Документ взят из кэша поисковой машины. Адрес оригинального документа : http://www.stsci.edu/sms-deliv/2005320-161806-smssa32.text Дата изменения: Wed Nov 16 19:18:06 2005 Дата индексирования: Fri Feb 28 17:02:58 2014 Кодировка: Поисковые слова: guide 8.0

To : Distribution
From : Science Planning and Scheduling Team, STScI
Date : 16-Nov-2005 16:10:57 UT
SMS Supervisor : William Hathaway 410-338-5050 hathaway@stsci.edu

Subject : SMS SA325P00: distribution of final products


The Mission Scheduler and Command Loader processing for the final run
of SMS SA325P00 has been completed. The products have been reviewed
and approved for release and may be found at address SSSP1.HST.NASA.GOV,
while comments on the PASS errors are included below. This distribution
includes MEGG and MOSR products in addition to MS/CL products.

SMS Name : SA325P00
MS Run Name : SA325P00_F
CL Run Names : SA325P00_F1

Calendar Name : 053257G1
SMS Start Time : 2005.325:00:00:00
SMS End Time : 2005.331:21:30:00


The Operational Period Catalog and SPCs have been generated from the Command
Loads. The OPCat is:

/data/scheduling/spss_flight_data/pass/cl/sa325p00_f1/opc/op3182101.cat

CCS:
===
Product Notification Message, pnm_2005320161055.txt, fully enumerating
these products has been successfully transmitted via File Transport
Protocol (FTP) to the Control Center System (CCS) A,D,F,H strings.


PASS error analysis
===================

There are three of the usual benign 69 /3 type messages.

There is one occurance of the level-3 message:
471/ 3 MSGCEMIN 2005Y325D19H05M46.1538457 COENG
TOTAL REAL-TIME ENGINEERING DOWNLINK FOR THE TIME PERIOD 325 17:30:17 TO
325 19:05:46 IS 24 MIN. THIS IS LESS THAN THE DESIRED MINIMUM OF 30 MIN.

We have obtained additional or extended MAR contacts during this time
period, but due to a combination of antenna view restrictions, Full
Communication Outages now seen under 2-gyro control, limits on minimum
duration of usable contacts, and time reserved for NCC testing, we have
been unable to add enough to resolve the errors.
Such situations now occur nearly every week and are usually not
considered to be serious.


HST FINAL MODE LOAD APPROVAL FORM
=================================


SUBSYSTEM SIGN-OFF (ENTER NAME) DOY/TIME
--------- --------------------------- --------

DMS FC/SE
--------------------------- --------
EPS FC/SE
--------------------------- --------
I&C FC/SE
--------------------------- --------
OTA FC/SE
--------------------------- --------
PCS FC/SE
--------------------------- --------
SI FC/SE
--------------------------- --------
STSCI/SPST William Hathaway 320/16:10
--------------------------- --------

=======================================================================
FINAL AUTHORIZATION:


-------------------------------------------- -------------
MOSES FO MANAGER/MOSES SS APPROVAL TO UPLINK DOY/GMT

=======================================================================


Delivery Notes:
===============

This SMS has a non-standard end time of 331:21:30, to better
accomodate the scheduling of the calibration proposal 10771
(details of which are in the "Commanding Notes" section below.)


This SMS includes the monthly ACS calibration proposal 10733 CCD
Hot Pixel Annealing. The annealing period is centered around
the time 329:08:37:56. Normally, this Anneal occurs every four
weeks, which would have placed it on the following week's SMS,
but in this case it was deemed desirable to perform it prior to
the calibration proposal 10771. The regular scheduling of this
Anneal will resume on the 05360 SMS.


The Bay 5 thermal predictor model has found heat input predictions
exceeding the 4300 kJ threshhold

There are no excursions over the threshhold for uniform
transmitter usage.

Predicted excursions with actual transmitter operation

Start End Duration Peak (kJ) Peak Time
2005.325:11:05:00 - 2005.325:11:50:00 0:00:45:00 4324.3 2005.325:11:15:00
2005.325:12:15:00 - 2005.325:13:15:00 0:01:00:00 4350.9 2005.325:12:25:00
2005.328:23:05:00 - 2005.329:00:35:00 0:01:30:00 4357.6 2005.329:00:20:00
2005.329:01:25:00 - 2005.329:02:15:00 0:00:50:00 4321.5 2005.329:01:35:00


In the following description of the execution of the calibration
proposal 10771, real-time commanding must have forward uplink
opportunities of at least 7min on each of two different TDRS
in each of the following windows:
330:21:41:00 to 23:04:00
331:08:32:00 to 10:24:00

According to our reading of the scheduled contacts, these times
have been provided:

East - Forward 330:21:29:01 - 330:22:05:22
West - Forward 330:22:19:01 - 330:22:53:03
East - Forward 330:22:55:03 - 330:23:17:59

then:

West - Forward 331:08:35:15 - 331:09:26:15
East - Forward 331:09:28:31 - 331:09:58:31
West - Forward 331:10:18:45 - 331:10:52:47

We believe this more than satisfies the needs. FOT is invited
to double check that these contacts exist and are appropriate.


