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<!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:m="http://www.w3.org/1998/Math/MathML" xmlns:md="http://cnx.rice.edu/mdml/0.4" xmlns:bib="http://bibtexml.sf.net/" id="m0540"> 

  <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/">Communication with Satellites</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/">2.9</md:version>
  <md:created xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2000/08/11</md:created>
  <md:revised xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">2003/08/19 09:01:39.363 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="dhj">
      <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>
  </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="dhj">
      <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:maintainer>
    <md:maintainer xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/" id="jac3">
      <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>
      <md:email xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">jac3@rice.edu</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/">communication channels</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">geosynchronous orbits</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/">long-distance communication</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">long-distance transmission</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">satellite</md:keyword>
    <md:keyword xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">satellite communication</md:keyword>
  </md:keywordlist>

  <md:abstract xmlns:m="http://www.w3.org/1998/Math/MathML" xmlns:bib="http://bibtexml.sf.net/">Satellites may be used to transmit information over large distances.</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="p1">
      Global wireless communication relies on satellites.  Here,
      ground stations transmit to orbiting satellites that amplify the
      signal and retransmit it back to earth.  Satellites will move
      across the sky unless they are in <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/">geosynchronous
      orbits</term>, where the time for one revolution about the
      equator exactly matches the earth's rotation time of one day.
      TV satellites would require the homeowner to continually adjust
      his or her antenna if the satellite weren't in geosynchronous
      orbit.  Newton's equations applied to orbiting bodies predict
      that the time <m:math display="inline"><m:ci>T</m:ci></m:math>
      for one orbit is related to distance from the earth's center
      <m:math display="inline"><m:ci>R</m:ci></m:math> 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="eq0001">
	<m:math display="block">
	  <m:apply>
	    <m:eq/>
	    <m:ci>R</m:ci>
	    <m:apply>
	      <m:root/>
	      <m:degree><m:cn type="integer">3</m:cn></m:degree>
	      <m:apply>
		<m:divide/>
		<m:apply>
		  <m:times/>
		  <m:ci>G</m:ci>
		  <m:ci>M</m:ci>
		  <m:apply>
		    <m:power/>
		    <m:ci>T</m:ci>
		    <m:cn>2</m:cn>
		  </m:apply>
		</m:apply>
		<m:apply>
		  <m:times/>
		  <m:cn>4</m:cn>
		  <m:apply>
		    <m:power/>
		    <m:pi/>
		    <m:cn>2</m:cn>
		  </m:apply>
		</m:apply>
	      </m:apply>
	    </m:apply>
	  </m:apply>
	</m:math>
      </equation>

      where <m:math display="inline"><m:ci>G</m:ci></m:math> is the
      gravitational constant and <m:math display="inline"><m:ci>M</m:ci></m:math> the earth's mass.
      Calculations yield

      <m:math display="inline">
	<m:apply>
	  <m:eq/>
	  <m:ci>R</m:ci>
	  <m:apply>
	    <m:times/>
	    <m:cn>42200</m:cn>
	    <m:ci>km</m:ci>
	  </m:apply>
	</m:apply>
      </m:math>, which corresponds to an altitude of 
      <m:math display="inline">
	<m:apply>
	  <m:times/>
	  <m:cn>35700</m:cn>
	  <m:ci>km</m:ci>
	</m:apply>
      </m:math>.  This altitude greatly exceeds that of the
      ionosphere, requiring satellite transmitters to use frequencies
      that pass through it.  Of great importance in satellite
      communications is the transmission delay.  The time for
      electromagnetic fields to propagate to a geosynchronous
      satellite and return is 0.24 s, a significant delay.
    </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="exercise1">
      <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="prob1">
	  In addition to delay, the propagation attenuation
	  encountered in satellite communication far exceeds what
	  occurs in ionospheric-mirror based communication.  Calculate
	  the attenuation incurred by radiation going to the satellite
	  (one-way loss) with that encountered by Marconi (total going
	  up and down).  Note that the attenuation calculation in the
	  ionospheric case, assuming the ionosphere acts like a
	  perfect mirror, is not a straightforward application of 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="m0101" target="p2" strength="5">propagation
	  loss formula</cnxn>.
	</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="sol1">
	  Transmission to the satellite, known as the uplink,
	  encounters inverse-square law power losses.  Reflecting off
	  the ionosphere not only encounters the same loss, but twice.
	  Reflection is the same as transmitting exactly what arrives,
	  which means that the total loss is the <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/">product
	  </emphasis>of the uplink and downlink losses.  The
	  geosynchronous orbit lies at an altitude of
	  <m:math display="inline">
	    <m:apply>
	      <m:times/>
	      <m:cn>35700</m:cn>
	      <m:ci>km</m:ci>
	    </m:apply>
	  </m:math>.  The ionosphere begins at an altitude of about
	  50 km.  The amplitude loss in the satellite case is
	  proportional to

	  <m:math display="inline">
	    <m:cn type="e-notation">2.8<m:sep/>-8</m:cn> </m:math>;
	  for Marconi, it was proportional to
	  
	  <m:math display="inline">
	    <m:cn type="e-notation">4.4<m:sep/>-10</m:cn>
	  </m:math>.  
	  Marconi was  <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/">very </emphasis>lucky.
	</para>
      </solution>
    </exercise>

  </content>
</document>
