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Photo Credit: https://www.azernews.az/region/63312.html

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Photo Credit: http://blog.relearningtoteach.com/2015/11/day-44-swedish-fusion.html

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the innermost layer of the Earth

where the Sun's energy comes from

where nuclear fusion occurs

hotter than 15 million degrees Kelvin

Credit: https://phys.org/news/2017-08-sun-core-rotates-faster-surface.html

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between the core and convective zone

energy from nuclear fusion travels through it to get to the convective zone

tachocline separates it and the convective zones (the two layers rotate differently)

5 million degrees Kelvin

Credit: http://www.passmyexams.co.uk/GCSE/physics/structure-of-the-sun.html

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2 million degrees Kelvin

convection currents occur here

convection currents carry the energy to the Sun's surface

Credit: http://www.passmyexams.co.uk/GCSE/physics/structure-of-the-sun.html

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the surface of the Sun

can see sunspots

can see granules

densest part of the solar atmosphere

Credit: https://www.britannica.com/science/photosphere

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above the photosphere

can be more clearly seen during solar eclipses

means "color sphere"

lower atmosphere

Credit: https://en.wikipedia.org/wiki/Chromosphere

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upper atmosphere

can be clearly seen during solar eclipses

2 million degrees Kelvin

can also be seen using a coronagraph

Credit: https://spaceplace.nasa.gov/sun-corona/en/

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planet sized dark spots on the surface of the Sun

aren't as hot as the area surrounding it

have a penumbra and umbra

caused by disturbances in the Sun's magnetic field

can last a few days to up to even months

Credit: https://en.wikipedia.org/wiki/Sunspot

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a large, bright feature extending from the surface of the Sun

"solar eruptions"

Credit: https://www.nasa.gov/content/goddard/what-is-a-solar-prominence/

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eruptions of electromagnetic radiation from the Sun

Credit: https://en.wikipedia.org/wiki/Solar_flare

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a "light show" caused by the Sun

during a coronal mass ejection, the Sun releases a bubble of gas that travels through space very quickly

particles from this interact with the gases in our atmosphere, resulting in auroras

Credit: https://apod.nasa.gov/apod/ap180410.html

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https://sciencing.com/suns-core-5371274.html

http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html

https://www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html

http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Conzone.html

https://www.windows2universe.org/sun/atmosphere/photosphere.html

https://www.britannica.com/science/chromosphere

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

https://www.britannica.com/science/corona-Sun

https://scied.ucar.edu/solar-corona

https://www.windows2universe.org/sun/atmosphere/sunspots.html

https://www.nasa.gov/content/goddard/what-is-a-solar-prominence

https://www.britannica.com/science/solar-prominence

https://www.swpc.noaa.gov/phenomena/solar-flares-radio-blackouts

https://spaceplace.nasa.gov/aurora/en/