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When charged particles from the sun strike atoms in Earth's atmosphere, they cause electrons in the atoms to move to a higher-energy state. When the electrons drop back to a lower energy state, they release a photon: light.

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sudden, rapid, and intense variation in brightness

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a large, bright, gaseous feature extending outward from the Sun's surface, often in a loop shape

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darker, cooler areas on the surface of the sun in a region called the photosphere. They look dark only in comparison with the brighter and hotter regions of the photosphere around them.

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Extends millions of kilometers into space and is most easily seen during a total solar eclipse, but it is also observable with a corona graph.

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Reddish and glowing layer of gas above a star's (or Sun's) photosphere.

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The visible glowing surface of the sun.

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A region of turbulent plasma between a star's core and its visible photosphere at the surface, through which energy is transferred by convection.

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layer of a star's interior where energy is primarily transported toward the exterior by means of radiative diffusion and thermal conduction, rather than by convection.

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The central region of the Earth; it extends fourteen hundred to eighteen hundred miles from the Earth's center.

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Google images
https://www.nasa.gov/content/goddard/what-is-solar-activity