Statistics: # IMAGE NPIX MEAN RMS MIN MAX ACIS_nov01_total.fits 6004901 5.905 14.294 0.0 14331.0 ACIS_nov01_total I2 Node 0 262654 5.332285 4.630499 0.0 175.0 ACIS_nov01_total I2 Node 1 262654 6.409459 8.562094 0.0 303.0 ACIS_nov01_total I2 Node 2 262654 7.448263 13.059591 0.0 404.0 ACIS_nov01_total I2 Node 3 262654 8.156453 17.050854 0.0 506.0 ACIS_nov01_total I3 Node 0 262654 8.495412 17.983638 0.0 502.0 ACIS_nov01_total I3 Node 1 262654 7.650540 13.657848 0.0 545.0 ACIS_nov01_total I3 Node 2 262654 6.488144 9.005573 0.0 312.0 ACIS_nov01_total I3 Node 3 262654 5.238881 4.496267 0.0 174.0 ACIS_nov01_total S2 Node 0 262397 6.106297 51.337795 0.0 14331.0 ACIS_nov01_total S2 Node 1 262397 6.899862 14.868258 0.0 303.0 ACIS_nov01_total S2 Node 2 262397 6.112642 7.455193 0.0 3469.0 ACIS_nov01_total S2 Node 3 262397 5.837445 2.702221 0.0 37.0 ACIS_nov01_total S3 Node 0 262397 10.835135 3.859614 0.0 82.0 ACIS_nov01_total S3 Node 1 262397 12.967328 6.325135 0.0 69.0 ACIS_nov01_total S3 Node 2 262397 13.115421 5.178487 0.0 79.0 ACIS_nov01_total S3 Node 3 262397 10.972130 4.054595 0.0 180.0
Statistics: # IMAGE NPIX MEAN RMS MIN MAX ACIS_total.fits 6004901 255.59 474.17 0.0 404123.0 ACIS_total I2 node 0 262654 152.545234 122.420427 40.0 9330.0 ACIS_total I2 node 1 262654 182.112490 256.131781 100.0 8275.0 ACIS_total I2 node 2 262654 207.903596 394.983931 108.0 11559.0 ACIS_total I2 node 3 262654 224.642678 523.162252 0.0 14302.0 ACIS_total I3 node 0 262654 241.704063 517.203810 125.0 13943.0 ACIS_total I3 node 1 262654 221.836682 385.335458 123.0 11030.0 ACIS_total I3 node 2 262654 186.509469 249.251098 46.0 8038.0 ACIS_total I3 node 3 262654 150.166622 109.904024 0.0 4453.0 ACIS_total S2 node 0 262397 306.411102 335.725447 104.0 51434.0 ACIS_total S2 node 1 262397 387.438473 986.476460 114.0 19302.0 ACIS_total S2 node 2 262397 349.740957 257.077932 139.0 126052.0 ACIS_total S2 node 3 262397 341.492361 75.415179 0.0 757.0 ACIS_total S3 node 0 262397 689.531062 613.759180 174.0 4575.0 ACIS_total S3 node 1 262397 826.884080 673.787660 0.0 69416.0 ACIS_total S3 node 2 262397 560.522685 139.472073 170.0 3212.0 ACIS_total S3 node 3 262397 495.080557 134.206874 0.0 2968.0
Observations with cold radiator temperature deviation larger than 0.5 C from the nominal value of -127.92905 C are dropped (after DOM 200).
Mean CTI observed when FPT~ -119 C and no testing modes (Squeegy, cuckoo, etc.) (average of 4 nodes per chip). CTI's are computed for Mn K alpha, and defined as slope/intercept x10^4 of row # vs ADU. Data file here
CTI slopes were computed for data point after DOM 200 and inside of 1 sigma deviation. Using only data point in 1 sigma range, we drop high temperature observations, squeegy observations, and other outliers. A independent variable is date, and a dependent variable is CTI. Note: Unit is cti/day from this month report. Front Side Illuminated S Array Node 0 Node 1 Node 2 Node 3 CCD4 1.415e-8 1.797e-8 1.848e-8 1.645e-8 CCD6 1.406e-8 1.700e-8 1.607e-8 1.498e-8 CCD8 1.257e-8 1.306e-8 1.273e-8 1.171e-8 CCD9 1.298e-8 1.632e-8 1.496e-8 1.102e-8 AVG 1.264e-8 Front Side Illuminated I Array Node 0 Node 1 Node 2 Node 3 CCD0 1.288e-8 1.724e-8 1.706e-8 1.451e-8 CCD1 1.367e-8 1.570e-8 1.620e-8 1.245e-8 CCD2 1.406e-8 1.643e-8 1.630e-8 1.269e-8 CCD3 1.299e-8 1.536e-8 1.484e-8 1.373e-8 AVG 1.336e-8 Detrended AVG 1.246e-8 Back Side Illuminated S Array Node 0 Node 1 Node 2 Node 3 CCD5 5.414e-9 6.310e-9 6.508e-9 2.852e-9 AVG: 4.930e-9 CCD7 3.138e-9 4.633e-9 4.813e-9 3.075e-9 AVG 3.979e-9
The Mean (max) FPT: -118.06 std dev: 1.22 mean width: 0.32 std dev: 0.11
DOY | Focal Temp | S.D. |
---|---|---|
306.92 | -118.58 | 0.32 |
309.49 | -118.41 | 0.24 |
312.02 | -118.90 | 0.23 |
314.41 | -119.22 | 0.16 |
314.86 | -117.93 | 0.48 |
317.48 | -117.61 | 0.38 |
320.09 | -118.25 | 0.31 |
325.39 | -114.86 | 0.51 |
328.05 | -118.74 | 0.26 |
New Plots!
