Geomagnetic Storms Auroras Solar Activity Coronal Mass Ejections Solar Storms Aurora Borealis Solar Flares Solar Wind Geomagnetic Storm Geomagnetic Activity Solar Phenomena Geomagnetic Phenomena Magnetic Storms Effects on Earth Impact on Earth Coronal Mass Ejection Magnetosphere NOAA Effects on Technology Northern Lights Radio Blackouts Geomagnetic Disturbances Effects on Planets Solar Cycle Solar Physicist Prediction Center Space Weather Prediction Center Solar Eruption Solar Emissions Radio Disruptions Prediction Solar System Data Collection Magnetic Fields Forecasting Forecasting Challenges Satellites Solar Observation NOAA Reports Data Analysis Geomagnetism Cosmic Particles Energetic Particles Impact on Technology Magnetic Activity Communication Disruptions Solar Energetic Particles NOAA SWPC Aurora Forecast Aurora Viewing Radio Bursts Solar Cycles Expertise Space Weather Monitoring Interplanetary Shocks Solar Events Satellite Operations Cosmic Radiation NOAA Predictions Solar Corona Space Weather Prediction Coronagraphs Space Travel Ionosphere Monitoring Solar Observations Satellite Development Northern Lights Display
A coronal mass ejection interacting with a fast solar‑wind stream could push auroras south, with visibility dependent on real‑time conditions.
