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Chromosphere

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Chromosphere
The chromosphere (literally, "color sphere") is a thin layer of the Sun's atmosphere just above the photosphere, roughly 10,000 kilometers deep (approximating to, if a little less than, the diameter of the Earth).

 


Chromosphere
From LoveToKnow 1911
CHROMOSPHERE (from Gr. xpiepa, colour, and c4aipa, a sphere), in astronomy, the red-coloured envelope of the sun, outside of the photosphere.

Chromosphere
The chromosphere is the second most outer layer of the Sun. Several thousand kilometres thick, it resides above the photosphere and beneath the corona.

Chromosphere
Related Category: Astronomy: General
(kr´msfr´´) [Gr.

chromosphere
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Chromosphere
The chromosphere is a narrow layer above the photosphere that raises in temperature with height. Normally, it can't be seen by the naked eye because the light from the photosphere of the Sun overpowers it.

Chromosphere
This entry contributed by Dana Romero
The layer of the Sun lying just above the photosphere.

The chromosphere is also home to spikes of gas called spicules that rise through it at the edges of the large convection cells that exist within the layer (so called supergranules).

Definition: chromosphere: The lower level of the solar atmosphere between the photosphere and the corona.
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Chromosphere
Wikipedia, the free encyclopedia - Cite This Source
The chromosphere (literally, "color sphere") is a thin layer of the Sun's atmosphere just above the photosphere, roughly 10,000 kilometers deep (approximating to, ...

CHROMOSPHERE AND CORONA
The ordinary solar spectrum is produced by the photosphere; during an eclipse the brilliant photosphere is blocked out by the Moon and three objects are visible: (1) a thin, ...

chromosphere -- the lower atmosphere of the Sun that appears as a thin rosy ring around the edge of the solar disk during a total eclipse.
corona -- the upper atmosphere of the Sun that appears as a halo around the Sun during a total eclipse.

Chromosphere. The layer of the solar atmosphere above the photosphere and beneath the transition region and the corona. It is seen during eclipses as a bright red ring around the Sun, and the term burning prairie has been used to describe it.

chromosphere The Sun's lower atmosphere, lying just above the visible photosphere.

chromosphere
a layer in a star's atmosphere lying below the corona and above the photosphere
circumpolar ...

Chromosphere- that part of the sun's atmosphere that lies just above its visible surface, or photosphere
Circumpolar stars- stars that never set when seen from a given location
Colles- small hills or knobs ...

Chromosphere
the layer of the solar atmosphere that is located above the photosphere and beneath the transition region and the corona. The chromosphere is hotter than the photosphere but not as hot as the corona.

Chromosphere
A line layer of gas just above the photosphere of the sun, it is often marked by solar eruptions called solar flares and prominence.
Chromatic Aberration ...

Chromosphere--a reddish layer in the Sun´s atmosphere, the transition between the photosphere and the corona ...

chromosphere
The lower layer of the atmosphere of the Sun.
circumpolar
Areas of the night sky which do not travel below the horizon over the course of a year, from a particular location on the Earth.

chromosphere: Bright gases just above the photosphere of the sun.
circular velocity: The velocity required to remain in a circular orbit about a body.

Chromosphere - The part of the Sun's atmosphere between the photosphere and the corona
Circle - A curve on which all points are equidistant from the center ...

CHROMOSPHERE - Region immediately above a star’s photosphere.

Chromosphere
The next layer up is the Chromosphere. Even though this layer is further from the surface of the Sun, the temperature of the chromosphere is greater than that of the photosphere, typically about 10,000 K.

The Chromosphere
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The chromosphere is an irregular layer above the photosphere where the temperature rises from 6000° C to about 20,000° C.

Chromosphere
The middle layer of the solar atmosphere between the photosphere and the corona. The chromosphere is roughly 10,000 kilometers (6,200 miles) thick and is composed primarily of hydrogen.

Chromosphere The part of the Sun just above the photosphere. Thousands of miles thick, it is mostly hydrogen gas. It looks like a red ring during an eclipse. The corona is just above the chromosphere.

Chromosphere: A layer of the Sun's atmosphere lying above the photosphere with a width of about 2000 km. It has a lower gas density than the photosphere but a higher temperature.

Chromosphere
Part of the Sun's atmosphere, it is visible during a total solar eclipse.
Circumpolar star ...

Chromosphere
The part of the Sun's atmosphere just above the surface.
Circumpolar Star
A star that never sets but always stays above the horizon. This depends on the location of the observer.

Chromosphere - The part of the Sun's atmosphere between the photosphere and the corona
Circle - A curve on which all points are equidistant from the center ...

