Solar Flare Index Prediction Using SDO/HMI Vector Magnetic Data Products with Statistical and Machine Learning Methods
Hewei Zhang, Qin Li, Yanxing Yang, Ju Jing, Jason T.L. Wang, Haimin, Wang, Zuofeng Shang

TL;DR
This study employs statistical and machine learning techniques to predict solar flare activity, specifically the Flare Index, using magnetic data from SDO/HMI, achieving improved accuracy over existing methods for forecasting space weather hazards.
Contribution
Introduces novel machine learning approaches and a comprehensive analysis of SHARP magnetic parameters for accurate 1-day ahead solar flare prediction.
Findings
Machine learning methods outperform traditional models in FI prediction.
SHARP parameters' importance varies, with some being more predictive.
Prediction accuracy improves notably for high FI values.
Abstract
Solar flares, especially the M- and X-class flares, are often associated with coronal mass ejections (CMEs). They are the most important sources of space weather effects, that can severely impact the near-Earth environment. Thus it is essential to forecast flares (especially the M-and X-class ones) to mitigate their destructive and hazardous consequences. Here, we introduce several statistical and Machine Learning approaches to the prediction of the AR's Flare Index (FI) that quantifies the flare productivity of an AR by taking into account the numbers of different class flares within a certain time interval. Specifically, our sample includes 563 ARs appeared on solar disk from May 2010 to Dec 2017. The 25 magnetic parameters, provided by the Space-weather HMI Active Region Patches (SHARP) from Helioseismic and Magnetic Imager (HMI) on board the Solar Dynamics Observatory (SDO),…
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Taxonomy
TopicsSolar and Space Plasma Dynamics
