Performance of solar far-side active regions neural detection
E. G. Broock, T. Felipe, A. Asensio Ramos

TL;DR
This study evaluates a neural network's ability to detect far-side solar active regions using helioseismic data, demonstrating improved sensitivity and detection rates over traditional methods, confirmed by EUV observations.
Contribution
The paper introduces and validates a neural network approach that enhances the detection sensitivity of far-side solar active regions compared to standard seismic methods.
Findings
Neural network shows 47% more true detections at similar false positive rates.
Approximately 96% of standard method detections correspond to EUV active regions.
Neural network can detect weaker active regions by adjusting detection thresholds.
Abstract
Context. Far-side helioseismology is a technique used to infer the presence of active regions in the far hemisphere of the Sun based on the interpretation of oscillations measured in the near hemisphere. A neural network has been recently developed to improve the sensitivity of the seismic maps to the presence of far-side active regions. Aims. Our aim is to evaluate the performance of the new neural network approach and to thoroughly compare it with the standard method commonly applied to predict far-side active regions from seismic measurements. Methods. We have computed the predictions of active regions using the neural network and the standard approach from five years of far-side seismic maps as a function of the selected threshold in the signatures of the detections. The results have been compared with direct extreme ultraviolet observations of the far hemisphere acquired with the…
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