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      <title>Solar Activity by Ryan Meadows</title>
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      <description>Made with love</description>
      <language>en-us</language>
      <pubDate>2019-08-08 00:10:36 UTC</pubDate>
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         <title>SOLAR ACTIVITY</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373649473</link>
         <description><![CDATA[<div>By: Ryan Meadows</div>]]></description>
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         <pubDate>2019-08-08 00:14:08 UTC</pubDate>
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         <title>Sun:</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373649623</link>
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         <pubDate>2019-08-08 00:15:43 UTC</pubDate>
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         <title>Sun Layers and Properties:</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373649759</link>
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         <pubDate>2019-08-08 00:17:04 UTC</pubDate>
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         <title>Core: The temperature at the very center of the Sun is about 15,000,000° C (27,000,000° F) and the density is about 150 g/cm³ (approximately 10 times the density of gold, 19.3 g/cm³ or lead, 11.3 g/cm³). </title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373650163</link>
         <description><![CDATA[<div>https://lh4.googleusercontent.com/KQul_XuHm5P_QKOpO4LarmvwILtuxqUguS213_IyR_PzljVc5sKzeA7xOqYKnL0QEdXrDzAawlKluE3ZmLcm8UHEWAqw6VZ8vg=w1920-h907</div>]]></description>
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         <pubDate>2019-08-08 00:21:04 UTC</pubDate>
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         <title>Radiative Zone: The density drops from 20 g/cm³ (about the density of gold) down to only 0.2 g/cm³ (less than the density of water) from the bottom to the top of the radiative zone. The temperature falls from 7,000,000° C to about 2,000,000° C over the same distance.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373651365</link>
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         <pubDate>2019-08-08 00:30:46 UTC</pubDate>
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         <title>Convective Zone: The convection zone is the outer-most layer of the solar interior. It extends from a depth of about 200,000 km right up to the visible surface. At the base of the convection zone the temperature is about 2,000,000° C. This is &quot;cool&quot; enough for the heavier ions (such as carbon, nitrogen, oxygen, calcium, and iron) to hold onto some of their electrons. Density is only 0.0000002 gm/cm³ (about 1/10,000th the density of air at sea level).</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373651973</link>
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         <pubDate>2019-08-08 00:35:48 UTC</pubDate>
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         <title>Photosphere: The photosphere is the visible surface of the Sun that we are most familiar with. Since the Sun is a ball of gas, this is not a solid surface but is actually a layer about 100 km thick (very, very, thin compared to the 700,000 km radius of the Sun).</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373652525</link>
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         <pubDate>2019-08-08 00:41:02 UTC</pubDate>
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         <title>Corona: The corona is usually hidden by the bright light of the Sun&#39;s surface. However, the corona can be seen during a total solar eclipse.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373652780</link>
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         <pubDate>2019-08-08 00:43:37 UTC</pubDate>
         <guid>https://padlet.com/11384731/neuwqid62odn/wish/373652780</guid>
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         <title>Chromospere: A reddish gaseous layer immediately above the photosphere of the sun or another star. Together with the corona, it constitutes the star&#39;s outer atmosphere.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373653079</link>
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         <pubDate>2019-08-08 00:46:32 UTC</pubDate>
         <guid>https://padlet.com/11384731/neuwqid62odn/wish/373653079</guid>
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         <title>Sunspots: Dark, planet-sized regions that appear on the &quot;surface&quot; of the Sun. Sunspots are &quot;dark&quot; because they are cooler than their surroundings</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373653544</link>
         <description><![CDATA[<div>https://lh5.googleusercontent.com/5vZ5YwSRBK9bvctLfe-UiOi6QA4UMrHiJXg7MWs5I7vN77BdXZ6BUf9TbIPs80zxK2R1Cv2VKdlcQU3McuuHmDSRFNp2K9eI=w1920-h907</div>]]></description>
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         <pubDate>2019-08-08 00:51:13 UTC</pubDate>
         <guid>https://padlet.com/11384731/neuwqid62odn/wish/373653544</guid>
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         <title>Prominence: A large, bright, gaseous feature extending outward from the Sun&#39;s surface, often in a loop shape.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373653788</link>
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         <pubDate>2019-08-08 00:54:06 UTC</pubDate>
         <guid>https://padlet.com/11384731/neuwqid62odn/wish/373653788</guid>
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         <title>Flare: A solar flare is a sudden flash of increased brightness on the Sun, usually observed near its surface and in close proximity to a sunspot group.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373654320</link>
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         <pubDate>2019-08-08 00:58:14 UTC</pubDate>
         <guid>https://padlet.com/11384731/neuwqid62odn/wish/373654320</guid>
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         <title>Aurora: When charged particles emitted from the sun during a solar flare penetrate the earth&#39;s magnetic shield and collide with atoms and molecules in our atmosphere. These collisions result in photons, which make up the aurora.</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373654524</link>
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         <pubDate>2019-08-08 01:00:01 UTC</pubDate>
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         <title>Cites:</title>
         <author>11384731</author>
         <link>https://padlet.com/11384731/neuwqid62odn/wish/373654688</link>
         <description><![CDATA[<div>https://www.aurorahunter.com/what-are-the-northern-lights.html<br><a href="https://en.wikipedia.org/wiki/Solar_flare">https://en.wikipedia.org/wiki/Solar_flare</a><br><a href="https://en.wikipedia.org/wiki/Solar_prominence">https://en.wikipedia.org/wiki/Solar_prominence</a><br>https://scied.ucar.edu/sunspots<br><a href="https://en.wikipedia.org/wiki/Chromosphere">https://en.wikipedia.org/wiki/Chromosphere</a><br>https://spaceplace.nasa.gov/sun-corona/<br>https://solarscience.msfc.nasa.gov/surface.shtml<br><a href="https://solarscience.msfc.nasa.gov/interior.shtml">https://solarscience.msfc.nasa.gov/interior.shtml</a></div>]]></description>
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         <pubDate>2019-08-08 01:02:19 UTC</pubDate>
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