Daimian Hou, Fuzhen Liu, Hai Peng, Yanchao Gu, Guodong Tang
{"title":"单站 TEC 模型的时序卷积网络构建与分析","authors":"Daimian Hou, Fuzhen Liu, Hai Peng, Yanchao Gu, Guodong Tang","doi":"10.1016/j.jastp.2024.106309","DOIUrl":null,"url":null,"abstract":"<div><p>Ionosphere is one of the main error sources of global navigation satellite system (GNSS) precise positioning, and affecting communicate services such as communication, broadcasting, and radar positioning. Total electron content (TEC) is a key parameter to characterize the state of the ionosphere. Establishing a high-precision TEC model and making accurate predictions can effectively improve positioning accuracy and improve communication quality. The traditional TEC model has limited ability to describe the changes of TEC under extreme conditions such as magnetic storms. Based on the temporal convolution network (TCN) model, this paper conducts experiments on TEC grid data in six low latitude regions and six mid latitude regions, and compares them with Long short term memory (LSTM), gated recurrent units (GRU) and bidirectional long short term memory (BiLSTM) models. Results show that the mean average error (MAE) of TCN (1.2385 TECU) is lower in most areas compared with LSTM (1.2727 TECU), GRU (1.2602 TECU) and BiLSTM (1.2767 TECU). And the TCN model shows better performance in the mid latitude regions (0.8778 TECU) than low latitude regions (1.5992 TECU). Then, this paper takes 1st October to 31st December 2021. as an example to calculate the prediction accuracy of the TCN model in the magnetic quiet period and the magnetic storm period. During the sample time, there were 4 weak geomagnetic storms, 1 strong geomagnetic storm, and there was a continuous long magnetic resting period at the same time, with a variety of different geomagnetic activities. The results show that the MAE distribution of the TCN model is more concentrated in the magnetostatic period, and the model error in the mid latitude region is normally distributed between -4-4.5 TECU. During the magnetic storm period, the TCN model has the lowest proportion of errors exceeding 5 TECU, and the proportions in the mid latitude and low latitude regions are 2.8% and 10.4%, respectively, which are better than the comparison model. Finally, we discuss the performance of short-term TEC prediction and the possible causes of obvious errors. The accuracy of the TCN model reaches 1.07 TECU, which is better than the long-term prediction result (1.24 TECU), and the accuracy is the best among the four models. After the detection of TEC anomaly disturbance, we believe that the obvious errors in the three experimental grids in north america are related to hurricane ELSA.</p></div>","PeriodicalId":15096,"journal":{"name":"Journal of Atmospheric and Solar-Terrestrial Physics","volume":"262 ","pages":"Article 106309"},"PeriodicalIF":1.8000,"publicationDate":"2024-07-17","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":"{\"title\":\"Temporal convolutional network construction and analysis of single-station TEC model\",\"authors\":\"Daimian Hou, Fuzhen Liu, Hai Peng, Yanchao Gu, Guodong Tang\",\"doi\":\"10.1016/j.jastp.2024.106309\",\"DOIUrl\":null,\"url\":null,\"abstract\":\"<div><p>Ionosphere is one of the main error sources of global navigation satellite system (GNSS) precise positioning, and affecting communicate services such as communication, broadcasting, and radar positioning. Total electron content (TEC) is a key parameter to characterize the state of the ionosphere. Establishing a high-precision TEC model and making accurate predictions can effectively improve positioning accuracy and improve communication quality. The traditional TEC model has limited ability to describe the changes of TEC under extreme conditions such as magnetic storms. Based on the temporal convolution network (TCN) model, this paper conducts experiments on TEC grid data in six low latitude regions and six mid latitude regions, and compares them with Long short term memory (LSTM), gated recurrent units (GRU) and bidirectional long short term memory (BiLSTM) models. Results show that the mean average error (MAE) of TCN (1.2385 TECU) is lower in most areas compared with LSTM (1.2727 TECU), GRU (1.2602 TECU) and BiLSTM (1.2767 TECU). And the TCN model shows better performance in the mid latitude regions (0.8778 TECU) than low latitude regions (1.5992 TECU). Then, this paper takes 1st October to 31st December 2021. as an example to calculate the prediction accuracy of the TCN model in the magnetic quiet period and the magnetic storm period. During the sample time, there were 4 weak geomagnetic storms, 1 strong geomagnetic storm, and there was a continuous long magnetic resting period at the same time, with a variety of different geomagnetic activities. The results show that the MAE distribution of the TCN model is more concentrated in the magnetostatic period, and the model error in the mid latitude region is normally distributed between -4-4.5 TECU. During the magnetic storm period, the TCN model has the lowest proportion of errors exceeding 5 TECU, and the proportions in the mid latitude and low latitude regions are 2.8% and 10.4%, respectively, which are better than the comparison model. Finally, we discuss the performance of short-term TEC prediction and the possible causes of obvious errors. The accuracy of the TCN model reaches 1.07 TECU, which is better than the long-term prediction result (1.24 TECU), and the accuracy is the best among the four models. After the detection of TEC anomaly disturbance, we believe that the obvious errors in the three experimental grids in north america are related to hurricane ELSA.