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http://study.com/cimahges/multiimags/16.the-structure-of-the-sun-600x518.png
https://i.ytimg.com/vi/HFT7ATLQQx8/maxresdefault.jpg
http://i1-news.softpedia-static.com/images/news2/Sun-039-s-Core-Rotates-Slower-Than-Previously-Thought-2.jpg
http://study.com/cimages/multimages/16/sun_parts_big.jpg
http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Images/chromosphere.gif
http://images.csmonitor.com/csm/2013/02/sunspot.jpg?alias=standard_600x400

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The sun provides energy for aurora. These auroras may appear as red, pink and white, violet, or blue.

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The sun releases heat and energy when a sudden eruption of magnetic energy is released into the atmosphere.

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An arched, gaseous feature that extends out from the surface of the sun, similar a solar flare.

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Sunspots are an occasional phenomena which occurs on the surface of the sun. They are an area of reduced temperature and appear darker than the rest.

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The corona is a field plasma that surrounds the sun and extends millions of miles into the space. It is most easily seen during solar eclipses.

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Literally named the "Sphere of color", the chromosphere is the layer of the sun situated above the photosphere and serves as layer of the suns's atmosphere.

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The visible surface of the sun. This layer is km thick and is gaseous like the rest of the sun.

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An area of plasma between the core and the photosphere where energy is transferred by a process of convection.

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The radiative zone of the sun is the layer just outside the core, which transports energy and light to the exterior regions through radiative diffusion. In this zone, energy travels in the form of radiative photons.

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This is the innermost region of the sun where all nuclear activity occurs-hydrogen is consumed to form helium and energy and light are produced as a result.

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1. Core
2. Radiative zone
3. Convective zone
4. Photosphere
5. Chromosphere
6. Corona
7. Sunspot
8. Granules
9. Prominence