Predicting Solar Energetic Particles Using SDO/HMI Vector Magnetic Data Products and a Bidirectional LSTM Network
Yasser Abduallah, Vania K. Jordanova, Hao Liu, Qin Li, Jason T. L., Wang, Haimin Wang

TL;DR
This paper introduces a bidirectional LSTM deep learning model that predicts solar energetic particle events based on solar magnetic data, flare, and CME associations, improving prediction accuracy over existing methods.
Contribution
The study develops a novel biLSTM model utilizing SDO/HMI magnetic data for SEP prediction, demonstrating superior performance compared to previous machine learning approaches.
Findings
biLSTM outperforms related algorithms in SEP prediction
Model effectively incorporates flare and CME data
Potential for probabilistic forecasting and calibration
Abstract
Solar energetic particles (SEPs) are an essential source of space radiation, which are hazards for humans in space, spacecraft, and technology in general. In this paper we propose a deep learning method, specifically a bidirectional long short-term memory (biLSTM) network, to predict if an active region (AR) would produce an SEP event given that (i) the AR will produce an M- or X-class flare and a coronal mass ejection (CME) associated with the flare, or (ii) the AR will produce an M- or X-class flare regardless of whether or not the flare is associated with a CME. The data samples used in this study are collected from the Geostationary Operational Environmental Satellite's X-ray flare catalogs provided by the National Centers for Environmental Information. We select M- and X-class flares with identified ARs in the catalogs for the period between 2010 and 2021, and find the associations…
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Taxonomy
MethodsSigmoid Activation · Tanh Activation · Long Short-Term Memory · Bidirectional LSTM
