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Dec 31st Radiation Telecon and Summary:
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Due to elevated ACE P3 rates, a telecon was held at 11:45am today. At the time of the telecon, the 2 hr average P3 rate was slightly above the alert limit of 50000. One of the two predicted CME's had passed, and one more was expected.
Based on the elevated rates and expectation for continued high rates for another day, the consensus was to protect the science instruments by manually activating SCS-107. SCS-107 ran nominally, starting at 2024:366:17:17:09.
It is expected that the radiation will quiet down in the next two days. The current target for uplink of return to science loads is the comm pass on DSS-65 at 10:15 PM Thu 02-Jan (2025:003:03:15:00). The current plan is for a "pickup" replan, following the original DEC2324 two-week loads and potentially appending the JAN0625 loads. This is subject to evaluation by FOT and SOT MP.
Although we prefer to quote CTI values of the cleanest data (FT <= -119.7 C, int time > 7000sec), the data that fulfills these conditions are getting rare. We now quote CTI based on temperature corrected data for Focal plane temperature <= -118.5 C).
The unit is now CTI/year not CTI/day.
Average of ACIS-I CCDs (MnKa) slope: | 5.214e-02 CTI/year | (1.428e-04 CTI/day) |
---|---|---|
Detrended slope: | 4.865e-02 CTI/year | (1.333e-04 CTI/day) |
We display all bad pixels that have showed up in past, and, if any, previously unknown bad pixels appeared in the last 14 days. We also list hot pixels (defined as 1000 above the average of bias background). Warm columns 509-514 are probably due to boundaries.
New definitions of warm pixels and flickering pixels (May 15, 2014). If a pixel displays the level beyond a threshold for more than 70% of the time in the past two weeks, the pixel is categorized as a "warm" pixel. If a pixel is above the threshold more than 30% of time but less than 70% of the time in the past two weeks, the pixel is categorized as a "flickering" pixel.
CCD0 | CCD1 | CCD2 | CCD3 | CCD4 | CCD5 | CCD6 | CCD7 | CCD8 | CCD9 | |
---|---|---|---|---|---|---|---|---|---|---|
Previously Unknown Bad Pixels | ||||||||||
Current Warm Pixels | (985,393) (910,239) | (837,378) (178,149) (803,225) (104,31) (526,66) (99,899) | (21,95) | (670,387) | (335,412) | |||||
Flickering Warm Pixels | (283,278) | (370,70) (427,125) (802,665) | (726,537) (665,25) (353,201) | (931,553) (680,391) (617,159) (394,80) (811,637) | (161,206) (367,511) (282,385) (233,227) (357,303) (263,317) (877,408) (233,102) (369,376) (669,577) (728,340) | (849,169) (1000,214) (884,31) | (597,187) (881,53) (838,239) (893,490) (332,324) (139,109) (675,304) (182,474) (275,393) (136,65) | (150,374) (749,477) | ||
Current Hot Pixels | ||||||||||
Flickering Hot Pixels | ||||||||||
Warm column candidates | 512 510 1022 | 512 1022 | ||||||||
Flickering Warm column candidates |
For this period, 6 peaks are observed.
Day (DOY) | Temp (C) | Width (Days) | |
---|---|---|---|
359.40 | -116.00 | 0.11 | |
359.64 | -108.74 | 0.62 | |
360.32 | -107.97 | 0.53 | |
361.04 | -106.31 | 0.74 | |
361.94 | -109.86 | 0.97 | |
363.66 | -103.10 | 4.25 |
Weekly focal plane temperature with sun angle, earth angle, and altitude overplotted. Sun angle is the solar array angle, that is the angle between the sun and the optical axis (+X axis). The earth angle is the angle between earth and the ACIS radiator (+Z axis). Altitude varies from 34 kkm to 128 kkm.
17 TSC moves this period
weekly average time/step | 0.00135 s |
---|---|
mission average time/step | 0.00132 s |
New violations or new extrema are shown in blue cells.
