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https://solarscience.msfc.nasa.gov/interior.shtml
https://solarscience.msfc.nasa.gov/surface.shtml
https://solarscience.msfc.nasa.gov/chromos.shtml
https://solarscience.msfc.nasa.gov/corona.shtml
https://solarscience.msfc.nasa.gov/flares.shtml
https://solarscience.msfc.nasa.gov/feature1.shtml#Sunspots

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The Sun's core is the central region where nuclear reactions consume hydrogen to form helium. These reactions release the energy that ultimately leaves the surface as visible light. These reactions are highly sensitive to temperature and density.

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The radiative zone extends outward from the outer edge of the core to the interface layer or tachocline at the base of the convection zone. The radiative zone is characterized by the method of energy transport - radiation. The energy generated in the core is carried by light that bounces from particle to particle through the radiative zone.

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The convection zone is the outer-most layer of the solar interior. It extends from a depth of about 200,000 km right up to the visible surface. At the base of the convection zone the temperature is about 2,000,000° C. This is "cool" enough for the heavier ions to hold onto some of their electrons. This makes the material more opaque so that it is harder for radiation to get through. This traps heat that ultimately makes the fluid unstable and it starts to "boil" or convect.

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The photosphere is the visible surface of the Sun that we are most familiar with.

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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. At these higher temperatures hydrogen emits light that gives off a reddish color. This colorful emission can be seen in prominences that project above the limb of the sun during total solar eclipses.

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The Corona is the Sun's outer atmosphere. It is visible during total eclipses of the Sun as a pearly white crown surrounding the Sun. The corona displays a variety of features including streamers, plumes, and loops.

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Sunspots appear as dark spots on the surface of the Sun. Temperatures in the dark centers of sunspots drop to about 3700 K. They typically last for several days, although very large ones may live for several weeks.

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Solar flares are tremendous explosions on the surface of the Sun. In a matter of just a few minutes they heat material to many millions of degrees and release as much energy as a billion megatons of TNT. They occur near sunspots, usually along the dividing line between areas of oppositely directed magnetic fields.

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Auroras are basically light shows in the sky. They are best seen at night and are actually caused by the sun. When a solar storm comes toward us, some of the energy and small particles can travel down the magnetic field lines at the north and south poles into Earth’s atmosphere. There, the particles interact with gases in our atmosphere resulting in beautiful displays of light in the sky. Oxygen gives off green and red light. Nitrogen glows blue and purple.