Oct_10_1999_M79.txt Shift M79 Start at 1999:283:20:30:00 GMT = 1999 Oct 10 4:30pm EDT End 1999 Oct 10 7:00pm EDT See http://asc.harvard.edu/acis/SOT_reports/sot-shift.html, or /proj/ascwww/AXAF/extra/science/htdocs/acis/SOT_reports/Oct_01_1999_M70.txt. SOT Lead Bill Podgorski SOT SC/ACA FOT-SI HRC-SI ACIS-SI OTHER Plan: - Running P21b load, SHORT eclipse (OBA setpoint raised) EVENTS DONE OBSID -------------- ---- ----- Start Shift 283:2030 ----- Out of Contact ------ AOS DSS-54 (Madrid) 283:2130 62355 ----- Real time------ DSS-54 (Madrid) Chandra State at AOS was nominal (see note 1) Eclipse start 283:2230 Eclipse end (see note 2) 283:2309 LOS End of shift 283:2350 NOTES/ISSUES/PROBLEMS --------------------- 1) Chandra's state at AOS was as follows: UTC 1999:283:21:31:01 (Sun Oct 10) OBT 1999:283:21:30:34 CTUVCDU 4585983 FMT2_NORM OBC s/w NRML OBC Errs 1 OBT 55978234.55 ONLVCDU 4585976 OBSID 62355 EPState SUN SIM TTpos -99616 HETG Angle 81.3 PCADMODE NPNT RA 97.697 Bus V 30.55 SIM FApos -467 LETG Angle 81.3 PCONTROL NPNT Dec -50.700 Bus I 65.30 AOFSTAR GUID Roll 79.485 ACA Object SSSSSSSS Dither ENAB HRC-I HV OFF ACA ImFunc TTTTTNNN Dith Yang -1.72 Yaw Rate 0.01 HRC-S HV OFF ACA CCD Temp -10.4 Dith Zang -7.99 Pitch Rate 0.24 OBSMode NEXT ACA Int Time 1.698 Roll Rate -0.44 Door OP UNAC AOACSTAT OK FSS SunAlfa SUN Door CL UNAC FSS Alfa -0.30 Batt 1 SOC 100.00% Avg HRMA Temp 70.61 FSS Beta -0.16 Batt 2 SOC 100.00% Avg OBA Temp 50.50 SA Resolv 89.97 Batt 3 SOC 100.00% ACIS Stat7-0 66 OBA Tavg Fault NFLT SA Sun Pres ILLM Cold Rad -120.7 OBA Trng Fault NFLT Warm Rad -82.0 HRMA power 83.50 OBA power 70.20 EPHIN Geom LARG INT cnt 121 Roll Mom. 5.203 P41GM cnt 0 Pitch Mom. -1.319 A-Leak 0.1720 Yaw Mom. 17.148 B-Leak 0.0280 2) Eclipse performance was acceptable. The OBA temp went up to just above 53 degrees (setpoint raised to 55 degrees). At LOS the OBA temp was about 52.8 degrees and slowly trending downward. The peak bus voltage reached was about 33 volts. The power draw characteristics of the OBA were not exactly as expected and this issue must be understood so that future eclipse performance can be accurately predicted.