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Citation

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The core is the innermost layer of the Sun. Nuclear reactions occur here. They consume hydrogen, which then form helium.

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It is named by the method of energy transport: radiation. Energy is generated in the core and is carried by light (photons), which bounce from particle to particle through the radiative zone.

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This is the outermost inner layers of the Sun. Gases such as oxygen, nitrogen, and calcium hold their electrons. This is the layer where heat is transported to the outer layers.

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It is the deepest layer of the Sun that we can observe directly. Most of the photosphere is covered by granulation. The temperature ranges from 11,000 and 6,700 degrees Fahrenheit.

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The chromosphere is above the photosphere. The temperature rises as farther away the layer goes from the core.

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This is the outermost layer. the temperature is approximately 900,000 degrees Fahrenheit. The only way from the corona to be seen with a naked eye is during a total solar eclipse .

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Sunspots are spots in the Sun's photsphere that appear darker than the rest. The reduced temperature makes it appear darker. Their intense magnetic fields inhibit the rise of heat from the solar interior.

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It is a large, bright feature extending outward from the Sun's surface. Prominence's are anchored to the Sun's surface in the photosphere and extend outwards into the corona.

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Solar flares are powerful bursts of radiation. This can affect Earth"s communication and GPS signals.

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Auroras can happen when a giant cloud of gas from the sun, a coronal mass ejection or CME, which then collides with Earth's magnetic fields.

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https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html
https://solarscience.msfc.nasa.gov/interior.shtml
Corona Picture
Chromosphere picture
Photosphere Picture
Radiative Zone
Convection Zone
Core
Sunspots picture
Prominence
Solar Flare
Auroras