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| subject: | 4\17 Pt 2 HST Daily Rpt No 3343 |
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17 April 2003
HUBBLE SPACE TELESCOPE
DAILY REPORT #3343
PERIOD COVERED: DOY 106
Part 2 of 2
WFPC2 9594
WFPC2 CYCLE 11 SUPPLEMENTAL DARKS pt2/3
This dark calibration program obtains 3 dark frames every day to
provide data for monitoring and characterizing the evolution of hot
pixels
STIS 9606
CCD Dark Monitor-Part 2
Monitor the darks for the STIS CCD.
STIS 9608
CCD Bias Monitor - Part 2
Monitor the bias in the 1x1, 1x2, 2x1, and 2x2 bin settings at
gain=1, and 1x1 at gain = 4, to build up high-S/N superbiases and
track the evolution of hot columns.
STIS 9614
STIS CCD Imaging Flats C11
Investigate flat-field stability over a monthly period.
STIS 9615
Cycle 11 MAMA Dark Monitor
This test performs the routine monitoring of the MAMA detector dark
noise. This proposal will provide the primary means of checking on
health of the MAMA detectors systems through frequent monitoring of
the background count rate. The purpose is to look for evidence of
change in dark indicative of detector problem developing.
STIS/CAL 9628
MAMA Sensitivity and Focus Monitor Cycle 11
Monitor sensitivity of each MAMA grating mode to detect any change
due to contamination or other causes. Also monitor the STIS focus in
a spectroscopic and imaging mode.
ACS 9649
ACS internal CTE monitor
The charge transfer efficiency {CTE} of the ACS CCD detectors will
decline as damage due to on-orbit radiation exposure accumulates.
This degradation will be closely monitored at regular intervals,
because it is likely to determine the useful lifetime of the CCDs.
All the data for this program is acquired using internal targets
{lamps} only, so all of the exposures should be taken during Earth
occultation time {but not during SAA passages}. This program
emulates the ACS pre-flight ground calibration and post-launch SMOV
testing {program 8948}, so that results from each epoch can be
directly compared. Extended Pixel Edge Response {EPER} and First
Pixel Response {FPR} data will be obtained over a range of signal
levels for both the Wide Field Channel {WFC}, and the High Resolution
Channel {HRC}.
ACS 9658
ACS Earth Flats
This program will obtain sequences of flat field images by observing
the bright Earth. Several UV filters from the interim calibration
program {9564} require additional exposures to obtain the required
illumination. A few UV filters from this program will be repeated to
monitor for changes in the flat fields and to verify the interim
results. Since no streaks are observed in the UV, the wavelength
coverage is extended to longer wavelengths in order to explore the
severity of streaks in the flats from clouds in the FOV. We have
added exposures for the HRC in the visible filters to verify the
results derived from the L-flat campaign and to explore the severity
of streaks. We have also added exposures on WFC using the minimum
exposure time and using filters which will not saturate the brightest
WFC pixel by more than 10 times the full well.
ACS 9673
CCD Daily Monitor
This program consists of basic tests to monitor, the read noise, the
development of hot pixels and test for any source of noise in ACS CCD
detectors. This programme will be executed once a day for the entire
lifetime of ACS
STIS 9706
STIS Pure Parallel Imaging Program: Cycle 10
This is the default archival pure parallel program for STIS during
cycle 10.
WFPC2 9709
POMS Test Proposal: WFII parallel archive proposal
This is the generic target version of the WFPC2 Archival Pure
Parallel program. The program will be used to take paralell images of
random areas of the sky, following the recommendations of the 2002
Parallels Working Group.
WFPC2 9710
POMS Test Proposal: WFII backup parallel archive proposal
FLIGHT OPERATIONS SUMMARY:
Significant Spacecraft Anomalies:
(The following are preliminary reports of potential non-nominal
performance that will be investigated.)
HSTARs:
8991 - Failure of Track to schedule for TDRS-J Test {at} 099/1306z
COMPLETED OPS REQs:
None
OPS NOTES EXECUTED:
1098-0 - Document limits for FSW Main Bus C Voltage Monitor {at}
106/1852z
SCHEDULED SUCCESSFUL FAILURE TIMES
FGS GSacq 4 4
FGS REacq 12 12
FHST Update 7 7
LOSS of LOCK
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