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chromosphere

   Also found in: Medical, Encyclopedia, Wikipedia 0.01 sec.
chro·mo·sphere  (krm-sfîr)
n.
1. An incandescent, transparent layer of gas, primarily hydrogen, several thousand miles in depth, lying above and surrounding the photosphere of a star, such as the sun, but distinctly separate from the corona.
2. A gaseous layer similar to a chromosphere around a star.

chromo·spheric (-sfîrk, -sfr-) adj.

chromosphere [ˈkrəʊməˌsfɪə]
n
(Astronomy) a gaseous layer of the sun's atmosphere extending from the photosphere to the corona and visible during a total eclipse of the sun
chromospheric  [ˌkrəʊməˈsfɛrɪk] adj

chromosphere  (krm-sfîr)
A glowing, transparent layer of gas surrounding the photosphere of a star. The Sun's chromosphere is several thousand kilometers thick, is composed mainly of hydrogen at temperatures of 6,000° to 20,000°K, and gives off reddish light.
ThesaurusLegend:  Synonyms Related Words Antonyms
Noun1.chromosphere - a gaseous layer of the sun's atmosphere (extending from the photosphere to the corona) that is visible during a total eclipse of the sun
layer - a relatively thin sheetlike expanse or region lying over or under another
Sun - the star that is the source of light and heat for the planets in the solar system; "the sun contains 99.85% of the mass in the solar system"; "the Earth revolves around the Sun"


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Specific topics include the origin of solar white-light flares, modeling the hemispheric pattern of solar filaments, stellar atmospheres and the diamagnetic effect, observations of running waves in a sunspot chromosphere, and acoustic shocks in the quiet solar chromosphere.
This ultrasharp image of the sun's chromosphere, a layer sandwiched between the star's visible surface and its outer atmosphere, reveals a surprisingly complex array of filaments of roiling gas, some as small as 70 kilometers across, says Richard Fisher, director of NASA'S heliophysics division in Washington, D.
Papers from a July 2005 meeting in Stein's honor are presented here, in sections on solar surface observations, surface diagnostics, magneto-convection and dynamos, sub-surface solar structures, flux emergence and active regions, sunspots, chromospheric observations and models, and connections between the photosphere, chromosphere, and corona.
 
 
 
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