Abstract

X-rays emitted by the Sun can damage electronic devices of spaceships, satellites, positioning systems and electricity distribution grids. Thus, the forecasting of solar X-rays is needed to warn organizations and mitigate undesirable effects. Traditional mining classification methods categorize observations into labels, and we aim to extend this approach to predict future X-ray levels. Therefore, we developed the “SeMiner” method, which allows the prediction of future events. “SeMiner” processes X-rays into sequences employing a new algorithm called “Series-to-Sequence” (SS). It employs a sliding window approach configured by a specialist. Then, the sequences are submitted to a classifier to generate a model that predicts X-ray levels. An optimized version of “SS” was also developed using parallelization techniques and Graphical Processing Units, in order to speed up the entire forecasting process. The obtained results indicate that “SeMiner” is well-suited to predict solar X-rays and solar flares within the defined time range. It reached more than 90% of accuracy for a 2-day forecast, and more than 80% of True Positive (TPR) and True Negative (TNR) rates predicting X-ray levels. It also reached an accuracy of 72.7%, with a TPR of 70.9% and TNR of 79.7% when predicting solar flares. Moreover, the optimized version of “SS” proved to be 4.36 faster than its initial version.

Highlights

  • Solar Flares are sudden releases of large amounts of energy (1025 –1032 erg) from the active regions of the solar atmosphere

  • Rate was 86.5%, using the IBK classifier. These results show a strong balance between True Positive (TP) and True Negative (TN) rates, a desirable feature considering that the solar data relevant to this task is very imbalanced

  • This work has been developed in the context of sun X-Ray flux emissions, and solar flare predictions

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Summary

Introduction

Solar Flares are sudden releases of large amounts of energy (1025 –1032 erg) from the active regions of the solar atmosphere. These phenomena can last from tens of seconds up to a few hours, depending on the intensity, emitting a broad spectrum of electromagnetic radio waves radio, such as X-rays or even gamma-rays. Solar Flares impact High Frequency (HF) and Very High Frequency (VHF) radio communications because of the X-ray influence on HF/VHF paths inside the ionosphere [1,2]. Solar flares and their high X-rays emissions can impact the Global Positioning System (GPS), and electricity power

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