The Suns Structure

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Across
  1. 3. The outermost layer where temperatures can reach 2 million degrees Celsius.
  2. 7. These can disrupt Earth’s magnetic field and come from solar flares, solar prominences and coronal mass ejections.
  3. 8. The layer in which light is radiated out into space.
  4. 11. 99.8% of all the mass in the solar system. It is the center of our solar system.
  5. 12. The coolest layer of the sun located above the photosphere.
  6. 14. This layer creates the sun’s magnetic field through convection currents.
Down
  1. 1. The sun is 330,000 times more massive than this planet.
  2. 2. The unit of measure for power.
  3. 4. The product or result of nucleosynthesis in our sun.
  4. 5. The area where Hydrogen is fused to Helium through a process called nucleosynthesis.
  5. 6. The type of star our sun will swell to when it runs out of Hydrogen.
  6. 9. The element our sun uses to form Helium in the process of nucleosynthesis, it is found in the core of the sun.
  7. 10. Areas of magnetic disturbances on the surface of the sun.
  8. 13. An area of ionized gas (plasma) where energy in the form of photons is transported outward.