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These happen suddenly and rapidly. They are made when magnetic energy is released and can release intense variation in bright light.
https://cdn.cnn.com/cnnnext/dam/assets/170914181101-earth-ducks-a-cosmic-bullet-opinion-lincoln-exlarge-169.jpg

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https://cdn.images.express.co.uk/img/dynamic/151/590x/worldwide-617284.jpg

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https://www.nasa.gov/sites/default/files/styles/full_width_feature/public/images/678410main_layerzoo_full.jpg

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http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html
http://csep10.phys.utk.edu/astr162/lect/sun/interior.html
http://solarscience.msfc.nasa.gov/interior.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/photosphere.html
http://solarscience.msfc.nasa.gov/surface.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/chromosphere.html
http://csep10.phys.utk.edu/astr162/lect/sun/corona.html
https://www.eso.org/public/outreach/eduoff/vt-2004/mt-2003/mt-2003-sun-corona-normal.jpg
https://upload.wikimedia.org/wikipedia/commons/d/d4/Sun_poster.svg
http://coolcosmos.ipac.caltech.edu/ask/11-Why-does-the-Sun-have-spots-
http://www.enchantedlearning.com/subjects/astronomy/sun/prominences.shtml
http://www.nasa.gov/mission_pages/sunearth/news/News022411-monsterprom.html#.VmoKlfmrTIV
http://hesperia.gsfc.nasa.gov/sftheory/flare.htm
http://pwg.gsfc.nasa.gov/polar/EPO/auroral_poster/aurora_all.pdf
https://www.astronomynotes.com/starsun/s2.htm

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This layer is the most visible to us on Earth. It is a very thin layer that is 1/7,000 of the total of Earth's radius. On this layer, the temperature also drops, and it would be very hard to see on this layer.https://www.astronomynotes.com/starsun/sunsurf.jpg

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These are the arcs of gas/plasma that erupt from the photophere. Some can last from a few hours to months. Even today scientists aren't completely sure how these form.
https://www.astronomynotes.com/starsun/prominencesm.jpg

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Theses are created when the sun's magnetic field gets twisted all around the inside of the sun. The magnetic field rises up and then pokes through, creating these spots.
https://www.astronomynotes.com/starsun/granulationsm.gif

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This layer is the outer atmosphere of the sun. Here, temperature reaches millions of degrees. The pressure and density of this layer is much lower than that of Earth's atmosphere. You can only see this during a total solar eclipse or with a corona graph.
https://www.astronomynotes.com/nakedeye/TSE73.jpeg

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This layer is 2,000 - 3,000 km thick and can only be seen during a good total solar eclipse. It also glows a slight red color.https://www.astronomynotes.com/starsun/chromosphere.jpg

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https://www.astronomynotes.com/starsun/s2.htm
http://hesperia.gsfc.nasa.gov/sftheory/flare.htm
http://coolcosmos.ipac.caltech.edu/ask/11-Why-does-the-Sun-have-spots-
http://www.enchantedlearning.com/subjects/astronomy/sun/prominences.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/chromosphere.html
http://csep10.phys.utk.edu/astr162/lect/sun/corona.html
http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html
http://media.web.britannica.com/eb-media/04/92904-034-7C3D6409.jpg
http://csep10.phys.utk.edu/astr162/lect/sun/interior.html
http://solarscience.msfc.nasa.gov/interior.shtml
http://csep10.phys.utk.edu/astr162/lect/sun/photosphere.html
http://solarscience.msfc.nasa.gov/surface.shtml

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These are energy charged particles that flow out of the sun and towards the Earth by solar winds. This energy reacts with Earth's magnetic field by changing the energy and creating a huge hole.
https://apod.nasa.gov/apod/image/1804/DragonAurora_Bastoni_960.jpg

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This layer is just below the Earth's surface and is considered the interior of the sun. The sun's temperature is very unstable because it is moving so quickly and unstable. This allows energy to diffuse outwards from the sun by convective fluid. When the fluid rises it cools and expands.
http://www.passmyexams.co.uk/GCSE/physics/images/sun-04.jpg

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This is the layer between the core and the convective zone. Here, energy made by nuclear fusion moves outward in the form of electromagnetic radiation. This zone occupies about 70% of the space of the sun. This zone is smaller and also is has a cooler temperature in comparison to the sun.
http://www.passmyexams.co.uk/GCSE/physics/images/sun-03.jpg

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This is the innermost layer of the sun and what the sun draws its energy from. Inside, temperatures are extremely hot and everything is packed together. This allows for nuclear reactions to happen in and on the sun.
http://www.passmyexams.co.uk/GCSE/physics/images/sun-02.jpg