实时自动检测多类别太阳射电暴

IF 1.8 4区 物理与天体物理 Q3 ASTRONOMY & ASTROPHYSICS
Jingyu Deng, Guowu Yuan, Hao Zhou, Hao Wu, Chengming Tan
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引用次数: 0

摘要

精确的太阳射电暴(SRB)实时探测对于太阳物理研究和空间天气预报至关重要。目前,关于太阳射电暴探测的大多数研究都集中在单类识别和简单判别上。现有的多类别检测研究非常有限。本文提出了一种多类别太阳射电暴实时探测方法,以满足太阳射电暴实时探测、探测精度和分类精度的要求。首先,从 e-CALLISTO 收集太阳射电暴频谱。利用 LabelImg 对频谱进行标注,建立了包含 II 型、III 型、IIIs 型、IV 型和 V 型太阳射电暴的数据集。其次,在 YOLOv8n 模型的主干模块中引入了全维度动态卷积,增强了模型的特征提取能力。第三,创建了基于 ConvNeXt 的多尺度特征融合网络,以防止特征信息丢失并优化损失函数。实验结果表明,在已建立的太阳射电暴数据集上,所提出的方法达到了 82.4% 的平均检测精度。与最初的 YOLOv8n 模型相比,准确率提高了 3.5%。此外,该模型以每秒 140.9 帧的速度运行,每帧代表一个持续 15 分钟的频谱。因此,改进后的 YOLOv8n 模型提高了太阳射电暴的探测精度和速度,实现了对 II 型、III 型、IIIs 型、IV 型和 V 型太阳射电暴的自动探测和定位。
本文章由计算机程序翻译,如有差异,请以英文原文为准。

Real-time automated detection of multi-category solar radio bursts

Real-time automated detection of multi-category solar radio bursts

Accurate real-time solar radio burst (SRB) detection is crucial for solar physics research and space weather forecasting. Currently, most studies on solar radio burst detection focus on single-category identification and simple discrimination of bursts. There are limited existing studies on multi-category detection. This paper proposes a real-time multi-category solar radio burst detection method to meet the requirements of real-time detection, detection accuracy, and classification accuracy in solar radio bursts. First, solar radio burst spectrums were collected from e-CALLISTO. The spectrums are labeled using LabelImg, and a dataset containing solar radio bursts of Type II, Type III, Type IIIs, Type IV, and Type V was established. Second, a full-dimensional dynamic convolution was introduced in the backbone module of the YOLOv8n model, enhancing the model’s feature extraction capability. Third, a multi-scale feature fusion network based on ConvNeXt was created to prevent feature information loss and optimize the loss function. The experimental results show that the proposed method achieves an average detection accuracy of 82.4% on the established solar radio burst dataset. Compared with the original YOLOv8n model, the accuracy increased by 3.5%. Additionally, the model operates at 140.9 frames per second, with each frame representing a spectrum of 15 minutes duration. Thus, the improved YOLOv8n model enhances the detection accuracy and speed of solar radio bursts, enabling automatic detection and localization of solar radio bursts of Type II, Type III, Type IIIs, Type IV, and Type V.

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来源期刊
Astrophysics and Space Science
Astrophysics and Space Science 地学天文-天文与天体物理
CiteScore
3.40
自引率
5.30%
发文量
106
审稿时长
2-4 weeks
期刊介绍: Astrophysics and Space Science publishes original contributions and invited reviews covering the entire range of astronomy, astrophysics, astrophysical cosmology, planetary and space science and the astrophysical aspects of astrobiology. This includes both observational and theoretical research, the techniques of astronomical instrumentation and data analysis and astronomical space instrumentation. We particularly welcome papers in the general fields of high-energy astrophysics, astrophysical and astrochemical studies of the interstellar medium including star formation, planetary astrophysics, the formation and evolution of galaxies and the evolution of large scale structure in the Universe. Papers in mathematical physics or in general relativity which do not establish clear astrophysical applications will no longer be considered. The journal also publishes topically selected special issues in research fields of particular scientific interest. These consist of both invited reviews and original research papers. Conference proceedings will not be considered. All papers published in the journal are subject to thorough and strict peer-reviewing. Astrophysics and Space Science features short publication times after acceptance and colour printing free of charge.
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