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<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="m11540">
  <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/">Convolution - Analog</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/">1.7</md:version>
  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/08/06 08:22:01 GMT-5</md:created>
  <md:revised xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/08/08 04:14:26.951 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="richb">
      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Richard</md:firstname>
      <md:othername xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">G.</md:othername>
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Baraniuk</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">richb@rice.edu</md:email>
    </md:author>
    <md:author xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="Anders">
      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Anders</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Gjendemsjo</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">gjendems@NO-SPAM.tele.ntnu.no</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="Anders">
      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Anders</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Gjendemsjo</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">gjendems@NO-SPAM.tele.ntnu.no</md:email>
    </md:maintainer>
  </md:maintainerlist>
  
  <md:keywordlist xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Convolution</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Derivation</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Analog</md:keyword>
  </md:keywordlist>

  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Introduces convolution for analog signals.</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="s0p1">
	In this module we examine convolution for continuous
	time signals. This will
	result in the convolution integral and
	its <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/" document="m10088">properties</cnxn>.
	These concepts are very important in Electrical
	Engineering and will make any engineer's life a lot easier if
	the time is spent now to truly understand what is going on.
      </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="s0p2">
	In order to fully understand convolution,
	you may find it useful to look at 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/" document="m10087">discrete-time convolution</cnxn> as well.
	Accompanied to this module there is a fully worked out <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/" document="m11541">example</cnxn> with mathematics and figures.
	It will also be helpful to experiment with the <link xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" src="http://www.jhu.edu/~signals/convolve/">Convolution
        - Continuous time</link> applet available from
	<link xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" src="http://www.jhu.edu">Johns Hopkins University</link>.  These resources offers different approaches
	to this crucial concept.
      </para>

    <section 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="s2">
      <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/">Derivation of the convolution integral</name>
      <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="s2p1">
	The derivation used here closely follows the one discussed in
	the motivation	section above.  To begin this, it is necessary to state the
	assumptions we will be making.  In this instance, the only
	constraints on our system are that it be linear and
	time-invariant.

	<list 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="list1" type="enumerated">
	  <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/">Brief Overview of Derivation Steps:</name>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">An impulse input leads to an impulse response output.</item>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	    A shifted impulse input leads to a shifted impulse response
	    output.  This is due to the time-invariance of the system.
	  </item>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	    We now scale the impulse input to get a scaled impulse
	    output.  This is using the scalar multiplication property of
	    linearity.
	  </item>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	    We can now "sum up" an infinite number of these scaled
	    impulses to get a sum of an infinite number of scaled
	    impulse responses.  This is using the additivity attribute
	    of linearity.
	  </item>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	    Now we recognize that this infinite sum is nothing more than
	    an integral, so we convert both sides into integrals.
	  </item>
	  <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	    Recognizing that the input is the function
	    <m:math display="inline">
	      <m:apply>
		<m:ci type="function">f</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	    </m:math>, we also recognize that the output is exactly the
	    convolution integral.
	  </item>
	</list>
      </para>

      <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="f1">
	<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="ctimpresp1.png"/>
	<caption xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	  We begin with a system defined by its impulse response,
	  <m:math display="inline">
	    <m:apply>
	      <m:ci type="function">h</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	  </m:math>.
	</caption>
      </figure>

      <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="f2">
	<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="ctimpresp2.png"/>
	<caption xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	  We then consider a shifted version of the input impulse.
	  Due to the time invariance of the system, we obtain a
	  shifted version of the output impulse response.
	</caption>
      </figure>

      <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="fig3">
	<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="ctimpresp3.png"/>
	<caption xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	  Now we use the scaling part of linearity by scaling the
	  system by a value,
	  <m:math display="inline">
	    <m:apply>
	      <m:ci type="function">f</m:ci>
	      <m:ci>τ</m:ci>
	    </m:apply>
	  </m:math>,
	  that is constant with respect to the system variable,
	  <m:math><m:ci>t</m:ci></m:math>.
	</caption>
      </figure>

