Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters
文献类型:期刊论文
作者 | Wang, Jianhang1; Guo, Deyu1; Xiang, Zheng1,2; Ni, Binbin1; Liu, Yangxizi1; Dong, Junhu1 |
刊名 | ADVANCES IN SPACE RESEARCH |
出版日期 | 2023 |
卷号 | 71期号:1页码:275-285 |
ISSN号 | 0273-1177 |
关键词 | Flux prediction Artificial neural network Geosynchronous orbit Solar wind parameters |
DOI | 10.1016/j.asr.2022.10.013 |
英文摘要 | There are hundreds of satellites operating at the geosynchronous (GEO) orbit where relativistic electrons can cause severe damage. Thus, predicting relativistic electron fluxes is significant for spacecraft safety. In this study, using GOES satellite data during 2011-2020, we propose two neural network models with two hidden layers to predict geosynchronous relativistic electron fluxes at two energy chan-nels (>0.8 MeV and > 2 MeV). The number of input neurons of the two channels (>0.8 MeV and > 2 MeV) are determined to be 36 and 44, respectively. The > 0.8 MeV model has 22 and 9 neurons in the hidden layers, while the > 2 MeV model has 25 and 15 neurons in the hidden layers. The input parameters include the north-south component of the interplanetary magnetic field, solar wind speed, solar wind dynamic pressure and solar wind proton density. Through the analysis of different time delays, we determine that the optimal time delays of two energy channels (>0.8 MeV and > 2 MeV) are 8 days and 10 days, respectively. The training set and validation set (Jan 2011-Dec 2018) are divided by the 10-fold cross-validation method, and the remaining data (Jan 2019-Feb 2020) is used to analyze the model performance as a test set. The prediction results of both energy channels show good agreement with satellite observations indi-cated by low RMSE (-0.3 cm-2sr-1s-1), high PE (-0.8) and CC (-0.9). These results suggest that only using solar wind parameters is capable of obtaining reasonable predictions of geosynchronous relativistic electron fluxes.(c) 2022 COSPAR. Published by Elsevier B.V. All rights reserved. |
WOS关键词 | RADIATION BELT ELECTRONS ; GEOSTATIONARY ORBIT ; MAGNETOSPHERIC PLASMA ; MODEL ; MECHANISMS ; DROPOUTS ; POINT ; WAVES |
资助项目 | National Natural Science Foundation of China[42188101] ; National Natural Science Foundation of China[42174190] ; National Natural Science Foundation of China[42025404] ; National Natural Science Foundation of China[41904143] ; China National Space Administration[D020308] ; China National Space Administration[D020104] ; Fundamental Research Funds for the Central Universities[2042021kf0016] ; B-type Strategic Priority Program of the Chinese Academy of Sciences[XDB41000000] ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences[DQXX2021-04] ; China Postdoctoral Science Foundation Project[2019M662700] |
WOS研究方向 | Engineering ; Astronomy & Astrophysics ; Geology ; Meteorology & Atmospheric Sciences |
语种 | 英语 |
出版者 | ELSEVIER SCI LTD |
WOS记录号 | WOS:000913077100001 |
资助机构 | National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration ; China National Space Administration ; China National Space Administration ; China National Space Administration ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration ; China National Space Administration ; China National Space Administration ; China National Space Administration ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration ; China National Space Administration ; China National Space Administration ; China National Space Administration ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; National Natural Science Foundation of China ; China National Space Administration ; China National Space Administration ; China National Space Administration ; China National Space Administration ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; Fundamental Research Funds for the Central Universities ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; B-type Strategic Priority Program of the Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; open project of Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project ; China Postdoctoral Science Foundation Project |
源URL | [http://ir.iggcas.ac.cn/handle/132A11/106854] |
专题 | 地质与地球物理研究所_中国科学院地球与行星物理重点实验室 |
通讯作者 | Xiang, Zheng |
作者单位 | 1.Wuhan Univ, Sch Elect Informat, Dept Space Phys, Wuhan, Hubei, Peoples R China 2.Chinese Acad Sci, Inst Geol & Geophys, Key Lab Earth & Planetary Phys, Beijing, Peoples R China |
推荐引用方式 GB/T 7714 | Wang, Jianhang,Guo, Deyu,Xiang, Zheng,et al. Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters[J]. ADVANCES IN SPACE RESEARCH,2023,71(1):275-285. |
APA | Wang, Jianhang,Guo, Deyu,Xiang, Zheng,Ni, Binbin,Liu, Yangxizi,&Dong, Junhu.(2023).Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters.ADVANCES IN SPACE RESEARCH,71(1),275-285. |
MLA | Wang, Jianhang,et al."Prediction of geosynchronous electron fluxes using an artificial neural network driven by solar wind parameters".ADVANCES IN SPACE RESEARCH 71.1(2023):275-285. |
入库方式: OAI收割
来源:地质与地球物理研究所
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