🌄 Last night's sky was a sight to behold! 🤩 If you missed it, check out these stunning photos, and thousands others circulating online. Usually observed in polar regions, auroras are caused by solar particles interacting with Earth's magnetic field. When solar eruptions occur… pic.twitter.com/uZ1WZd5Of3

Not much going on with the solar wind this afternoon to indicate we've had any recent significant solar storm arrivals. We'll check back in with ya later this evening. Meanwhile, please consider giving us a follow on Facebook, we sometimes do longer, more detailed posts over…

THOUGHTS ON AURORA VISIBILITY TONIGHT, MAY 11: Good evening. After last night's historic storm, the solar wind monitors are finally beginning to calm down this evening, the greatest indication of this being the total strength of the magnetic field, which has recently been around… pic.twitter.com/elm5UUNrEs

Current interplanetary and storm conditions: no Radio storm, S1 Radiation storm, and G3 Geomagnetic storm. The solar wind speed is still very high (almost 900 km/s!), but the magnetic field displays rather low magnitudes and the Bz component is still oscillating around the zero. pic.twitter.com/V0WSPC5HVw