In the SMS 053257g1, there is one case of a large (~70")
integrated T3 slew within an orbit preceeding a guide star
reacquisition. The start and end times of this reacquisition are:

331:15:23:04 331 331:15:31:13

This activity occurs during one of the executions of special test
calibration proposal 10771.



The Commanding Team has completed its review of
Flight SMS 053257G1 and has found no problems.
Our formal input for this delivery follows:

****************************************
Commanding Notes for Flight SMS 053257G1
****************************************

This SMS contains special commanding for calibration proposal 10771
which modifies the TEC temperature setpoints of the ACS WFC and HRC CCDs.
During the execution of the proposal, each CCD for a period of time
reaches both a warmer and cooler temperature plateau.
During the time the CCDs are at these plateau temperatures, data is taken
to characterize the behavior of the CCDs at these non-nominal temperatures.

The test begins on day 330 at 20:00 UT. The HRC CCD is set to begin
warming and the WFC CCD is set to cooling below nominal temperatures.

Assuming the WFC cooldown is completed in the expected 99 minutes,
then real-time commanding must SET the ACS event Flag8 to prevent
stored commanding from aborting the test and returning the WFC to
its nominal setpoint. Therefore, real-time commanding must set Flag8
prior to day 330 23:05 UT for the test to proceed.
There is no corresponding concern or action required for the
warming of the HRC CCD.

For the next part of the test, the HRC CCD is cooled and the WFC CCD
is warmed. Thus, assuming the HRC cooldown is completed in the expected
time of 32 minutes, then real-time commanding must SET the ACS event Flag9
to prevent stored commanding from aborting the test and returning the
HRC to its nominal setpoint. Therefore, real-time commanding must set
Flag9 prior to day 331 at 10:24 UT for the test to proceed.
Again there is no corresponding concern or action required for the
warming of the WFC CCD.

After the completion of the tests on day 331 at 20:19 UT, both CCDs
are returned to their nominal setpoint temperatures and both event
Flags 8 and 9 are cleared.

In summary, assuming the specified plateau temperatures are reached
in the specified times (both will be in the OPS request), event
Flags 8 and 9 will need to be set for the tests to proceed to completion.


Ron Pitts FSE/STScI x -4932

Ancillary information and reports:
==================================


The following proposals are scheduled on this SMS:
08791 NICMOS Post-SAA calibration - CR Persistence - PART 2
10092 The COSMOS 2-Degree ACS Survey
10135 Unveiling the Progenitors and Physics of Cosmic Explosions
10143 Ultracool companions to the nearest L dwarfs
10173 Infrared Snapshots of 3CR Radio Galaxies
10396 Star Clusters, Stellar Populations, and the Evolution of the Small Mag
ellanic Cloud
10410 Anisotropy and obscuration in the near-nuclear regions of powerful rad
io galaxies
10435 Merger-Induced Populations in Early-Type Galaxy Cores
10481 HST Observations of Astrophysically Important Visual Binaries
10496 Decelerating and Dustfree: Efficient Dark Energy Studies with Supernov
ae and Clusters
10497 Cepheid Calibrations of the Luminosity of Two Reliable Type Ia Superno
vae and a Re-determination of the Hubble Constant
10505 The Onset of Star Formation in the Universe: Constraints from Nearby
Isolated Dwarf Galaxies.
10514 Kuiper Belt Binaries: Probes of Early Solar System Evolution
10523 The Halo Shape and Metallicity of Massive Spiral Galaxies
10524 Blue Stragglers: a key stellar population to probe internal cluster dy
namics
10525 Characterizing the Near-UV Environment of M Dwarfs: Implications for E
xtrasolar Planetary Searches and Astrobiology
10526 Dynamics of the Polarization Structure of the Crab Nebula
10527 Imaging Scattered Light from Debris Disks Discovered by the Spitzer Sp
ace Telescope Around 20 Sun-like Stars
10539 Coronagraphic Imaging of Bright New Spitzer Debris Disks
10540 Imaging Nearby Dusty Disks
10541 Probing the jet mattter content of quasar PKS 0637-752
10548 Near-UV Snapshot Survey of Low Luminosity AGNs
10549 SAINTS - Supernova 1987A INTensive Survey
10556 Neutral Gas at Redshift z=0.5
10576 An ACS Imaging Survey of the Galaxies Hosting Strong Mg II Absorption
10587 Measuring the Mass Dependence of Early-Type Galaxy Structure
10606 Ultraviolet Snapshots of 3CR Radio Galaxies
10610 Astrometric Masses of Extrasolar Planets and Brown Dwarfs
10613 Calibrating the Mass-Luminosity Relation at the End of the Main Sequen
ce
10626 A Snapshot Survey of Brightest Cluster Galaxies and Strong Lensing to
z = 0.9
10629 Are Field OB Stars Alone?
10702 The COSMOS 2-Degree ACS Survey NICMOS Parallels
10727 Low frequency flatfield test for NICMOS Camera 1
10729 ACS CCDs daily monitor
10733 CCD Hot Pixel Annealing
10737 CCD Stability Monitor
10738 Earth Flats
10745 WFPC2 CYCLE 14 INTERNAL MONITOR
10748 WFPC2 CYCLE 14 Standard Darks
10771 CTE and QE measurement for ACS CCDs at three different temperatures
10772 WF4 Anomaly Characterization
NICSA NICMOS DETECTOR POWER MANAGEMENT AROUND THE SAA
POINT SPSS GENERIC POINTING PROPOSAL
TABLE MISCELLEANEOUS SI TABLE LOADS (SPSS)



