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      <title>Solar Activity by Xitlalli Fortoso</title>
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      <description>By: Xitlalli Fortoso</description>
      <language>en-us</language>
      <pubDate>2017-05-10 11:21:16 UTC</pubDate>
      <lastBuildDate>2017-05-10 11:56:17 UTC</lastBuildDate>
      <webMaster>hello@padlet.com</webMaster>
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      <item>
         <title>Picture of the Sun</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170975892</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="http://abyss.uoregon.edu/~js/images/not_the_great_pumpkin.jpg" width="575" height="575"><figcaption class="caption"></figcaption></figure></div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:25:07 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170975892</guid>
      </item>
      <item>
         <title>Suns Layers</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170976222</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="http://www.astronoo.com/images/soleil/soleil-structure-layers.jpg" width="1024" height="677"><figcaption class="caption"></figcaption></figure></div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:27:15 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170976222</guid>
      </item>
      <item>
         <title>Core of the Sun</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170976465</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="https://astrobob.areavoices.com/astrobob/images/SunLayers.jpg" width="500" height="470"><figcaption class="caption"></figcaption></figure>The <strong>Sun's core</strong> is the central region where nuclear reactions consume hydrogen to form helium.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:28:45 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170976465</guid>
      </item>
      <item>
         <title>Radiative Zone</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170976794</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="http://astro.ic.ac.uk/sites/default/files/imagecache/XLarge/SolarInterior.jpg" width="596" height="597"><figcaption class="caption"></figcaption></figure>The Sun's <strong>radiative zone</strong> is the section of the solar interior between the innermost core and the outer convective <strong>zone</strong>.<br><br></div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:31:08 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170976794</guid>
      </item>
      <item>
         <title>Convective Zone</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170977019</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="https://www.cora.nwra.com/~werne/eos/images/interior.jpg" width="600" height="600"><figcaption class="caption"></figcaption></figure>It extends from a depth of 200,000 km up to the visible surface of the Sun. Energy is transported by <strong>convection</strong> in this region. </div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:32:56 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170977019</guid>
      </item>
      <item>
         <title>Photosphere</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170977282</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:335,&quot;url&quot;:&quot;http://study.com/cimages/multimages/16/the_sun_by_the_atmospheric_imaging_assembly_of_nasas_solar_dynamics_observatory_-_20100819.jpg&quot;,&quot;width&quot;:352}" data-trix-content-type="image"><img src="http://study.com/cimages/multimages/16/the_sun_by_the_atmospheric_imaging_assembly_of_nasas_solar_dynamics_observatory_-_20100819.jpg" width="352" height="335"><figcaption class="caption"></figcaption></figure>The&nbsp;</div><div><strong>photosphere</strong> is the lowest layer of the <strong>Sun</strong> visible from Earth. This thin layer is the lowest level in the <strong>Sun's</strong> atmosphere. Energy finally escapes the <strong>Sun</strong> from the <strong>photosphere</strong>, so it is significantly cooler than the solar interior.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:34:50 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170977282</guid>
      </item>
      <item>
         <title>Chromosphere</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170977439</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="http://classconnection.s3.amazonaws.com/733/flashcards/2034733/jpg/convection_zone1352128867756.jpg" width="700" height="540"><figcaption class="caption"></figcaption></figure>A reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star's outer atmosphere.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:36:05 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170977439</guid>
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      <item>
