COVER INFORMATION Station: URUMQI (Code Ur ) Experiment: InSight tracking Exp. Code: ed045b Schedule Version: 1.00 Processed by SCHED version: 11.50 Development version 11.5. Started Apr. 2 PI: Dominic Dirxx Address: Delft The Netherlands Phone: +31 15 27 8886 EMAIL: d.dirkx@tudelft.nl Fax: Phone during observation: Observing mode: Mk5 at 8 GHz Notes: Spacecraft signal on X band Single pol RCP Schedule for URUMQI (Code Ur ) Page 2 InSight tracking UP: D => Below limits; H => Below horizon mask; W => still slewing at end; blank => Up. Early: Seconds between end of slew and start. Dwell: On source seconds. Disk: GBytes recorded to this point. TPStart: Recording start time. Frequencies are LO sum (band edge). SYNC: Time correlator is expected to sync up. ---------------------------------------------------------------------------------------- Start UT Source Start / Stop Early Disk TPStart Stop UT LST EL AZ HA UP ParA Dwell GBytes SYNC ---------------------------------------------------------------------------------------- --- Sun 23 Feb 2020 Day 54 --- Next scan frequencies: 8400.49 8416.49 8432.49 8448.49 Next BBC frequencies: 300.49 316.49 332.49 348.49 Next scan bandwidths: 16.00 16.00 16.00 16.00 02 30 00 J1924-2914 18 28 34 16.1 167.0 -1.0 -10.8 0 0 02 30 00 02 33 00 =1921-293 18 31 35 16.3 167.6 -0.9 -10.3 180 6 02 30 01 02 33 00 MARS0240 18 31 35 22.8 182.9 0.2 2.3 -19 6 No stop 02 35 00 --- 18 33 35 22.8 183.4 0.2 2.7 101 10 02 33 01 02 35 00 J1820-2528 18 33 35 21.0 182.8 0.2 2.2 -7 10 No stop 02 38 00 =1817-254 18 36 35 21.0 183.5 0.2 2.8 173 15 02 35 01 02 38 00 MARS0240 18 36 35 22.8 184.1 0.3 3.3 -7 15 No stop 02 40 00 --- 18 38 36 22.7 184.6 0.3 3.7 113 19 02 38 01 02 40 00 J1820-2528 18 38 36 21.0 184.0 0.3 3.2 -7 19 No stop 02 43 00 =1817-254 18 41 36 20.9 184.7 0.3 3.8 173 25 02 40 01 02 43 00 MARS0240 18 41 36 22.7 185.4 0.4 4.3 -7 25 No stop 02 45 00 --- 18 43 37 22.6 185.9 0.4 4.7 113 29 02 43 01 02 45 00 J1820-2528 18 43 37 20.9 185.2 0.4 4.2 -7 29 No stop 02 48 00 =1817-254 18 46 37 20.8 185.9 0.4 4.7 173 35 02 45 01 02 48 00 MARS0240 18 46 37 22.6 186.6 0.4 5.2 -6 35 No stop 02 50 00 --- 18 48 37 22.5 187.1 0.5 5.6 114 38 02 48 01 02 51 00 MARS0300 18 49 38 22.5 187.3 0.5 5.8 58 38 02 51 00 03 10 00 --- 19 08 41 21.9 192.0 0.8 9.5 1140 75 02 51 01 03 11 00 MARS0320 19 09 41 21.9 192.3 0.8 9.7 58 75 03 11 00 03 20 00 --- 19 18 42 21.5 194.4 1.0 11.4 540 92 03 11 01 03 21 00 MARS0340 19 19 42 21.5 194.7 1.0 11.6 58 92 03 21 00 03 40 00 --- 19 38 46 20.5 199.2 1.3 15.1 1140 129 03 21 01 03 41 00 MARS0400 19 39 46 20.4 199.4 1.3 15.3 58 129 03 41 00 04 00 00 --- 19 58 49 19.1 203.9 1.6 18.7 1140 165 03 41 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess120.X256 --- WARNING --- This group does not match an entry in the frequency catalog. This might be ok because the catalog is not complete. But be very careful to be sure that the setup is correct. Setup group: 4 Station: URUMQI Total bit rate: 256 Format: MARK5B Bits per sample: 2 Sample rate: 32.000 Number of channels: 4 DBE type: DBBC_DDC Speedup factor: 1.00 Disk used to record