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The sun sends us more than heat and light; it sends lots of other energy and small particles our way. Sometime more particles than others.

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A solar flare occurs when magnetic energy that has built up in the solar atmosphere is suddenly released.

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A prominence is a large, bright, gaseous feature extending outward from the Sun's surface, often in a loop shape. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the Sun's corona.

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Sunspots are spots or patches appearing from time to time on the sun's surface, appearing dark by contrast with its surroundings.

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The chromosphere is a layer in the Sun between about 250 miles and 1300 miles above the solar surface. The temperature in the chromosphere varies between about 4000 K at the bottom (the so-called temperature minimum) and 8000 K at the top (6700 and 14,000 degrees F).

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The photosphere is the deepest layer of the Sun that we can observe directly. It reaches from the surface visible at the center of the solar disk to about 250 miles (400 km) above that. The temperature in the photosphere varies between about 6500 K at the bottom and 4000 K at the top (11,000 and 6700 degrees F, 6200 and 3700 degrees C). Most of the photosphere is covered by granulation.

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It extends from a depth of 200,000 km up to the visible surface of the Sun. Energy is transported by convection in this region. The surface of the convection zone is where light (photons) is created.

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The Sun's radiative zone is the section of the solar interior between the innermost core and the outer convective zone. In the radiative zone, energy generated by nuclear fusion in the core moves outward as electromagnetic radiation. In other words, the energy is conveyed by photons.

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The core is the source of all the Sun's energy. Fortunately for life on earth, the Sun's energy output is just about constant so we do not see much change in its brightness or the heat it gives off. The Sun's core has a very high temperature, more than 15 million degrees Kelvin, and the material in the core is very tightly packed or dense. It is a combination of these two properties that creates an environment just right for nuclear reactions to occur.

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http://www.astronoo.com/en/articles/journey-of-the-photon.html
https://www.mindmeister.com/520025900/sun
http://solar.physics.montana.edu/ypop/Spotlight/SunInfo/Core.html
http://www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html
http://astronimate.com/article/layers-of-the-sun-explained/
http://sc663dtk.weebly.com/the-sun.html
https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html