<?xml version="1.0" encoding="utf-8" standalone="no"?>
<!DOCTYPE document PUBLIC "-//CNX//DTD CNXML 0.5 plus MathML//EN" "http://cnx.rice.edu/cnxml/0.5/DTD/cnxml_mathml.dtd">
<document xmlns="http://cnx.rice.edu/cnxml" 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="new13">
  <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/">Power</name>
  <metadata xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
  <md:version xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">**new**</md:version>
  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/06/13 10:29:17.887 GMT-5</md:created>
  <md:revised xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/06/13 13:33:01.272 GMT-5</md:revised>
  <md:authorlist xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
    <md:author xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="wlw">
      <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@rice.edu</md:email>
    </md:author>
  </md:authorlist>

  <md:maintainerlist xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
    <md:maintainer xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="wlw">
      <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@rice.edu</md:email>
    </md:maintainer>
    <md:maintainer xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="lizzardg">
      <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/">lizzardg@rice.edu</md:email>
    </md:maintainer>
    <md:maintainer xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="jsilv">
      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Jeffrey</md:firstname>
      
      <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/">jsilv@rice.edu</md:email>
    </md:maintainer>
  </md:maintainerlist>
  
  

  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">How to calculate the power that flows into and out of a line, as well as average power.</md:abstract>
</metadata>

  <content xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
    <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">You might be tempted to now say that
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:msub>
	    <m:mi>P</m:mi>
	    <m:mi>in</m:mi>
	  </m:msub>
	  <m:apply>
	    <m:times/>
	    <m:msub>
	      <m:mi>V</m:mi>
	      <m:mi>in</m:mi>
	    </m:msub>
	    <m:msub>
	      <m:mi>I</m:mi>
	      <m:mi>in</m:mi>
	    </m:msub>
	  </m:apply>
	</m:apply>
      </m:math>, but that is incorrect for sinusoidal excitation.  
      <m:math>
	<m:msub>
	  <m:mi>V</m:mi>
	  <m:mi>in</m:mi>
	</m:msub>
      </m:math> and
      <m:math>
	<m:msub>
	  <m:mi>I</m:mi>
	  <m:mi>in</m:mi>
	</m:msub>
      </m:math> are <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">phasors</emphasis>! So let's digress for
      a second to see (or review, I hope) how to find power when the
      voltage and current are phasor quantities. What really matters
      is not the absolute phase angle of the two quantities, but
      rather the phase angle between them.  Suppose we have a voltage
      phasor, <m:math><m:ci>V</m:ci></m:math> which has zero phase
      angle and a complex impedance
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:ci>Z</m:ci>
	  <m:apply>
	    <m:times/>
	    <m:apply>
	      <m:abs/>
	      <m:ci>Z</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:exp/>
	      <m:apply>
		<m:times/>
		<m:imaginaryi/>
		<m:msub>
		  <m:mi>θ</m:mi>
		  <m:mi>z</m:mi>
		</m:msub>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:apply>
      </m:math>. Obviously, the current is given by
      <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:mover>
	      <m:mi>I</m:mi>
	      <m:mo>˜</m:mo>
	    </m:mover>
	    <m:apply>
	      <m:divide/>
	      <m:mover>
		<m:mi>V</m:mi>
		<m:mo>˜</m:mo>
	      </m:mover>
	      <m:mover>
		<m:mi>Z</m:mi>
		<m:mo>˜</m:mo>
	      </m:mover>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:apply>
		  <m:abs/>
		  <m:ci>V</m:ci>
		</m:apply>
		<m:apply>
		  <m:abs/>
		  <m:ci>Z</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:exp/>
		<m:apply>
		  <m:minus/>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>
	
      To find power, we can not work just with phasors, we have to go
      back to the complete function of time as well so we write:

