Automated Classification of Auroral Images with Deep Neural Networks

Author:

Shang Zhiyuan12,Yao Zhonghua12,Liu Jian34ORCID,Xu Linli56,Xu Yan12,Zhang Binzheng789,Guo Ruilong1011ORCID,Wei Yong12

Affiliation:

1. Key Laboratory of Earth and Planetary Physics, Institute of Geology and Geophysics, Chinese Academy of Sciences, Beijing 100000, China

2. College of Earth and Planetary Sciences, University of Chinese Academy of Sciences, Beijing 100000, China

3. School of Nuclear Science and Technology, University of Science and Technology of China, Hefei 230026, China

4. Advanced Algorithm Joint Lab, Shandong Computer Science Center, Qilu University of Technology, Jinan 250014, China

5. Anhui Province Key Laboratory of Big Data Analysis and Application, School of Computer Science and Technology, University of Science and Technology of China, Hefei 230026, China

6. Anhui Province Key Laboratory of Big Data Analysis and Application, School of Computer Science and Technology, University of Science and Technology of China, State Key Laboratory of Cognitive Intelligence, Hefei 230026, China

7. Department of Earth Sciences, The University of Hong Kong, Hong Kong SAR, China

8. Laboratory for Space Research, The University of Hong Kong, Hong Kong SAR, China

9. High Altitude Observatory, National Center for Atmospheric Research, Boulder, CO 80301, USA

10. Laboratory of Optical Astronomy and Solar-Terrestrial Environment, Institute of Space Sciences, School of Space Science and Physics, Shandong University, Weihai 264200, China

11. Laboratory for Planetary and Atmospheric Physics, STAR Institute, Université de Liège, Liège 4000-4032, Belgium

Abstract

Terrestrial auroras are highly structured that visualize the perturbations of energetic particles and electromagnetic fields in Earth’s space environments. However, the identification of auroral morphologies is often subjective, which results in confusion in the community. Automated tools are highly valuable in the classification of auroral structures. Both CNNs (convolutional neural networks) and transformer models based on the self-attention mechanism in deep learning are capable of extracting features from images. In this study, we applied multiple algorithms in the classification of auroral structures and performed a comparison on their performances. Trans-former and ConvNeXt models were firstly used in the analysis of auroras in this study. The results show that the ConvNeXt model can have the highest accuracy of 98.5% among all of the applied algorithms. This study provides a direct comparison of deep learning tools on the application of classifying auroral structures and shows promising capability, clearly demonstrating that auto-mated tools can help to minimize the bias in future auroral studies.

Funder

The National Science Foundation of China

Key Research Program of the Institute of Geology & Geophysics CAS

Publisher

MDPI AG

Subject

General Physics and Astronomy

Reference32 articles.

1. The development of the auroral substorm;Akasofu;Planet. Space Sci.,1964

2. Magnetospheric impulse response for many levels of geomagnetic activity;Bargatze;J. Geophys. Res. Space Phys.,1985

3. Polar views of the Earth’s aurora with Dynamics Explorer;Frank;Geophysical Res. Lett.,1982

4. Satellite studies of magnetospheric substorms on August 15, 1968: 4. Ogo 5 magnetic field observations;McPherron;J. Geophys. Res. Atmos.,1973

5. Syrjäsuo, M., and Pulkkinen, T. (1999, January 27–29). Determining the skeletons of the auroras. Proceedings of the 10th International Conference on Image Analysis and Processing, Washington, DC, USA.

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