(NEW File - Corrected Observing Date) CORE-3038 (Continuous Observations of the Rotation of the Earth-3038) 2001 November 28 Notes prepared by Nancy Vandenberg and Cynthia Thomas,NVI/GSFC Schedule name: nov01/c3038.skd on CDDISA Nominal Start: 18:30 U.T. on November 28 (day 332) first observation at 18:30 U.T. on 1300+580 Nominal Stop: 18:30 U.T. on November 29 (day 333) last observation at 18:18 U.T. on 0552+398 for GC last observation at 18:23 U.T. on 2234+282 for NY last observation at 18:25 U.T. on 2255-282 for MA-WZ last observation at 18:26 U.T. on 1741-038 for KK-WF Observing Mode: 2F (with barrel roll, see details below) Correlator: Bonn 1 letter 2 letter Station Code Code # of tapes # of obs Occupation Code Fairbanks A Gc 1 (TT) 391 40476601 Kokee K Kk 2 (TT) 325 72983001 Matera I Ma 2 (TT) 384 72435701 Ny Alesund N Ny 1 (TT) 372 73313301 Westford E Wf 2 (TT) 360 72097301 Wettzell V Wz 1 (TT) 417 72247801 Purpose ======= The CORE-3 sessions marked the start of the regular CORE oberving program. These sessions will provide a bi-weekly 48-hour continuous data set from January through July (NEOS + CORE-3) and a weekly 48-hour continuous data set from July through December. The CORE-3 sessions will be recorded in a Mark 4 mode which requires that the participating stations have Mark 4 capability. Observing Mode ============== This is the first CORE series that uses a "Mark 4" style observing mode. The mode for CORE-3 uses fan-out and records on all 32 tracks to achieve a data rate of 128 Mb/s, more than twice that of the standard geodetic Mode C which is 56 Mb/s. CORE Mode "2F" (twice the standard mode C, fanned out) ----------------------------------------------------------------- Number of frequencies 14 (standard wide-band frequency sequence modified to avoid RFI at Matera) Number of channels 16 (14 USB + 2 LSB) Channel bandwidth 4.0 MHz Sample rate 8 Mb/s Bits per sample 1 Total data rate 128 Mb/s Data rate on tape 4 Mb/s/track Fan-out 1:2 Tape speed 80 ips Tracks per pass 32 Passes per tape 14 Barrel roll yes (*) Track frame format Mark4 and VLBA (*) The 16 recorded channels are comprised of the standard 14-channel USB frequency sequence plus the LSB channels of the first and last frequencies at X-band. The two outer X-band LSB channels give extra sensitivity. They also slightly narrow the peak of the delay resolution function, resulting in better group delay precision. *The stations with VLBA backends, Fairbanks and Kokee, will use barrel roll during this session and record in VLBA (non-data replacement) format. Stations with Mark 4 formatters cannot barrel roll. Schedule ======== This schedule was made by C. Thomas using sked. Schedule setup parameters: Early start 10 sec Minimum scan length 30 sec Maximum scan length 600 sec Minimum SNR 20 at X-band, margin of 5 15 at S-band, margin of 3 Automatic scheduling setup: optimize for uniform sky coverage at all stations, maximize the number of observations, minimize slewing time, minimize time between scans, consider the top 50% of ranked scans for selection, consider the last 1 hour of scans for sky coverage calculations, minimum 50 min between scans on the same source. The characteristics of the generated schedule are listed below. These will vary slightly for each schedule that is generated. The characteristics also will change when Matera and Ny Alesund are used in the network instead of Medicina and Onsala. Schedule characteristics: Average scan length 87 seconds Median SNR 35.0 at X-band 25.0 at S-band Number of observations 3481 observations Average scans per station 374 scans Parity ====== This schedule was made with a minimum scan time of less than the 55 seconds required for parity checks. As a result, some parity checks in the schedule may give bad results even though there is nothing wrong. The next release of the FS, 9.5, will correct this problem. In the meantime, please check when a parity check fails to see if the cause is a short scan. If the problem is presistent and occurs frequently at your station for a given schedule type, you may want to disable parity checks for specific experiments of that type. You can do this by creating empty "checkf80" and "checkr80" procedures (or "checkf135" and "checkr135" if you are using thick tape) in the EXPERIMENT procedure library for the effected experiment. If you do this, it is strongly recommend that you verify recorder performance before the experiment by recording some tape in both directions using the experiment set-up and check it with the appropriate parity check procedures. Flux Information ================ Program snranal compares the measured performance of a session with respect to the predicted. The program calculates an empirical flux density for each source. In order to account for changes in the flux catalog since the last update based on source modeling, the