NASA Analysis Report for Z22164 ($22JUN13MH) This report is a contributed analysis report that does not correspond to the database maintained by the IVS Data Centers for this session. (Analyzed by Sergei Bolotin, NVI, Inc. / NASA Goddard Space Flight Center. Spoolfile source: interactive solve/nuSolve analysis.) Problems: None. Number of observations rejected during correlation: 1 observation of 0727-115 at 06:32:27 Number of observations not usable by the software: 4 observation 4, HOBART12:HART15M , 0537-441, 06:38:04, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 18, HOBART12:HART15M , 0537-441, 06:57:43, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 25, HOBART12:HART15M , 0736+017, 07:07:00, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 33, HOBART12:HART15M , 0537-441, 07:18:23, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 3 observation 1, HOBART12:HART15M , 0420-014, 06:30:15, which fits at -3768.9 +/- 53.7 ps observation 2, HOBART12:HART15M , 0458-020, 06:31:18, which fits at -3871.9 +/- 60.3 ps observation 38, HOBART12:HART15M , 0332-403, 07:27:52, which fits at -256.9 +/- 72.8 ps Other comments: None. Parameterization: 6 parameters: UT1 offset atmosphere offset for: HART15M HOBART12 clock offset, first order term, and second order term for: HOBART12 Clock breaks: None Session statistics Observations: 120 scheduled 39 correlated (included in the database) 35 recoverable (usable in Solve/nuSolve) 32 used Session fit: 46.966 ps UT1 formal error: 15.74 microsec Source Performance Number of Observations Scheduled Correlated* Used 0131-522 6 2 2 0308-611 9 3 3 0332-403 9 3 2 0346-279 9 3 3 0402-362 12 4 4 0405-385 9 3 3 0420-014 3 1 0 0437-454 3 1 1 0454-234 6 2 2 0458-020 9 3 2 0537-286 6 2 2 0537-441 9 3 0 0646-306 3 1 1 0648-165 6 2 2 0727-115 9 2 2 0736+017 3 1 0 1057-797 9 3 3 ------------ --------- ---------- ------ Source Total 120 39 32 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.