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http://cdn.alaskaphotographics.com/wp-content/uploads/2015/11/ak1ds-2727.jpg

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Auroras are light shows put on by the Sun, near the North and South poles. particles sent to Earth by the Sun interact with gasses in our atmosphere and cause the beautiful northern and southern lights.

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http://www.sciencemag.org/sites/default/files/styles/article_main_large/public/images/sn-solarflare.jpg?itok=RBiAYo6R

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A solar flare occurs when there is an eruption on the sun, caused by magnetic fields realigning.

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https://www.nasa.gov/sites/default/files/thumbnails/image/faq1.jpg

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A solar prominence is a large, bright feature extending outwards into the Sun's Corona.

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https://www.weather.gov/images/fsd/astro/Sun_sunspot.jpg

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The Sun is covered in sunspots- darker, cooler areas appearing on the photosphere of the Sun. They can be very large, and are caused by magnetic reactions we do not quite understand.

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The corona is the Sun's outer atmosphere. It is mostly visible during complete solar eclipses as a pearly white "crown" surrounding the Sun.

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The chromosphere is the irregular layer above the photosphere. The chromosphere has a reddish glow to it surrounding the sun. Changes in solar flares occur in the chromosphere.

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https://solarscience.msfc.nasa.gov/surface.shtml

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The photosphere is the visible surface of the Sun most of us recognize. This is a layer about 100 km thick, and has visible sun spots.

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The convective zone is the outermost layer of the interior of the Sun. This layer traps heat and other ions.

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http://astronimate.com/wp-content/uploads/2016/10/layers-of-the-sun-interior-convective-zone.png?x70168

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The radiative zone extends from the outer surface of the core, to the base of the convection zone. The radiative zone is characterized by the means of energy transport- radiation.

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https://sohowww.nascom.nasa.gov/gallery/images/large/cutaway00.jpg

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https://solarscience.msfc.nasa.gov/interior.shtml

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The Sun's core is the central region where nuclear reactions consume hydrogen, in turn forming helium. The center core of the Sun is approximately 27,000,000 degrees Fahrenheit.

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http://www.astronoo.com/images/soleil/soleil-structure-layers.jpg