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There is a page named "Solar prominences" on Wikipedia
- extremely hot plasma, prominences contain much cooler plasma, similar in composition to that of the chromosphere. Prominences form over timescales of...17 KB (1,885 words) - 08:42, 22 June 2024
- Several smaller prominences were also visible on the eastern limb, though because of the eclipse's relatively high magnitude, prominences on both limbs...74 KB (6,783 words) - 03:21, 24 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 (9,734 words) - 04:47, 23 June 2024
- and a prominence. Some prominences are so powerful that they eject matter at speeds ranging from 600 km/s to more than 1000 km/s. Other prominences form...48 KB (5,256 words) - 16:14, 12 June 2024
- Stellar corona (redirect from Solar corona)region of plasma populated by intermittent coronal structures known as solar prominences or filaments. The Sun's corona lies above the chromosphere and extends...62 KB (7,681 words) - 09:59, 26 May 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...169 KB (18,751 words) - 03:54, 24 June 2024
- its surface, which along with the internal process that leads to solar prominences, caused material to be ejected repeatedly from the sun. Due to the...2 KB (342 words) - 11:54, 30 November 2023
- emission nebulae and from features in the Sun's atmosphere, including solar prominences and the chromosphere. According to the Bohr model of the atom, electrons...7 KB (856 words) - 14:17, 7 April 2024
- of helium by both Pierre Janssen and Norman Lockyer, who observed Solar prominences with spectroscopes. Fritsch Bullock Rennoldson Herschel Tietjen Spörer...9 KB (918 words) - 10:18, 9 November 2023
- which the corona and prominences was visible. Other observers 1 to 5 miles away were clouded out. In San Blas, the corona and prominences were still visible...9 KB (1,020 words) - 02:10, 5 June 2024
- Retrieved 3 April 2015. "1185: The first description of solar prominences" (PDF). History of Solar Physics: A Time Line of Great Moments. 2015. Archived...14 KB (589 words) - 05:04, 12 June 2024
- Structure of the Sun Solar core Radiative zone Convection zone Photosphere Chromosphere Corona Solar granulation Sunspots Solar prominences Solar flares Physical...12 KB (1,048 words) - 18:37, 5 June 2024
- Eclipse (redirect from Solar and Lunar Eclipses)a bigger one. The term eclipse is most often used to describe either a solar eclipse, when the Moon's shadow crosses the Earth's surface, or a lunar...41 KB (4,657 words) - 12:01, 13 May 2024
- understood. Associated with solar flares are flare sprays. They involve faster ejections of material than eruptive prominences, and reach velocities of 20...42 KB (4,404 words) - 01:31, 22 June 2024
- 14th-century Laurentian Chronicle with the first detailed description of solar prominences. They were described as flame-like tongues of live embers: On the...17 KB (1,604 words) - 05:04, 14 April 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...47 KB (3,483 words) - 13:13, 19 June 2024
- Coronal mass ejection (category Solar phenomena)observed to support prominences, also known as filaments, composed of much cooler material than the surrounding coronal plasma. Prominences are embedded in...58 KB (6,845 words) - 21:51, 19 May 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...3 KB (282 words) - 17:17, 6 April 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...24 KB (2,873 words) - 10:43, 14 June 2024
- solar prominences plural of solar prominence
- Chromosphere and Solar Prominences by Charles Augustus Young 584670Popular Science Monthly Volume 4 February 1874 — The Chromosphere and Solar Prominences1874Charles
- outer atmosphere of the Sun much more rapidly. The study of the solar corona and prominences without eclipses (George Darwin Lecture) in Monthly Notices of
- timescales of about a day, and stable prominences may persist in the corona for several months. Some prominences break apart and give rise to coronal mass