ED‐AttConvLSTM: An Ionospheric TEC Map Prediction Model Using Adaptive Weighted Spatiotemporal Features

Author:

Li Liangchao1ORCID,Liu Haijun1ORCID,Le Huijun234ORCID,Yuan Jing5,Wang Haoran1,Chen Yi1ORCID,Shan Weifeng1,Ma Li6,Cui Chunjie7

Affiliation:

1. Institute of Intelligent Emergency Information Processing Institute of Disaster Prevention Langfang China

2. Key Laboratory of Earth and Planetary Physics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

3. College of Earth and Planetary Sciences University of the Chinese Academy of Sciences Beijing China

4. Heilongjiang Mohe National Observatory of Geophysics Institute of Geology and Geophysics Chinese Academy of Sciences Beijing China

5. School of Information Engineering Institute of Disaster Prevention Langfang China

6. College of Art Hebei University of Economics and Business Shijiazhuang China

7. Beijing Jingwei Textile Machinery New Technology Co., Ltd. Beijing China

Abstract

AbstractIn this paper, we propose a novel Total Electron Content (TEC) map prediction model, named ED‐AttConvLSTM, using a Convolutional Long Short‐Term Memory (ConvLSTM) network and attention mechanism based on encoder‐decoder structure. The inclusion of the attention mechanism enhances the efficient utilization of spatiotemporal features extracted by the ConvLSTM, emphasizing the significance of crucial spatiotemporal features in the prediction process and, as a result, leading to an enhancement in predictive performance. We conducted experiments in East Asia (10°N–45°N, 90°E−130°E). The ED‐AttConvLSTM was trained and evaluated using the International GNSS Service TEC maps over a period of six years from 2013 to 2015 (high solar activity years) and 2017 to 2019 (low solar activity years). We compared our ED‐AttConvLSTM with IRI‐2016, COPG, LSTM, GRU, ED‐ConvLSTM and ED‐ConvGRU. The results indicate that our model surpasses the comparison models in forecasting both high and low solar activity years, across most months and UT moments in a day. Moreover, our model exhibits notably superior prediction performance during the most severe phases of a magnetic storm when compared to the comparison models. Subsequently, we then also discuss how the prediction performance of our model is affected by latitude. Finally, we discuss the diminishing performance of our model in multi‐day predictions, demonstrating that its reliability for forecasts ranging from one to 4 days in advance. Beyond the fifth day, there is a pronounced decline in the model's performance.

Funder

National Natural Science Foundation of China

Youth Innovation Promotion Association

Natural Science Foundation of Hebei Province

Publisher

American Geophysical Union (AGU)

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