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  <title>How strong can a geomagnetic storm be?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/how-strong-can-geomagnetic-storm-be</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;How strong can a geomagnetic storm be?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T12:50:43-07:00" title="Wednesday, February 2, 2022 - 12:50" class="datetime"&gt;Wed, 02/02/2022 - 12:50&lt;/time&gt;
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        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/Ovation_20140912.png?itok=aT8z8t_f" width="926" height="554" alt="Aurora forecast after a strong geomagnetic storm on September 13, 2014" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;Aurora forecast after a strong geomagnetic storm on September 13, 2014.&lt;/p&gt;

          &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;A geomagnetic superstorm from the Sun can be very strong but it does not happen frequently. However just like with natural disasters like fires and tornados we need to be prepared. Scientists measure the strength or energy of a geomagnetic storm in Watts, which measures how much energy is transferred in 1 second. A superstorm can dump as much as 5,000 GW (10^9 W) into Earth’s atmosphere at its peak time. That is more than the energy consumption rate of the US (~3,300GW).&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 19:50:43 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">376 at https://www2.hao.ucar.edu</guid>
    </item>
<item>
  <title>What protects the Earth from the Sun’s space weather?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/what-protects-earth-suns-space-weather</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;What protects the Earth from the Sun’s space weather?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T12:37:36-07:00" title="Wednesday, February 2, 2022 - 12:37" class="datetime"&gt;Wed, 02/02/2022 - 12:37&lt;/time&gt;
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        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/470162main_magnetosphere-orig_full.jpg?itok=Zj2g0ZK2" width="926" height="713" alt="The Earth's magnetosphere" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;The Earth's magnetosphere.&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;NASA/Goddard/Aaron Kaase&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;Earth sits within a bubble formed by Earth’s strong magnetic field. This magnetic field is constantly exposed to the wind from the Sun and therefore shaped like a teardrop with a tail pointing away from Earth and Sun. This protective bubble is called the magnetosphere, and is responsible for deflecting most of the high energy particles from Earth.&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 19:37:36 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">375 at https://www2.hao.ucar.edu</guid>
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<item>
  <title>What is space weather?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/what-space-weather</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;What is space weather?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T11:57:13-07:00" title="Wednesday, February 2, 2022 - 11:57" class="datetime"&gt;Wed, 02/02/2022 - 11:57&lt;/time&gt;
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        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/1-whyweshouldw.jpg?itok=kg8-UmLg" width="926" height="716" alt="Space weather" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;Space weather from Sun to Earth, in this case caused by a &lt;a href="https://www2.hao.ucar.edu/education/pictorial/coronal-mass-ejection"&gt;coronal mass ejection&lt;/a&gt; (CME).&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;NASA&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;Space weather is a branch of space physics and heliophysics, the science of understanding the Sun and its connection with the solar system.&amp;nbsp;&lt;/p&gt;

&lt;p&gt;Like Earth's weather, space weather describes the variable conditions in the space environment between Earth and the Sun. Extreme space weather can impact our technology in space such as satellites, but also interfere with communication systems, global navigation satellite systems such as GPS, and damage our power electric power grid. Therefore space weather is &lt;a href="https://www.swpc.noaa.gov"&gt;monitored continuously&lt;/a&gt; to protect our infrastructure.&lt;/p&gt;&lt;/div&gt;
      
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</description>
  <pubDate>Wed, 02 Feb 2022 18:57:13 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">374 at https://www2.hao.ucar.edu</guid>
    </item>
<item>
  <title>How does the Sun affect our climate?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/how-does-sun-affect-our-climate</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;How does the Sun affect our climate?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T11:42:59-07:00" title="Wednesday, February 2, 2022 - 11:42" class="datetime"&gt;Wed, 02/02/2022 - 11:42&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;The Sun drives the weather on planet Earth. The winds and circulation of ocean patterns are all affected by the Sun's energy output. The differential heating of the planet, due to the tilt of the rotation axis of the Earth with respect to the Sun, generates the winds and major ocean currents as well as providing us with our seasons. Furthermore, it is believed that the &lt;a href="https://www2.hao.ucar.edu/education/pictorial/sunspot-cycle"&gt;11-year solar cycle&lt;/a&gt; has an impact on our climate.&amp;nbsp;&lt;/p&gt;


