Session Notes for RD0701 Prepared by D. Behrend, NVI, Inc./GSFC =========================================================== PURPOSE AND GENERAL NOTES =========================================================== The purpose of rd0701 is to continue the series of Gb/s tests and to check new stations in Gigabit mode (station checkout). HartRAO and Matera run their first Gb/s test in an IVS session. This session has all stations fully scheduled. HartRAO was given double weight. The schedule uses the 80 best sources. Wettzell will observe INT I07052 and join rd0701 at about 1950 UT. This schedule was generated using ultra-high minimum SNRs of 80 at X-band and 60 at S-band. An extra 3 seconds is added at the start of each scan for correlator synchronization. These extra seconds are not included in the calculation of the scan SNR. This session must be recorded on Mk5 disks. Multiple disk modules will be required. Stations must plan for disk changes by referring to the drudg listings that display the number of Gb recorded during the experiment. Refer to the last sections of these notes for reminders about testing and setup for the Gb/s recording mode. Testing prior to the experiment is essential for success. =========================================================== Parameter values for experiment RD0701 Experiment description: R&D-01 2007 Scheduler: dbb Correlator: HAYSTACK Nominal start: 2007-052-18:00:00 Nominal end: 2007-053-18:00:00 Current yyyyddd: 2007052 (2007.14) ( 14153 MJD, WED. 21FEB.) Greenwich sidereal time: 4: 5: 6.00 (18: 0: 0 UT) Sun's RA and DEC: 22h 18.7m -10d 30.2 =========================================================== First observations Observation listing from file ./rd0701.skd for experiment RD0701 Source Start DURATIONS name yyddd-hhmmss Hh Ma Ny Wf Wz 0235+164 07052-180000| 199 87 109 199 | 4C39.25 07052-180832| 67 40 67 | 1044+719 07052-181024| 101 56 101 | ...... 0607-157 07052-195021| 40 40 40| 1156+295 07052-195537| 332 306 332| ...... End of listing. =========================================================== Last observations Observation listing from file ./rd0701.skd for experiment RD0701 Source Start DURATIONS name yyddd-hhmmss Hh Ma Ny Wf Wz ...... CTA26 07053-174815| 348 93 151 348 63| 0955+476 07053-175206| 49 49 40| 1128+385 07053-175342| 79 79 70| 1803+784 07053-175616| 72 69 72 62| 1739+522 07053-175803| 46 47 47| End of listing. =========================================================== SKED Summary from file ./rd0701.skd for experiment RD0701 (all scans with at least one subnet station) Average number of obs. per baseline per source (normalized by up-time) = 6.4 Min = .0 Max = 65.5 (Baseline Hh-Ny on CTA26 ) RMS = 9.9 Total time: 1439 minutes ( 24.0 hours). Key: Hh=HARTRAO Ma=MATERA Ny=NYALES20 Wf=WESTFORD Wz=WETTZELL Hh Ma Ny Wf Wz Avg % obs. time: 43 38 28 28 31 34 % cal. time: 2 4 2 2 3 3 % slew time: 41 24 11 9 8 19 % idle time: 13 34 58 60 57 45 total # scans: 212 304 212 173 267 233 # scans/hour : 9 13 9 7 11 10 Avg scan (sec): 175 109 112 139 100 126 Total GBytes: 5350 4753 3423 3467 3846 4168 Total GB(M5): 4756 4225 3043 3082 3419 3705 # of tapes : .1 .1 .1 .1 .1 tape change times (hhmm): Total number of tapes: .7 Total GBytes (M5) recorded: 18524.0 # OF OBSERVATIONS BY BASELINE | Hh Ma Ny Wf Wz StnTotal ----------------------------------- Hh| 206 86 61 172 525 Ma| 179 134 260 779 Ny| 149 167 581 Wf| 127 471 Wz| 726 Number of 2-station scans: 62 Number of 3-station scans: 113 Number of 4-station scans: 135 Number of 5-station scans: 33 Total # of scans, observations: 343 1541 =========================================================== Recording mode Name Code GEOSX8N 8F Recording mode setup for: HARTRAO MATERA NYALES20 WESTFORD WETTZELL Mode Tot.Rate Tot.BandW #chan #bits Barrel Mk341:2 1012.736 Mbits 506.368 MHz 14 2 NONE Chan.BW #Subpasses Tracks(*fan) Tot.tracks Speed 16.00 MHz 1 16(*2) 32 .02 X-band spanned bw= 720.0 MHz rms spanned bw= 280.4 MHz S-band spanned bw= 140.0 MHz rms spanned bw= 50.9 MHz Effective number of channels recorded per sub-pass X S Total 19.780 11.868 31.648 =========================================================== Tape