A solar flare is a relatively intense, localized emission of electromagnetic radiation in the Sun's atmosphere. Flares occur in active regions and are often, but not always, accompanied by coronal mas
Image artifacts (diffraction spikes and vertical streaks) appearing in a CCD image of a major solar flare due to the excess incident radiation
An X3.2-class solar flare observed in different wavelengths. Clockwise from top left: 304, 335, 131, and 193 Å
Electric currents in Earth's dayside ionosphere can be strengthened during a large solar flare.
Richard Carrington's sketch of the first recorded solar flare (A and B mark the initial bright points which moved over the course of five minutes to C and D before disappearing.)
Superflares are very strong explosions observed on stars with energies up to ten thousand times that of typical solar flares. The stars in this class satisfy conditions that should make them solar ana
Solar flare
…Sun in fiction Superflare NOAA Space Weather Prediction Center's near real-time solar flare data and resources: GOES X-Ray Flux (1-minute data) GOES Solar Ultraviolet Imager…
Artist's impression of a superflare from EV Lacertae