NASA Analysis Report for Z22290 ($22OCT17MH) 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: 0 Number of observations not usable by the software: 5 observation 7, HOBART12:HART15M , 1334-127, 06:40:46, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 8, HOBART12:HART15M , 1647-296, 06:42:28, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 9, HOBART12:HART15M , 1758-651, 06:45:01, quality code X: 0 S: 9, fringe code X: ' ' S: ' ' observation 14, HOBART12:HART15M , 1243-072, 06:59:52, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' observation 25, HOBART12:HART15M , 1657-261, 07:21:29, quality code X: 9 S: 0, fringe code X: ' ' S: ' ' Number of observations rejected during analysis: 1 observation 27, HOBART12:HART15M , 1546+027, 07:26:00, which fits at 170.5 +/- 60.9 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: 29 scheduled 29 correlated (included in the database) 24 recoverable (usable in Solve/nuSolve) 23 used Session fit: 60.767 ps UT1 formal error: 14.30 microsec Source Performance Number of Observations Scheduled Correlated* Used 0308-611 2 2 2 0530-727 2 2 2 1004-500 1 1 1 1057-797 2 2 2 1144-379 2 2 2 1213-172 1 1 1 1243-072 1 1 0 1244-255 1 1 1 1334-127 2 2 1 1351-018 1 1 1 1406-076 2 2 2 1424-418 2 2 2 1451-375 2 2 2 1502+036 1 1 1 1508-055 1 1 1 1538+149 1 1 1 1546+027 1 1 0 1606+106 1 1 1 1647-296 1 1 0 1657-261 1 1 0 1758-651 1 1 0 ------------ --------- ---------- ------ Source Total 29 29 23 * Correlated means included in database. Please note that the number of recoverable (usable) observations cannot be broken down by source for Intensive solutions.