&lt;figure class="media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/010417_TS_atlantic-current_main.jpg?itok=j2GGpMee" width="926" height="495" alt="Ocean currents" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;Ocean currents.&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;JPL-CALTECH/NASA&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;An excellent review of the climatic impact of the Sun on Earth can be found at the &lt;a href="https://www.swpc.noaa.gov/impacts/space-weather-impacts-climate"&gt;Space Weather Prediction Center&lt;/a&gt; (NOAA).&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 18:42:59 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">373 at https://www2.hao.ucar.edu</guid>
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<item>
  <title>How does the Sun affect communications?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/how-does-sun-affect-communications</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;How does the Sun affect communications?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T11:34:56-07:00" title="Wednesday, February 2, 2022 - 11:34" class="datetime"&gt;Wed, 02/02/2022 - 11:34&lt;/time&gt;
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        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/AEHF_1.jpg?itok=LkxuSnDW" width="926" height="661" alt="Communication satellite" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;Communication satellite.&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;Wikipedia&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;In our technology-based economy we depend heavily on satellites and various forms of high frequency communication systems. Communications and navigation systems used by commercial airliners can be affected by geomagnetic storms which are caused by solar activity. Geomagnetic storms can actually cause the atmosphere of Earth to expand, affecting satellite orbits. An excellent review of these issues can be found at the &lt;a href="https://www.swpc.noaa.gov/impacts/space-weather-and-earths-climate/"&gt;Space Weather Prediction Center &lt;/a&gt;(NOAA).&amp;nbsp;&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 18:34:56 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">372 at https://www2.hao.ucar.edu</guid>
    </item>
<item>
  <title>What are the aurorae?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/what-are-aurorae</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;What are the aurorae?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T11:09:25-07:00" title="Wednesday, February 2, 2022 - 11:09" class="datetime"&gt;Wed, 02/02/2022 - 11:09&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;The northern lights occur near the north pole of earth. The phenomena is known as the aurora borealis when it occurs in the northern hemisphere and as the aurora australis when it occurs in the southern hemisphere. The name aurora borealis comes from the Latin for northern dawn.&lt;/p&gt;


&lt;figure class="align-left media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/mechanism-aurora.jpg?itok=tJpty6Jg" width="926" height="682" alt="The mechanism for aurorae" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;The mechanism for aurorae.&lt;/p&gt;

          &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;We now know what causes these spectacular displays in the sky. The interaction of the solar wind with the geomagnetic field of the Earth cause energetic particles (primarily electrons and protons) — a million tons of it — to enter into the Earth's upper atmosphere. There they interact with molecules of nitrogen and oxygen to produce the red and green light seen in the auroral phenomena.&lt;/p&gt;

&lt;p&gt;Auroral phenomena have been observed on other planets of our solar system, including Jupiter, Saturn, and even Mars.&lt;br&gt;
&amp;nbsp;&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 18:09:25 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">371 at https://www2.hao.ucar.edu</guid>
    </item>
<item>
  <title>How does the Sun work?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/how-does-sun-work</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;How does the Sun work?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T10:28:50-07:00" title="Wednesday, February 2, 2022 - 10:28" class="datetime"&gt;Wed, 02/02/2022 - 10:28&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;The Sun is a giant, natural thermonuclear reactor that converts hydrogen to helium in its core to produce the heat we sense on our faces as sunshine.&amp;nbsp;&lt;/p&gt;


&lt;figure class="align-right media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/SunFusion.jpg?itok=TSotmkeB" width="926" height="843" alt="The outward pressure of fusion balances the inward force of gravity" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;The outward pressure of fusion balances the inward force of gravity.&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;https://cnx.org/contents/22C4lQHJ@8/Nuclear-Fusion&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;Why does this reactor not explode as a thermonuclear bomb? The Sun is held together in an equilibrium state by the mutual gravitational attraction between all its atoms acting to compress the solar center. These gravitational forces produce and contain the nuclear reactions taking place there. The solar atmosphere outside the energy generating core adjusts itself to carry the enormous amount of energy that emerges from the surface in the form of radiation.&amp;nbsp;&lt;/p&gt;