CHROMOSPHERE
The chromosphere is the inner, reddish layer in the sun's atmosphere, between the and the . The chromosphere is visible during a total .

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.

Lower chromosphere of the Sun, a comparatively cool region in which radiation at certain wavelengths is absorbed from the continuous spectrum emitted from the Sun's photosphere. [A84]
Reynolds Number ...

The thin chromosphere is visible in this solar eclipse picture.
Corona
When the new Moon covers up the photosphere during a total solar eclipse, you can see the pearly-white corona around the dark Moon.

Above the chromosphere lies the transition region, where the temperature increases rapidly on a distance of only around 100 km.

discoverer of Pluto's moon Charon (331k jpg (Jim is the seated figure at left)) chromosphere the lower level of the solar atmosphere between the photosphere and the corona colles small hills or knobs.

chromosphere (NASA Thesaurus / NASA SP-7, 1965) A thin layer or relatively transparent gases above the photosphere of the sun. chronoisotherm (NASA SP-7, 1965) See isotherm, note. chronometer noon (NASA SP-7, 1965) See solar noon.

The photosphere, chromosphere. and corona.
Courtesy of Univ of Herts, UK
The Solar Corona, as seen in a
total eclipse ...

The photosphere, chromosphere and corona
This composite image presents the three most visible elements of space weather: a storm from the Sun, aurora as seen from space, and aurora as seen from the Earth.

A bright gaseous stream (SURGE) emanating from the CHROMOSPHERE. BRIGHT SURGE ON THE LIMB (BSL). A large gaseous stream (SURGE) that moves outward more than 0.15 solar radius above the LIMB. BURST.

(Most such high- speed stars have lower metal abundances, a result of their coming to us from a different part of the Galaxy.) Like the Sun, the star is magnetically active with a chromosphere and X-ray-radiating corona heated to roughly 5 million ...

This is the one opportunity for humans to view the next, higher layer of the solar atmosphere, called the chromosphere. Immense plumes of hot gas propelled through the chromosphere appear as tiny luminous threads on the Sun's unraveling edge.

Above the photosphere lies a region called the chromosphere. It has this name because this layer of the Sun's atmosphere can be seen during the last moments before totality in a solar eclipse as a pinkish layer (hence color, or chromo).

In addition, there are two layers of gas above the photosphere called the chromosphere and the corona. Events which occur on the Sun include sunspots, solar flares, solar wind, and solar prominences.

A solar flare is a sudden intense brightening of a small part of the Sun's chromosphere in the vicinity of a plage or facula and often near a sunspot group. The flare develops in a few minutes and may last several hours.

The Sun's faint corona will be visible, and even the chromosphere, solar prominences, and possibly even a solar flare may be visible.

The chromosphere, which extends for several thousand kilometers above the photosphere, has a temperature near 30,000 K (about 54,000° F).

Above the photosphere is another layer of gas, about 2,000km thick, called the chromosphere. Its temperature is higher, with a typical value of 105K.

Its greater sensitivity allowed Jansen and Lockyer to photograph the spectral lines in the Sun's chromosphere and discover the element Helium. It was not isolated in a laboratory until 1895.

A magnetic storm is a temporary perturbation (disruption) of the Earth's magnetic field, caused by solar flares, which eject plasma from the Sun's chromosphere.

coronagraph - An instrument for photographing the chromosphere and corona of the sun outside of eclipse.
cosmic background radiation - The microwave radiation coming from all directions that is believed to be the redshifted glow of the big bang.

The pattern of large cells seen in the sun's chromosphere, when viewed in the light of the strong emission line of ionized hydrogen.
superior planet - (n.)
Any planet whose orbit lies beyond the earth's orbit around the sun.

transition zone The region of rapid temperature increase that separates the Sun's chromosphere from the corona.
transverse motion Motion perpendicular to a particular line of sight, which does not result in Doppler shift in radiation received.

sunspots and faculae in the photosphere
plages, fibrils, and filaments in the chromosphere
coronal condensations in the corona.
Solar flares are also associated with active regions.

Astronomers describe different "layers" of our Sun based on what can be seen when looking at different colors (wavelengths) of light. The layers we can most easily see are the photosphere, chromosphere, and the corona.

"The most significant damage [to biological systems] associated with ultraviolet light occurs from UV-C [short-wave ultraviolet], which is produced in enormous quantities in the photosphere of hotter F-type stars and further out, in the chromospheres, ...

Past indications of a planetary companion around Epsilon Eridani have been difficult to verify because the young star is "jittery" with a very active chromosphere.

See also: Solar, Sun, Light, Corona, Atmosphere