      <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:ci type="fn">V</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:abs/>
		<m:ci>V</m:ci>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:apply>
		  <m:times/>
		  <m:ci>ω</m:ci>
		  <m:ci>t</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="eq3">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:ci type="fn">I</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:apply>
		  <m:abs/>
		  <m:ci>V</m:ci>
		</m:apply>
		<m:apply>
		  <m:abs/>
		  <m:ci>Z</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:apply>
		  <m:minus/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</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="eq4">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:ci type="fn">I</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:abs/>
		<m:ci>I</m:ci>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:apply>
		  <m:minus/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>The power as a function of time is given as
      <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="eq5">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:ci type="fn">P</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:ci type="fn">I</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	      <m:apply>
		<m:ci type="fn">V</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:abs/>
		<m:ci>V</m:ci>
	      </m:apply>
	      <m:apply>
		<m:abs/>
		<m:ci>V</m:ci>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:apply>
		  <m:times/>
		  <m:ci>ω</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:apply>
		  <m:minus/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>We remember a useful trig identity:
      <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="eq6">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:cos/>
	      <m:apply>
		<m:minus/>
		<m:ci>A</m:ci>
		<m:ci>B</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:plus/>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:cos/>
		  <m:ci>A</m:ci>
		</m:apply>
		<m:apply>
		  <m:cos/>
		  <m:ci>B</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:sin/>
		  <m:ci>A</m:ci>
		</m:apply>
		<m:apply>
		  <m:sin/>
		  <m:ci>B</m:ci>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>Hence:
      <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="eq7">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:cos/>
	      <m:apply>
		<m:minus/>
		<m:apply>
		  <m:times/>
		  <m:ci>ω</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
		<m:msub>
		  <m:mi>θ</m:mi>
		  <m:mi>z</m:mi>
		</m:msub>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:plus/>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:cos/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		</m:apply>
		<m:apply>
		  <m:cos/>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:sin/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		</m:apply>
		<m:apply>
		  <m:sin/>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>which makes
      <m:math>
	<m:apply>
	  <m:ci type="fn">P</m:ci>
	  <m:ci>t</m:ci>
	</m:apply>
      </m:math>

      <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="eq8">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:ci type="fn">P</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:plus/>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:power/>
		  <m:apply>
		    <m:cos/>
		    <m:apply>
		      <m:times/>
		      <m:ci>ω</m:ci>
		      <m:ci>t</m:ci>
		    </m:apply>
		  </m:apply>
		  <m:cn>2</m:cn>
		</m:apply>
		<m:apply>
		  <m:cos/>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:cos/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		</m:apply>
		<m:apply>
		  <m:sin/>
		  <m:apply>
		    <m:times/>
		    <m:ci>ω</m:ci>
		    <m:ci>t</m:ci>
		  </m:apply>
		</m:apply>
		<m:apply>
		  <m:sin/>
		  <m:msub>
		    <m:mi>θ</m:mi>
		    <m:mi>z</m:mi>
		  </m:msub>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>We are really interested in finding <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">average
	power</emphasis> since energy which flows into and then back
      out of the line does no work for us. Clearly the second term
      in <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="eq8"/> (going as
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:apply>
	    <m:cos/>
	    <m:apply>
	      <m:times/>
	      <m:ci>ω</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	  </m:apply>
	  <m:apply>
	    <m:sin/>
	    <m:apply>
	      <m:times/>
	      <m:ci>ω</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	  </m:apply>
	</m:apply>
      </m:math>) has an average value of zero, and so we can forget
      about it. Time for one more trig identity:
      <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="eq9">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:power/>
	      <m:apply>
		<m:cos/>
		<m:ci>A</m:ci>
	      </m:apply>
	      <m:cn>2</m:cn>
	    </m:apply>
	    <m:apply>
	      <m:plus/>
	      <m:apply>
		<m:divide/>
		<m:cn>1</m:cn>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:divide/>
		  <m:cn>1</m:cn>
		  <m:cn>2</m:cn>
		</m:apply>
		<m:apply>
		  <m:cos/>
		  <m:apply>
		    <m:times/>
		    <m:cn>2</m:cn>
		    <m:ci>A</m:ci>
		  </m:apply>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>
      <m:math>
	<m:apply>
	  <m:cos/>
	  <m:apply>
	    <m:times/>
	    <m:cn>2</m:cn>
	    <m:ci>ω</m:ci>
	    <m:ci>t</m:ci>
	  </m:apply>
	</m:apply>
      </m:math> has zero average value as well, so we are left with
      the following for the average value of the power
      <m:math>
	<m:apply>
	  <m:mean/>
	  <m:apply>
	    <m:ci type="fn">P</m:ci>
	    <m:ci>t</m:ci>
	  </m:apply>
	</m:apply>
      </m:math>
      <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="eq10">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:mean/>
	      <m:apply>
		<m:ci type="fn">P</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:apply>
		  <m:times/>
		  <m:apply>
		    <m:abs/>
		    <m:ci>V</m:ci>
		  </m:apply>
		  <m:apply>
		    <m:abs/>
		    <m:ci>I</m:ci>
		  </m:apply>
		</m:apply>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:msub>
		  <m:mi>θ</m:mi>
		  <m:mi>z</m:mi>
		</m:msub>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:apply>
		  <m:power/>
		  <m:apply>
		    <m:abs/>
		    <m:ci>V</m:ci>
		  </m:apply>
		  <m:cn>2</m:cn>
		</m:apply>
		<m:apply>
		  <m:times/>
		  <m:cn>2</m:cn>
		  <m:apply>
		    <m:abs/>
		    <m:ci>Z</m:ci>
		  </m:apply>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:msub>
		  <m:mi>θ</m:mi>
		  <m:mi>z</m:mi>
		</m:msub>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>
      Note that one useful way that people sometimes use to express
      this is to say
      <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="eq11">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:mean/>
	      <m:apply>
		<m:ci type="fn">P</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:cn>1</m:cn>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:mover>
		  <m:mi>V</m:mi>
		  <m:mo>˜</m:mo>
		</m:mover>
		<m:msup>
		  <m:mover>
		    <m:mi>V</m:mi>
		    <m:mo>˜</m:mo>
		  </m:mover>
		  <m:mo>*</m:mo>
		</m:msup>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>

