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      <title>The Doppler Effect by ‫איתיאל וילק‬‎</title>
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      <pubDate>2016-08-04 16:55:38 UTC</pubDate>
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         <title>The Doppler Effect</title>
         <author>itielmwilk</author>
         <link>https://padlet.com/itielmwilk/mmqcxczwl505/wish/117552319</link>
         <description><![CDATA[<div><br><br><br><br></div><div><strong>Doppler Effect in Light: Red Shift &amp; Blue Shift</strong></div><div><br></div><div>the nature of a light wave means that if the object is moving there will be a shift in the spectral lines of that object. Light waves from a moving source experience something called "The Doppler Effect" to result in either a red shift or blue shift in the light's frequency(as seen. This is in a fashion similar (though not identical) to other types of waves, i.e. sound waves. The major difference is that light waves do not require a medium for travel, so the<a href="http://physics.about.com/od/wavessound/a/dopplereffect.htm"> classical application of the Doppler effect</a> doesn't apply precisely to this situation.</div><div><br><br><br></div><div><strong>Relativistic Doppler Effect for Light</strong></div><div><br></div><div>Consider two objects: the light source and the "listener" (or observer). Since light waves traveling in empty space have no medium, we analyze the Doppler effect for light in terms of the motion of the source relative to the listener.</div><div><br></div><div>We set up our coordinate system so that the positive direction is from the listener toward the source. So if the source is moving away from the listener, its velocity <em>v</em> is positive, but if it is moving toward the listener, then the <em>v</em> is negative. The listener, in this instance, is <em>always</em> considered to be at rest (so <em>v</em> is really the total<a href="http://physics.about.com/od/glossary/g/velocity.htm"> relative velocity</a> between them).</div><div><br><br><br><br><br></div><div><strong>Red Shift &amp; Blue Shift</strong></div><div><br></div><div>A light source moving <em>away</em> from the listener (<em>v</em> is positive) would provide an <em>fL</em> that is less than <em>fS</em>. In the<a href="http://physics.about.com/od/lightoptics/a/vislightspec.htm"> visible light spectrum</a>, this causes a shift toward the red end of the light spectrum, so it is called a <em>red shift</em>. When the light source is moving <em>toward</em> the listener (<em>v</em> is negative), then <em>fL</em> is greater than <em>fS</em>. In the<a href="http://physics.about.com/od/lightoptics/a/vislightspec.htm"> visible light spectrum</a>, this causes a shift toward the high-frequency (hf) end of the light spectrum, this is called a <em>blue shift</em>. Obviously, in the area of the<a href="http://physics.about.com/od/lightoptics/a/electrspectrum.htm"> electromagnetic spectrum</a> outside<a href="http://chemistry.about.com/od/chemistryglossary/g/visible-spectrum-definition.htm"> of the visible light spectrum</a>, these alterations might not actually be toward red and blue. If you're in the infrared, for example, you're ironically&nbsp; shifting <em>away</em> from red when you experience a "red shift."</div><div><br><br></div><div><figure class="attachment attachment-preview" data-trix-attachment="{&quot;contentType&quot;:&quot;image&quot;,&quot;height&quot;:270,&quot;url&quot;:&quot;https://lh3.googleusercontent.com/2beFkP9WPPXZpzx9NXl5WvcGDgBIQSEulHd5YR7h6rMGl-mLGIgXK_yqxle3I9cWqqdeW1v85ff0F2bYSITCLmbrWtXTyMtvuxTjWcPynNscoV5wOTp1ZC6HksRXFgAm2He0hq1D&quot;,&quot;width&quot;:401}" data-trix-content-type="image"><img src="https://lh3.googleusercontent.com/2beFkP9WPPXZpzx9NXl5WvcGDgBIQSEulHd5YR7h6rMGl-mLGIgXK_yqxle3I9cWqqdeW1v85ff0F2bYSITCLmbrWtXTyMtvuxTjWcPynNscoV5wOTp1ZC6HksRXFgAm2He0hq1D" width="401" height="270"><figcaption class="caption"></figcaption></figure></div><div><br><br></div><div><em>fL</em> = sqrt [(<em>c</em> - <em>v</em>)/(<em>c</em> + <em>v</em>)] * <em>fS</em></div><div><br></div><div><strong>Applications</strong></div><div><br></div><div>Police put this property to use in the radar boxes they use to track speed.<a href="http://space.about.com/od/astronomydictionary/g/Radio-Waves.htm"> Radio waves</a> are transmitted out, collide with a vehicle, and bounce back. The speed of the vehicle (which acts as the source of the reflected wave) determines the change in frequency, which can be detected with the box. (Similar applications can be used to measure wind velocities in the atmosphere, which is the "<a href="http://physics.about.com/od/physicsintherealworld/f/dopplerradar.htm">Doppler radar</a>" of which meteorologists are so fond.)</div><div><br></div><div>This Doppler shift is also used to track satellites. By observing how the frequency changes, you can determine the velocity relative to your location, which allows ground-based tracking to analyze the movement of objects in space.</div><div><br></div><div>In astronomy, these shifts prove helpful. When observing a system with two stars, you can identify which is moving toward you and which away by analyzing how the frequencies alter.</div><div><br></div><div>Even more significantly, evidence from the analysis of light<a href="http://space.about.com/od/Stargazing-Guides/ss/Octobers-Special-Sky-Sights_5.htm"> from distant galaxies</a> shows that the light experiences a red shift. These galaxies are moving away from the Earth. In fact, the results of this are a bit beyond the mere Doppler effect. This is actually<a href="http://physics.about.com/od/physicsqtot/g/spacetime.htm"> a result of spacetime</a> itself expanding, as predicted by<a href="http://physics.about.com/od/relativisticmechanics/a/relativity_3.htm"> general relativity</a>. Extrapolations of this evidence, along with other findings, support the "<a href="http://physics.about.com/od/astronomy/f/BigBang.htm">big bang</a>" picture of the origin of the universe.</div><div><br><br><br><br><br></div>]]></description>
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         <pubDate>2016-08-04 16:51:07 UTC</pubDate>
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         <author>itielmwilk</author>
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         <pubDate>2016-08-03 17:05:20 UTC</pubDate>
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