      <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="f4">
	<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="ctimpresp4.png"/>
	<caption xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">
	  We can now use the additivity aspect of linearity to add an
	  infinite number of these, one for each possible
	  <m:math><m:ci>τ</m:ci></m:math>.  Since an infinite sum
	  is exactly an integral, we end up with the integration known
	  as the Convolution Integral.  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/" document="m11478" target="s2s1">
	  sampling property</cnxn>, we recognize the left-hand side simply as the input
	  <m:math>
	    <m:apply>
	      <m:ci type="fn">f</m:ci>
	      <m:ci>t</m:ci>
	    </m:apply>
	  </m:math>.
	</caption>
      </figure>
    </section>
    
    <section 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="s3">
      <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/">Convolution Integral</name>
      <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="s3p1">
	As mentioned above, the convolution integral provides an easy
	mathematical way to express the output of an LTI system based
	on an arbitrary signal,
	<m:math>
	  <m:apply>
	    <m:ci>x</m:ci>
	    <m:ci>t</m:ci>
	  </m:apply>
	</m:math>, and the system's impulse response,
	<m:math>
	  <m:apply>
	    <m:ci>h</m:ci>
	    <m:ci>t</m:ci>
	  </m:apply>
	</m:math>.  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/">convolution integral</term> is expressed 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="eqn1">
	  <m:math>
	    <m:apply>
	      <m:eq/>
	      <m:apply>
		<m:ci>y</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	      <m:apply>
		<m:int/>
		<m:bvar>
		  <m:ci>τ</m:ci>
		</m:bvar>
		<m:lowlimit>
		  <m:apply>
		    <m:minus/>
		    <m:infinity/>
		  </m:apply>
		</m:lowlimit>
		<m:uplimit>
		  <m:infinity/>
		</m:uplimit>
		<m:apply>
		  <m:times/>
		  <m:apply>
		    <m:ci>x</m:ci>
		    <m:ci>τ</m:ci>
		  </m:apply>
		  <m:apply>
		    <m:ci>h</m:ci>
		    <m:apply>
		      <m:minus/>
		      <m:ci>t</m:ci>
		      <m:ci>τ</m:ci>
		    </m:apply>
		  </m:apply>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:math>
	</equation>

	Convolution is such an important tool that it is represented
	by the symbol *, and can be written 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="eqn2">
	  <m:math>
	    <m:apply>
	      <m:eq/>
	      <m:apply>
		<m:ci>y</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	      <m:apply>
		<m:csymbol definitionURL="http://cnx.rice.edu/cd/cnxmath.ocd#convolve"/>
		<m:apply>
		  <m:ci>x</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
		<m:apply>
		  <m:ci>h</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:math>
	</equation>

	By making a simple change of variables into the convolution
	integral,
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:ci>τ</m:ci>
	    <m:apply>
	      <m:minus/>
	      <m:ci>t</m:ci>
	      <m:ci>τ</m:ci>
	    </m:apply>
	  </m:apply>
	</m:math>,
	we can easily show that convolution is
	<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/">commutative</term>:

	<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="eqn3">
	  <m:math>
	    <m:apply>
	      <m:eq/>
	      <m:apply>
		<m:csymbol definitionURL="http://cnx.rice.edu/cd/cnxmath.ocd#convolve"/>
		<m:apply>
		  <m:ci>x</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
		<m:apply>
		  <m:ci>h</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
	      </m:apply>
	      <m:apply>
		<m:csymbol definitionURL="http://cnx.rice.edu/cd/cnxmath.ocd#convolve"/>
		<m:apply>
		  <m:ci>h</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
		<m:apply>
		  <m:ci>x</m:ci>
		  <m:ci>t</m:ci>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:math>
	</equation> which gives an equivivalent form of <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="eqn1"/>
	<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="eqn4">
	    <m:math>
	        <m:apply>
		    <m:eq/>
		    <m:apply>
			<m:ci>y</m:ci>
			<m:ci>t</m:ci>
		    </m:apply>
		    <m:apply>
			<m:int/>
			<m:bvar><m:ci>τ</m:ci></m:bvar>
			<m:lowlimit><m:apply><m:minus/><m:infinity/></m:apply></m:lowlimit>
			<m:uplimit><m:infinity/></m:uplimit>
			<m:apply>
			    <m:times/>
			    <m:apply>
				<m:ci>x</m:ci>
				<m:apply>
				    <m:minus/>
				    <m:ci>t</m:ci>
				    <m:ci>τ</m:ci>
				</m:apply>
			    </m:apply>
		  	    <m:apply>
			        <m:ci>h</m:ci>
				<m:ci>τ</m:ci>
			    </m:apply>
			</m:apply>
		    </m:apply>
	        </m:apply>
	    </m:math>
	</equation>
	

