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#44926
Tue 26 May 2009 12:39:PM
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Joined: Feb 2001
Posts: 381,903
Launch Director
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OP
Launch Director
Joined: Feb 2001
Posts: 381,903 |
HUBBLE SPACE TELESCOPE - Continuing to collect World Class Science
DAILY REPORT #4852
PERIOD COVERED: 5am May 22 - 5am May 26, 2009 (DOY 142/0900z-146/0900z)
OBSERVATIONS SCHEDULED
S/C/FGS 11457
Verify Guide Star Acquisition with Continuing FGSs
After the shuttle deploys HST at the end of SM4 and at the beginning of
SMOV4, it will be necessary to test and demonstrate HST's ability to
acquire guide stars with the FGSs. This is a major pre-requisite for all
observations by HST's SIs when precision pointing under guide star
control is needed. This proposal will test the ability of each of the
unreplaced FGSs to acquire a primary guide star while another FGS
acquires a secondary guide star. After acquiring the guide star pair,
HST will track these stars in finelock for approximately 10 minutes.
When possible, use guide stars that have been successfully acquired and
tracked in the past.
S/C/ACS 11365
Load and Dump Onboard Memory
This proposal is a test and verification of the ACS dump of memory
capability. Areas of Control Section (CS) to dump include: EDAC RAM,
EEPROM, and CS PROM (with the CS in Operate). Areas of MIE memory to
dump include: MIE RAM and MIE PROM (with the MIE in Operate). Note that
the MIE memory must first be copied to CS buffer RAM as images, which
are then dumped.
S/C 11364
Vehicle Disturbance Test
The purpose of the VDT is to measure and characterize uncompensated
environmental disturbances acting upon the HST during normal operation.
The VDT is a passive test (not a forced-response test) used to obtain
signatures for both externally induced (e.g. SCM, SA-3, SSM thermal
gradients) and internally induced (e.g. HGA, RWA, COS and WFC3
mechanisms) disturbances affecting HST LOS pointing. The disturbances
observed will be used as the nominal on-orbit disturbances in pointing
control simulations until the next VDT is run.
The test occurs after release, and most of the VDT can be run during the
BEA period. The -V1 sunpoint portion of the VDT usually occurs after the
BEA period is complete. The VDT shall consist of two separate tests that
need not occur consecutively. The overall duration of the VDT is at
least 13 orbits of spacecraft time including (1) at least 8 orbits at
+V3 sunpoint after achieving thermal equilibrium (at least 36-hours at
+V3 sunpoint) and three out of 8-orbits have RWA Friction Compensation
turned Off, and (2) at least 5 orbits at -V1 sunpoint (all or part of
this segment have RWA Friction Compensation turned Off). At the
beginning of each test, the attitude control law gains are switched to
maneuver gains, and the gyros are commanded to low mode. The nominal
attitude control law configuration will be restored at the end of each
test.
Each test is initiated via SMS execution of stored program macros in the
HST flight computer to switch the attitude control law gains to
low-bandwidth maneuver gains, command the gyros into low mode, terminate
Velocity aberration and parallax (VAP) processing, and manage the status
of on-board RWA Friction Compensation. The nominal attitude control law
configuration will be restored at the end of each test via SMS execution
of stored program macros. The stored program command macros are
developed specifically for the VDT by the Flight Software and Pointing
Control System groups.
S/C/COS 11353
COS Dump Test and Verification of COS Memory Loads
This proposal is a test and verification of the COS dump of memory
capability. Areas of Control Section (CS) to dump include: EXEC RAM,
EEPROM, and CS PROM (with the CS in Operate). Areas of DIB memory to
dump include: DIB RAM and DIB PROM (with the DIB in Operate). Areas of
DCE memory to dump include: the DCE code image. Note that the DIB and
DCE memory must first be copied to CS buffer RAM as images, which are
then dumped. Supports Activity COS-02
FLIGHT OPERATIONS SUMMARY:
Significant Spacecraft Anomalies: (The following are preliminary reports
of potential non-nominal performance that will be investigated.)
HSTARS:
11845 - During FGS-2 ITS test at 142/11:48 - Trans mode failed with no
S-curve detected in y-axis. FGS-2 did achieve Fine Lock and LOS scan was
also successful.
11847 - WFC3 safed on IMEB1ST @ 145/13:02z
COMPLETED OPS REQUEST:
18436-2 - Open COS FUV DVA door @ 142/15:26z
18441-0 - VDT Macro Installation - IP-170 @ 143:10:50z
18442-0 - Execute Vehicle Disturbance Test - IP-170 Section B and C @ 144/01:34z
18451 0 - Recover WFC3 to Boot @ 145/13:50z
18444-1 - Reset WFC3 setpoints after recovery @ 145/14:04z
18452-4 - Recover WFC3 from Boot to Operate @ 145/16:16z
18448-0 - ACS CEB-R ASIC FSW Timing Pattern Update @ 146/16:22z
18446-1 - Clear ACS WFC TEC Event Flag 8 @ 145/17:22z
COMPLETED OPS NOTES: (None)
SCHEDULED SUCCESSFUL
FGS GSAcq 19 19
FGS REAcq 00 00
OBAD with Maneuver 22 22
SIGNIFICANT EVENTS:
Flash Reports:
-COS successfully transition to operate at ~ 142/10:32. The FUV DCE
successfully transition to operate at 142/10:52. No limit violation
observed and the instrument is performing nominally.
COS internal pressure is currently at 3.5x10-6 torr, we are on schedule
for opening the FUV DVA door at 11:00am EST Friday morning.
-The COS and ACS memory that was collected was dumped from the SSR
at 142/13:40z, these dumps were analyzed and report to be as expected.
-The COS FUV door was successfully opened at 142/15:22. All power and position
telemetry was as expected. A small increase in pressure was measured by the COS internal
and ESM ion gauges.
-VDT data collection successful. The Vehicle Disturbance Test at the +V3
sunpoint attitude was successfully completed at 2009/144/01:34 with the
nominal gains restored to the vehicle control law. An LBBIAS was
uplinked to the vehicle to ensure minimal bias errors at the following
Guide Star Acquisition. That subsequent acquisition at 144/03:45
succeeded.
-At 145/1100 WFC3 recovery from Protect Safe mode began via
stored commanding. At 145/1302 during the transition to Protect Operate,
the instrument safed as a result of a limit check violation of an
SES-collected thermistor on the unpowered MEB.
-WFC3 was recovered to Protect Operate. At 145/1631 WFC3 successfully
intercepted the SMS timeline to dump EEPROM, Exec RAM, and PROM memory.
SSR playback is currently in progress and the memory dumps will be analyzed
by the Payload FSW team.
-WFC3 EEPROM, Exec RAM, and PROM memory dumps were collected via SMS
starting at 145/1631. The SSR playback of these dumps began at 145/1651.
The Payload FSW team has verified the contents of the memory dumps are
as expected.
WFC3 remains in Protect Operate.
-The FSW team completed the COS analysis of the
zero-filled pattern loaded to and dumped from CS Buffer memory at 145/1700.
In summary, no bit flips in CS Buffer memory were observed.
David Cottle
UBB Owner & Administrator
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