https://padlet.com/emilee_hines/70i48ck19b5f en-us 2018-01-04 15:38:56 UTC 2023-01-19 06:07:41 UTC hello@padlet.com emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218765641 Citation ]]> 2018-01-04 15:42:55 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218765641 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766327 2018-01-04 15:45:36 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766327 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766683 This is the outermost layer. the temperature is approximately 900,000 degrees Fahrenheit. The only way from the corona to be seen with a naked eye is during a total solar eclipse . ]]> 2018-01-04 15:46:59 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766683 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766995 The chromosphere is above the photosphere. The temperature rises as farther away the layer goes from the core. ]]> 2018-01-04 15:48:11 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218766995 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767118 It is the deepest layer of the Sun that we can observe directly. Most of the photosphere is covered by granulation. The temperature ranges from 11,000 and 6,700 degrees Fahrenheit. ]]> 2018-01-04 15:48:37 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767118 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767253 This is the outermost inner layers of the Sun. Gases such as oxygen, nitrogen, and calcium hold their electrons. This is the layer where heat is transported to the outer layers. ]]> 2018-01-04 15:49:05 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767253 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767335 It is named by the method of energy transport: radiation. Energy is generated in the core and is carried by light (photons), which bounce from particle to particle through the radiative zone. ]]> 2018-01-04 15:49:23 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767335 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767458 The core is the innermost layer of the Sun. Nuclear reactions occur here. They consume hydrogen, which then form helium. ]]> 2018-01-04 15:49:42 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218767458 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218771512 https://www.nasa.gov/mission_pages/iris/multimedia/layerzoo.html
https://solarscience.msfc.nasa.gov/interior.shtml
Corona Picture
Chromosphere picture
Photosphere Picture
Radiative Zone   
Convection Zone
Core
Sunspots picture
Prominence
Solar Flare
Auroras ]]> 2018-01-04 16:02:57 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218771512 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218780890 Sunspots are spots in the Sun's photsphere that appear darker than the rest. The reduced temperature makes it appear darker. Their intense magnetic fields inhibit the rise of heat from the solar interior. ]]> 2018-01-04 16:30:58 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218780890 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218783824 It is a large, bright feature extending outward from the Sun's surface. Prominence's are anchored to the Sun's surface in the photosphere and extend outwards into the corona.]]> 2018-01-04 16:39:21 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218783824 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218786063 Solar flares are powerful bursts of radiation. This can affect Earth"s communication and GPS signals. ]]> 2018-01-04 16:46:14 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218786063 emilee_hines https://padlet.com/emilee_hines/70i48ck19b5f/wish/218790214 Auroras can happen when a giant cloud of gas from the sun, a coronal mass ejection or CME, which then collides with Earth's magnetic fields.]]> 2018-01-04 17:00:06 UTC https://padlet.com/emilee_hines/70i48ck19b5f/wish/218790214