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      <title>Solar Activity  by Taylor Scism</title>
      <link>https://padlet.com/taylor_scism/8wq50hmzikpj</link>
      <description>Taylor Scism</description>
      <language>en-us</language>
      <pubDate>2019-05-22 20:58:13 UTC</pubDate>
      <lastBuildDate>2023-03-07 23:19:06 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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      <item>
         <title>The Sun&#39;s layers</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362714849</link>
         <description><![CDATA[<div>https://science.howstuffworks.com/sun5.htm<br>http://www.thesuntoday.org/solar-facts/powering-the-sun/</div>]]></description>
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         <pubDate>2019-05-22 21:01:31 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362714849</guid>
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      <item>
         <title>The Core</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715085</link>
         <description><![CDATA[<div>The core is the inner most layer of the Sun which powers the it, allowing for the Sun to produce heat and light</div>]]></description>
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         <pubDate>2019-05-22 21:02:43 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715085</guid>
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      <item>
         <title>The Radiative Zone</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715620</link>
         <description><![CDATA[<div>The area around the core is where the plasma density is high and radiation gets bounced around for about hundreds of thousands of years, until it makes it to the top of this zone.</div>]]></description>
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         <pubDate>2019-05-22 21:05:18 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715620</guid>
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      <item>
         <title>The Convective Zone</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715756</link>
         <description><![CDATA[<div>This is the layer after the Radiative Zone. In this layer the temperature drops to about 2 million Kelvin and convection currents form large bubbles of hot plasma on the surface.</div>]]></description>
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         <pubDate>2019-05-22 21:05:55 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715756</guid>
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      <item>
         <title>The Photosphere</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715804</link>
         <description><![CDATA[<div>The Photosphere is the layer after the Convective Zone. This layer is the Sun's visible surface and the temperature is about 5,800 kelvin.</div>]]></description>
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         <pubDate>2019-05-22 21:06:10 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715804</guid>
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      <item>
         <title>The Chromosphere</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715870</link>
         <description><![CDATA[<div>The Chromosphere layer is the layer above the Photosphere. This layer is very thin and appears bright red.</div>]]></description>
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         <pubDate>2019-05-22 21:06:33 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715870</guid>
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      <item>
         <title>The Corona</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715921</link>
         <description><![CDATA[<div>The Corona is the last layer of the sun. This layer's temperature is about 2 million Kelvin and can get hotter when in a flare.</div>]]></description>
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         <pubDate>2019-05-22 21:06:45 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715921</guid>
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         <title>Sunspots</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715979</link>
         <description><![CDATA[<div>Sunspots are dark, cooler areas on the sun caused by the 11 year solar cycle.</div>]]></description>
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         <pubDate>2019-05-22 21:07:03 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362715979</guid>
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      <item>
         <title>Prominence</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716015</link>
         <description><![CDATA[<div>These are plasma hoops that connect two sunspots.</div>]]></description>
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         <pubDate>2019-05-22 21:07:13 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716015</guid>
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         <title>Flare</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716037</link>
         <description><![CDATA[<div>Solar Flares occur when the sun has violent explosions.</div>]]></description>
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         <pubDate>2019-05-22 21:07:20 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716037</guid>
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      <item>
         <title>Aurora</title>
         <author>taylor_scism</author>
         <link>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716055</link>
         <description><![CDATA[<div>When radiation and several other particles meet Earth's magnetic field, auroras occur at the poles.</div>]]></description>
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         <pubDate>2019-05-22 21:07:29 UTC</pubDate>
         <guid>https://padlet.com/taylor_scism/8wq50hmzikpj/wish/362716055</guid>
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