Predicting Solar Proton Events of Solar Cycles 22-24 using GOES Proton & soft X-Ray flux features
Aatiya Ali, Viacheslav Sadykov, Alexander Kosovichev, Irina N., Kitiashvili, Vincent Oria, Gelu M. Nita, Egor Illarionov, Patrick M. O'Keefe,, Fraila Francis, Chun-Jie Chong, Paul Kosovich, Russell D. Marroquin

TL;DR
This study uses machine learning models, specifically XGBoost and SVM, on GOES satellite data to predict Solar Proton Events across solar cycles 22-24, highlighting the transferability challenges of models trained on different cycles.
Contribution
It introduces a comprehensive catalog of SPEs and flux data across multiple solar cycles and evaluates the cross-cycle transferability of ML-based SPE prediction models.
Findings
XGBoost outperforms SVM and operational forecasts in accuracy.
Transferability of models trained on one cycle to others is limited.
Long-term data validation is crucial for robust SEP forecasting.
Abstract
Solar Energetic Particle (SEP) events and their major subclass, Solar Proton Events (SPEs), can have unfavorable consequences on numerous aspects of life and technology, making them one of the most harmful effects of solar activity. Garnering knowledge preceding such events by studying operational data flows is essential for their forecasting. Considering only Solar Cycle (SC) 24 in our previous study, Sadykov et al. 2021, we found that it may be sufficient to utilize only proton and soft X-ray (SXR) parameters for SPE forecasts. Here, we report a catalog recording 10 MeV 10 particle flux unit SPEs with their properties, spanning SCs 22-24, using NOAA's Geostationary Operational Environmental Satellite flux data. We report an additional catalog of daily proton and SXR flux statistics for this period, employing it to test the application of machine learning (ML) on the…
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Taxonomy
TopicsSolar and Space Plasma Dynamics · Solar Radiation and Photovoltaics
