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Update embedded youtube videos in the glossary
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@dgarciabriseno
dgarciabriseno committed Feb 22, 2022
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30 changes: 15 additions & 15 deletions dialogs/glossary.html
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<!--
Helioviewer.org Visual Glossary
Dimensions to use for movies/screenshots:
1280x960
Hint: on a 1920x1080 display using the Chrome web browser with bookmarks
hidden, you would want to resize the browser to 1898x1157 to be able
to create full-viewport Helioviewer.org videos with the desired dimensions.
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<div class='glossary-text'>2,500 km thick (1,600 mi) layer of plasma above the Sun’s photosphere. Temperatures range from ~4500 K to 60,000 K (110,000 to 8,000°F). The word chromosphere means, literally, “color sphere” and refers to its reddish color when seen with the naked eye during a total solar eclipse.</div>
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<!-- Convection -->
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<!--CME-->
<tr name='cme' class='g-basic g-fe'>
<td>
<iframe class="youtube-player" type="text/html" src="http://www.youtube.com/embed/TWySQHjIRSg" frameborder="0"></iframe>
<iframe class="youtube-player" type="text/html" src="https://www.youtube.com/embed/TWySQHjIRSg" frameborder="0"></iframe>
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<td>
<div class='glossary-title'>Coronal Mass Ejection (CME)</div>
<div class='glossary-text'>A catastrophic expansion of a part of the coronal magnetic field that causes a huge bubble of plasma and magnetic field to erupt from the Sun. A CME can last for several hours and travels though space at a million miles per hour. CMEs are usually accompanied by a solar flare. The charged particles and magnetic fields associated with CMEs can cause power and communications outages, damage to satellites, and health problems for astronauts. They usually take about three days to reach Earth, but very fast ones can arrive in under a day.</div>
<div class='glossary-text'>A catastrophic expansion of a part of the coronal magnetic field that causes a huge bubble of plasma and magnetic field to erupt from the Sun. A CME can last for several hours and travels though space at a million miles per hour. CMEs are usually accompanied by a solar flare. The charged particles and magnetic fields associated with CMEs can cause power and communications outages, damage to satellites, and health problems for astronauts. They usually take about three days to reach Earth, but very fast ones can arrive in under a day.</div>
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<iframe class="youtube-player" type="text/html" src="http://www.youtube.com/embed/dU0sJm2wgYc" frameborder="0"></iframe>
<iframe class="youtube-player" type="text/html" src="https://www.youtube.com/embed/dU0sJm2wgYc" frameborder="0"></iframe>
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<div class='glossary-title'>Flare</div>
<div class='glossary-text'>A rapid release of vast magnetic energy in a sunspot region, causing temperatures to rise tens of millions of degrees in a small area above the solar surface. The resulting radiation surge can cause blackouts of communication signals and damage to satellites. Flares can produce dangerous EUV radiation, X-rays, gamma rays, and high-energy protons.</div>
<div class='glossary-text'>A rapid release of vast magnetic energy in a sunspot region, causing temperatures to rise tens of millions of degrees in a small area above the solar surface. The resulting radiation surge can cause blackouts of communication signals and damage to satellites. Flares can produce dangerous EUV radiation, X-rays, gamma rays, and high-energy protons.</div>
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<div class='glossary-title'>Ionization</div>
<div class='glossary-text'>A process that produces ions, typically collisions between atoms or electrons, or by interaction with electromagnetic radiation.
<div class='glossary-text'>A process that produces ions, typically collisions between atoms or electrons, or by interaction with electromagnetic radiation.
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<div class='glossary-title'>Magnetogram</div>
<div class='glossary-text'>A magnetogram is an image of the Sun's magnetic flux. They are derived by using emission lines which are magnetically sensitive, which allows the magnetic flux present to be calculated. Currently, only line-of-sight magnetic flux measurements - the amount of magnetic flux that lies along the line-of-sight between the instrument and Sun - are available on Helioviewer.org, from the HMI and MDI instruments. Magnetograms are important as the Sun's magnetic field is thought to play an important role in solar activity.</div>
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<!--Magnetosphere-->
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<div class='glossary-title'>Maunder Minimum</div>
<div class='glossary-text'>From 1645 to 1715, scientists believe there was a decrease in the total energy output from the Sun, as indicated by little or no sunspot activity. This period coincided with a climate event on Earth known as the Little Ice Age.</div>
<div class='glossary-text'>From 1645 to 1715, scientists believe there was a decrease in the total energy output from the Sun, as indicated by little or no sunspot activity. This period coincided with a climate event on Earth known as the Little Ice Age.</div>
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<iframe class="youtube-player" type="text/html" src="http://www.youtube.com/embed/BosmntuHHLo" frameborder="0"></iframe>
<iframe class="youtube-player" type="text/html" src="https://www.youtube.com/embed/BosmntuHHLo" frameborder="0"></iframe>
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<div class='glossary-title'>Prominence</div>
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<i>More Info:</i><br />
<div class='glossary-links'>
<a href='http://www.nasa.gov/mission_pages/sdo/main/index.html' target="_blank">SDO Homepage</a>
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<div class='glossary-text'>Dark areas on the Sun created by strong magnetic fields beneath the Sun’s surface. Sunspots appear dark because they are cooler than the surrounding areas of the photosphere. They range in size from 2,400 km (1,500 mi) to several times Earth’s size. Sunspots usually occur in pairs or groups of opposite magnetic polarity that rotate with the surface of the Sun. They are the footprints of magnetic loops pushing through the surface and holding plasma below. Manifesting intense magnetic activity, sunspots host secondary phenomena such as coronal loops and reconnection events. Most solar flares and coronal mass ejections originate in magnetically active regions around visible sunspot groupings. Similar phenomena indirectly observed on stars are commonly called starspots and both light and dark spots have been measured.</div>
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<div class='glossary-text'>A cluster of multiple sunspots.</div>
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<!--Total Solar Irradiance-->
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