Modeling the Dynamic Global Distribution of the Ring Current Oxygen Ions Using Artificial Neural Network Technique

被引:1
作者
Wang, Qiushuo [1 ]
Yue, Chao [1 ]
Li, Jinxing [2 ]
Bortnik, Jacob [2 ]
Ma, Donglai [2 ]
Jun, Chae-Woo [3 ]
机构
[1] Peking Univ, Inst Space Phys & Appl Technol, Beijing, Peoples R China
[2] Univ Calif Los Angeles, Dept Atmospher & Ocean Sci, Los Angeles, CA USA
[3] Nagoya Univ, Inst Space Earth Environm Res ISEE, Nagoya, Japan
来源
SPACE WEATHER-THE INTERNATIONAL JOURNAL OF RESEARCH AND APPLICATIONS | 2024年 / 22卷 / 06期
基金
中国国家自然科学基金;
关键词
ring current oxygen; machine learning; artificial neural network; INNER MAGNETOSPHERE; ISOTROPIC BOUNDARY; CURRENT SHEET; PLASMA SHEET; PRECIPITATION; SCATTERING; PROTONS;
D O I
10.1029/2023SW003779
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The ring current is an important component of the Earth's near-space environment, as its variations are the direct driver of geomagnetic storms that can disrupt power grids, satellite communications, and navigation systems, thereby impacting a wide range of technological and human activities. Oxygen ions (O+) are one of the major components of the ring current and play a significant role in both the enhancement and depletion of the ring current during geomagnetic storms. Although a standard statistical study can provide average global distributions of ring current ions, it can't offer insight into the short-term dynamic variations of the global distribution. Therefore, we employed the Artificial Neural Network technique to construct a global ring current O+ ion model based on the Van Allen Probes observations. Through optimization of the combination of input geomagnetic indices and their respective time history lengths, the model can well reproduce the spatiotemporal variation of the oxygen ion flux distributions and demonstrates remarkable accuracy and minimal errors. Additionally, the model effectively reconstructs the temporal variation of ring current O+ ions for non-training set data. Furthermore, the model provides a comprehensive and dynamic representation of global ring current O+ ion distribution. It accurately captures the dynamics of O+ ions during a geomagnetic storm with the oxygen ion fluxes enhancement and decay, and reveals distinct characteristics for different energy levels, such as injection from the plasma sheet, outflow from the ionosphere, and magnetic local time asymmetry. The ring current, a significant part of Earth's space environment, is closely linked to geomagnetic disturbances that can disrupt power grids, satellite communications, and navigation systems, affecting our daily lives. Oxygen ions (O+) are a key component of the ring current during geomagnetic active time. In our study, we use a powerful tool called Artificial Neural Networks to create a model for ring current O+ behavior. This model only requires F10.7 and geomagnetic indices as inputs. By carefully selecting the best combination of the geomagnetic indices and their time history, we built a model that can accurately mimic the behavior of oxygen ions observed by satellites. Our model demonstrates that the levels of O+ ion fluxes rise and fall at various locations during geomagnetic disturbance, which is consistent with previous observational trend. The model also helps us to understand the global distribution of O+ ions in real time. During a test case of a geomagnetic storm, the model revealed details about energy-dependent O+ ion flux enhancement and decay. An artificial neural network model was built to reconstruct ring current oxygen ions using geomagnetic indices as input The model shows high accuracy in predicting non-training set data and successfully captures the enhancement and decay of oxygen ion fluxes The model successfully reproduces the variation of global distribution for oxygen ions of different energies during geomagnetic storms
引用
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页数:14
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