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Predicting the Loci of Solar Eruptions
2017
Proceedings of the International Astronomical Union
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AbstractThe longitudinal distribution of solar active regions shows non-homogeneous spatial behaviour, which is often referred to as Active Longitude (AL). Evidence for a significant statistical relationships between the AL and the longitudinal distribution of flare and coronal mass ejections (CME) occurrences is found in Gyenge et al. 2017 (ApJ, 838, 18). The present work forecasts the spatial position of AL, hence the most flare/CME capable active regions are also predictable. Our forecast
doi:10.1017/s1743921317008006
fatcat:au2qpez72rgarmcz5v7bhssivm