	For more information on the characteristics of the convolution
	integral, read about 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/" document="m10088">Properties of Convolution</cnxn>.
      </para>
    </section><!-- end section s3-->

    
    <section 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="s4">
      <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/">Implementation of Convolution</name>
      <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="s4p1">
	Taking a closer look at the convolution integral, we find that
	we are multiplying the input signal by the time-reversed
	impulse response and integrating.  This will give us the value
	of the output at one given value of <m:math display="inline"><m:ci>t</m:ci></m:math>.  If we then shift
	the time-reversed impulse response by a small amount, we get
	the output for another value of <m:math display="inline"><m:ci>t</m:ci></m:math>.  Repeating this for
	every possible value of <m:math display="inline"><m:ci>t</m:ci></m:math>, yields the total
	output function.  While we would never actually do this
	computation by hand in this fashion, it does provide us with
	some insight into what is actually happening.  We find that we
	are essentially reversing the impulse response function and
	sliding it across the input function, integrating as we go.
	This method, referred to as 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/">graphical method</term>,
	provides us with a much simpler way to solve for the output
	for simple (contrived) signals, while improving our intuition
	for the more complex cases where we rely on computers.  In
	fact <link xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" src="http://www.ti.com">Texas Instruments</link>
	develops <link xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" src="http://dspvillage.ti.com/docs/toolssoftwarehome.jhtml">Digital
	Signal Processors</link> which have special instruction sets
	for computations such as convolution.
      </para>
    </section>

    <section 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="s5">
        <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/">Summary</name>
	<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="s5p1">
	    Convolution is a truly important concept, which <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/">must</emphasis>
	    be well understood.
	</para>
        <note 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="convoltion integral">

	  <m:math>
	    <m:apply>
	      <m:eq/>
	      <m:apply>
		<m:ci>y</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	      <m:apply>
		<m:int/>
		<m:bvar>
		  <m:ci>τ</m:ci>
		</m:bvar>
		<m:lowlimit>
		  <m:apply>
		    <m:minus/>
		    <m:infinity/>
		  </m:apply>
		</m:lowlimit>
		<m:uplimit>
		  <m:infinity/>
		</m:uplimit>
		<m:apply>
		  <m:times/>
		  <m:apply>
		    <m:ci>x</m:ci>
		    <m:ci>τ</m:ci>
		  </m:apply>
		  <m:apply>
		    <m:ci>h</m:ci>
		    <m:apply>
		      <m:minus/>
		      <m:ci>t</m:ci>
		      <m:ci>τ</m:ci>
		    </m:apply>
		  </m:apply>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:math>

	</note>
	<note 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="convoltion integral">
	  <m:math>
	    <m:apply>
	      <m:eq/>
	      <m:apply>
		<m:ci>y</m:ci>
		<m:ci>t</m:ci>
	      </m:apply>
	      <m:apply>
		<m:int/>
		<m:bvar>
		  <m:ci>τ</m:ci>
		</m:bvar>
		<m:lowlimit>
		  <m:apply>
		    <m:minus/>
		    <m:infinity/>
		  </m:apply>
		</m:lowlimit>
		<m:uplimit>
		  <m:infinity/>
		</m:uplimit>
		<m:apply>
		  <m:times/>
		  <m:apply>
		    <m:ci>h</m:ci>
		    <m:ci>τ</m:ci>
		  </m:apply>
		  <m:apply>
		    <m:ci>x</m:ci>
		    <m:apply>
		      <m:minus/>
		      <m:ci>t</m:ci>
		      <m:ci>τ</m:ci>
		    </m:apply>
		  </m:apply>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:math>

	</note>
    </section>
      
   <section 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="s6">
        <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="s6p1">
	    Go to? 
	    <list 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="l1" type="inline">
	        <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/"><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/" document="m11542">Introduction</cnxn></item>
	        <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/"><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/" document="m11541">Convolution - Full example</cnxn></item>
	        <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/"><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/" document="m10087">Convolution - Discrete time</cnxn></item>
	        <item xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/"><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/" document="m10088">Properties of convolution</cnxn></item>
	    </list>
	</para>
    </section>

  </content>
  
</document>
