利用多尺度 TransUNet 识别无线电频率干扰

IF 3.3 3区 物理与天体物理 Q2 ASTRONOMY & ASTROPHYSICS Publications of the Astronomical Society of the Pacific Pub Date : 2024-06-27 DOI:10.1088/1538-3873/ad54ef
Xuan Zhang, Bo Liang, Longfei Hao, Song Feng, Shoulin Wei, Wei Dai and Yihang Dao
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引用次数: 0

摘要

无线电观测是一种利用无线电波进行天文观测的方法。射电观测中的一个常见挑战是射频干扰(RFI),它是指射频频段内其他无线信号源对无线电信号的无意或有意干扰。这种干扰会污染射电望远镜接收到的天文信号,严重影响时频域天文观测和研究。因此,识别 RFI 至关重要。在本文中,我们采用了一种深度学习方法来检测观测数据中存在的射频干扰,并提出了一种基于 TransUNet 的改进网络结构。该网络利用了多尺度卷积注意机制的原理。它引入了提取高维图像信息的辅助分支和用于提取特征图的增强型坐标注意机制,从而能够更全面、更准确地识别时频图像中的射频干扰。我们引入了一种名为多尺度 TransUNet 网络(简称 MS-TransUNet)的新型架构。我们利用云南天文台 40 米射电望远镜的观测数据作为数据集,对网络进行训练、验证和测试。与之前的深度学习网络(U-Net、RFI-Net、R-Net、DSC、EMSCA-UNet)相比,该网络的召回率和 f2 得分均有显著提高。具体来说,召回率至少提高了 2.99%,f2 分数至少提高了 2.46%。实验证明,该网络在确保高精度的同时,还能更全面地识别 RFI。
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Identification of Radio Frequency Interference Using Multi-scale TransUNet
Radio observation is a method for conducting astronomical observations using radio waves. A common challenge in radio observations is Radio Frequency Interference (RFI), which refers to the unintentional or intentional interference of radio signals from other wireless sources within the radio frequency band. Such interference contaminates the astronomical signals received by radio telescopes, significantly affecting time–frequency domain astronomical observations and research. Consequently, identifying RFI is crucial. In this paper, we employ a deep learning approach to detect RFI present in observation data and propose an improved network structure based on TransUNet. This network leverages the principles of a multi-scale convolutional attention mechanism. It introduces an auxiliary branch to extract high-dimensional image information and an enhanced coordinate attention mechanism for feature map extraction, enabling more comprehensive and accurate identification of RFI in time–frequency images. We introduce a novel architecture named the Multi-Scale TransUNet Network, abbreviated as MS-TransUNet. We utilized observation data from the 40 m radio telescope at the Yunnan Observatory as a data set for training, validating, and testing the network. Compared with previous deep learning networks (U-Net, RFI-Net, R-Net, DSC, EMSCA-UNet), the recall rate and f2 score have been significantly improved. Specifically, the recall rate is improved by at least 2.99%, and the f2 score is improved by at least 2.46%. Experiments demonstrate that this network is exceptional in identifying RFI more comprehensively while ensuring high precision.
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来源期刊
Publications of the Astronomical Society of the Pacific
Publications of the Astronomical Society of the Pacific 地学天文-天文与天体物理
CiteScore
6.70
自引率
5.70%
发文量
103
审稿时长
4-8 weeks
期刊介绍: The Publications of the Astronomical Society of the Pacific (PASP), the technical journal of the Astronomical Society of the Pacific (ASP), has been published regularly since 1889, and is an integral part of the ASP''s mission to advance the science of astronomy and disseminate astronomical information. The journal provides an outlet for astronomical results of a scientific nature and serves to keep readers in touch with current astronomical research. It contains refereed research and instrumentation articles, invited and contributed reviews, tutorials, and dissertation summaries.
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