基于深度学习的风暴期全球电离层 TEC 预测:混合 CNN-BiLSTM 方法

Space Weather Pub Date : 2024-07-01 DOI:10.1029/2024sw003877
Xiaochen Ren, Biqiang Zhao, Zhipeng Ren, Yan Wang, Bo Xiong
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摘要

深度学习在高精度电离层参数预测中的应用已成为空间天气研究的重点之一。本研究提出了一种名为混合卷积神经网络(CNN)-双长短期记忆的改进模型,用于预测未来电离层总电子含量(TEC)。利用现有最长(25 年)全球电离层地图-TEC 对模型进行了训练,并评估了电离层风暴预测的准确性。结果表明,与地心坐标系相比,使用太阳地理参照系中的历史 TEC 作为输入驱动数据可获得更高的预测精度。此外,通过比较不同的输入参数,发现将 Kp、ap 和 Dst 指数作为模型的输入可有效提高其准确性,尤其是在长期预报中,R2 提高了 3.49%,均方根误差降低了 13.48%。与 BiLSTM-深度神经网络(DNN)和 CNN-BiLSTM 相比,混合 CNN-BiLSTM 模型的预测精度最高。这表明利用 CNN 模块处理空间信息,并结合 DNN 模块纳入地磁指数进行结果校正。此外,在短期预测中,该模型准确预测了电离层风暴的演变过程。在延长预测长度时,虽然存在预测误差的情况,但模型仍然捕捉到了电离层风暴的整个过程。此外,预测结果受经度、磁纬度和当地时间的影响很大。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
Deep Learning‐Based Prediction of Global Ionospheric TEC During Storm Periods: Mixed CNN‐BiLSTM Method
The application of deep learning in high‐precision ionospheric parameter prediction has become one of the focus in space weather research. In this study, an improved model called Mixed Convolutional Neural Networks (CNN)—Bi‐Long Short Term Memory is proposed for predicting future ionospheric Total Electron Content (TEC). The model is trained using the longest available (25 years) Global Ionospheric Maps‐TEC and evaluated the accuracy of ionospheric storm predictions. The results indicate that using historical TEC in the solar‐geographical reference frame as input driving data achieves higher prediction accuracy compared to that in the geocentric coordinate system. Additionally, by comparing different input parameters, it is found that incorporating the Kp, ap, and Dst indices as inputs to the model effectively improves its accuracy, especially in long‐term forecasting where R2 increased by 3.49% and Root Mean Square Error decreased by 13.48%. Compared with BiLSTM‐Deep Neural Networks (DNN) and CNN‐BiLSTM, the Mixed CNN‐BiLSTM model has the highest prediction accuracy. It suggests that the utilization of CNN modules for processing spatial information, along with the incorporation of DNN modules to incorporate geomagnetic indices for result correction. Moreover, in short‐term predictions, the model accurately forecasts the evolution process of ionospheric storms. When extending the predicted length, although there are cases of prediction errors, the model still captures the entire process of ionospheric storms. Furthermore, the predicted results are significantly influenced by longitude, magnetic latitude, and local time.
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