&lt;p&gt;This is the basic idea behind the existence of all stars beginning with gravitational attraction and compression of a gas cloud to the beginning of nuclear energy generation and, finally, to the exhaustion of the nuclear fuel and death of the star.&lt;br&gt;
&amp;nbsp;&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 17:28:50 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">370 at https://www2.hao.ucar.edu</guid>
    </item>
<item>
  <title>What tools do scientists use to study the Sun?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/what-tools-do-scientists-use-to-study-sun</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;What tools do scientists use to study the Sun?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T09:49:18-07:00" title="Wednesday, February 2, 2022 - 09:49" class="datetime"&gt;Wed, 02/02/2022 - 09:49&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;Scientists study the Sun using satellites and ground-based telescopes, observing everything from the sun's outer atmosphere to its surface and interior.&lt;/p&gt;


&lt;figure class="align-right media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/Solar_Dynamics_Observatory_1.jpg?itok=FfJ3mBla" width="926" height="521" alt="Solar Dynamics Observatory (SDO)" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;Artist rendering of Solar Dynamics Observatory (SDO) in orbit (launched in 2010).&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;NASA&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;Since the magnetic field of the Sun is so important, scientists observe the Sun in as many wavelengths as possible near the various emission and absorption lines of atoms near the Sun's surface.&lt;/p&gt;

&lt;p&gt;Since we cannot see the interior of the Sun, scientists must use indirect methods. For instance, if you strike an object, you can tell something about its substance by the way it vibrates in response (a bell will ring, and jello will just wiggle). The same applies to the Sun. The movement of material inside the Sun (such as dynamic flares and &lt;a href="https://www2.hao.ucar.edu/education/pictorial/coronal-mass-ejection"&gt;CMEs&lt;/a&gt;) produces pressure waves that make the Sun’s surface vibrate. With very accurate telescopes the vibrations can be measured, and then carefully analyzed to determine properties of the interior. This is a very exciting new field, &lt;a href="https://en.wikipedia.org/wiki/Helioseismology"&gt;helioseismology&lt;/a&gt;.&lt;br&gt;
&amp;nbsp;&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 16:49:18 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">369 at https://www2.hao.ucar.edu</guid>
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<item>
  <title>Why is it important to study the Sun?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/why-it-important-study-sun</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;Why is it important to study the Sun?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T09:19:32-07:00" title="Wednesday, February 2, 2022 - 09:19" class="datetime"&gt;Wed, 02/02/2022 - 09:19&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;Variations of the Sun's output do occur, and these affect the Earth's climate. Indeed, tree ring studies and ice core studies indicate a correlation between Earth's ice ages and the Sun's activity.&lt;/p&gt;


&lt;figure class="align-right media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/Coronal%20mass%20ejections.jpg?itok=wQu-IZMX" width="926" height="890" alt="Coronal Mass Ejection" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;A large coronal mass ejection (CME) blasting solar material into space.&lt;/p&gt;

              &lt;p class&gt;&lt;small&gt;&lt;em&gt;SOHO (ESA/NASA)&lt;/em&gt;&lt;/small&gt;&lt;/p&gt;
      &lt;/figcaption&gt;
  &lt;/figure&gt;