The following times of eng. formats have been scheduled in the SMS.

Format Start Time End Time
HN Start of SMS 2005.327:15:22:00
FN 2005.327:15:22:00 2005.327:16:06:16
HN 2005.327:16:06:16 2005.330:02:55:39
FN 2005.330:02:55:39 2005.330:03:39:38
HN 2005.330:03:39:38 Beyond End of SMS



SOLAR ARRAY OPTIMIZATION SUMMARY REPORT
2005.318 20:11:16 VERSION= 3.3


Command: smsg -eps 053257g1 -offset

CALENDAR START= 2005.325:00:00:00 CALENDAR END= 2005.331:21:30:00

CALENDAR ID= 053257G1

NUMBER OF SA SLEWS= 20

SA COMMAND TIME +V1/SA-NORMAL SA_SLEW_DUR SA_SLEW_ANG
yyyy.ddd:hh:mm:ss (DEG) (SEC) (DEG)
----------------- ------ ----- ------
2005.325:00:29:00 62.35 539 68.36
2005.325:06:58:41 82.98 296 20.64
2005.327:06:52:31 115.95 374 32.97
2005.327:11:45:13 76.75 408 39.20
2005.327:14:28:50 147.66 549 70.91
2005.327:16:27:33 77.44 547 70.22
2005.328:07:47:25 170.96 631 93.52
2005.328:09:57:46 91.14 583 79.82
2005.328:14:50:05 117.19 333 26.05
2005.328:17:35:24 167.11 461 49.92
2005.328:19:34:32 80.27 608 86.83
2005.329:06:04:35 160.07 583 79.79
2005.329:13:05:44 92.26 537 67.81
2005.329:14:39:50 128.75 394 36.49
2005.329:16:12:39 140.90 227 12.15
2005.330:02:00:47 61.12 583 79.78
2005.330:04:01:35 83.16 306 22.04
2005.330:08:08:49 128.14 438 44.99
2005.330:11:39:45 62.57 528 65.58
2005.330:17:51:14 78.94 264 16.37





LEGEND:
Col 1 (SA COMMAND TIME) The time of the SASLWLIM EPS SMS statement.

Col 2 (+V1/SA-NORMAL) The angle between the V1 axis and the SA normal
vector, measured clockwise from V1 in the same
direction as the Sun, in degrees.
This is the EPS SMS SA angle following the SA slew.

Col 3 (SA_SLEW_DUR) The solar array slew duration, in seconds.

Col 4 (SA_SLEW_ANG) The solar array slew angle, in degrees:




Slew summary of Calendar 053257G1

Start Stop V1-SUN Beta Bay 5
ddd:hh:mm:ss ddd:hh:mm:ss RA DEC PA OR Angle Angle Incid

