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The magnetic field of sunspot AR1719 erupted on April 11th at 0716 UT,
producing an M6-class solar flare and the following alerts:
Thu, 11 Apr 2013 10:15:09 -0400 (EDT)
A Radiation violation of GOES 13 P5 (40-80 MeV) has occurred indicating a possible EPHIN P41GM value of 1/3 the threshold.
Value: 0.27 p/cm2-s-sr-MeV
Limit: 0.25
Fri, 12 Apr 2013 01:10:04 -0400 (EDT)
A Radiation violation of P3 (130keV) scaled from P6 (761keV) has been observed by ACE
Observed = 1.2007e+08
(limit = fluence of 1.2e8 particles/cm2-ster-MeV within 2 hours)
Although we have quoted CTI values of the cleanest data (FT <= -119.7 C, int time > 7000sec), the data fills these conditions are getting rare. We quote CTI temperature factor corrected ones. The values in the parentheses are CTI based on the cleanest data.
Average of ACIS-I CCDs (MnKa) slope: | 2.515e-9 CTI/day | (1.636e-9 CTI/day) |
---|---|---|
Detrended slope: | 7.148e-9 CTI/day | (6.837e-9 CTI/day) |
We display all bad pixels 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 a computational artificial effect due to boundaries.
CCD0 | CCD1 | CCD2 | CCD3 | CCD4 | CCD5 | CCD6 | CCD7 | CCD8 | CCD9 | |
---|---|---|---|---|---|---|---|---|---|---|
Previously Unknown Bad Pixels | ||||||||||
Current Warm Pixels | (233,315) (233,321) (233,322) (233,323) (233,324) (233,325) (233,327) (233,326) (258,797) (263,317) (280,313) (352,544) (369,376) (669,577) (792,313) | (881,53) | ||||||||
Flickering Warm Pixels | (153,205) (692,141) (117,749) (667,782) | (427,125) (802,665) (910,239) | (526,66) (764,98) | (703,739) (847,364) | (247,364) | (233,329) (282,385) (367,511) (641,669) (745,313) (1023,166) (233,328) (109,1) | (884,31) (843,420) (1000,214) | (335,412) | (139,109) (587,544) (1024,454) (1024,455) (1024,456) (1024,457) (1024,458) (197,241) (356,902) (833,325) (182,474) (1024,453) (913,165) | (636,819) |
Current Hot Pixels | ||||||||||
Flickering Hot Pixels | ||||||||||
Warm column candidates | ||||||||||
Flickering Warm Column Candidates | 509 518 | 509 514 1021 | 509 518 | 509 | 518 509 514 1021 | 509 514 1021 | 509 |
For this period, 5 peaks are observed.
Day (DOY) | Temp (C) | Width (Days) | |
---|---|---|---|
96.05 | -118.27 | 0.25 | |
96.56 | -105.85 | 0.95 | |
99.02 | -117.61 | 0.34 | |
99.30 | -115.60 | 0.23 | |
100.29 | -116.44 | 1.06 |
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.
5 TSC moves this period
weekly average time/step | 0.00144 s |
---|---|
mission average time/step | 0.00133 s |
New violations or new extrema are shown in blue cells.
MSID | 04/05/13 | 04/06/13 | 04/07/13 | 04/08/13 | 04/09/13 | 04/10/13 | 04/11/13 | yellow limits (lower) upper | red limits (lower) upper | Units | Description |
1DPAMZT | 304.33 | (4.00) 30.00 | (-37.50) 40.50 |
C | DPA -Z PANEL TEMP | ||||||
5EPHINT | 331.46 | 334.66 | 333.02 | 335.75 | (272.0) 313.7 | (270.0) 322.0 |
K | EPHIN TEMP | |||
HKEBOXTEMP | 339.18 | 338.12 | 341.39 | (268.0) 320.0 | (253.0) 348.0 |
K | EPHIN HOUSEKEEPING EBOX: TEMPERATURE (5EHSE300) | ||||
HKABIASLEAKI | 1.00 | 1.00 | 1.00 | 1.00 | 1.00 | 1.00 | 1.00 | (-100.0) 1.0 | (-200.0) 1.01 |
uA | EPHIN HOUSEKEEPING A-BIAS: LEAKAGE CURRENT (5EHSE400) |
HKBBIASLEAKI | 1.00 | 1.00 | (-100.0) 1.0 | (-200.0) 1.01 |
uA | EPHIN HOUSEKEEPING B-BIAS: LEAKAGE CURRENT (5EHSE500) | |||||
HKCBIASLEAKI | 45.20 | 45.20 | 45.20 | 45.20 | 45.20 | 45.20 | (-100.0) 45.2 | (-200.0) 45.21 |
uA | EPHIN HOUSEKEEPING C-BIAS: LEAKAGE CURRENT (5EHSE600) | |
HKDBIASLEAKI | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | (-100.0) 45.1 | (-200.0) 45.11 |
uA | EPHIN HOUSEKEEPING D-BIAS: LEAKAGE CURRENT (5EHSE700) |
HKEBIASLEAKI | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | 45.10 | (-100.0) 45.1 | (-200.0) 45.11 |
uA | EPHIN HOUSEKEEPING E-BIAS: LEAKAGE CURRENT (5EHSE800) |
TEIO | 348.12 | 348.12 | 349.70 | (253.0) 333.15 | (250.2) 358.15 |
K | EPHIN ELECTRONICS HOUSING TEMP | ||||
