证结果的稳定性。实验结果表明,该方法在精度上接近于射电全息测量,在速度上接近于实时性。
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来源期刊
Experimental Astronomy
Experimental Astronomy 地学天文-天文与天体物理
CiteScore
5.30
自引率
3.30%
发文量
57
审稿时长
6-12 weeks
期刊介绍: Many new instruments for observing astronomical objects at a variety of wavelengths have been and are continually being developed. Furthermore, a vast amount of effort is being put into the development of new techniques for data analysis in order to cope with great streams of data collected by these instruments. Experimental Astronomy acts as a medium for the publication of papers of contemporary scientific interest on astrophysical instrumentation and methods necessary for the conduct of astronomy at all wavelength fields. Experimental Astronomy publishes full-length articles, research letters and reviews on developments in detection techniques, instruments, and data analysis and image processing techniques. Occasional special issues are published, giving an in-depth presentation of the instrumentation and/or analysis connected with specific projects, such as satellite experiments or ground-based telescopes, or of specialized techniques.
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