Aug_13_1999_L22.txt Shift L22 (A22) Start at 1999:225:10:00 GMT = 1999 Aug 13 6:00am EDT End 1999 Aug 13 2:00pm EDT See http://asc.harvard.edu/acis/SOT_reports/sot-shift.html, or /proj/ascwww/AXAF/extra/science/htdocs/acis/SOT_reports/Aug_13_1999_L22.txt. SOT Lead Ed Kellogg SOT SC/ACA Mark Freeman FOT-SI HRC-SI James Reeves ACIS-SI Yousaf Butt (Times will be given in GMT on day 225. not precise.) EVENTS PLAN DONE OBSID -------------- ---- ---- ----- Start shift (06am EDT 13 Aug 1999) 1000 1000 62563 Gyro scale factor & misalignment SOP 6F003 ongo Changed from Goldstone to Canberra 1124 LGA A to B 1147 ACIS radiation entry 1500 Finish SOP 6F003 1530 1310 End shift (2pm EDT 12 Aug) day 225 1800 1853 Canberra LOS 1955 CAP 252 powers down earth sensors Goldstone AOS 2240 Start PCAD checkouts 2300 End radiation day 226 0050 Start ACIS, SAP 61044 0100 NOTES/ISSUES/PROBLEMS --------------------- At H-to-L shift change, 225:1000, Chandra 10.5 hrs before perigee ACA in the Gyro scale factor & misalignment procedure HRC on, low voltage power only EPHIN nominal ACIS Flight Contamination source Monitoring, looking at whatever was in the field of view as we went through the scale factor & misalignment procedure, which does a series of slews to various locations on the sky, with a dwell and ACA lock on the stars, to give data for updating the gyro scale factors and offsets. As of 1220, spacecraft configuration: IU-A, CTU-A, RCTUs A Side, OBC-A Online, OBC-B Offline. PCAD: VDE-A IOE-A, ADE-A, SPE-A/B, FSS-A/B, IRU-1 = LO, IRU-2 = LO. Commanded attitude monitor enabled, Autonomous unloading & RW momentum bias disabled, Momentum monitor fault safing action (SCS #9) disabled, Auto transition to NPM function disabled (temporary) Pointing is NMM sun pointed, 120 deg SA angle Vacuum 4.5e-6 torr, Link via Canberra-DSN direct-512-LGA-B. The gyro scale factor & misalignment procedure was completed successfully. At the last maneuver back to normal sun mode, looking at the South Ecliptic Pole, we acquired 6 out of a possible 8 stars in ACA. For the 8 pointings done in this procedure, we got enough stars on each occasion to expect a successful calculation. While tracking stars, we also saw an instance of a cosmic ray hit that caused the tracking box to shift over a bit. The ACA recovered quickly and centered the star in the box again. This is an example of the recovery behavior that we were certain exists when tracking stars, but which is not as yet available when tracking fidlites. At 2300, we plan to start PCAD checkout activities. These could be done as early as 226:0300, 7 1/2 hours earlier than the planned start of OFLS scheduled activities. We should be prepared to use that time effectively.