@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@ @ @ @ MTA Monitoring Report 3/31/00 - 4/06/00 @ @ @ @@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@@ ************ CTI trend ************* No changes are observed. Attached email from Catherine. ************** MTA Problem Tracking. ***************** No new problems are reported this week; only same preoblems keep coming: C28VMONB, CUSOB28V, CIUB5V, CIUB15V, CTUB15V, AWD2TQI, AWD5TQI, SEHSE400, 2CE01ATM, 2IMINATM, 2IMHVATM, 2CE00ATM, AWD6TQI ******** Trending *********** In general, no new trends are observed, however, HRMA Struts, HSTRTGRD1,2,4, and 5 show strong trend, and may violate the limits in 2-4 months, if the tends contiune. Also we are changing a few more mta limits in future (suggested values below): Spacecraft Struts: HSSTRTGRD4 -0.50 1.50 -1.00 2.00 TFTE: HTFTEGRD4 -0.50 1.00 -1.00 1.20 TFTE: HTFTEGRD5 -0.50 1.00 -1.00 1.20 TFTE: HTFTEGRD6 -1.80 0.50 -2.00 1.00 *********** ACIS Focal Temperature ******** We had usual peaks around DOY 91, 93.8, 96.2. The peaks reached -106, -110, and -108 C, respectively. ************* Telemetry *********** Nothing special happened. There are usal violations in HRMA, and many jumps due to possible software bugs. *********** Photon Page ************ Mkn observations show good round images; no distotion. BSID DETECTOR GRATING TARGET ANALYSIS --------------------------------------------------------- 907 ACIS-I NONE QB1429-008A,B OK 857 ACIS-S NONE B2 0331+39 OK 944 ACIS-I NONE SGR B2 NO DATA POSTED 896 ACIS-I NONE ABELL 2219 NO SKY NICE PIC 418 ACIS-S NONE MITG J0414+0534 OK 1522 NO INFORMATION NO SKY 604 ACIS-S HETG ALGOL NO DATA POSTED 851 AICS-I NONE BAL 1044+3656 OK 867 ACIS-S NONE Q 1331+170 OK 858 ACIS-S NONE B2 0755+37 OK 446 ACIS-I NONE MKN 421, ZOFF-2 OK 664 ACIS-I NONE 1735-269 OK 140 ACIS-S NONE E0102-72.3 CHIPS3 OK 440 ACIS-S NONE MKN 421, YOFF-15 NO SKY 900 ACIS-I NONE MKW 3S NO SKY 425 ACIS-S NONE SBSG 1520+530 NO DATA POSTED 439 ACIS-S NONE MKN 421,YOFF-10 OK ************ Some Comments from Exparts ******** ----------------------------------------------------------- From Catherine Grant (4/6/00) --- email sent to SOT ----------------------------------------------------------- Estimating the change in CTI since Jan 29 (when we decreased the focal plane temperature to -120C) depends strongly on the correlation you assume between the measured CTI and the cosmic ray background as measured by the S3 amplitude rejected count rate. The data used in this analysis covers the span of Jan. 29 to Apr. 2. Fitting this correlation in a number of ways to different groupings of the available CTI data, the worst case CTI change is: +1.21 x 10-8 / day A conservative guestimate of the error is our CTI measurement accuracy over the measurement span or 2e-6 / 64 = 3.12 x 10-8 / day These numbers can be compared to Dan Schwartz's ACE fluence numbers.