<h2> Cassini and Saturn's moons ephemeris at AMDA </h2>
<br/>
<br/> <UL>
  <li> Cassini/Titan/Enceladus Ephemeris are calculated by <b>Joseph Groene</b>
  of University of Iowa based on CASSINI SPICE kernels. 
  All data are taken from <a href="http://www-pw.physics.uiowa.edu/~jbg/cas.html" TARGET=_BLANK>Joseph Groene site</a>
 
   <li> Ephemeris are presented in geographic Saturn barycentric coordinates
        and include 
        <UL>
           <li> <b>Western Longitude_IAU,</b><br/>
                based on the Voyager determination of the period of Saturn kilometric radiation
               (SKR).<br/>
              Seidelmann et al.:2002, "Report on the IAU/IAG Working Group
              on Cartographic Coordinates and Rotational Elements of the
              Planets and Satellites: 2000", CELESTIAL MECHANICS AND
              DYNAMICAL ASTRONOMY 82: 83-110, 2002. 
           <li> <b>Western Longitude_SLS3,</b><br/>
                based on Cassini SKR measurements.<br/> 
                The SLS3 longitude system is only valid for time period:
                <b>01.01.2004 - 10.08.2007.</b><br/>
                <a href="http://www.agu.org/pubs/crossref/2008/2007JA012861.shtml" TARGET=_BLANK>Kurth et al. (2008)</a>, An update to a Saturnian longitude system based on 
               kilometric radio emissions, Journal of Geophysical Research, Volume 113, 
               Issue A5, CiteID A05222  
           <li> <b>Latitude</b>
           <li><b>Local Time</b>
           <li> <b>L-shell</b> (dipole) value
           <li> <b>Radius</b> 
        </UL>    
 </UL>