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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/">Noise and Interference</name>

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  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2000/07/27</md:created>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Don</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Johnson</md:surname>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">dhj@rice.edu</md:email>
    </md:author>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Don</md:firstname>
      
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Joe</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Montgomery</md:surname>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Adan</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Galvan</md:surname>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Erin</md:firstname>
      
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Snavely</md:surname>
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      <md:firstname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">John</md:firstname>
      <md:othername xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Austin</md:othername>
      <md:surname xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Cottrell</md:surname>
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  </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/">communication channels</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">information communication</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">interference</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">noise</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">power spectrum</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">white noise</md:keyword>
  </md:keywordlist>

  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Introduction to noise and noise filtering.
</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="intro"> We have mentioned that communications are, to
      varying degrees, subject to interference and noise. It's time to
      be more precise about what these quantities are and how they
      differ.  </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="second">
      <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/">Interference</term> represents man-made signals. Telephone
      lines are subject to power-line interference (in the United
      States a distorted 60 Hz sinusoid). Cellular telephone
      channels are subject to adjacent-cell phone conversations using
      the same signal frequency. The problem with such interference is
      that it occupies the same frequency band as the desired
      communication signal, and has a similar structure.
    </para>

    <exercise 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="exer1">
      <problem 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="exer1a">
	  Suppose interference occupied a different frequency band; how would
	  the receiver remove it?
	</para>
      </problem>
      <solution 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="exer1b">
	  If the interferer's spectrum does not overlap that of our
	  communications channel—the interferer is
	  out-of-band—we need only use a bandpass filter that
	  selects our transmission band and removes other portions of
	  the spectrum.
	</para>
      </solution>
    </exercise>

    <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="third"> 

      We use the notation 
      <m:math><m:apply><m:ci type="fn">i</m:ci><m:ci>t</m:ci></m:apply>
      </m:math> 
      to represent interference. Because interference has man-made
      structure, we can write an explicit expression for it that may contain
      some unknown aspects (how large it is, for 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="fourth">
      <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/">Noise</term> signals have little structure and arise from
      both human and natural sources.  Satellite channels are subject
      to deep space noise arising from electromagnetic radiation
      pervasive in the galaxy. Thermal noise plagues
      <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/">all</emphasis> electronic circuits that contain
      resistors. Thus, in receiving small amplitude signals, receiver
      amplifiers will most certainly add noise as they boost the
      signal's amplitude. All channels are subject to noise, and we
      need a way of describing such signals despite the fact we can't
      write a formula for the noise signal like we can for
      interference. The most widely used noise model 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/">white
      noise</term>. It is defined entirely by its frequency-domain
      characteristics.  </para>

    <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="noise">
      <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/">
	White noise has constant power at all frequencies.
      </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/">
	At each frequency, the phase of the noise spectrum is totally
	uncertain: It can be any value in between
	<m:math><m:mn>0</m:mn></m:math> and
	<m:math><m:apply><m:times/><m:cn>2</m:cn><m:ci>π</m:ci></m:apply></m:math>,
	and its value at any frequency is unrelated to the phase at
	any other frequency.
      </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/">
	When noise signals arising from two different sources add, the
	resultant noise signal has a power equal to the sum of the
	component powers.
      </item>
    </list> 

    <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="power">
      Because of the emphasis here on frequency-domain power, we are
      lead to define 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/">power spectrum</term>. Because 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/" document="m0047" target="parseval" strength="8">Parseval's
      Theorem</cnxn>, we define the power spectrum
      <m:math><m:apply><m:ci type="fn"><m:msub><m:mi>P</m:mi><m:mi>s</m:mi></m:msub></m:ci><m:ci>f</m:ci></m:apply></m:math>
      of a non-noise signal <m:math><m:apply><m:ci type="fn">s</m:ci><m:ci>t</m:ci></m:apply></m:math> to be the
      magnitude-squared of its Fourier transform.

      <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="a0000">
	<m:math>
	  <m:apply>
	    <m:equivalent/>
	    <m:apply>
	      <m:ci type="fn"><m:msub>
		  <m:mi>P</m:mi>
		  <m:mi>s</m:mi>
		</m:msub></m:ci>
	      <m:ci>f</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:power/>
	      <m:apply>
		<m:abs/>
		<m:apply>
		  <m:ci type="fn">S</m:ci><m:ci>f</m:ci>
		</m:apply>
	      </m:apply>
	      <m:cn>2</m:cn>
	    </m:apply>
	  </m:apply>
	  
	</m:math>
      </equation>

      Integrating the power spectrum over any range of frequencies
      equals the power the signal contains in that band. Because signals
      <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> have negative frequency components that
      mirror positive frequency ones, we routinely calculate the power in a
      spectral band as the integral over positive frequencies multiplied by
      two.
      
