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Loto’aniu, P., Rodriguez, J., Redmon, R., Machol, J., Kress, B., Seaton, D., Darnel, J., Rowland, W., Tilton, M., Denig, W., Boudouridis, A., Codrescu, S. and Claycomb, A. (2017) Space Weather Monitoring with GOES-16: Instruments and Data Products. Geophysical Research Abstracts, 19, 9663.

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• TITLE: The Dependence between Solar Flare Emergence and the Average Background Solar X-Ray Flux Emission

  AUTHORS: Yael Peleg, Rami Babayew, Itzhak Orion

  KEYWORDS: Space Weather, Solar Flare, Solar Activity, Sunspots, Solar Cycle

  JOURNAL NAME: International Journal of Astronomy and Astrophysics, Vol.14 No.3, July 30, 2024

  ABSTRACT: Solar flares, sudden bursts of intense electromagnetic radiation from the Sun, can significantly disrupt technological infrastructure, including communication and navigation satellites. To mitigate these risks, accurate forecasting of solar activity is crucial. This study investigates the potential of the Sun’s background X-ray flux as a tool for predicting solar flares. We analyzed data collected by solar telescopes and satellites between the years 2013 and 2023, focusing on the duration, frequency, and intensity of solar flares. We compared these characteristics with the background X-ray flux at the time of each flare event. Our analysis employed statistical methods to identify potential correlations between these solar phenomena. The key finding of this study reveals a significant positive correlation between solar flare activity and the Sun’s background X-ray flux. This suggests that these phenomena are interconnected within the framework of overall solar activity. We observed a clear trend: periods with increased occurrences of solar flares coincided with elevated background flux levels. This finding has the potential to improve solar activity forecasting. By monitoring background flux variations, we may be able to develop a more effective early warning system for potentially disruptive solar flares. This research contributes to a deeper understanding of the complex relationship between solar flares and the Sun’s overall radiative output. These findings indicate that lower-resolution X-ray sensors can be a valuable tool for identifying periods of increased solar activity by allowing us to monitor background flux variations. A more affordable approach to solar activity monitoring is advised.