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

Author:

Wang Qiushuo1,Yue Chao1ORCID,Li Jinxing2ORCID,Bortnik Jacob2ORCID,Ma Donglai2ORCID,Jun Chae‐Woo3ORCID

Affiliation:

1. Institute of Space Physics and Applied Technology Peking University Beijing China

2. Department of Atmospheric and Oceanic Sciences University of California, Los Angeles Los Angeles CA USA

3. Institute for Space‐Earth Environmental Research (ISEE) Nagoya University Nagoya Japan

Abstract

AbstractThe 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.

Funder

National Natural Science Foundation of China

Publisher

American Geophysical Union (AGU)

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