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photosphere
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photosphere

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The structure of the Sun. Nuclear reactions at the core release vast amounts of energy in the form of light and heat that radiate out to the photosphere and corona. Surges of glowing gas rise as prominences from the surface of the Sun and cooler areas, known as sunspots, appear as dark patches on the star's surface.

Visible surface of the Sun, which emits light and heat. About 300 km/200 mi deep, it consists of incandescent gas at a temperature of 5,800 K (5,530°C/9,980°F).

Rising cells of hot gas produce a mottling of the photosphere known as granulation, each granule being about 1,000 km/620 mi in diameter. The photosphere is often marked by large, dark patches called sunspots.



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CaX), which is the highest ionization stage of a chemical element ever discovered in a photospheric stellar spectrum.
In introducing 54 papers that presented a sample of its first results and related theoretical models at the 2007 ASP conference, Matthews (UCL Mullard Space Science Laboratory, Surrey, UK) and coauthors from NASA and the National Astronomical Observatory of Japan explain Hinode's mission to provide information on how solar magnetic fields are formed, evolve, and interact with plasmas to create the photospheric and chromospheric phenomena observed.
Eighty contributions are organized into sections on photospheric magnetism, radiative transfer methods and inversion techniques, new solar polarimeters and techniques, atomic spectro- polarimetry, theory of collisional polarization, laboratory experiments and molecular spectro-polarimetry, stellar spectro- polarimetry, and chromospheric electromagnetism.
 
 
 
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