Bernese GNSS Software Version 5.2 Tutorial

7 Additional ExamplesThe table at the end of the program output provides an overview of the clock quality:...REFERENCE CLOCK SELECTION FOR OUTPUT FILE-----------------------------------------Selected reference station:...WTZR 14201M010STATISTICS ON THE CLOCKS IN THE OUTPUT FILE-------------------------------------------# per file rms of poly. fit (ns)Clock name out 001 n = 0 n = 1 n = 2-------------------------------------------------------------------WTZR 14201M010 288 288 1.473 0.000 0.000WSRT 13506M005 288 288 4.522 0.030 0.030MATE 12734M008 288 288 29.164 0.054 0.052PTBB 14234M001 288 288 0.398 0.058 0.043ONSA 10402M004 284 284 5.625 0.081 0.076LAMA 12209M001 288 288 2.928 2.933 2.932JOZ2 12204M002 288 288 3.062 3.067 3.069HERT 13212M010 288 288 3.317 3.322 3.328ZIMM 14001M004 288 288 4.277 4.091 3.833TLSE 10003M009 288 288 5.174 4.892 4.735ZIM2 14001M008 287 287 5.297 5.021 4.712GANP 11515M001 288 288 6.752 6.689 6.629WTZZ 14201M014 288 288 0.3E+06 0.3E+06 0.3E+06G01 59 59 21.052 0.132 0.133G02 113 113 53.422 0.141 0.125G29 93 93 40.743 0.154 0.132G18 111 111 42.206 0.159 0.160G20 83 83 14.258 0.174 0.174G07 105 105 3.159 0.186 0.141G11 87 87 89.780 0.192 0.190G19 103 103 91.491 0.192 0.137G25 83 83 32.991 0.199 0.064G13 86 86 10.746 0.220 0.173G15 102 102 104.649 0.221 0.197G23 98 98 32.848 0.228 0.111G12 86 86 37.991 0.234 0.156G14 111 111 111.496 0.240 0.235G16 108 108 87.316 0.242 0.237G31 113 113 71.218 0.264 0.160G22 110 110 14.928 0.268 0.243G21 102 102 45.147 0.289 0.253G05 111 111 65.893 0.356 0.310R02 98 98 44.931 0.370 0.271G06 93 93 248.956 0.371 0.342R13 103 103 22.465 0.377 0.343R04 99 99 4.507 0.409 0.382G32 87 87 299.992 0.419 0.270R05 124 124 19.777 0.577 0.500R19 100 100 20.052 0.590 0.313...7.3.4 Further suggestions• Switch the “Var-covar wrt epoch parameters” in panel “GPSEST 6.7: General Options forEpoch Parameters” from SIMPLIFIED to CORRECT.• Compute a PPP for one of the stations in the zero difference network solution.Compare the coordinates and clocks from the PPP with the results from the networksolution. Exchange the orbits, EOP, and satellite clock corrections from yoursolution by products from other sources (e.g., CODE or IGS).• Use the PPP approach to screen the residuals of the Bernese zero difference observationfiles. This has to be done station by station. Make sure that you use aconsistent set of orbits, EOP, and satellite clocks (e.g., IGS final products or CODEfinal solution).Page 132AIUB