      <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="a0001">
	<m:math>
	  <m:mtext>Power in</m:mtext>
	  <m:apply>
	    <m:eq/>
	    <m:interval>
	      <m:ci><m:msub><m:mi>f</m:mi><m:mn>1</m:mn></m:msub></m:ci>
	      <m:ci><m:msub><m:mi>f</m:mi><m:mn>2</m:mn></m:msub></m:ci>
	    </m:interval> 
	    <m:apply>
	      <m:times/>
	      <m:cn>2</m:cn>
	      <m:apply>
		<m:int/><m:bvar><m:ci>f</m:ci></m:bvar>
		<m:lowlimit>
		  <m:ci><m:msub><m:mi>f</m:mi><m:mn>1</m:mn></m:msub></m:ci>
		</m:lowlimit>
		<m:uplimit>
		  <m:ci><m:msub><m:mi>f</m:mi><m:mn>2</m:mn></m:msub></m:ci>
		</m:uplimit>
		<m:apply>
		  <m:ci type="fn"><m:msub><m:mi>P</m:mi><m:mi>s</m:mi></m:msub></m:ci><m:ci>f</m:ci>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>

      Using the notation <m:math><m:apply><m:ci type="fn">n</m:ci><m:ci>t</m:ci></m:apply></m:math> to represent
      a noise signal's waveform, we define noise in terms of its power
      spectrum. For white noise, the power spectrum equals the
      constant

      <m:math> 
	<m:apply>
	  <m:divide/>
	  <m:ci><m:msub><m:mi>N</m:mi><m:mn>0</m:mn></m:msub></m:ci>
	  <m:cn>2</m:cn>
	</m:apply>
      </m:math>.  With
      this definition, the power in a frequency band equals 
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:ci><m:msub><m:mi>N</m:mi><m:mn>0</m:mn></m:msub></m:ci>
	  <m:apply>
	    <m:minus/>
	    <m:ci><m:msub><m:mi>f</m:mi><m:mn>2</m:mn></m:msub></m:ci>
	    <m:ci><m:msub><m:mi>f</m:mi><m:mn>1</m:mn></m:msub></m:ci>
	  </m:apply>
	</m:apply>
      </m:math>.  
    </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="final"> 
      When we pass a signal through a linear, time-invariant system, the
      output's spectrum equals 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="m0048" target="spectrum" strength="8">product</cnxn> of the system's
      frequency response and the input's spectrum. Thus, the power
      spectrum of the system's output 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="a0002">
	<m:math>
	  <m:apply>
	    <m:eq/>
	    <m:apply>
	      <m:ci type="fn"><m:msub><m:mi>P</m:mi><m:mi>y</m:mi></m:msub></m:ci>
	      <m:ci>f</m:ci>
	    </m:apply>
	    <m:apply>
	      <m:times/>
	      <m:apply>
		<m:power/>
		<m:apply>
		  <m:abs/>
		  <m:apply>
		    <m:ci type="fn">H</m:ci>
		    <m:ci>f</m:ci>
		  </m:apply>
		</m:apply>
		<m:cn>2</m:cn>
	      </m:apply>
	      <m:apply>
		<m:ci type="fn"><m:msub><m:mi>P</m:mi><m:mi>x</m:mi></m:msub></m:ci>
		<m:ci>f</m:ci>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math> 
      </equation>

      This result applies to noise signals as well. When we pass white
      noise through a filter, the output is also a noise signal but with
      power spectrum
      <m:math>
	<m:apply>
	  <m:times/>
	  <m:apply>
	    <m:power/>
	    <m:apply>
	      <m:abs/>
	      <m:apply>
		<m:ci type="fn">H</m:ci>
		<m:ci>f</m:ci>
	      </m:apply>
	    </m:apply>
	    <m:cn>2</m:cn>
	  </m:apply>
	  <m:apply>
	    <m:divide/>
	    <m:ci><m:msub><m:mi>N</m:mi><m:mn>0</m:mn></m:msub></m:ci>
	    <m:cn>2</m:cn>
	  </m:apply>
	</m:apply>
      </m:math>.
    </para>
    

  </content>
</document>
