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The core is the center of the sun and its hottest part.Thermonuclear energy is created here.

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Energy moves slowly outward.

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Heated and cooled gas create convection currents that push energy further out towards the surface.

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The rapid release of the magnetic energy of the sun.

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The deepest observable layer of the sun.

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The layer above the photosphere which is also observable.

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Ionized elements glow in x-ray and ultraviolet wavelengths.

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Unstable plasma that extends from the Photosphere and loops out into space.

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https://www.google.com/imghp?hl=en&tab=wi&authuser=0

https://www.nasa.gov

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Cooler places on the sun that appear darker.

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Particles from solar storms travel down lines of our magnetic field and interact with gases in the atmosphere.