types ID Station Tape length Density Passes Hh HARTRAO Mark5A Ma MATERA Mark5A Ny NYALES20 Mark5A Wf WESTFORD Mark5A Wz WETTZELL Mark5A =========================================================== SNR Targets Minimum SNR by baseline for multi-baseline scans X-band (margin 0) S-band (margin 0) Hh Ma Ny Wf Hh Ma Ny Wf Ma 80 Ma 60 Ny 80 80 Ny 60 60 Wf 80 80 80 Wf 60 60 60 Wz 80 80 80 80 Wz 60 60 60 60 ====================================================================== TESTING AND SETUP ====================================================================== This session requires 4 ribbon cables between the Formatter and the Mark 5 Recorder. If one of these cables is missing, the correlator will not be able to read any of the data. Recording 1GB/s data should be verified for your station if you have not already done so. To do this, Mark 4 stations should run ftp://web.haystack.edu/pub/mark5/SNAP/chk1024.snp with ftp://web.haystack.edu/pub/mark5/SNAP/chk1024.prc VLBA4 stations such as Kokee Park, should run ftp://web.haystack.edu/pub/mark5/SNAP/vchk1024.snp and ftp://web.haystack.edu/pub/mark5/SNAP/vchk1024.prc If you have FS 9.9.0 or later installed, you may have already installed these files as part of the upgrade. If not, they are available in /usr2/fs/systests directory. Instructions on installing, using, and analyzing the results of this test can be found in "systests.txt" in the same directory. Regardless of where you get the .snp and .prc files, you should use the systests "chk1024" script to analyze the results of the test. For more information, please try the shell command: chk1024 -h or try: chk1024 logfile for a summary of the results from "logfile". Please be sure to start a new log (i.e., rename the existing old one) each time you run one of the test .snp schedules mentioned above. If the results from "chk1024" aren't completely positive (all setups, particularly "1g" shown as 64 tracks tested, "100% good", and NO "other tracks present" clause), please send a copy of the log to dsmythe@haystack.mit.edu, or put a copy in the ivsmisc area in ivscc (please use a unique name for your file so that your log is not overwritten by others), with a follow-up e-mail to dsmythe. Do not touch any of the cables between the Formatter and the Mark 5 Recorder after this test has been run without any errors. ====================================================================== DISK MODULE CHANGES ====================================================================== This session will require 2, 3 or 4 disk modules, depending on the sizes that you have available at your station. DRUDG does not know the sizes, so it shows an ever-increasing GByte count. Please be aware that you will have to change modules several times during this session, and plan accordingly. There are a few of things to consider: 1) It is desriable to precondition all modules ahead of time that you will use for the session. Recording at the 1 Gigabit/second often works better if the modules have been preconditioned since their last shipment. If you don't have time to precondition all the modules that are needed, plus one or two spares, please precondition as many as you can. 2) Mark module change times. Select the modules you will use for this session, note their sizes, and then mark by hand the places in the schedule where a module change will be necessary, and which bank will need to be changed. You can use the drudg Option 5 listing for this purpose. Unfortunately it is not possible to predict the module change times exactly. For various reasons, a module can be finished at a different time, usually earlier than expected. As long as a module does not end a great deal earlier than expected, this should not cause a problem. 3) Change modules promptly. When a module is full, the FS will automatically switch to the next one and put up a notice that you should change the old one. It is good practice to change the module as soon as it's called for, because then a new one is available in case the module in use should end prematurely for some reason. If you have any questions, please contact Ed Himwich (weh@ivscc.gsfc.nasa.gov).