MSID | 12/27/24 | 12/28/24 | 12/29/24 | 12/30/24 | 12/31/24 | 01/01/25 | 01/02/25 | yellow limits (lower) upper | red limits (lower) upper | Units | Description |
AFTBLKHDT | 308.47 | 308.62 | 310.14 | (260.2) 303.0 |
(250.2) 308.0 |
TEMP | AFT BULKHEAD TEMP | ||||
AWD1TQI | (-3.39) | (-1.22) 1.22 |
(-3.3) 3.3 |
AMP | WHEEL 1 TORQUE CURRENT | ||||||
AWD4TQI | (-3.43) | (-1.22) 1.22 |
(-3.3) 3.3 |
AMP | WHEEL 4 TORQUE CURRENT | ||||||
AWD6TQI | (-3.47) | (-3.39) | (-1.22) 1.22 |
(-3.3) 3.3 |
AMP | WHEEL 6 TORQUE CURRENT | |||||
CALPALV | (112.00) | (126.0) 128.0 |
(125.0) 129.0 |
V | Cal Pulser Amplitude | ||||||
CTXBPWR | (0.00) | (0.00) | (0.00) | (0.00) | (36.12) 37.0 |
(36.0) 38.0 |
DBM | TRANSMITTER B OUTPUT POWER | |||
HRMAAVG | (304.47) | (304.70) | (306.0) 308.0 |
(305.0) 309.0 |
K | AVG OF HRMA METRICS | |||||
IMHBLV | (0.00) | (126.0) 128.0 |
(125.0) 129.0 |
(2IMHBLV) | Imaging Bot & Top MCP HV Monitor | ||||||
IMHVLV | (79.00) | (126.0) 128.0 |
(125.0) 129.0 |
(2IMHVLV) | Imaging Bot MCP HV Monitor | ||||||
MZOBACONE | 313.50 | 315.11 | 311.83 | 315.32 | 313.82 | 314.07 | (260.2) 303.0 |
(250.2) 308.0 |
CONE | -Z SIDE OBA CONE | |
OBAAVG | 306.15 | 304.32 | 306.57 | 305.03 | (282.5) 300.0 |
(281.4) 301.0 |
K | OBA/TFTE TEMP | |||
OBADIAGRAD | 4.65 | 4.59 | 4.44 | 4.34 | 4.56 | 4.42 | 4.59 | (-1.11) 3.5 |
(-2.78) 3.9 |
K | OBA DIAM GRAD |
PZOBACONE | 309.70 | 310.95 | 308.45 | 311.40 | 309.42 | 312.40 | 309.94 | (260.2) 303.0 |
(250.2) 308.0 |
CONE | +Z SIDE OBA CONE |
TCYZ_RW6 | (276.07) | (288.15) 363.15 |
(278.15) 404.15 |
K | RWA -6 TEMP (RWA CRNR COMP) | ||||||
TFTERANGE | 48.10 | 49.78 | 48.89 | 49.19 | 48.78 | (16.7) 37.5 |
(11.1) 45.0 |
K | TFTE VENT/RAD TEMP |
Gyro Bias Drift | Gyro Bias Drift Histogram |
---|---|
OBSID | DETECTOR | GRATING | TARGET | ANALYSIS | ACA |
---|---|---|---|---|---|
30697 | ACIS-67 | NONE | NGC1300 | OK | OK |
30502 | ACIS-56789 | HETG | Vela X-1 | OK/NA | OK |
30081 | ACIS-0123 | NONE | NGC1977 point | OK | OK |
28561 | ACIS-67 | NONE | PSO J170.8326+20.2083 | OK | OK |
30503 | ACIS-56789 | HETG | Vela X-1 | OK/NA | OK |
30444 | HRC-I | NONE | HE 1353-1917 | OK | OK |
30687 | ACIS-67 | NONE | 2MASXJ06591070+2401400 | OK | OK |
30164 | ACIS-3678 | NONE | NGC4207 | OK | OK |
29841 | ACIS-0123 | NONE | PSR J1958+2846 | OK | OK |
29635 | ACIS-0123 | NONE | Perseus cluster E | OK | OK |
28078 | ACIS-67 | NONE | PS15bva KISS15s | OK | OK |
30695 | ACIS-67 | NONE | Gaia DR2 3428357798930628096 | OK | OK |
30698 | ACIS-67 | NONE | NGC1300 | OK | OK |
30699 | ACIS-0123 | NONE | PSR J1958+2846 | OK | OK |
30699 | ACIS-0123 | NONE | PSR J1958+2846 | OK | OK |
30486 | HRC-I | NONE | SN 2002ap | OK | OK |
30038 | ACIS-567 | NONE | ACT-CL J2151.9+1113 | OK | OK |
28631 | ACIS-0123 | NONE | Abell 370 | OK | OK |
30497 | ACIS-56789 | HETG | Vela X-1 | OK/NA | OK |
30690 | ACIS-0123 | NONE | UGC 03698 | OK | OK |
30700 | ACIS-0123 | NONE | PSR J1958+2846 | OK | OK |
30550 | HRC-S | LETG | NGC 5548 | OK/NA | OK |
30707 | ACIS-0123 | NONE | Orion Nebula Cluster | OK | OK |
30552 | HRC-S | LETG | NGC 5548 | OK/NA | OK |
29750 | ACIS-678 | NONE | 1eRASS J012710.5-285542 | OK | OK |
30708 | ACIS-0123 | NONE | Orion Nebula Cluster | OK | OK |
This week's focus is Gratings
Last reported on
Oct 17.
Only the most interesting or representative msids are shown below.
For a full listing choose the bulletted link.
MSID | Mean | RMS | Delta/Yr | Delta/Yr/Yr | Unit | Description | |
---|---|---|---|---|---|---|---|
4hposaro | -0.155 | 0.029 | 67.81 +/- 20.17 | 0.76 +/- 0.83 | na | NA | |
4hposbro | -0.151 | 0.029 | 68.39 +/- 20.39 | 0.77 +/- 0.84 | na | NA | |
4lposaro | 0.036 | 0.018 | 73.94 +/- 12.47 | 0.28 +/- 0.47 | na | NA | |
4lposbro | 0.038 | 0.019 | 72.99 +/- 12.82 | 0.36 +/- 0.48 | na | NA | |
4mp28av | 0.013 | 0.001 | 0.41 +/- 0.73 | -0.01 +/- 0.02 | V | MCE A: +28 VOLT MONITOR | |
4mp28bv | 0.079 | 0.005 | 2.02 +/- 3.22 | -0.03 +/- 0.12 | V | MCE B: +28 VOLT MONITOR | |
4mp5av | 0.019 | 0.001 | 0.49 +/- 0.78 | -0.01 +/- 0.03 | V | MCE A: +5 VOLT MONITOR | |
4mp5bv | 0.014 | 8.331e-04 | 0.37 +/- 0.59 | -0.01 +/- 0.02 | V | MCE B: +5 VOLT MONITOR |
If you have any questions, please contact: swolk@head.cfa.harvard.edu