TEPHIN | 332.41 | 335.56 | 333.98 | 337.13 | (272.8) 313.7 | (270.0) 322.0 |
K | EPHIN SENSOR HOUSING TEMP | |||
OHRTHR43 | 294.20 | 294.20 | 294.11 | 294.12 | 294.28 | (292.4) 294.1 | (280.2) 308.0 |
K | RT 134: PERISCOPE | ||
3TSMXCET | 265.81 | 263.31 | 263.31 | 270.79 | (153.0) 263.0 | (148.0) 353.0 |
K | -X TURTLE SHELL NR HRC CEA | |||
3TSMXSPT | 298.23 | 303.22 | 295.74 | 303.22 | 303.22 | 300.72 | 305.71 | (203.0) 283.0 | (148.0) 353.0 |
K | -X TURTLE SHELL NR ACIS SS |
TB1T1 | (270.09) | (270.09) | (270.09) | (270.09) | (270.2) 298.0 | (268.0) 300.8 |
p008 | BATT 1 TEMP 1 K |
OBSID | DETECTOR | GRATING | TARGET | ANALYSIS | ACA |
---|---|---|---|---|---|
15220 | ACIS-0123 | NONE | COSMOS Legacy | OK | OK |
15222 | ACIS-0123 | NONE | COSMOS Legacy | OK | OK |
15225 | ACIS-0123 | NONE | COSMOS Legacy | OK | OK |
15085 | ACIS-012367 | NONE | Antlia Cluster E5 | OK | OK |
15294 | ACIS-01236 | NONE | Centaurus A | OK | OK |
14941 | ACIS-0123 | NONE | Sgr A* | OK | OK |
14900 | ACIS-23567 | NONE | ESO318-021 | OK | OK |
14641 | ACIS-7 | NONE | 2S 1553-542 | OK | OK |
14576 | ACIS-235678 | NONE | IC 5148 | OK | OK |
15092 | ACIS-23678 | NONE | 3C 444 | OK | OK |
14799 | ACIS-235678 | NONE | SN 2013ai | OK | OK |
15201 | ACIS-01236 | NONE | Cen A Northern Lobe 1 | OK | OK |
15489 | ACIS-01236 | NONE | A1795 | CAL | OK |
15202 | ACIS-01236 | NONE | Cen A Northern Lobe 2 | OK | OK |
15175 | ACIS-01236 | NONE | RXCJ1514.9-1523 | OK | OK |
15488 | ACIS-01236 | NONE | A1795 | CAL | OK |
15221 | ACIS-0123 | NONE | COSMOS Legacy | OK | OK |
15344 | ACIS-678 | NONE | SDSS J1310+5601 | OK | OK |
15624 | ACIS-7 | NONE | 2MASS J19094043+4930050 | OK | OK |
This week's focus is Ground Computed Gradients.
Last reported on
Jan 17.
Only the most interesting or representative msids are shown below.
For a full listing choose the bulletted link.
Min/max envelopes in dark blue appear on the trending plots. The envelopes are 4th degree fits to the monthly minimum and maximum values for each MSID. The final polynomial form and binning are still being experimented with. We will soon add to the trending pages a report of the fits and predictions they give on future limit violations. The light blue curve is our original smoothing of all the data over 30 day moving boxcars. The green/yellow line is a linear fit to all the data; the break occurs at a limit change.
Gradients HRMA FAP | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
HFAPGRD1 | -0.01 | 4.155e-02 | -3.507e-04 | 8.404e-05 | K | RT1-RT2: HRMA Forward Aperture Plate |
HFAPGRD2 | 0.04 | 1.056e-02 | -8.666e-04 | -1.417e-04 | K | RT1-RT4: HRMA Forward Aperture Plate |
HFAPGRD3 | 0.04 | 1.453e-02 | -2.308e-03 | 3.305e-04 | K | RT2-RT3: HRMA Forward Aperture Plate |
HFAPGRD4 | 0.07 | 5.044e-03 | -1.010e-03 | -8.025e-05 | K | RT2-RT5: HRMA Forward Aperture Plate |
HFAPGRD5 | -0.02 | 1.356e-02 | 1.729e-03 | 7.509e-05 | K | RT3-RT1: HRMA Forward Aperture Plate |
HFAPGRD6 | 0.02 | 2.781e-03 | 3.826e-05 | 6.596e-05 | K | RT3-RT6: HRMA Forward Aperture Plate |
HFAPGRD7 | 0.02 | 3.779e-03 | 6.474e-05 | -3.232e-05 | K | RT4-RT5: HRMA Forward Aperture Plate |
HFAPGRD8 | -0.02 | 7.789e-04 | -8.849e-05 | -4.282e-06 | K | RT5-RT6: HRMA Forward Aperture Plate |
HFAPGRD9 | 1.714e-03 | 3.598e-03 | -1.847e-04 | 9.490e-05 | K | RT6-RT4: HRMA Forward Aperture Plate |
Gradients HRMA Struts | ||||||
MSID | MEAN | RMS | DELTA/YR | DELTA/YR/YR | UNITS | DESCRIPTION |
HSTRTGRD1 | -2.96 | 0.18 | -8.083e-02 | 3.120e-03 | K | RT25-RT26: HRMA STRUTS |
HSTRTGRD2 | -2.13 | 0.38 | -1.284e-01 | 4.316e-03 | K | RT26-RT27: HRMA STRUTS |
HSTRTGRD3 | -0.29 | 7.779e-02 | 9.295e-03 | 8.397e-04 | K | RT27-RT28: HRMA STRUTS |
HSTRTGRD4 | 1.85 | 0.46 | 1.442e-01 | 8.478e-03 | K | RT28-RT29: HRMA STRUTS |
HSTRTGRD5 | 3.11 | 0.18 | 6.952e-02 | -4.084e-03 | K | RT29-RT30: HRMA STRUTS |
HSTRTGRD6 | 0.80 | 0.28 | -3.804e-02 | 1.836e-03 | K | RT30-RT25: HRMA STRUTS |
If you have any questions, please contact: swolk@head.cfa.harvard.edu