IVS Analysis Report for R1992 ($21MAR29XA) This report is the official IVS analysis report that corresponds to the database maintained by the IVS Data Centers for this session. (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: - Many non-detections in both bands of AGGO. Parameterization comments: two clock breaks were added to YARRA12M. Other comments: NYALE13S was tagged along. ----------------------------------------- Session Statistics Observations: 2283 scheduled 2265 correlated (in database) 1748 recoverable (usable) 1713 used Session fit: 35.126 ps ----------------------------------------- Station Performance Number of Observations Scheduled Recoverable* Used % of scheduled obs used AGGO 431 245 240 55.7% HART15M 701 501 491 70.0% MATERA 915 729 710 77.6% NYALE13S 431 319 314 72.9% SEJONG 677 496 485 71.6% WETTZ13N 979 872 862 88.0% YARRA12M 432 334 324 75.0% --------------- --------- ----------- --------- ------ Station Total** 2283 1748 1713 75.0% * Recoverable: can be included in the solution. ** Total includes distinct observations only. MISSED: Station was scheduled, but it did not observe. NOT CORR: Station was scheduled but not correlated. NOT USED: Usable data was generated for this station, but the analyst rejected it all. ----------------------------------------- Source Performance Number of Observations Scheduled Correlated* Used % of scheduled obs used 3C345 14 14 13 92.9% NGC1218 12 12 7 58.3% 0826-373 17 17 9 52.9% 2325-150 9 6 4 44.4% 2037+216 44 44 4 9.1% 1737-081 3 3 2 66.7% 3C279 28 28 26 92.9% 1150+497 29 29 21 72.4% 0010+405 5 5 4 80.0% 0346+800 5 5 3 60.0% 1928+154 11 11 9 81.8% 2325+093 11 11 10 90.9% 0059+581 193 193 122 63.2% 0104-408 20 20 17 85.0% 0119+115 34 32 26 76.5% 0454-234 108 108 97 89.8% 0537-441 13 13 7 53.8% 0727-115 92 92 88 95.7% 1034-293 6 6 2 33.3% 1057-797 17 17 11 64.7% 1124-186 19 19 15 78.9% 1144-379 15 15 13 86.7% 1418+546 24 24 20 83.3% 1451-375 14 14 12 85.7% NGC6251 3 3 3 100.0% 1749+096 74 74 66 89.2% 1921-293 20 20 17 85.0% 3C418 216 216 166 76.9% 2052-474 16 16 10 62.5% 3C446 139 136 97 69.8% 0420-014 112 112 101 90.2% 1244-255 71 71 52 73.2% 1324+224 28 28 26 92.9% 1846+322 16 16 13 81.2% 2229+695 89 89 83 93.3% 0307+380 5 5 4 80.0% 0529+483 80 80 68 85.0% 0536+145 18 18 4 22.2% 0641+392 7 7 4 57.1% 1059+282 23 23 17 73.9% 2214+350 8 8 7 87.5% 0322+222 15 15 11 73.3% 1015+057 6 6 1 16.7% 1759-396 9 9 2 22.2% 2008-159 83 81 54 65.1% 0308-611 73 73 16 21.9% 0332-403 35 35 30 85.7% 1502+036 17 17 16 94.1% 0017+200 14 14 10 71.4% 0202+319 183 178 145 79.2% 1030+415 41 41 33 80.5% 1406-076 134 134 113 84.3% 1504+377 5 2 2 40.0% ------------ --------- ---------- ------ ------ Source Total 2283 2265 1713 75.0% * Correlated: included in database ----------------------------------------- Baseline Performance Number of Observations Scheduled Recoverable* Used % of scheduled obs used AGGO-HART15M 212 111 107 50.5% AGGO-MATERA 90 57 56 62.2% AGGO-NYALE13S 12 0 DESELECTED 0.0% AGGO-SEJONG 0 NOT CORR NOT CORR 0.0% AGGO-WETTZ13N 88 69 69 78.4% AGGO-YARRA12M 29 8 8 27.6% HART15M-MATERA 163 128 123 75.5% HART15M-NYALE13S 21 13 13 61.9% HART15M-SEJONG 53 39 39 73.6% HART15M-WETTZ13N 176 156 155 88.1% HART15M-YARRA12M 76 54 54 71.1% MATERA-NYALE13S 122 107 103 84.4% MATERA-SEJONG 136 78 76 55.9% MATERA-WETTZ13N 354 325 319 90.1% MATERA-YARRA12M 50 34 33 66.0% NYALE13S-SEJONG 121 63 62 51.2% NYALE13S-WETTZ13N 126 120 120 95.2% NYALE13S-YARRA12M 29 16 16 55.2% SEJONG-WETTZ13N 177 148 147 83.1% SEJONG-YARRA12M 190 168 161 84.7% WETTZ13N-YARRA12M 58 54 52 89.7% ----------------- --------- ----------- ---------- ------ Baseline Total 2283 1748 1713 75.0% * Recoverable: can be included in the solution. MISSED: Baseline was scheduled, but at least one of the sites did not observe. NOT CORR: Baseline was scheduled but not correlated. NO DATA: The baseline's stations were both correlated, but they did not observe together. DESELECTED: Usable data was generated for the baseline, but the analyst rejected it.