         <title>Corona</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170977800</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:327,&quot;url&quot;:&quot;https://sohowww.nascom.nasa.gov/explore/img/mdigraphic.gif&quot;,&quot;width&quot;:422}" data-trix-content-type="image"><img src="https://sohowww.nascom.nasa.gov/explore/img/mdigraphic.gif" width="422" height="327"><figcaption class="caption"></figcaption></figure>The rarefied gaseous envelope of the sun and other stars. The sun's corona is normally visible only during a total solar eclipse when it is seen as an irregularly shaped pearly glow surrounding the darkened disk of the moon.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:38:04 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170977800</guid>
      </item>
      <item>
         <title>Sun Spots</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170978521</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:366,&quot;url&quot;:&quot;https://upload.wikimedia.org/wikipedia/commons/6/67/Sunspots_1302_Sep_2011_by_NASA.jpg&quot;,&quot;width&quot;:634}" data-trix-content-type="image"><img src="https://upload.wikimedia.org/wikipedia/commons/6/67/Sunspots_1302_Sep_2011_by_NASA.jpg" width="634" height="366"><figcaption class="caption"></figcaption></figure>A spot or patch appearing from time to time on the sun's surface, appearing dark by contrast with its surroundings.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:41:45 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170978521</guid>
      </item>
      <item>
         <title>Prominence</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170978680</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:1054,&quot;url&quot;:&quot;https://www.nasa.gov/sites/default/files/thumbnails/image/faq5.jpg&quot;,&quot;width&quot;:1080}" data-trix-content-type="image"><img src="https://www.nasa.gov/sites/default/files/thumbnails/image/faq5.jpg" width="1080" height="1054"><figcaption class="caption"></figcaption></figure></div><div>A large, bright feature extending outward from the Sun's surface.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:42:42 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170978680</guid>
      </item>
      <item>
         <title>Flare</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170978854</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview"><img src="http://the-levant.com/wp-content/uploads/2015/09/sun-big-solar-flare-100910-02.jpg" width="512" height="419"><figcaption class="caption"></figcaption></figure>A <strong>flare</strong> is defined as a sudden, rapid, and intense variation in brightness.</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:43:51 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170978854</guid>
      </item>
      <item>
         <title>Aurora</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170979314</link>
         <description><![CDATA[<div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:541,&quot;url&quot;:&quot;http://i.dailymail.co.uk/i/pix/2014/03/13/article-2579940-1C3FF72600000578-0_964x541.jpg&quot;,&quot;width&quot;:964}" data-trix-content-type="image"><img src="http://i.dailymail.co.uk/i/pix/2014/03/13/article-2579940-1C3FF72600000578-0_964x541.jpg" width="964" height="541"><figcaption class="caption"></figcaption></figure>The result of charged particles colliding, creating bright lights in the sky. An example of <strong>aurora</strong> is when the <strong>sun</strong> just begins to rise.&nbsp;</div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:46:24 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170979314</guid>
      </item>
      <item>
         <title>Sources</title>
         <author>8615614</author>
         <link>https://padlet.com/8615614/bzviet1nwa5d/wish/170979863</link>
         <description><![CDATA[<div><a href="https://www.google.com/search?q=aurora+sun+definition&amp;source=lnms&amp;sa=X&amp;ved=0ahUKEwin-qamoOXTAhUHNSYKHavgBWgQ_AUIBSgA&amp;biw=1366&amp;bih=630&amp;dpr=1&amp;safe=active&amp;ssui=on">https://www.google.com/search?q=aurora+sun+definition&amp;source=lnms&amp;sa=X&amp;ved=0ahUKEwin-qamoOXTAhUHNSYKHavgBWgQ_AUIBSgA&amp;biw=1366&amp;bih=630&amp;dpr=1&amp;safe=active&amp;ssui=on</a><br><a href="http://the-levant.com/wp-content/uploads/2015/09/sun-big-solar-flare-100910-02.jpg">http://the-levant.com/wp-content/uploads/2015/09/sun-big-solar-flare-100910-02.jpg</a><br><a href="https://www.google.com/search?q=sunspots&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;ved=0ahUKEwjCgsHjnuXTAhWC4SYKHdRrCrsQ_AUICigB&amp;biw=1366&amp;bih=630&amp;safe=active&amp;ssui=on#imgrc=_">https://www.google.com/search?q=sunspots&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;ved=0ahUKEwjCgsHjnuXTAhWC4SYKHdRrCrsQ_AUICigB&amp;biw=1366&amp;bih=630&amp;safe=active&amp;ssui=on#imgrc=_</a><br><a href="https://www.google.com/search?q=prominence+sun&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;sqi=2&amp;pjf=1&amp;ved=0ahUKEwimtdu3n-XTAhXBQiYKHe5bDWcQ_AUIBigB&amp;biw=1366&amp;bih=630&amp;safe=active&amp;ssui=on#imgrc=q6gHfeHZJ0xrQM:">https://www.google.com/search?q=prominence+sun&amp;source=lnms&amp;tbm=isch&amp;sa=X&amp;sqi=2&amp;pjf=1&amp;ved=0ahUKEwimtdu3n-XTAhXBQiYKHe5bDWcQ_AUIBigB&amp;biw=1366&amp;bih=630&amp;safe=active&amp;ssui=on#imgrc=q6gHfeHZJ0xrQM:</a></div>]]></description>
         <enclosure url="" />
         <pubDate>2017-05-10 11:49:35 UTC</pubDate>
         <guid>https://padlet.com/8615614/bzviet1nwa5d/wish/170979863</guid>
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