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      <title>Solar Activity by </title>
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      <language>en-us</language>
      <pubDate>2019-07-10 20:22:39 UTC</pubDate>
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         <title></title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641087</link>
         <description><![CDATA[]]></description>
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         <pubDate>2019-08-07 22:39:18 UTC</pubDate>
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      <item>
         <title>Bibliography (1) ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641144</link>
         <description><![CDATA[<div><a href="https://www.express.co.uk/news/science/1138008/earth-orbit-change-dying-sun-asteroid-mining-solar-sail-space-news">https://www.express.co.uk/news/science/1138008/earth-orbit-change-dying-sun-asteroid-mining-solar-sail-space-news</a><br><br><a href="https://www.nasa.gov/mission_pages/sunearth/science/Sunlayers.html">https://www.nasa.gov/mission_pages/sunearth/science/Sunlayers.html</a><br><br><a href="https://www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html">https://www.windows2universe.org/sun/Solar_interior/Sun_layers/radiative_zone.html</a><br><br><a href="https://study.com/academy/lesson/the-suns-photosphere-definition-temperature-quiz.html">https://study.com/academy/lesson/the-suns-photosphere-definition-temperature-quiz.html</a></div>]]></description>
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         <pubDate>2019-08-07 22:40:16 UTC</pubDate>
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         <title></title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641335</link>
         <description><![CDATA[]]></description>
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         <pubDate>2019-08-07 22:42:11 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641335</guid>
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         <title>Core ~ </title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641453</link>
         <description><![CDATA[<div>The Sun's core is the central region where nuclear reactions consume hydrogen to form helium. These reactions release the energy that ultimately leaves the surface as visible light.</div>]]></description>
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         <pubDate>2019-08-07 22:43:47 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641453</guid>
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      <item>
         <title>Radiative + Convection Zones~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641497</link>
         <description><![CDATA[<div>In the radiative zone, energy generated by nuclear fusion in the core moves outward as electromagnetic radiation. In the convection zone, hot plasma rises, cools as it nears the surface, and falls to be heated and rise again.</div>]]></description>
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         <pubDate>2019-08-07 22:44:23 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641497</guid>
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         <title>Photosphere ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641715</link>
         <description><![CDATA[<div>The Sun's photosphere is a very thin layer made up of numerous granules (transient convective cells) where hot gases rise and give off light and heat.</div>]]></description>
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         <pubDate>2019-08-07 22:47:24 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641715</guid>
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      <item>
         <title>Bibliography (2) ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641825</link>
         <description><![CDATA[<div><a href="https://www.assignmentpoint.com/science/physics/chromosphere.html">https://www.assignmentpoint.com/science/physics/chromosphere.html</a><br><br><a href="https://www.washingtonpost.com/news/speaking-of-science/wp/2017/08/02/august-total-solar-eclipse-gives-scientists-rare-chance-to-study-suns-corona/?noredirect=on">https://www.washingtonpost.com/news/speaking-of-science/wp/2017/08/02/august-total-solar-eclipse-gives-scientists-rare-chance-to-study-suns-corona/?noredirect=on</a><br><br><a href="https://www.weather.gov/fsd/sunspots">https://www.weather.gov/fsd/sunspots</a><br><br><a href="http://www.daviddarling.info/encyclopedia/S/solar_flare.html">http://www.daviddarling.info/encyclopedia/S/solar_flare.html</a><br><br><a href="https://spaceplace.nasa.gov/aurora/en/">https://spaceplace.nasa.gov/aurora/en/</a></div>]]></description>
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         <pubDate>2019-08-07 22:48:50 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641825</guid>
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      <item>
         <title>Chromosphere ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641962</link>
         <description><![CDATA[<div>The chromosphere is an irregular layer above the photosphere where the temperature rises from 6000°C to about 20,000°C. At these higher temperatures hydrogen emits light that gives off a reddish color (H-alpha emission).</div>]]></description>
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         <pubDate>2019-08-07 22:50:08 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373641962</guid>
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         <title>Corona ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373642624</link>
         <description><![CDATA[<div>A corona is an aura of plasma that surrounds the Sun and other stars. </div>]]></description>
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         <pubDate>2019-08-07 22:59:43 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373642624</guid>
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         <title>sunspots ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373642998</link>
         <description><![CDATA[<div>Sunspots are darker, cooler areas on the surface of the sun in a region called the photosphere.</div>]]></description>
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         <pubDate>2019-08-07 23:03:51 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373642998</guid>
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         <title>prominence ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373643159</link>
         <description><![CDATA[<div>A prominence is a large, bright, gaseous feature extending outward from the Sun's surface, often in a loop shape. </div>]]></description>
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         <pubDate>2019-08-07 23:06:05 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373643159</guid>
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      <item>
         <title>flare ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373643511</link>
         <description><![CDATA[<div>Sometimes a sudden, rapid, and intense variation in brightness is seen on the Sun. That is a solar flare. A solar flare occurs when magnetic energy that has built up in the solar atmosphere is suddenly released.</div>]]></description>
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         <pubDate>2019-08-07 23:10:24 UTC</pubDate>
         <guid>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373643511</guid>
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         <title>aurora ~</title>
         <author>seleneberry02</author>
         <link>https://padlet.com/seleneberry02/ibx2t3dbv81o/wish/373643735</link>
         <description><![CDATA[<div>The Aurora is an incredible light show caused by collisions between electrically charged particles released from the sun that enter the earth's atmosphere and collide with gases such as oxygen and nitrogen.</div>]]></description>
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         <pubDate>2019-08-07 23:12:58 UTC</pubDate>
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