Related Category: Astronomy: General
More on Prominences
Chromosphere - (kr´msfr´´) [Gr.
at HighBeam Research
Pictures from Google Image Search ...
Definition: prominence: A strand of relatively cool gas in the solar corona which appears bright when seen at the edge of the Sun against the blackness of space.
Space Tragedies9 Planets in Nine DaysAstronomy 101
Related Articles ...
You can see the form, rise up, and then erupt away into space over the course of one day, on October 6-7, 2012. Sometimes this material rains back down to the surface, and sometimes it escapes entirely.
A prominence is a large bright feature extending outward from the Sun's surface, often in a loop configuration. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the Sun's corona.
An arched lifts off from the Sun, propelled by magnetic forces. This image was taken by the Skylab Space Station. It shows the Sun in ultraviolet light.
Return to the StarChild Main Page ...
A prominence is made up of relatively cold, dense plasma supported by the local magnetic field from falling back into the sun. They can survive like this for 200 days. The temperature of the plasma in a prominence is about 5000 K.
A solar (also known as a filament) is an arc of gas that erupts from the surface of the Sun. s can loop hundreds of thousands of miles into space.
Prominences are dense clouds of material suspended above the surface of the Sun by loops of magnetic field.
is a structure in the Sun's corona consisting of cool plasma supported by magnetic fields. s are bright structures when seen over the solar limb, but appear dark when seen against the bright solar disk.
prominence Loop or sheet of glowing gas ejected from an active region on the solar surface, which then moves through the inner parts of the corona under the influence of the Sun's magnetic field.
: Complex structures of relatively cool, dense solar material that extend into the outer chromosphere and inner corona. They are generally static and believed to be supported by magnetic forces.
prominence -- a large-scale gaseous formation above the surface of the Sun.
. A term identifying cloud-like features in the solar atmosphere. The features appear as bright structures in the corona above the solar limb and as dark filaments when seen projected against the solar disk.
Prominence, solar- a loop of cooler gas seen above the sun's surface, which sometimes erupts outwards into space
Proton- a positively charged particle that forms part of the nucleus of an atom ...
- Structure that occurs above the photosphere of the Sun. s may reach high into the corona, often as graceful loops that may hang suspended for many days.
A looping column of gas ejected from the surface of the Sun.
The initial stage of planetary formation. A protoplanet is a small clump of material that may accumulate material to become a planet.
Eruptions of the solar surface. Visible during total solar eclipses.
Proper Motion ...
an explosion of hot gas that erupts from the Sun's surface. Solar prominences are usually associated with sunspot activity and can cause interference with communications on Earth due to their electromagnetic effects on the atmosphere.
s. A mass of glowing gas, mainly hydrogen, that rises from the surface of the Sun.
Proper motion. The movement of an individual star on the celestial sphere.
A feature of the lower part of the solar corona which when observed in the red line of hydrogen at 653nm (Ha), look like flames leaping up from the surface of the Sun.
- A region of cool gas embedded in the corona. s are bright when seen above the Sun's limb, but appear as dark filaments when seen against the Sun's disk ...
Prominence A cloud of cooler plasma extending high above the Sun"s visible surface, rising above the photosphere into the corona.
A region of cool (104 K), high-density gas embedded in the hot (106 K), low-density Solar corona. s are the flamelike tongues of gas that appear above the limb of the Sun.
Rise to prominence
Alcibiades first rose to prominence when he began advocating aggressive Athenian action after the signing of the Peace of Nicias
Peace of Nicias ...
An eruption of gas from the chromosphere of a star. Solar s are visible as part of the corona during a total solar eclipse.
Cloud of gas elevated above the solar surface.
The apparent drift of a star across the sky, compounded from the motion of the star and the sun.
Solar gas protruding over the limb, visible to the naked eye only at eclipses but also observed outside of eclipses by its emission line spectrum. s are at approximately the same temperature as the chromosphere.
A prominence beginning to erupt on the Sun's limb, caused by a cascade of rippling Alfven waves sparked by small-scale flares. Image: NASA/SDO/AIA.
A seen in projection on the Solar disk. [H76]
An instrument used with a telescope for visually measuring small angular separations (as between binary stars). [H76]
Fine Structure ...
This image was acquired from NASA's Skylab space station on December 19, 1973. It shows one of the most spectacular solar flares ever recorded, propelled by magnetic forces, lifting off from the Sun.
A solar as seen by SOHO. Image credit: Solar and Heliospheric Observatory (SOHO). SOHO is a project of international cooperation between ESA and NASA.
A solar prominence is an arc of gas that erupts from the surface of the . Prominences can loop hundreds of thousands of miles into space and can last for many months.
Finally, solar s rise up through the chromosphere from the photosphere, sometimes reaching altitudes of 150,000 kilometers. These gigantic plumes of gas are the most spectacular of solar phenomena, aside from the less frequent solar flares.
prominence A filamentlike protuberance from the chromosphere of the sun. See flocculi. Compare flare.
ACTIVE A displaying material motion and changes in appearance over a few minutes of time. ACTIVE REGION (AR) A localized, transient volume of the solar atmosphere in which PLAGEs, SUNSPOTS, FACULAe, FLAREs, etc.
solar prominence (NASA Thesaurus) Filamentlike protuberances from the chromosphere of the sun. Used for filaments (solar physics). solar prominence (NASA SP-7, 1965) = prominence.
prism proper motion angular change of a star's direction from the Sun in one year. protein large molecule composed of hundreds to thousands of amino acids joined together by peptide links making up the DNA molecule.
A rather twisted prominence. Both images courtesy of SOHO/EIT consortium. SOHO is a project of international cooperation between ESA and NASA.
If I can see solar s with the naked eye during a total eclipse, why do I need a hydrogen-alpha filter to see them at other times?
See also: Earth, Sun, Astro, Solar, Period