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<br />receivers were <br /> <br />The following Ashtech Z12 and FXHE geodetic dual-frequency <br />used: <br /> <br />Ashtech Z12 receiver LP0018 and antenna C587 with accessories <br /> <br />with accessories <br /> <br />Ashtech Z12 receiver LP0124 and antenna C421 <br /> <br />1 <br /> <br />1 <br /> <br />11 <br /> <br />J <br /> <br /> <br />I: <br /> <br />with accessories <br /> <br />Ashtech Z12 receiver LP0259 and antenna C311 <br /> <br />Il <br /> <br />Software: <br /> <br />I} <br /> <br />v2.505 <br /> <br />Ashtech static and kinematic processor, <br /> <br />PNAV <br />WinPrism <br /> <br />Ashtech processing and adjustment package, v2.0 <br /> <br />" <br /> <br />Advanced GPS post-processing software, TerraSat, v2.0 <br /> <br />Least squares gps adjustment package, v3.0 <br /> <br />GeoGenius <br /> <br />11 <br /> <br />J <br /> <br /> <br /> <br />IJ <br /> <br />Fillnet <br /> <br />IJ <br /> <br />Data Processing and Adjustment <br /> <br />The following NGS control points were used <br /> <br />IJ <br /> <br />Quality <br /> <br />Vertical <br /> <br />Horizontal Quality <br /> <br />10 <br /> <br />Site <br /> <br />Name <br /> <br />First, Class <br /> <br />First <br /> <br />2590 <br /> <br />0259 <br /> <br />IJ <br /> <br />Class <br /> <br />First, <br /> <br />First <br /> <br />259A <br /> <br />A259 <br /> <br />IJ <br /> <br />Second <br /> <br />First, Class <br />(Ellipsoidal) <br /> <br />First <br /> <br />First <br /> <br />DIDO <br /> <br />BECH <br /> <br />DIDO <br /> <br />BECHTOLT <br /> <br />1 <br /> <br />Fourth, Class <br />(Ellipsoidal) <br /> <br />First <br /> <br />BE11 <br /> <br />11 <br /> <br />BE <br /> <br />I <br /> <br />.J <br /> <br />IJ <br /> <br />The NGS data sheets are included in appendix <br /> <br />The data was observed at 10 second update rates for kinematic/rapid static <br />processing, thinned to 30 seconds for static processing. Occupation times <br />averaged at least fifteen minutes. Earlier sessions (not included in the <br />adjustment) were observed at 30 second epochs for approximately an hour, <br />to anticipate problems due to the solar max I ionospheric disturbance issues <br /> <br />2 <br /> <br />Ii <br />-l <br /> <br />I, <br /> <br />... <br /> <br />I: <br /> <br />.J <br /> <br /> <br />I <br />