From this month, we are using 10 period moving averages to show trends of peak temperatures and peak widths. Note, the gaps in the width plot are due to missing/corrupted data.
The following pixels consistently showed a bias level more than 5 sigma away the chip's mean level during this period.
CCD0 | CCD2 | CCD3 | CCD4 | CCD5 | CCD6 | CCD7 | CCD8 | |
---|---|---|---|---|---|---|---|---|
New for This Month | (811,637) | |||||||
Previously Reported Warm Pixels | (526,66) | (247,364) |
(1-3,775-1022) (226,565) (232-245,313) (510-511,775-1022) (512,775) (513,776-1024) (607,281) (1022,166) |
(360,249) (766,501) |
(1-3, 1-1024) (510-515,775-1024) (1022,775) |
(64,482) (587,544) | ||
Previously Reported - Healed ? | (483,816) | (453,1) | ||||||
Flickering ? | (995,200) | (509,spurious rows) | (360,249) |
(4,spurious rows) (509,spurious rows) (516,spurious rows) |
Hot Pixels - No new hot pixels observed this month.
Previously reported:
Pixel 1022,166 of Quad 4 CCD 5.
We define a hot pixel as a pixel with the count
rate 1000 counts above the average
From: Royce Buehler Subject: FEP Power cycling commands Here are the specifics on the changes we've just made to add FEP power cycling to the ACIS tables. Dan, let me know who else to forward this to. What was changed: Every science run which actually calls for a bias, and which previously called out a WSVIDALLDN command. What was not changed: Science runs which do not actually call for a bias. (This includes configurations like TN_00156B, which do not call for a bias although the offline system thinks they do. Such exceptional simodes all begin with TN or CN.) Science runs which did not previously call out a WSVIDALLDN command. There were around 150 of these, all archaic. The parameter generation system can no longer assign any of these to an observation. What exactly changed: The command WSVIDALLDN, followed by a delay of 18 seconds on orbit, was replaced by the 3 commands AA00000000 (stop science) followed by 4 second delay AA00000000 " " " " WSPOW00000 (power down all feps and video boards) followed by a 24 second delay. The next command in all of these science runs is a WSPOW which tells the BEP to power up all FEPs and the specific video boards needed for the run. We had a premonition long ago that we wouldn't always be certain of having juice to the FEPs at the start of a science runt, so we decided to explicitly power on the FEPs and to provide sufficient following delay (63 seconds) to power up six video boards, and six FEPs, and to load all the FEPs. Consequently, there was no need to adjust this or any of the remaining commands. Next week, we'll be saving ourselves 27 seconds of science on each bias run by moving the two dump commands (dump sys config and dump Huffman tables) to run after the start science command.
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_11_2001.fits 16777216 0.01685 0.13099 0.0 6.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCI_08_1999_11_2001.fits 16777216 1.22396 3.18807 0.0 462.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_11_2001.fits 16777216 0.05182 0.31624 0.0 37.0
IMAGE NPIX MEAN STDDEV MIN MAX HRCS_08_1999_11_2001.fits 16777216 4.10397 10.34303 0.0 1815.0
We plot the width of the zero order streak of ACIS/HETG observations and
the width of the zero order image for HRC/LETG observations of point sources.
No significant defocusing trend is seen at this time. See
Gratings Focus
pages.
