Facula: Difference between revisions
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:''For the [[genus]] of [[gossamer-winged butterflies]], see ''[[Facula (butterfly)]]. |
:''For the [[genus]] of [[gossamer-winged butterflies]], see ''[[Facula (butterfly)]]. |
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[[Image:Sun at 304 Angstroms.jpg|thumb|right|256px|The bright areas visible here on the Sun are ''faculae''.]]A '''facula''' (plural: '''faculae'''), Latin for "little torch", is literally a "bright spot." It is used in [[planetary nomenclature]] for naming certain surface features of planets and moons, and is also a type of surface phenomenon on the [[Sun]]. |
[[Image:Sun hi at 304 Angstroms.jpg|thumb|right|256px|The bright areas visible here on the Sun are ''faculae''.]]A '''facula''' (plural: '''faculae'''), Latin for "little torch", is literally a "bright spot." It is used in [[planetary nomenclature]] for naming certain surface features of planets and moons, and is also a type of surface phenomenon on the [[Sun]]. |
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'''Solar faculae''' are bright spots that form in the canyons between [[Granule (solar physics)|solar granules]], short-lived convection cells several thousand kilometers across that constantly form and dissipate over timescales of several minutes. Faculae are produced by concentrations of magnetic field lines. |
'''Solar faculae''' are bright spots that form in the canyons between [[Granule (solar physics)|solar granules]], short-lived convection cells several thousand kilometers across that constantly form and dissipate over timescales of several minutes. Faculae are produced by concentrations of magnetic field lines. |
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Revision as of 00:01, 31 January 2012
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- For the genus of gossamer-winged butterflies, see Facula (butterfly).
A facula (plural: faculae), Latin for "little torch", is literally a "bright spot." It is used in planetary nomenclature for naming certain surface features of planets and moons, and is also a type of surface phenomenon on the Sun.
Solar faculae are bright spots that form in the canyons between solar granules, short-lived convection cells several thousand kilometers across that constantly form and dissipate over timescales of several minutes. Faculae are produced by concentrations of magnetic field lines.
The chromosphere is above the photosphere. Solar energy passes through this region on its way out from the center of the Sun. Faculae and flares arise in the chromosphere. Faculae are bright luminous hydrogen clouds which form above regions where sunspots are about to form. Flares are bright filaments of hot gas emerging from sunspot regions. Sunspots are dark depressions on the photosphere with a typical temperature of 4,000°C (7,000°F).