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ORIGINAL RESEARCH article

Front. Astron. Space Sci.

Sec. Space Physics

Volume 12 - 2025 | doi: 10.3389/fspas.2025.1629056

This article is part of the Research TopicPredicting Near-Earth Space Environment: New Perspective and Capabilities in the AI AgeView all 4 articles

Modeling Ring Current Proton Distribution using MLP, CNN, LSTM, and Transformer Networks

Provisionally accepted
  • 1University of California, Los Angeles, Los Angeles, United States
  • 2University of California Riverside, Riverside, United States

The final, formatted version of the article will be published soon.

This study aims at developing ring current proton flux models using four neural network architectures: a multilayer perceptron (MLP), a convolutional neural network (CNN), a long short-term memory (LSTM) network, and a Transformer network. All models take time sequences of geomagnetic indices as inputs. Experimental results demonstrate that the LSTM and Transformer models consistently outperform the MLP and CNN models by achieving lower mean squared errors on the test set, possibly due to their intrinsic capability to process temporal sequential input data. Unlike MLP and CNN models, which require a fixed input history length even though proton lifetime varies with altitude, the LSTM and Transformer models accommodate variable-length sequences during both training and inference. Our findings indicate that the LSTM and Transformer architectures are well suited for modeling ring current proton behavior when GPU Deleted: s resources are available, and the Transformer slightly underperforms the LSTM model due to the restriction on the number of total heads. For resource-constrained environments, however, the MLP model offers a practical alternative, with faster training and inference times, while maintaining competitive accuracy.

Keywords: Ring current, magentospheric physics, MLP (multi layer perceptron), CNN - convolutional neural network, LSTM (Long Short Term Memory Networks), Transformer Neural Network, geomagenetic storm, proton

Received: 15 May 2025; Accepted: 09 Sep 2025.

Copyright: © 2025 Li, Bortnik, Wang and Wen. This is an open-access article distributed under the terms of the Creative Commons Attribution License (CC BY). The use, distribution or reproduction in other forums is permitted, provided the original author(s) or licensor are credited and that the original publication in this journal is cited, in accordance with accepted academic practice. No use, distribution or reproduction is permitted which does not comply with these terms.

* Correspondence: Jinxing Li, University of California, Los Angeles, Los Angeles, United States

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