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A large transequatorial coronal hole opened on the Sun in mid-February 2026, sending high-speed solar wind streams directly toward Earth. This video explains how coronal holes differ from explosive solar eruptions, why this particular opening triggered G2-level geomagnetic storms, and what effects occurred during February 14-17, 2026. We explore the complete physics behind auroras, how solar wind interacts with Earth's magnetic field, and why space weather monitoring matters for satellite systems and power grids. By the end, you'll understand the Sun-Earth connection, what creates those northern lights visible across northern states, and what to expect as we continue through Solar Cycle 25's maximum phase. Based on NOAA space weather data and documented observations from the February 2026 event. Have you ever witnessed an aurora from your location? If you live in northern regions (above 45° latitude), we'd love to hear about your experience during this February 2026 event or any previous sightings. Share your observations in the comments below! 🌌 If you found this informative, like and subscribe for more in-depth explorations. #SpaceWeather #CoronalHole #Aurora #SolarScience #Astrophysics ⚠️ Disclaimer: The information included in this video originates from multiple publicly available sources and has been compiled for educational and informational use. While accuracy and relevance have been prioritized, certain interpretations or analyses may differ as new data becomes available. The imagery and visuals displayed throughout this video have been created using artificial intelligence for representation purposes only.