Solar flares are huge explosions on the Sun. A flare appears as a sudden, intense brightening of a region on the Sun, typically lasting several minutes.
Flares occur when intense magnetic fields on the Sun become too tangled. Like a rubber band that snaps when it is twisted too far, the tangled magnetic fields release energy when they “snap”. Solar flares emit huge bursts of electromagnetic radiation, including X-rays, ultraviolet radiation, visible light, and radio waves. The energy emitted by a solar flare is more than a million times greater than the energy from a volcanic explosion on Earth!
Although solar flares can be visible in white light, they are often more readily noticed via their bright X-ray and ultraviolet emissions. Coronal mass ejections often accompany solar flares, though scientists are still trying to determine exactly how the two phenomena are related. Solar flares burst forth from the intense magnetic fields in the vicinity of active regions on the Sun. Solar flares are most common during times of peak solar activity, the “solar max” years of the sunspot cycle.