EP1 ยท Space & Solar Storms
Flares, ejections and the geomagnetic response at Earth across the observed window, with the solar cycle and the great historical storms for scale.
Alert me when
A solar flare is a flash of X-rays from the Sun's surface, sorted into classes A, B, C, M and X, where each letter is ten times the last and the number is the strength within it. The X-rays arrive in eight minutes and disturb radio and GPS on the daylight side, but they do not cause storms on the ground.
When a CME sweeps past, it shakes Earth's magnetic field. The planetary Kp index measures that shaking every three hours on a 0 to 9 scale, and NOAA maps Kp onto the G storm scale: Kp 5 is a G1, Kp 6 a G2, up to Kp 9 for a G5. This window peaked at Kp 6.3, a G2.
A moving magnetic field induces electric currents in long conductors: power lines, pipelines and rail. These geomagnetically induced currents are the mechanism by which a storm in space becomes a problem on the ground, pushing grid transformers towards saturation and, in a severe storm, towards damage. That is how a CME becomes a grid operator's problem rather than an astronomer's.
Space weather is the one natural peril with no geography. A Carrington-class storm does not strike a country; it couples into the whole sunlit and night side at once, so exposures that are normally uncorrelated fail together.