      Back to our example:
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:msub>
	    <m:mi>V</m:mi>
	    <m:mi>in</m:mi>
	  </m:msub>
	  <m:cn type="complex-polar">4.18<m:sep/>38</m:cn>
	</m:apply>
      </m:math> and
      <m:math>
	<m:apply>
	  <m:eq/>
	  <m:msub>
	    <m:mi>I</m:mi>
	    <m:mi>in</m:mi>
	  </m:msub>
	  <m:cn type="complex-polar">0.144<m:sep/>21</m:cn>
	</m:apply>
      </m:math> Thus

      <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="eq12">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:mean/>
	      <m:apply>
		<m:ci type="fn">
		  <m:msub>
		    <m:mi>P</m:mi>
		    <m:mi>in</m:mi>
		  </m:msub>
		</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:cn>1</m:cn>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:times/>
		<m:cn>4.18</m:cn>
		<m:cn>0.144</m:cn>
	      </m:apply>
	      <m:apply>
		<m:cos/>
		<m:cn>59</m:cn>
	      </m:apply>
	      <m:mtext>Watts</m:mtext>
	    </m:apply>
	    <m:cn>0.155</m:cn>
	  </m:apply>
	</m:math>
      </equation>As an alternative way of calculating the power into
      the line note that we <emphasis xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">know</emphasis> the magnitude of
      the current through both the capacitor and the resistor of the
      apparent
      <m:math>
	<m:msub>
	  <m:mi>Z</m:mi>
	  <m:mi>in</m:mi>
	</m:msub>
      </m:math>. They are just two elements in series, and so they both
      have the same current flowing through them, namely,
      <m:math>
	<m:msub>
	  <m:mi>I</m:mi>
	  <m:mi>in</m:mi>
	</m:msub>
      </m:math>. No power is dissipated in the capacitor, so we could
      just as well have said
      <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="eq13">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:mean/>
	      <m:apply>
		<m:ci type="fn">
		  <m:msub>
		    <m:mi>P</m:mi>
		    <m:mi>in</m:mi>
		  </m:msub>
		</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:divide/>
		<m:cn>1</m:cn>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:power/>
		<m:apply>
		  <m:abs/>
		  <m:ci>I</m:ci>
		</m:apply>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:ci>R</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:times/>
		<m:apply>
		  <m:divide/>
		  <m:cn>1</m:cn>
		  <m:cn>2</m:cn>
		</m:apply>
		<m:apply>
		  <m:power/>
		  <m:cn>0.144</m:cn>
		  <m:cn>2</m:cn>
		</m:apply>
	      </m:apply>
	      <m:cn>15</m:cn>
	    </m:apply>
	    <m:cn>0.155</m:cn>
	  </m:apply>
	</m:math>
      </equation> and gotten the answer in an even easier fashion!
      (Note that we still have to keep the factor of "1/2" to account
      for the time average of a sinusoidal product.) For reasons I do
      not understand, students have always had an aversion to finding
      power. It is not that hard, and in the end, is usually the
      "bottom line" with regard to how a system will perform. Go back
      over this section until it makes sense, as you may see power
      crop up someplace else one of these days!
    </para>   
  </content>
  
</document>

