https://padlet.com/bryschug/r6sjgnsmo547 en-us 2019-04-28 19:20:59 UTC 2026-01-27 01:53:40 UTC hello@padlet.com https://imgglb.padletcdn.com/v13/image?t=g_auto&url=https%3A%2F%2Fpadlet.net%2Ficons%2Fpng%2F2600.png bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/354837440 2019-04-28 23:51:54 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/354837440 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355144149 The sun's core is the hottest part of the sun because the pressure on the gasses is so immense. This is where nuclear fusion happens, giving the sun light, heat, and energy.]]> 2019-04-29 18:01:47 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355144149 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355149491 2019-04-29 18:10:56 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355149491 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355154429 The energy from nuclear fission in the core comes outward as electromagnetic radiation.]]> 2019-04-29 18:19:01 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355154429 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355161246 Heat and energy move outward and flowing in masses called convection cells.]]> 2019-04-29 18:32:53 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355161246 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355275708 2019-04-30 02:42:05 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355275708 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355276053 This is where the light that we get on earth is emitted from. It is also one of the cooler areas of the sun. It is also the densest part of the sun's atmosphere.]]> 2019-04-30 02:43:39 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355276053 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355276850 2019-04-30 02:47:40 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355276850 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355473101 The chromosphere is 2,500 km thick. The hydrogen alpha emitted from this layer forms lighter "plages" and darker "filament" features.]]> 2019-04-30 15:03:14 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355473101 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355637743 2019-04-30 21:38:12 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355637743 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355637949 The temperature here is a large as a few million degrees kelvin. It is the sun's outer atmosphere and emits high amounts of radiation as x-rays. Coronal holes allow for solar wind that extends into outer space and appear white on the surface. ]]> 2019-04-30 21:39:17 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355637949 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355638700 2019-04-30 21:43:33 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355638700 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355638995 Sunspots are areas on the sun that are much cooler than the surrounding areas. These sunspots are caused by the sun's magnetic field rising up to the photosphere.]]> 2019-04-30 21:45:16 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355638995 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355644837 2019-04-30 22:20:27 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355644837 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355645754 Prominence is the glowing loop of electrically charged hydrogen and helium that forms a plasma. It is formed from the sun's magnetic field changing and bursts out.]]> 2019-04-30 22:26:21 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355645754 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355646551 http://astronomy.com/news-observing/ask%20astro/2010/07/i%20heard%20that%20the%20light%20from%20nuclear%20fusion%20reactions%20in%20the%20suns%20core%20takes%20about%20200000%20years%20to%20reach%20its%20surface%20i%20thought%20the%20speed%20of%20light%20is%20constant%20why%20does%20it%20take%20so%20long
https://www.nasa.gov/content/goddard/what-is-a-solar-prominence
http://planetfacts.org/the-center-of-the-sun/
https://www.windows2universe.org/sun/solar_activity.html
https://hesperia.gsfc.nasa.gov/sftheory/flare.htm]]> 2019-04-30 22:30:40 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355646551 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355647159 2019-04-30 22:33:55 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355647159 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355648690 Flares occur from magnetic energy in the solar atmosphere builds up and explodes, creating a huge blast of different types of waves that have radiation.]]> 2019-04-30 22:45:59 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355648690 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355649496 2019-04-30 22:51:34 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355649496 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355649725 Auroras having to do with the sun are caused by coronal mass ejections that collide with Earth's magnetic field. The magnetic fields cause an unstable environment and allow the release of oxygen and nitrogen particles into the upper atmosphere causing auroras.]]> 2019-04-30 22:53:03 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355649725 bryschug https://padlet.com/bryschug/r6sjgnsmo547/wish/355651665 2019-04-30 23:05:47 UTC https://padlet.com/bryschug/r6sjgnsmo547/wish/355651665