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...
17 KB (1,885 words) - 08:42, 22 June 2024
frequent flares. Other forms of solar activity frequently associated with coronal mass ejections are eruptive prominences, coronal dimming, coronal waves...
48 KB (5,256 words) - 16:14, 12 June 2024
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...
84 KB (9,738 words) - 23:58, 20 August 2024
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...
78 KB (7,066 words) - 06:27, 15 August 2024
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...
2 KB (276 words) - 17:25, 30 June 2024
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...
48 KB (3,570 words) - 12:50, 22 August 2024
ejections, solar particle events, and other eruptive solar phenomena. The occurrence of solar flares varies with the 11-year solar cycle. Solar flares are...
49 KB (5,229 words) - 18:40, 15 August 2024
In topography, prominence or relative height (also referred to as autonomous height, and shoulder drop in US English, and drop in British English) measures...
27 KB (3,189 words) - 02:36, 7 August 2024
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...
38 KB (4,485 words) - 22:15, 9 August 2024
Sun (redirect from Solar diameter)
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...
178 KB (20,212 words) - 22:22, 22 August 2024