Session Notes for RD0802 Prepared by D. Behrend, NVI, Inc./GSFC =========================================================== PURPOSE AND GENERAL NOTES =========================================================== The purpose of rd0802 is to test 512 Mbps recording mode for possible usage in CONT08. The frequency setting is basically the R1 mode (256 Mbps) but using 2-bit sampling instead of 1-bit. The schedule was generated using SNRs of 40 at X-band and 30 at S-band for all stations but TIGO. TIGO has SNRs of 20 at X and 15 at S in order to increase their number of observations. The schedule uses the 80 best geodetic sources. TIGO has a weight factor of 5. Ny-Alesund was tagged along. Kokee Park and Wettzell will observe INT I08051 and join rd0802 at about 1950 UT. 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 may be required. Stations must plan for disk changes by referring to the drudg listings that display the number of Gb recorded during the experiment. =========================================================== Parameter values for experiment RD0802 Experiment description: R&D-02 2008 Scheduler: dbb Correlator: HAYSTACK Nominal start: 2008-051-18:00:00 Nominal end: 2008-052-18:00:00 Current yyyyddd: 2008051 (2008.14) ( 14517 MJD, WED. 20FEB.) Greenwich sidereal time: 4: 0:12.00 (18: 0: 0 UT) Sun's RA and DEC: 22h 14.0m -10d 57.1 =========================================================== First observations Observation listing from file ./rd0802.skd for experiment RD0802 Source Start DURATIONS name yyddd-hhmmss Kk Ny On Tc Wf Wz 0235+164 08051-180000| 165 305 305 121 | 2136+141 08051-180547| 480 480 299 | ...... 0454-234 08051-195003| 215 215 67| 0727-115 08051-195429| 40 40| 2136+141 08051-195442| 161 304 304 | End of listing. =========================================================== Last observations Observation listing from file ./rd0802.skd for experiment RD0802 Source Start DURATIONS name yyddd-hhmmss Kk Ny On Tc Wf Wz ...... 0454-234 08052-175350| 233 233 71| 1749+096 08052-175436| 40 40 | 0119+115 08052-175845| 43 54 54 40| End of listing. =========================================================== SKED Summary from file ./rd0802.skd for experiment RD0802 (all scans with at least one subnet station) Average number of obs. per baseline per source(normalized by up-time) = 7.9 Min = .0 Max = 135.0 (Baseline Ny-On on 1741-038) RMS = 12.4 Total time: 1440 minutes ( 24.0 hours). Key: Kk=KOKEE Ny=NYALES20 On=ONSALA60 Tc=TIGO Wf=WESTFORD Wz=WETTZELL Kk Ny On Tc Wf Wz Avg % obs. time: 31 29 51 48 53 31 40 % cal. time: 3 4 5 2 5 4 4 % slew time: 13 20 26 5 19 13 16 % idle time: 52 46 17 44 23 51 40 total # scans: 262 336 400 178 390 384 325 # scans/hour : 11 14 17 7 16 16 14 Avg scan (sec): 103 74 110 231 118 69 116 # data tracks: 32 32 32 32 32 32 # Mk5 tracks: 32 32 32 32 32 32 Total GBytes: 1934 1801 3164 2966 3301 1902 2511 Total GB(M5): 1719 1601 2812 2636 2934 1691 2232 # of tapes : .1 .1 .1 .1 .1 .1 tape change times (hhmm): Total number of tapes: .9 Total GBytes (M5) recorded: 13393.5 # OF OBSERVATIONS BY BASELINE | Kk Ny On Tc Wf Wz StnTotal ---------------------------------------- Kk| 144 133 115 235 136 763 Ny| 314 61 236 281 1036 On| 75 250 359 1131 Tc| 169 77 497 Wf| 236 1126 Wz| 1089 Number of 2-station scans: 60 Number of 3-station scans: 225 Number of 4-station scans: 136 Number of 5-station scans: 103 Number of 6-station scans: 16 Total # of scans, observations: 540 2821 =========================================================== Recording mode Name Code GEOSX8N 8F Recording mode setup for: KOKEE NYALES20 ONSALA60 TIGOCONC WESTFORD WETTZELL Mode Tot.Rate Tot.BandW #chan #bits Barrel Mk341:2 506.368 Mbits 253.184 MHz 14 2 NONE Chan.BW #Subpasses Tracks(*fan) Tot.tracks Speed 8.00 MHz 1 16(*2) 32 .01 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 Kk KOKEE Mark5A Ny NYALES20 Mark5A On ONSALA60 Mark5A Tc TIGOCONC Mark5A Wf WESTFORD Mark5A Wz WETTZELL Mark5A =========================================================== SNR Targets Minimum SNR by baseline for multi-baseline scans X-band (margin 5) S-band (margin 3) Kk Ny On Tc Wf Kk Ny On Tc Wf Ny 40 Ny 30 On 40 40 On 30 30 Tc 20 20 20 Tc 15 15 15 Wf 40 40 40 20 Wf 30 30 30 15 Wz 40 40 40 20 40 Wz 30 30 30 15 30 ====================================================================== DISK MODULE CHANGES ====================================================================== This session will require 1 or 2 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 may have to change modules 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 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 possible after it is 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 (Ed.Himwich@nasa.gov).