An Automated Detection Method for Solar Radio Type III Bursts Using Phase Clustering and Hierarchical Thresholding
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摘要: 太阳射电III型暴是太阳活动中最为常见的射电爆发类型之一, 其具有快速频率漂移等特征, 是耀斑爆发和日冕物质抛射等太阳活动事件的示踪器. 现有的识别方法面临连续爆发检测能力弱、小样本学习不足等问题, 导致误检率高和召回率低. 针对这些缺陷, 提出一种基于相位编组法的自适应轮廓检测算法, 该方法融合灰度梯度相位信息与多级阈值过滤, 通过形态学操作拟合太阳射电Ⅲ型暴频谱轮廓, 实现对太阳射电Ⅲ型暴频谱的自动识别, 通过计算对应的爆发起止时间、爆发起止频率、频率漂移率等有效信息, 对海量频谱观测数据进行快速批量识别与分析. 基于云南天文台澄江米波太阳射电望远镜的观测数据集开展应用, 经检验, 该方法在识别太阳射电Ⅲ型暴上实现了93.5%的召回率.Abstract: Solar radio type III bursts are among the most common types of radio bursts in solar activities. They are characterized by features such as rapid frequency drift and serve as a precursor tracer for solar activity events like solar flares and coronal mass ejections. Existing identification methods face problems such as weak capability in detecting continuous bursts and insufficient learning with small samples, leading to high false detection rates and low recall rates. To address these shortcomings, this paper proposes an adaptive contour detection algorithm based on the phase grouping method. This method integrates gray gradient phase information with multi-level threshold filtering, fits the spectral contour of solar radio type III bursts through morphological operations, and realizes the automatic identification of the spectrum of solar radio type III bursts. Applied to the observation dataset from the Chengjiang Meter-wave Solar Radio Telescope of Yunnan Observatory, it has been verified that this method achieves a 93.5% recall rate in identifying solar radio type III bursts.
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表 1 核尺寸连接性能对比表
Table 1. Comparison table of nuclear size connection performance
核尺寸 特征边缘连接正确率/(%) 噪声连接错误率/(%) 3×2 37.5 0.9 5×2 73.5 4.6 7×2 92.6 10.3 9×2 94.8% 39.8 -
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张洪瑞 男, 2000年7月出生于云南省普洱市, 现为云南大学信息学院硕士研究生, 主要研究方向为太阳射电暴频谱的自动识别、无线电环境测试等. E-mail:
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