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  <name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Introduction to Using the Smith Chart</name>
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  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2000/09/21</md:created>
  <md:revised xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2008/05/28 19:38:06.640 GMT-5</md:revised>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Bill</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Wilson</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">wlw@madriver.net</md:email>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Bill</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Wilson</md:surname>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Elizabeth</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Gregory</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">elizabeth.gregory@gmail.com</md:email>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Jeffrey</md:firstname>
      <md:othername xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">M</md:othername>
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Silverman</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">JSilverman@astro.berkeley.edu</md:email>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Gerard</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Wysocki</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">gerardw@rice.edu</md:email>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Scott</md:firstname>
      <md:othername xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">W</md:othername>
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Kravitz</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">swkravitz@gmail.com</md:email>
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    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">smith chart</md:keyword>
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  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Introducing the Smith Chart.</md:abstract>
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    <para xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="para1">Using the <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="fig1">Smith Chart</cnxn>,
    we will investigate some of the application and uses of the
    <term xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Smith Chart</term>. For the text, we will use my new "mini
    Smith Chart" which is reproduced below.  Clearly, there is not
    much detail here, and our answers will not be as accurate as they
    would be if we used a full size chart, but we want to get ideas
    across here, not the best number possible, and with the small
    size, we won't run out of paper before everything is done.
        
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="fig1">
	<name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">The Smith Chart</name>
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      </figure>
      
      Note that we have a couple of "extras" on the chart.  The two
      scales at the bottom of the chart can be used to either set or
      measure radial variables such as the magnitude of the reflection
      coefficient
      <m:math>
	<m:apply>
	  <m:abs/>
	  <m:ci>Γ</m:ci>
	</m:apply>
      </m:math>, or the VSWR, as it turns out that in practice, what
      one can actually measure on a line is the VSWR.  Remember, there
      is a direct relationship between the VSWR and the magnitude of
      the reflection coefficient.
      <equation xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="eq1">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:ci>VSWR</m:ci>
	    <m:apply>
	      <m:divide/>
	      <m:apply>
		<m:plus/>
		<m:cn>1</m:cn>
		<m:apply>
		  <m:abs/>
		  <m:ci>Γ</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:minus/>
		<m:cn>1</m:cn>
		<m:apply>
		  <m:abs/>
		  <m:ci>Γ</m:ci>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>

      <equation xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="eq2">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:abs/>
	      <m:ci>Γ</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:divide/>
	      <m:apply>
		<m:minus/>
		<m:ci>VSWR</m:ci>
		<m:cn>1</m:cn>
	      </m:apply>
	      <m:apply>
		<m:plus/>
		<m:ci>VSWR</m:ci>
		<m:cn>1</m:cn>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>
      Since
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:apply>
	    <m:abs/>
	    <m:apply>
	      <m:ci type="fn">r</m:ci>
	      <m:ci>s</m:ci>
	    </m:apply>
	  </m:apply>
	  <m:apply>
	    <m:abs/>
	    <m:ci>Γ</m:ci>
	  </m:apply>
	</m:apply>
      </m:math>, once we have the VSWR, we have
      <m:math>
	<m:apply>
	  <m:abs/>
	  <m:apply>
	    <m:ci type="fn">r</m:ci>
	    <m:ci>s</m:ci>
	  </m:apply>
	</m:apply>
      </m:math> and so we know how big a circle we need on the Smith
      Chart in order to go from one place to the next.  Note also that
      there is a scale around the outside of the chart which is given
      in fractions of a wavelength. Since 
      <m:math>
	<m:apply>
	  <m:ci type="fn">r</m:ci>
	  <m:ci>s</m:ci>
	</m:apply>
      </m:math> rotates around at a rate
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:cn>2</m:cn>
	  <m:ci>β</m:ci>
	  <m:ci>s</m:ci>
	</m:apply>
      </m:math> and
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:ci>β</m:ci>
	  <m:apply>
	    <m:divide/>
	    <m:apply>
	      <m:times/>
	      <m:cn>2</m:cn>
	      <m:pi/>
	    </m:apply>
	    <m:ci>λ</m:ci>
	  </m:apply>
	</m:apply>
      </m:math>, we could either show distance in cm or something, and
      then change the scale whenever we change wavelength.  Or, we
      could just use a distance scale in
      <m:math><m:ci>λ</m:ci></m:math>, and measure all
      distances in units of the wavelength.  This is what we shall do.
      Since the rate of rotation is
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:cn>2</m:cn>
	  <m:ci>β</m:ci>
	  <m:ci>s</m:ci>
	</m:apply>
      </m:math>, one trip around the Smith Chart is the same as going
      one half of a wavelength down the line. Rotation in a clockwise
      direction is the same as moving away from the load towards the
      generator, while motion along the line in the other direction
      (towards the load) calls for counterclockwise rotation. The
      scale is, of course, a relative one, and so we will have to
      re-set our zero, depending upon where the load etc. are really
      located. This will all become clearer as we do an example.
    </para>

    <para xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="para2">Let's start out with the simplest thing we can,
      with just a generator, line and load <cnxn xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" target="fig2"/>. Our
      task will be to find the input impedance,
      <m:math>
	<m:msub>
	  <m:mi>Z</m:mi>
	  <m:mi>in</m:mi>
	</m:msub>
      </m:math>, for the line, so that we can figure the input
      voltage.
      
      <figure xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="fig2"><name xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Transmission Line Problem</name><media xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" type="image/png" src="802.png">
<param name="print-width" value="3in"/>
</media></figure>

      For this first problem, we are going to start out with all the
      basics. In later examples, we probably will only give lengths in
      wavelengths, and impedances in terms of
      <m:math>
	<m:msub>
	  <m:mi>Z</m:mi>
	  <m:mn>0</m:mn>
	</m:msub>
      </m:math>, but let's do this the whole way through.
    


    </para>   
  </content>
  
</document>