&lt;p&gt;The Sun’s powerful eruptions can also disrupt life on Earth. &lt;a href="https://www2.hao.ucar.edu/education/pictorial/coronal-mass-ejection"&gt;Coronal mass ejections&lt;/a&gt; (or CMEs) occur when large amounts of material are ejected from the Sun’s corona into interplanetary space. &amp;nbsp;These CMEs can carry a million tons of material out towards the planets at a million miles an hour (almost a billion kg at 27 million m/s). When a portion of this material reaches the Earth's outer atmosphere, it impacts satellites, perturbing their orbits, scoring their surfaces, and disrupting communications. The solar material can slide down the Earth's magnetic field lines and cause the phenomenon known as &lt;a href="https://www2.hao.ucar.edu/education/about-the-sun/what-are-aurorae-2"&gt;aurora&lt;/a&gt;, and also burn out power grids. CMEs occur perhaps once a month or so during solar minimum, and up to twice or more a day at solar maximum (&lt;a href="https://www2.hao.ucar.edu/hao-science/science-topic/long-term-solar-variability-lsv"&gt;read more about the solar cycle&lt;/a&gt;).&lt;/p&gt;
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  <pubDate>Wed, 02 Feb 2022 16:19:32 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">368 at https://www2.hao.ucar.edu</guid>
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  <title>What are some historical observations of the Sun?</title>
  <link>https://www2.hao.ucar.edu/education/about-the-sun/what-are-some-historical-observations-sun</link>
  <description>&lt;span class="field field--name-title field--type-string field--label-hidden"&gt;What are some historical observations of the Sun?&lt;/span&gt;
&lt;span class="field field--name-uid field--type-entity-reference field--label-hidden"&gt;&lt;span&gt;kolinski&lt;/span&gt;&lt;/span&gt;
&lt;span class="field field--name-created field--type-created field--label-hidden"&gt;&lt;time datetime="2022-02-02T08:45:18-07:00" title="Wednesday, February 2, 2022 - 08:45" class="datetime"&gt;Wed, 02/02/2022 - 08:45&lt;/time&gt;
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            &lt;div class="clearfix text-formatted field field--name-field-body field--type-text-long field--label-hidden field__item"&gt;&lt;p&gt;The Sun has been studied by humans for a long time. Eclipses were likely first recorded prior to 1948 B.C. Astronomers in China noticed sunspots several thousand years ago: the I-Ching or "Book of Changes," which dates back to the 12th century B.C., mentions a "Ri Zhong Jian Mei," which means "a obscuration was seen within the Sun". The first written record of a sunspot sighting dates to 28 B.C (by Chinese astronomers).&lt;/p&gt;

&lt;p&gt;Telescopic observations of the Sun's surface began around 1610. It was at this time that the sunspots could be systematically observed and were, by &lt;a href="https://www2.hao.ucar.edu/education/scientists/galileo-galilei-1564-1642"&gt;Galileo&lt;/a&gt;, &lt;a href="https://www2.hao.ucar.edu/education/scientists/johannes-fabricius-1587-1616"&gt;Fabricius&lt;/a&gt;, &lt;a href="https://www2.hao.ucar.edu/education/scientists/christoph-scheiner-1575-1650"&gt;Scheiner&lt;/a&gt; and &lt;a href="https://www2.hao.ucar.edu/education/scientists/thomas-harriot-1560-1621"&gt;Harriot&lt;/a&gt;. For Galileo this was actually unlucky. Western religions expected the Sun to have no "blemishes" and the observations of sunspots did not further his career at all. He was forced to recant and placed under house arrest.&lt;/p&gt;

&lt;p&gt;Nevertheless, &lt;a href="https://www2.hao.ucar.edu/education/pictorial/sunspot-cycle"&gt;observations of sunspots&lt;/a&gt; and the Sun continued. Around 1645 the sunspot count became very low until 1715. During these 70 years, there were likely less than 15 sunspots observed. These days, the minimum number observed per year is more like 15, even when the Sun is in its "inactive" phase. Interestingly, Europe had cooler than normal temperatures at this same time. So there is some indication that variations occurred in the Sun at the same time which cooled Earth's climate. This time period is referred to as the "Little Ice Age", and the sunspot absence as the Maunder Minimum.&lt;/p&gt;


&lt;figure class="media media--type-image media--view-mode-default figure mb-1 mb-md-4"&gt;
  
        &lt;img loading="lazy" src="https://www2.hao.ucar.edu/sites/default/files/styles/extra_large/public/2022-02/Sunspot_Numbers.png?itok=g9hk58PI" width="926" height="386" alt="400 years of sunspot observations" class="image-style-extra-large img-fluid"&gt;



      &lt;figcaption class="figure-caption pb-1"&gt;
          &lt;p&gt;400 years of sunspot observations.&lt;/p&gt;

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  <pubDate>Wed, 02 Feb 2022 15:45:18 +0000</pubDate>
    <dc:creator>kolinski</dc:creator>
    <guid isPermaLink="false">367 at https://www2.hao.ucar.edu</guid>
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