# data[].attributes.body
The core is the source of all the Sun's energy. It has a temperature more that 15 million degrees Kelvin, and the material that makes up the core is very dense.

# data[].attributes.body
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.

# data[].attributes.body
In the convective zone, heat and energy are carried outward along with matter in swirling flows called convection cells. This motion is similar to the roiling flows seen in a pot of boiling water.

# data[].attributes.body
The photosphere is the visible surface of the Sun that we are most familiar with. Since the Sun is a ball of gas, this is not a solid surface but is actually a layer about 100 km thick.

# data[].attributes.body
The chromosphere is the layer above the photosphere. It appears as a red glow around the sun and is almost transparent.

# data[].attributes.body
Corona means crown and is the outermost layer of gases that surround the sun. It is only seen during a solar eclipse.

# data[].attributes.body
•dark spots that appear on the surface on the surface of the sun. They appear darker because they are cooler than the surround areas

# data[].attributes.body
A solar prominence is a large, bright feature extending outward from the Sun's surface. Prominences are anchored to the Sun's surface in the photosphere, and extend outwards into the Sun's corona. A prominence forms over timescales of about a day, and stable prominences may persist in the corona for several months, looping hundreds of thousands of miles into space.

# data[].attributes.body
A solar flare is an intense burst of radiation coming from the release of magnetic energy associated with sunspots. Flares are our solar system’s largest explosive events. They are seen as bright areas on the sun and they can last from minutes to hours. We typically see a solar flare by the photons (or light) it releases, at most every wavelength of the spectrum.

# data[].attributes.body
The aurora borealis and aurora australis are often called the northern lights and southern lights. These light shows are provoked by energy from the Sun
and fueled by electrically charged particles trapped in Earth’s magnetic eld.

# data[].attributes.body
http://ds9.ssl.berkeley.edu/solarweek/MONDAY/core.html

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

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

https://phys.org/news/2011-12-astronomers-reveal-rapidly-core-stars.html

http://nineplanets.org/sol.html

https://www.nasa.gov/mission_pages/hinode/solar_020.html

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

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

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

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

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