Motion | Monthly total | Annual Total | Mission Total | Monthly Delta |
---|---|---|---|---|
Nov00 thru Nov01 | Jul99 thru Nov01 | current - previous | ||
SIM | ||||
SIM FA (STEPS) | 8488.00 | 63806.0 | 229239. | 4848.00 |
SIM TSC (STEPS) | 5.43387e+06 | 5.91151e+07 | 1.32925e+08 | 1.42224e+06 |
SIM TSC (# Moves) | 46 | 484 | 1185 | 19 |
mean SIM TSC at ACIS-I/sdev/# obs | 92903.0/ 0.00000/ 7 | 92903.0/ 0.00000/ 77 | 92968.4/ 266.077/ 203 | 0.00000/ 3 |
mean SIM TSC at ACIS-S/sdev/# obs | 75473.4/ 409.854/ 16 | 75413.3/ 476.600/ 160 | 75427.6/ 457.953/ 405 | -150.117/ 7 |
mean SIM TSC at HRC-I/sdev/# obs | -50504.0/ 0.00000/ 1 | -50504.3/ 0.690410/ 25 | -50504.5/ 0.621535/ 75 | 0.500000/ -1 |
mean SIM TSC at HRC-S/sdev/# obs | -99615.9/ 0.363137/ 14 | -99621.2/ 45.2743/ 149 | -99614.3/ 58.6464/ 328 | 0.0312500/ 5 |
GRATINGS | ||||
No. HETG insertions | 2.00000 | 35.0000 | 100.000 | 0.00000 |
No. LETG insertions | 4.00000 | 21.0000 | 65.0000 | 2.00000 |
mean HETG inserted angles/sdev (A) | 6.33750/ 0.00000 | 6.34821/ 0.00401785 | 6.71250/ 0.428978 | 0.00000 |
mean HETG inserted angles/sdev (B) | 6.33750/ 0.00000 | 6.33750/ 0.00000 | 6.48230/ 0.143354 | 0.00000 |
mean LETG inserted angles/sdev (A) | 7.08750/ 0.00000 | 7.18125/ 0.0277549 | 8.67841/ 6.56852 | 0.00000 |
mean LETG inserted angles/sdev (B) | 4.46250/ 0.00000 | 5.19464/ 11.2567 | 4.57383/ 0.0566057 | 0.00000 |
mean HETG retracted angles/sdev (A) | 79.8375/ 0.00000 | 79.8482/ 0.00401786 | 80.5237/ 0.687656 | 0.00000 |
mean HETG retracted angles/sdev (B) | 80.5875/ 0.00000 | 80.6089/ 0.00779937 | 81.1407/ 0.589484 | 0.00000 |
mean LETG retracted angles/sdev (A) | 79.0875/ 0.00000 | 79.2482/ 0.0361607 | 80.3624/ 2.44248 | 0.00000 |
mean LETG retracted angles/sdev (B) | 78.3375/ 0.00000 | 78.4268/ 0.0267857 | 79.1048/ 0.753359 | 0.00000 |
Reaction Wheel Rotations | Past 12 Months | Jan00 thru current | ||
AORWDAY1 | 6.50341e+07 | 9.65357e+08 | 1.83934e+09 | -1.73500e+07 |
AORWDAY2 | 7.60810e+07 | 9.53524e+08 | 1.80955e+09 | -1.27631e+07 |
AORWDAY3 | 5.79744e+07 | 1.03597e+09 | 1.96097e+09 | -4.40048e+07 |
AORWDAY4 | 7.00865e+07 | 9.72498e+08 | 1.85409e+09 | -8.72968e+06 |
AORWDAY5 | 7.10277e+07 | 9.46432e+08 | 1.79712e+09 | -2.13856e+07 |
AORWDAY6 | 6.29508e+07 | 1.04169e+09 | 1.96460e+09 | -3.53428e+07 |
Since September 24, space weather forced 7 radiation-protection actions --- 4 autonomous and 3 commanded. All recoveries proceeded nominally. A total of about 1106 Ksec of scheduled science observing time has been lost due to radiation triggered (autonomous or manual) activations of SCS 107.
The most recent solar-proton storm reached severe (S4) levels. This is the 7th >=S3 event of this solar cycle and the 4th since September 24, of 7 expected for the solar cycle.
Rate of increase of the ACIS CCD CTI continues to fall within allocation. MIT/ Catherine Grant's most recent analysis (data through Nov 18 and consistent with SOT analysis through Nov 29) gives the following:
There is a natural desire to reduce this rate, especially to minimize the amount of gain re-calibration. After some initial discussions, the CXC SOT is examining quantitatively the potential benefits of scheduling the HRC or gratings during periods of high geomagnetic vulnerability.
SvT has completed software for generating the next Chandra Radiation Model database. This version incorporates Polar data with the Geotail data, to interpolate better the proton fluxes at high GSM latitudes, where Chandra spends much of its time. The database will be interchangeable with the existing one and contains version identifiers for CXC configuration management. SvT is currently exercising software to generate CRM database. We expect that SvT will complete populating the database by the end of 2002 January.
* This memo was originally sent out on Fri, 30 Nov 2001 16:43:18 by Steve O'Dell
Year | Month | |||||||||||
---|---|---|---|---|---|---|---|---|---|---|---|---|
1999 | Jul | Aug | Sep | Oct | Nov | Dec | ||||||
2000 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |
2001 | Jan | Feb | Mar | Apr | May | Jun | Jul | Aug | Sep | Oct | Nov | Dec |