In solar physics, a prominence, sometimes referred to as a filament, is a large plasma and magnetic field structure extending outward from the Sun's surface...

frequent flares. Other forms of solar activity frequently associated with coronal mass ejections are eruptive prominences, coronal dimming, coronal waves...

corona will be visible, and the chromosphere, solar prominences, coronal streamers and possibly even a solar flare may be seen. At the end of totality, the...

Sun's corona and solar prominences to be seen. Totality occurs only in a limited path across Earth's surface, with the partial solar eclipse visible over...

disturbance in the solar wind Solar cycle, an 11-year cycle of sunspot activity Solar cycle 25, the current cycle Solar prominence, a plasma and magnetic...

The solar storms of May 2024 were a series of powerful solar storms with extreme solar flares and geomagnetic storm components that occurred from 10–13...

ejections, solar particle events, and other eruptive solar phenomena. The occurrence of solar flares varies with the 11-year solar cycle. Solar flares are...

In topography, prominence or relative height (also referred to as autonomous height, and shoulder drop in US English, and drop in British English) measures...

a zone of energetic charged particles, most of which originate from the solar wind, that are captured by and held around a planet by that planet's magnetosphere...

gauss (0.001–0.01 T) in solar prominences. The magnetic field varies in time and location. The quasi-periodic 11-year solar cycle is the most prominent...