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一种X射线脉冲星信号特征提取算法

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利用脉冲星X射线信号对飞船进行导航是深空探测的一大热门研究领域.在X射线脉冲星导航中,对X射线脉冲星信号进行辨识非常重要.提出以时间周期峰度作为脉冲星信号的特征提取算法,并结合ResNet34对其训练验证.以辨识准确性超过90%作为辨识成功的标准,其中B0531+21、B0540-69和B1509-58三颗脉冲星完成辨识任务的最短观察时长分别为0.5 s、2.5 s和15 s.实验证明,TCK能快速、准确地完成X射线脉冲星信号的辨识任务.
An Algorithm for Identifying X-ray Pulsar Signals
The use of pulsar X-ray signals for spacecraft navigation is a hot research field in deep space exploration.In X-ray Pulsar-based Navigation(XNAV),identifying X-ray pulsar signals is extremely important.This article proposes the Time Cycle Kurtosis(TCK)as an identification algorithm for extracting pulsar signal features,and combines it with ResNet34 for training and verifica-tion.The criterion for successful identification is based on an accuracy of over 90%,with the shortest observation times for B0531+21,B0540-69,and B1509-58 pulsars to complete the identification task being 0.5 s,2.5 s,and 15 s,respectively.This article demon-strates through experiments that TCK can quickly and accurately complete the identification task of X-ray pulsar signals.

XNAVidentificationTCKfeature extractionResNet34

曾豪、杨乘

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贵州省教育厅汽车电子技术特色重点实验室,贵州 贵阳 550025

贵州师范大学 物理与电子科学学院,贵州 贵阳 550025

XNAV 辨识 TCK 特征提取 ResNet34

国家自然科学基金项目贵州省科学技术基金重点项目

62062025黔科合基础[2019]1432

2024

电脑与电信
广东省对外科技交流中心

电脑与电信

影响因子:0.117
ISSN:1008-6609
年,卷(期):2024.(5)