Predicting Major Solar Flares Using Convolutional Neural Networks and Multivariate Magnetic Field Time-Series Data

Abstract Predicting major solar flares, which pose significant risks to both space-based and terrestrial infrastructure, remains a critical challenge in space-weather research. In this paper, we propose a novel Convolutional Neural Network (CNN)-based framework that includes both a data preprocessing pipeline and a predictive model named $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> , designed to leverage Multivariate Time-Series (MVTS) data of solar magnetic field parameters to forecast flare events. Our framework is developed using a MVTS benchmark dataset SWAN-SF, which includes about 4100 Active Region (AR) sequences with 24 magnetic-field parameters sampled at 12-minute intervals. However, this dataset is characterized by over 10 million missing values, severe class imbalance, and strong temporal dependencies arising from its sliding-window construction. To address these challenges, we propose a new data preprocessing pipeline that incorporates an improved data-splitting strategy, designed to mitigate the scarcity and imbalance of major flares while preserving temporal independence between training and test sets. Experimental results show that, for predicting M-class or greater solar flares within 12 hours using SHARP magnetic-field data from 2010 – 2018, $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> achieves the highest overall True Skill Statistics (TSS) score of 0.86, outperforming eight existing MVTS-based approaches and three ablated variants of $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> . These findings demonstrate the effectiveness of our method in improving solar flare prediction and advancing space-weather forecasting.

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Publication Details

Journal
Solar Physics
Published
2026-02-01
DOI
https://doi.org/10.1007/s11207-026-02612-6
Primary Topic
Solar and Space Plasma Dynamics
Type
article
Field-Weighted Citation Impact
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article

Predicting Major Solar Flares Using Convolutional Neural Networks and Multivariate Magnetic Field Time-Series Data

Soheila Farokhi, Arash Azizian Foumani, Xiaojun Qi
Solar Physics
Solar and Space Plasma Dynamics
article

Predicting Major Solar Flares Using Convolutional Neural Networks and Multivariate Magnetic Field Time-Series Data

Soheila Farokhi, Arash Azizian Foumani, Xiaojun Qi
article en

Abstract

Abstract Predicting major solar flares, which pose significant risks to both space-based and terrestrial infrastructure, remains a critical challenge in space-weather research. In this paper, we propose a novel Convolutional Neural Network (CNN)-based framework that includes both a data preprocessing pipeline and a predictive model named $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> , designed to leverage Multivariate Time-Series (MVTS) data of solar magnetic field parameters to forecast flare events. Our framework is developed using a MVTS benchmark dataset SWAN-SF, which includes about 4100 Active Region (AR) sequences with 24 magnetic-field parameters sampled at 12-minute intervals. However, this dataset is characterized by over 10 million missing values, severe class imbalance, and strong temporal dependencies arising from its sliding-window construction. To address these challenges, we propose a new data preprocessing pipeline that incorporates an improved data-splitting strategy, designed to mitigate the scarcity and imbalance of major flares while preserving temporal independence between training and test sets. Experimental results show that, for predicting M-class or greater solar flares within 12 hours using SHARP magnetic-field data from 2010 – 2018, $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> achieves the highest overall True Skill Statistics (TSS) score of 0.86, outperforming eight existing MVTS-based approaches and three ablated variants of $Cmod$ <mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML"> <mml:mi>C</mml:mi> <mml:mi>m</mml:mi> <mml:mi>o</mml:mi> <mml:mi>d</mml:mi> </mml:math> . These findings demonstrate the effectiveness of our method in improving solar flare prediction and advancing space-weather forecasting.

Solar PhysicsVol. 301(2)
Utah State University (US)
Industry, innovation and infrastructure
Openalex Percentile: Top 66%
Solar and Space Plasma Dynamics
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