Temporal convolutional network construction and analysis of single-station TEC model

IF 1.8 4区 地球科学 Q3 GEOCHEMISTRY & GEOPHYSICS
Daimian Hou, Fuzhen Liu, Hai Peng, Yanchao Gu, Guodong Tang
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引用次数: 0

Abstract

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.

单站 TEC 模型的时序卷积网络构建与分析
电离层是全球导航卫星系统(GNSS)精确定位的主要误差源之一,并影响通信、广播和雷达定位等通信服务。电子总含量(TEC)是描述电离层状态的一个关键参数。建立高精度的 TEC 模型并进行准确预测可有效提高定位精度,改善通信质量。传统的 TEC 模型对磁暴等极端条件下的 TEC 变化描述能力有限。本文基于时间卷积网络(TCN)模型,对六个低纬度地区和六个中纬度地区的 TEC 电网数据进行了实验,并与长短期记忆(LSTM)、门控递归单元(GRU)和双向长短期记忆(BiLSTM)模型进行了比较。结果表明,与 LSTM(1.2727 TECU)、GRU(1.2602 TECU)和 BiLSTM(1.2767 TECU)相比,TCN(1.2385 TECU)在大多数区域的平均误差(MAE)较低。而 TCN 模型在中纬度地区(0.8778 TECU)的表现优于低纬度地区(1.5992 TECU)。然后,本文以 2021 年 10 月 1 日至 12 月 31 日为例,计算 TCN 模式在磁静止期和磁暴期的预测精度。在样本时间内,共发生了 4 次弱地磁暴、1 次强地磁暴,同时还存在连续较长的磁静止期,地磁活动多种多样。结果表明,TCN 模式的 MAE 分布在磁静止期较为集中,中纬度地区的模式误差在-4-4.5 TECU 之间呈正态分布。在磁暴期,TCN 模式误差超过 5 TECU 的比例最低,在中纬度和低纬度区域的比例分别为 2.8%和 10.4%,优于对比模式。最后,我们讨论了短期 TEC 预测的性能以及造成明显误差的可能原因。TCN模型的精度达到1.07 TECU,优于长期预测结果(1.24 TECU),精度是四个模型中最好的。经过对 TEC 异常扰动的检测,我们认为北美三个试验网格的明显误差与飓风 ELSA 有关。
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来源期刊
Journal of Atmospheric and Solar-Terrestrial Physics
Journal of Atmospheric and Solar-Terrestrial Physics 地学-地球化学与地球物理
CiteScore
4.10
自引率
5.30%
发文量
95
审稿时长
6 months
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.
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