An intense solar superstorm is currently underway, captivating millions worldwide with stunning auroras. The event began last night, and there are expectations for more auroras to grace the skies tonight. The remarkable geomagnetic storm has exceeded expectations, reaching extreme levels unseen in the past 20 years. The storm, fueled by powerful coronal mass ejections from the sun, has been described as a solar “superstorm,” rivaling the famous Halloween superstorm of November 2003.
Reports of auroras have poured in from various regions across the globe, starting from Europe and New Zealand and extending as far south as Mexico and as far north as Chile and Argentina in the Southern Hemisphere. While the peak activity may have passed, there is the possibility of further intensification as additional coronal mass ejections and high-speed solar winds are expected to impact Earth in the coming days. The recent X5.8 solar flare and the impending arrival of a coronal hole’s solar wind may prolong the superstorm activity.
Sun activity has remained very high, with a continuous stream of X flares and M flares being emitted. Active regions on the sun, particularly AR3664, have been prolific in producing flares, including the recent X5.8 flare. The increased solar activity has led to a severe geomagnetic storm, with Earth’s magnetic field currently experiencing significant disturbances.
Looking ahead, forecasts suggest a continuation of high flare activity, with a 99% chance of C flares, a 95% chance of M flares, and a 75% chance of X flares. The next expected coronal mass ejections associated with the recent X3.9 flare may arrive by May 12, potentially leading to further geomagnetic disturbances. Overall, the solar activity in recent days has been exceptional, with the sun displaying unprecedented levels of flare activity, captivating skywatchers and astronomers alike with its dazzling displays. Share your awe-inspiring sunspot and aurora photos with us, as we continue to marvel at the spectacle unfolding in the skies above.