data. 1st LO= 8100.00 8100.00 8100.00 8100.00 Net SB= U U U U IF SB = U U U U Pol. = RCP RCP RCP RCP BBC = 1 2 3 4 BBC SB= U U U U IF = A1 A1 A1 A1 The following frequency sets based on these setups were used. Frequency Set: 2 Setup file default. Used with PCAL = off LO sum= 8400.49 8416.49 8432.49 8448.49 BBC fr= 300.49 316.49 332.49 348.49 Bandwd= 16.00 16.00 16.00 16.00 Matching frequency sets: 2 Track assignments are: track1= 2, 4, 6, 8 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) * MARS0240 18 15 41.514224 * 18 18 44.520000 18 19 56.276787 0.00 -23 41 23.62156 *-23 40 08.40000 -23 39 34.76969 0.00 From catalog imbedded in main SCHED input file. * MARS0300 18 15 44.024744 * 18 18 47.030000 18 19 58.786326 0.00 -23 41 23.40400 *-23 40 08.00000 -23 39 34.29824 0.00 From catalog imbedded in main SCHED input file. * MARS0320 18 15 46.525225 * 18 18 49.530000 18 20 01.285882 0.00 -23 41 23.28572 *-23 40 07.70000 -23 39 33.92708 0.00 From catalog imbedded in main SCHED input file. * MARS0340 18 15 49.035747 * 18 18 52.040000 18 20 03.795421 0.00 -23 41 23.06817 *-23 40 07.30000 -23 39 33.45564 0.00 From catalog imbedded in main SCHED input file. * MARS0400 18 15 51.546270 * 18 18 54.550000 18 20 06.304959 0.00 -23 41 22.85061 *-23 40 06.90000 -23 39 32.98421 0.00 From catalog imbedded in main SCHED input file. 1817-254 18 17 52.332230 * 18 20 57.848697 18 22 10.574531 0.05 * J1820-2528 -25 29 37.39982 *-25 28 12.58410 -25 27 34.59171 0.09 J1820-25 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 656 observations. 1921-293 19 21 42.234126 * 19 24 51.055953 19 26 04.685816 0.00 * J1924-2914 -29 20 26.35397 *-29 14 30.12107 -29 12 05.33636 0.01 J1924-29 /home/guest/rmc/SCHED/sched11.5/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 63480 observations. SOURCE SCAN SUMMARY FOR SOURCES LISTED ABOVE Scan hours are for recording scans only. Baseline hours are only counted for scans above horizon at both ends. Source Setup file Frequency sets Observing hours (duplicates not shown) Scan Baseline MARS0240 sess120.X256 1 2 3 4 5 6 0.133 2.197 MARS0300 sess120.X256 1 2 3 4 5 6 0.317 6.650 MARS0320 sess120.X256 1 2 3 4 6 0.150 2.250 MARS0340 sess120.X256 1 2 3 4 6 0.317 3.167 MARS0400 sess120.X256 1 2 3 4 6 0.317 3.167 J1820-2528 sess120.X256 1 2 3 4 5 6 0.150 2.807 J1924-2914 sess120.X256 1 2 3 4 5 0.050 0.500 EFFECT OF SOLAR CORONA The solar corona can cause unstable phases for sources too close to the Sun. SCHED provides warnings at individual scans for distances less than 10 degrees. The distance from the Sun to each source in this schedule is: Source Sun distance (deg) MARS0240 59.4 MARS0300 59.4 MARS0320 59.4 MARS0340 59.4 MARS0400 59.4 J1820-2528 59.0 J1924-2914 45.6 Barry Clark estimates from predictions by Ketan Desai of IPM scattering sizes that the Sun will cause amplitude reductions on the longest VLBA baselines at a solar distance of 60deg F^(-0.6) where F is in GHz. For common VLBI bands, this is: 327 MHz 117. deg 610 MHz 81. deg 1.6 GHz 45. deg 2.3 GHz 36. deg 5.0 GHz 23. deg 8.4 GHz 17. deg 15.0 GHz 12. deg 22.0 GHz 9. deg 43.0 GHz 6. deg