Flare Forecasting Algorithms Based on High-Gradient Polarity Inversion Lines in Active Regions
Domenico Cicogna, Francesco Berrilli, Daniele Calchetti, Dario Del, Moro, Luca Giovannelli, Federico Benvenuto, Cristina Campi, Sabrina, Guastavino, Michele Piana

TL;DR
This paper introduces new metrics, including a topological parameter D, for predicting solar flares from active regions, demonstrating their effectiveness through machine learning validation on high-resolution solar data.
Contribution
The study presents a novel topological parameter D and an improved R value computation method, enhancing flare prediction accuracy using machine learning.
Findings
Both parameters significantly improve flare prediction performance.
Parameter D is consistently among the top predictors across tests.
The new R value computation exploits higher spatial resolution data.
Abstract
Solar flares emanate from solar active regions hosting complex and strong bipolar magnetic fluxes. Estimating the probability of an active region to flare and defining reliable precursors of intense flares is an extremely challenging task in the space weather field. In this work, we focus on two metrics as flare precursors, the unsigned flux R, tested on MDI/SOHO data and one of the most used parameters for flare forecasting applications, and a novel topological parameter D representing the complexity of a solar active region. More in detail, we propose an algorithm for the computation of the R value which exploits the higher spatial resolution of HMI maps. This algorithm leads to a differently computed R value, whose functionality is tested on a set of cycle 24th solar flares. Furthermore, we introduce a topological parameter based on the automatic recognition of magnetic…
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