fluxes in the flux catalog for the sources in the current source catalog were adjused using the following databases: Date Session ==== ========= 01JUL11 CORE-3020 01JUL03 CORE-C202 01JUL25 CORE-3022 01AUG08 CORE-3024 Simulation Results ================== Simulated data from this schedule was used in a global solution to estimate the formal errors. The table below lists the formal errors for Earth orientation parameters. These results meet the simulation goals for the CORE-3 network. Also shown in the table are the maximum correlations between the Earth orientation parameters and other parameters. Simulation for experiment $01NOV29ZZ -------------------------------------------------------------------| | | | Maximum | Correlating | | EOP | Formal | Correlation | Parameter | | Parameters | Errors | | | |------------+----------------+-------------+----------------------| | | | | | | X-Wobble | 67.0 muas | 0.11 | KOKEE Z COMPONENT | | Y-Wobble | 57.2 muas | 0.08 | WETTZELL Z COMPONENT | | UT1-TAI | 2.3 musec | 0.10 | GILCREEK Y COMPONENT | | UT1-Rate | 5.7 musec/d | 0.02 | NYALES20 Z COMPONENT | |------------|----------------|-------------|----------------------| Procedures ========== Please generate the procedures for this session using drudg. SKED Summary from file ./c3038.skd for experiment C3038 (all scans with at least one subnet station) SOURCE |0 6 12 18 | #SCANS #OBS #Obs/bl 0003-066I x x xx x x x x x x x x xx x x x I 17 31 6.1 0048-097I x x x x I 4 6 1.2 0059+581Ix x x x x x x x x x x x x x x x x x x I 19 255 18.8 0106+013I x x x x x x x x x x x x x x x x x I 17 52 7.9 0119+115Ix x x x x x x x x x x x x x x x xx I 18 85 10.0 0119+041I x x I 2 2 .3 0229+131I x x I 2 4 .5 0235+164I x x x x x x x x x x x x x x x x x x xI 19 107 11.5 CTA26 Ix x x x x x x x x x x x x x x x x xx I 19 51 7.1 0454-234Ix x x x x x x x x x I 10 14 5.0 0458-020I x x x x x xx x x x x xI 12 30 4.1 0528+134Ix x x x x x x x x x x x x x x x x x x x xI 21 91 10.4 0552+398I x x x xx x x x x x x x x x x x xx x x x xI 22 199 17.0 0556+238I x I 1 3 .3 0718+793Ix x x x x x x x x I 9 38 2.5 0727-115Ix x x x x x x x x x x x x x I 14 20 5.4 0749+540Ix x x x x x x x x x I 10 106 7.7 0804+499I x x x x x x x x I 8 105 8.5 0805+410I x x x x x x x x x I 9 70 5.5 0823+033I x x x x x x x x x x x x x x x x x x I 18 51 7.4 OJ287 I x x x x x x x x x x x x x x x x x x x x x I 21 120 12.3 0919-260I x x xx x I 5 5 2.0 4C39.25 I x x x x x x x x x x x x x xx x x x xI 19 158 13.4 OK290 I x x x x x x x x x I 9 19 1.8 0955+476I x x x x x x x x x x x x I 12 130 10.5 1044+719I x x x x x x x xI 8 106 7.3 1053+815I x x I 2 30 2.0 1124-186I x xx xx x x x x x x I 11 15 5.0 1128+385I x x x x x x x x x x x x x x xx x x xxI 20 183 15.8 1219+044I x x xx x x xx x x x x x x x x x x x xx I 21 61 8.6 1255-316I x x x x I 4 4 1.9 1300+580I x x x x x x x x x x x x x x x x x x x x xI 21 275 20.2 1313-333I I 0 0 .0 1334-127I x x x x x x x x x x x x x x x I 15 21 5.6 1351-018I x x x x x x x x x x x x xI 13 21 3.3 1357+769Ix x x x x x x x x x x x x x x x x x x x I 20 300 20.0 1606+106Ix x x x x x x x x x x x x x x x x x x x xx I 22 92 11.2 1622-253I I 0 0 .0 NRAO512 I x x x x x x x x x I 9 66 5.5 1726+455I x x x x x x x x x x x x x x xI 15 148 11.8 1739+522I x x x I 3 23 1.6 1741-038Ix x x x x x x x x x x x x x x x x x x x I 20 43 13.3 1749+096Ix x x x x x x xx x x x x x x x xx x x x x I 22 89 10.9 1908-201I x x x x x x x x I 8 12 4.1 1921-293I x x x x I 4 4 1.7 1958-179Ix x x x x x x x I 8 10 3.2 2121+053I x x x x x x x x x x x x x x x x I 16 55 7.6 2128-123I x x x x x x x x x x x I 11 17 5.1 2134+00 I xx x x x I 5 5 .7 2145+067Ix x x x x x x x x x I 10 43 5.8 2234+282I x x x x x x x x x x x x x x x x x I 17 100 9.4 2255-282I x x x xx x I 6 6 2.5 Total scans, obs: 628 3481 Average number of obs. per baseline per source (normalized by up-time) = 7.4 Min = .0 Max = 68.6 (Baseline Ny-Wz on 1741-038) RMS = 7.6 Total time: 1436 minutes ( 23.9 hours). Key: Gc=GILCREEK Kk=KOKEE Ma=MATERA Ny=NYALES20 Wf=WESTFORD Wz=WETTZELL Gc Kk Ma Ny Wf Wz Avg % obs. time: 27 43 43 31 43 36 37 % cal. time: 4 3 4 4 4 4 4 % slew time: 26 15 25 20 16 13 19 % idle time: 41 37 26 42 36 45 38 # of tapes : .8 1.1 1.2 .9 1.1 1.0 total # scans: 391 325 384 372 360 417 374 # scans/hour : 16 13 16 15 15 17 15.6 Avg scan (sec): 61 114 97 74 103 75 87 # OF OBSERVATIONS BY BASELINE | Gc Kk Ma Ny Wf Wz StnTotal -------------------------------------- Gc|391 303 171 267 258 203 1202 Kk| 325 90 184 211 117 905 Ma| 384 272 219 383 1135 Ny| 372 252 302 1277 Wf| 360 249 1189 Wz| 417 1254 Number of 2-station scans: 175 Number of 3-station scans: 164 Number of 4-station scans: 114 Number of 5-station scans: 99 Number of 6-station scans: 76 Total # of scans, observations: 628 3481 Average baseline components for all observations Average XY = 4959. Average XZ = 4374. Average YZ = 3183. Average length = 5322.