Cosmic-Ray-Constrained LSTM Model for Geomagnetic Storm Prediction
Zongyuan Ge, Chenwaner Zhang, Wei Zhou, Hongyu Zeng, Guiping Zhou

TL;DR
This paper introduces a physics-informed LSTM model that uses cosmic-ray flux data as a precursor to improve geomagnetic storm predictions, achieving better accuracy and longer warning times.
Contribution
It is the first to incorporate cosmic-ray flux modulation into an LSTM model for geomagnetic storm prediction, enhancing forecast skill with multi-source space-weather data.
Findings
Cosmic-ray data improves 48-hour forecast accuracy by up to 25.84%.
The model achieves RMSEs of 5.106 nT to 14.788 nT across 2- to 48-hour predictions.
Multi-source data integration enhances space-weather forecasting capabilities.
Abstract
Geomagnetic storms (GSTs) driven by solar wind-magnetosphere coupling can severely disrupt technological systems, motivating the need for improved prediction accuracy and longer warning times. In this study, we develop a physics-informed Long Short-Term Memory (LSTM) model that incorporates cosmic-ray flux modulation as an additional precursor signal. As coronal mass ejection (CME)-driven disturbances propagate through the heliosphere, enhanced turbulence and magnetic-field compression reduce galactic cosmic-ray (GCR) flux measured by ground-based neutron monitors (Forbush decreases), providing early information that can precede near-Earth solar-wind signatures by 1--3 days. We integrate multi-source space-weather data, spanning 1995-2020, including cosmic-ray observations, solar wind plasma parameters, interplanetary magnetic-field data, and geomagnetic indices. Based on these data, we…
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Taxonomy
TopicsIonosphere and magnetosphere dynamics · Solar and Space Plasma Dynamics · Earthquake Detection and Analysis
