https://padlet.com/andfli4971/ioch35h6h4q7 ~Made with love en-us 2018-10-12 01:05:10 UTC 2018-12-20 19:59:24 UTC hello@padlet.com https://padlet-assets.s3.amazonaws.com/icons/Growing.png andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271024 2018-12-20 19:20:29 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271024 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271145 2018-12-20 19:20:48 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271145 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271369 2018-12-20 19:21:25 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271369 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271584 The corona is the outermost part of the Sun's atmosphere.

Extremely High temperatures and is very thin. There are Heat Bombs and they explode and release their energy as heat

https://spaceplace.nasa.gov/sun-corona/en/]]> 2018-12-20 19:22:02 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316271584 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316272690 In the radiative zone, energy generated by nuclear fusion in the core moves outward as electromagnetic radiation

The Sun's radiative zone extends from the core outward to about 70% of the Sun's radius

https://www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html]]> 2018-12-20 19:25:18 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316272690 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316273956 At this point turbulent convective motions occur, similar to a pot of boiling water
The overturning motions inside the Sun are responsible for the granulation pattern seen on the Surface

https://www.windows2universe.org/sun/Solar_interior/Sun_layers/Convection_zone/convection_zone.html ]]> 2018-12-20 19:29:21 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316273956 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316275955 The solar core is made up of a really hot and dense gas (in the plasma state

15 million kelvins

The core is where the energy of the Sun is made. The density and temperature are just right for nuclear fusion reactions
https://www.windows2universe.org/sun/Solar_interior/Sun_layers/Core/core.html]]> 2018-12-20 19:34:46 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316275955 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316277440 Light emitted
Coolest region
densest part of the solar atmosphere
Disk with Sunspots
https://www.windows2universe.org/sun/atmosphere/photosphere.html


]]> 2018-12-20 19:40:03 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316277440 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316278255 just prior to and just after the peak of a total solar eclipse , the chromosphere appears as a thin reddish ring
The chromosphere is most easily viewed in emission lines such as Hydrogen alpha, where bright regions known as plages, and dark features called filaments are visible.
https://classroom.google.com/c/MTUzOTgzMDY0NjNa

]]> 2018-12-20 19:43:11 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316278255 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316279982 Sunspots are dark, planet-sized regions that appear on the surface of the Sun. Sunspots are dark because they are colder than the areas around them
https://www.windows2universe.org/sun/atmosphere/sunspots.html]]> 2018-12-20 19:49:51 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316279982 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316280844 Large impressive loop-like structures on the edge of the solar disk sometimes stand out brightly against the dark background of space
https://www.windows2universe.org/sun/atmosphere/prominence.html]]> 2018-12-20 19:53:00 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316280844 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316281126 Solar flares are essentially huge explosions on the Sun. Flares occur when intense magnetic fields on the Sun become too tangled
https://www.windows2universe.org/sun/atmosphere/solar_flares.html]]> 2018-12-20 19:54:00 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316281126 andfli4971 https://padlet.com/andfli4971/ioch35h6h4q7/wish/316281613 The aurora is formed when protons and electrons from the Sun travel along the Earth's magnetic field line
https://www.windows2universe.org/earth/Magnetosphere/aurora.html]]> 2018-12-20 19:55:51 UTC https://padlet.com/andfli4971/ioch35h6h4q7/wish/316281613