COVER INFORMATION Station: SVETLOE (Code Sv ) Experiment: Network Monitoring Experiment Exp. Code: N20X2 Schedule Version: 1.00 Processed by SCHED version: 11.60 Release 11.6; April 2020 PI: Olga Bayandina Address: JIVE Oude Hoogeveensedijk 4 7991PD Dwingeloo The Netherlands Phone: +31 521 596 508 EMAIL: bayandina@jive.eu Fax: Phone during observation: +31 521 596 508 Observing mode: Notes: 3.6cm NME and ftp fringe test for Session 3 2020 (2 Gbps, L+R, 2-bit sampling, 32 MHz filters, assumes use of v107 firmware for DBBCs) Please send the disk pack to JIVE as soon as possible, if appropriate COVER LETTER: This is the schedule for the 3.6cm NME and ftp fringe-test on 19 October 2020 involving the following antennas: Wb, Ef, Mc, Nt, On60, T6, Ur, Ys, Hh, Sv, Zc, Bd, Ir, Wz. The NME uses the 2Gbps setup that will follow in user experiments The schedule consists of long integrations on calibrators J1751+0939 and J2031+1219 for ftp-fringe tests. The following ftp-fringe tests are scheduled throughout the experiment (UT times): 12:10:00 (scan 1, 2 sec, J1751+0939) 12:40:00 (scan 3, 2 sec, J1751+0939) 13:10:00 (scan 5, 2 sec, J1751+0939) 13:40:00 (scan 7, 2 sec, J2031+1219) 14:10:00 (scan 9, 2 sec, J2031+1219) 14:40:00 (scan 11, 2 sec, J2031+1219) Good luck with the session! Olga Bayandina Mattermost: coms.evlbi.org Schedule for SVETLOE (Code Sv ) Page 2 Network Monitoring Experiment 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 ---------------------------------------------------------------------------------------- --- Mon 19 Oct 2020 Day 293 --- Next scan frequencies: 8319.49 8319.49 8319.49 8319.49 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 8511.49 8511.49 8511.49 8511.49 Next BBC frequencies: 239.49 239.49 239.49 239.49 303.49 303.49 303.49 303.49 367.49 367.49 367.49 367.49 431.49 431.49 431.49 431.49 Next scan bandwidths: 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 12 00 00 J1751+0939 15 52 49 34.5 503.4 -2.0 -17.3 0 0 12 00 00 12 12 00 =1749+096 16 04 51 35.3 506.8 -1.8 -15.8 720 185 12 00 01 12 17 00 J1751+0939 16 09 52 35.7 508.3 -1.7 -15.2 293 185 12 17 00 12 27 00 =1749+096 16 19 54 36.3 511.3 -1.5 -13.9 600 338 12 17 01 12 32 00 J1751+0939 16 24 55 36.6 512.8 -1.5 -13.2 293 338 12 32 00 12 42 00 =1749+096 16 34 56 37.1 515.8 -1.3 -11.8 600 492 12 32 01 12 47 00 J1751+0939 16 39 57 37.4 517.3 -1.2 -11.1 293 492 12 47 00 12 57 00 =1749+096 16 49 59 37.8 520.4 -1.0 -9.7 600 646 12 47 01 13 02 00 J1751+0939 16 55 00 38.0 521.9 -1.0 -8.9 293 646 13 02 00 13 12 00 =1749+096 17 05 01 38.4 525.0 -0.8 -7.4 600 800 13 02 01 13 17 00 J2031+1219 17 10 02 29.4 479.8 -3.4 -25.9 229 800 13 17 00 13 27 00 =2029+121 17 20 04 30.5 482.3 -3.2 -25.2 600 954 13 17 01 13 32 00 J2031+1219 17 25 04 31.0 483.6 -3.1 -24.8 293 954 13 32 00 13 42 00 =2029+121 17 35 06 32.0 486.2 -3.0 -24.0 600 1108 13 32 01 13 47 00 J2031+1219 17 40 07 32.5 487.6 -2.9 -23.5 293 1108 13 47 00 13 57 00 =2029+121 17 50 09 33.5 490.3 -2.7 -22.6 600 1262 13 47 01 14 02 00 J2031+1219 17 55 09 33.9 491.6 -2.6 -22.1 293 1262 14 02 00 14 12 00 =2029+121 18 05 11 34.8 494.4 -2.5 -21.1 600 1415 14 02 01 14 17 00 J2031+1219 18 10 12 35.3 495.8 -2.4 -20.6 293 1415 14 17 00 14 27 00 =2029+121 18 20 13 36.1 498.6 -2.2 -19.5 600 1569 14 17 01 14 32 00 J2031+1219 18 25 14 36.5 500.0 -2.1 -18.9 293 1569 14 32 00 14 42 00 =2029+121 18 35 16 37.3 502.9 -2.0 -17.7 600 1723 14 32 01 14 47 00 J2031+1219 18 40 17 37.6 504.4 -1.9 -17.0 293 1723 14 47 00 15 00 00 =2029+121 18 53 19 38.5 508.3 -1.7 -15.3 780 1923 14 47 01 SETUP FILE INFORMATION: NOTE: If DOPPLER, FREQ, or BW were used, see the individual scans for the final BBC settings. ======== Setup file: sess320.X2048 Matching groups in /home/guest/rmc/SCHED/sched11.6/catalogs/freq_RDBE.dat: kvzr_x Added by Des Small, 24 February 2012 Setup group: 1 Station: SVETLOE Total bit rate: 2048 Format: MARK5B Bits per sample: 2 Sample rate: 64.000 Number of channels: 16 DBE type: Speedup factor: 1.00 Disk used to record data. 1st LO= 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 8080.00 Net SB= L L U U L L U U L L U U L L U U IF SB = U U U U U U U U U U U U U U U U Pol. = RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP RCP LCP BBC = 1 9 1 9 2 10 2 10 3 11 3 11 4 12 4 12 BBC SB= L L U U L L U U L L U U L L U U IF = A B A B A B A B A B A B A B A B The following frequency sets based on these setups were used. Frequency Set: 10 Setup file default. Used with PCAL = off LO sum= 8319.49 8319.49 8319.49 8319.49 8383.49 8383.49 8383.49 8383.49 8447.49 8447.49 8447.49 8447.49 8511.49 8511.49 8511.49 8511.49 BBC fr= 239.49 239.49 239.49 239.49 303.49 303.49 303.49 303.49 367.49 367.49 367.49 367.49 431.49 431.49 431.49 431.49 Bandwd= 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 32.00 Matching frequency sets: 10 11 12 Track assignments are: track1= 18, 26, 2, 10, 20, 28, 4, 12, 22, 30, 6, 14, 24, 32, 8, 16 barrel=roll_off POSITIONS OF SOURCES USED IN RECORDING SCANS Source Source position (RA/Dec) Error (B1950) (J2000) (Date) (mas) 1749+096 17 49 10.387930 * 17 51 32.818574 17 52 30.329723 0.00 * J1751+0939 09 39 42.82586 * 09 39 00.72841 09 38 54.87769 0.00 J1751+09 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 192391 observations. 2029+121 20 29 32.681260 * 20 31 54.994267 20 32 53.297133 0.01 * J2031+1219 12 09 28.75299 * 12 19 41.34015 12 24 03.99787 0.02 J2031+12 /home/guest/rmc/SCHED/sched11.6/catalogs/sources.gsfc GSFC 2016a X/S astro solution, 4314 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 J1751+0939 sess320.X2048 1 2 3 4 5 6 7 8 9 10 14 0.867 78.867 J2031+1219 sess320.X2048 1 2 3 4 5 6 7 8 9 10 14 1.217 110.717 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) J1751+0939 66.2 J2031+1219 105.2 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