Longitudinal dependence of the forecast accuracy of the ionospheric total electron content in the equatorial zoneOAEI
Longitudinal dependence of the forecast accuracy of the ionospheric total electron content in the equatorial zone
The longitudinal dependence of the behavior of ionospheric parameters has been the subject of a number of works where significant variations are discovered.This also applies to the prediction of the iono-spheric total electron content(TEC),which neural network methods have recently been widely used.However,the results are mainly presented for a limited set of meridians.This paper examines the lon-gitudinal dependence of the TEC forecast accuracy in the equatorial zone.In this case,the methods are used that provided the best accuracy on three meridians:European(30° E),Southeastern(110° E)and American(75° W).Results for the stations considered are analyzed as a function of longitude using the Jet Propulsion Laboratory Global Ionosphere Map(JPL GIM)for 2015.These results are for 2 h ahead and 24 h ahead forecast.It was found that in this case,based on the metric values,three groups of archi-tectures can be distinguished.The first group included long short-term memory(LSTM),gated recurrent unit(GRU),and temporal convolutional networks(TCN)models as a part of unidirectional deep learning models;the second group is based on the recurrent models from the first group,which were supple-mented with a bidirectional algorithm,increasing the TEC forecasting accuracy by 2-3 times.The third group,which includes the bidirectional TCN architecture(BiTCN),provided the highest accuracy.For this architecture,according to data obtained for 9 equatorial stations,practical independence of the TEC prediction accuracy from longitude was observed under the following metrics(Mean Absolute Error MAE,Root Mean Square Error RMSE,Mean Absolute Percentage Error MAPE):MAE(2 h)is 0.2 TECU approximately;MAE(24 h)is 0.4 TECU approximately;RMSE(2 h)is less than 0.5 TECU except Niue station(RMSE(2 h)is 1 TECU approximately);RMSE(24 h)is in the range of 1.0-1.7 TECU;MAPE(2 h)<1%except Darwin station,MAPE(24 h)<2%.This result was confirmed by data from additional 5 stations that formed latitudinal chains in the equatorial part of the three meridians.The complete cor-respondence of the observational and predicted TEC values is illustrated using several stations for disturbed conditions on December 19-22,2015,which included the strongest magnetic storm in the second half of the year(min Dst=-155 nT).
Artem Kharakhashyan;Olga Maltseva
Institute for Physics,Southern Federal University,344090,Russia
IonosphereTotal electron contentForecastingBiGRUBiLSTMBiTCNTemporal convolution
《大地测量与地球动力学(英文版)》 2024 (005)
528-541 / 14
The authors are grateful to the developers of websites:http://omniweb.gsfc.nasa.gov/form/dx1.html,https://cddis.nasa.gov/archive/gnss/products/ionex/.The research was financially sup-ported by the Ministry of Science and Higher Education of the Russian Federation(State contract GZ0110/23-10-IF).
评论