</p></div>\",\"PeriodicalId\":15096,\"journal\":{\"name\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"volume\":\"262 \",\"pages\":\"Article 106309\"},\"PeriodicalIF\":1.8000,\"publicationDate\":\"2024-07-17\",\"publicationTypes\":\"Journal Article\",\"fieldsOfStudy\":null,\"isOpenAccess\":false,\"openAccessPdf\":\"\",\"citationCount\":\"0\",\"resultStr\":null,\"platform\":\"Semanticscholar\",\"paperid\":null,\"PeriodicalName\":\"Journal of Atmospheric and Solar-Terrestrial Physics\",\"FirstCategoryId\":\"89\",\"ListUrlMain\":\"https://www.sciencedirect.com/science/article/pii/S1364682624001378\",\"RegionNum\":4,\"RegionCategory\":\"地球科学\",\"ArticlePicture\":[],\"TitleCN\":null,\"AbstractTextCN\":null,\"PMCID\":null,\"EPubDate\":\"\",\"PubModel\":\"\",\"JCR\":\"Q3\",\"JCRName\":\"GEOCHEMISTRY & GEOPHYSICS\",\"Score\":null,\"Total\":0}","platform":"Semanticscholar","paperid":null,"PeriodicalName":"Journal of Atmospheric and Solar-Terrestrial Physics","FirstCategoryId":"89","ListUrlMain":"https://www.sciencedirect.com/science/article/pii/S1364682624001378","RegionNum":4,"RegionCategory":"地球科学","ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"Q3","JCRName":"GEOCHEMISTRY & GEOPHYSICS","Score":null,"Total":0}
Temporal convolutional network construction and analysis of single-station TEC model
Ionosphere is one of the main error sources of global navigation satellite system (GNSS) precise positioning, and affecting communicate services such as communication, broadcasting, and radar positioning. Total electron content (TEC) is a key parameter to characterize the state of the ionosphere. Establishing a high-precision TEC model and making accurate predictions can effectively improve positioning accuracy and improve communication quality. The traditional TEC model has limited ability to describe the changes of TEC under extreme conditions such as magnetic storms. Based on the temporal convolution network (TCN) model, this paper conducts experiments on TEC grid data in six low latitude regions and six mid latitude regions, and compares them with Long short term memory (LSTM), gated recurrent units (GRU) and bidirectional long short term memory (BiLSTM) models. Results show that the mean average error (MAE) of TCN (1.2385 TECU) is lower in most areas compared with LSTM (1.2727 TECU), GRU (1.2602 TECU) and BiLSTM (1.2767 TECU). And the TCN model shows better performance in the mid latitude regions (0.8778 TECU) than low latitude regions (1.5992 TECU). Then, this paper takes 1st October to 31st December 2021. as an example to calculate the prediction accuracy of the TCN model in the magnetic quiet period and the magnetic storm period. During the sample time, there were 4 weak geomagnetic storms, 1 strong geomagnetic storm, and there was a continuous long magnetic resting period at the same time, with a variety of different geomagnetic activities. The results show that the MAE distribution of the TCN model is more concentrated in the magnetostatic period, and the model error in the mid latitude region is normally distributed between -4-4.5 TECU. During the magnetic storm period, the TCN model has the lowest proportion of errors exceeding 5 TECU, and the proportions in the mid latitude and low latitude regions are 2.8% and 10.4%, respectively, which are better than the comparison model. Finally, we discuss the performance of short-term TEC prediction and the possible causes of obvious errors. The accuracy of the TCN model reaches 1.07 TECU, which is better than the long-term prediction result (1.24 TECU), and the accuracy is the best among the four models. After the detection of TEC anomaly disturbance, we believe that the obvious errors in the three experimental grids in north america are related to hurricane ELSA.
期刊介绍:
The Journal of Atmospheric and Solar-Terrestrial Physics (JASTP) is an international journal concerned with the inter-disciplinary science of the Earth''s atmospheric and space environment, especially the highly varied and highly variable physical phenomena that occur in this natural laboratory and the processes that couple them.
The journal covers the physical processes operating in the troposphere, stratosphere, mesosphere, thermosphere, ionosphere, magnetosphere, the Sun, interplanetary medium, and heliosphere. Phenomena occurring in other "spheres", solar influences on climate, and supporting laboratory measurements are also considered. The journal deals especially with the coupling between the different regions.
Solar flares, coronal mass ejections, and other energetic events on the Sun create interesting and important perturbations in the near-Earth space environment. The physics of such "space weather" is central to the Journal of Atmospheric and Solar-Terrestrial Physics and the journal welcomes papers that lead in the direction of a predictive understanding of the coupled system. Regarding the upper atmosphere, the subjects of aeronomy, geomagnetism and geoelectricity, auroral phenomena, radio wave propagation, and plasma instabilities, are examples within the broad field of solar-terrestrial physics which emphasise the energy exchange between the solar wind, the magnetospheric and ionospheric plasmas, and the neutral gas. In the lower atmosphere, topics covered range from mesoscale to global scale dynamics, to atmospheric electricity, lightning and its effects, and to anthropogenic changes.