325:00:29:00 325:03:47:15 188 21 128 0 62 8.6 81
325:03:47:15 325:06:58:41 188 21 128 0 62 8.5 81
325:06:58:41 325:08:25:17 141 8 109 0 98 8.5 80
325:08:25:17 325:17:58:55 200 43 144 0 71 8.4 80
325:17:58:55 325:23:01:37 20 -73 215 0 84 8.3 80
325:23:01:37 326:03:52:56 84 -69 155 0 89 8.1 80
326:03:52:56 326:08:18:49 77 -69 162 0 90 8.0 80
326:08:18:49 326:14:48:48 148 34 97 -10 101 7.8 70
326:14:48:48 326:20:18:59 17 -72 218 -1 83 7.6 79
326:20:18:59 326:21:16:01 15 -72 221 0 83 7.5 80
326:21:16:01 326:23:00:40 214 36 153 0 61 7.4 81
326:23:00:40 327:00:24:18 184 38 132 3 77 7.3 83
327:00:24:18 327:05:21:12 99 -75 139 -3 81 7.2 77
327:05:21:12 327:06:52:31 165 -4 110 0 73 7.0 80
327:06:52:31 327:08:21:50 112 -2 116 0 124 6.9 81
327:08:21:50 327:11:45:13 132 45 92 -2 116 6.8 79
327:11:45:13 327:14:28:50 202 49 146 2 77 6.7 82
327:14:28:50 327:16:27:33 87 1 115 -12 147 6.5 78
327:16:27:33 327:21:08:13 15 -73 221 0 82 6.3 80
327:21:08:13 327:22:53:06 144 -12 100 -11 91 6.1 69
327:22:53:06 328:00:30:59 144 -12 125 14 91 6.0 93
328:00:30:59 328:02:06:25 146 -24 110 0 85 5.9 80
328:02:06:25 328:04:05:50 241 43 177 -4 64 5.8 77
328:04:05:50 328:05:15:08 202 29 139 -1 61 5.7 80
328:05:15:08 328:07:47:25 6 -72 230 0 81 5.6 80
328:07:47:25 328:09:57:46 70 20 93 0 171 5.4 88
328:09:57:46 328:14:50:05 150 3 100 -11 91 5.2 69
328:14:50:05 328:17:35:24 79 -40 153 -8 117 4.9 74
328:17:35:24 328:19:34:32 74 23 83 0 167 4.7 87
328:19:34:32 329:00:42:20 6 -72 233 3 80 4.5 83
329:00:42:20 329:02:13:13 16 -71 222 0 83 4.2 80
329:02:13:13 329:06:04:35 205 70 146 0 94 4.0 80
329:06:04:35 329:08:16:00 60 10 187 0 170 3.8 88
329:08:16:00 329:10:59:52 92 48 54 0 143 3.5 84
329:10:59:52 329:13:05:44 59 12 194 0 171 3.3 88
329:13:05:44 329:14:39:50 140 -21 115 2 92 3.2 82
329:14:39:50 329:16:12:39 112 5 113 0 129 3.0 82
329:16:12:39 329:22:44:45 84 22 91 0 159 2.7 86
329:22:44:45 330:02:00:47 84 -29 144 -10 126 2.2 73
330:02:00:47 330:04:01:35 187 8 119 -1 61 2.0 80
330:04:01:35 330:05:21:42 182 43 121 -5 85 1.8 75
330:05:21:42 330:06:57:24 229 61 168 0 83 1.7 80
330:06:57:24 330:08:08:49 181 59 125 0 94 1.5 80
330:08:08:49 330:11:39:45 115 5 132 19 127 1.3 97
330:11:39:45 330:17:51:14 188 11 121 0 63 0.8 81
330:17:51:14 330:19:45:54 25 -61 229 14 93 0.4 93
330:19:45:54 330:21:20:14 19 -67 220 0 86 0.2 80
330:21:20:14 330:22:57:09 25 -61 200 -15 93 0.1 65
330:22:57:09 331:00:39:40 6 -72 233 0 79 -0.1 80
331:00:39:40 331:02:14:45 6 -72 233 0 79 -0.3 80
331:02:14:45 331:03:37:43 6 -72 233 0 79 -0.5 80
331:03:37:43 331:10:15:32 189 62 135 4 94 -0.9 84
331:10:15:32 331:13:03:33 189 62 135 4 94 -1.4 84
331:13:03:33 331:16:39:00 6 -72 233 0 79 -1.8 80
331:16:39:00 331:18:14:04 6 -72 233 -1 79 -2.1 79
331:18:14:04 331:21:11:24 6 -72 233 0 79 -2.3 80
331:21:11:24 331:21:20:04 6 -72 234 0 79 -2.5 80





Note: The following gaps of more than 4 hours
between activities exist on this Calendar:

Separation Time Activity Next Activity Al after Gap
(ddd:hh:mm) (ddd:hh:mm) (ddd:hh:mm)





COMCON Block Summary
SMS FILE NAME: 053257G1
Calendar FILE NAME: 053257G1

Start Time End Time Duration Service T H Rate Prop Prg Ob Al Vn
------------ ------------ --------- ------- - - --- ------------------



Distance between target and 1-star acq guide star
SMS FILE NAME: /data/scheduling/spss_flight_data/pass/msin/sa325p00.sms

LABELS: START TIMES: DELTA PRI TAR RA/ TAR DEC/ TARGET
SLEW/ SI GSACQ/ TIME FGS GS RA GS DEC DIST
GSACQ NAME NEXT SLEW (SEC) (DEG) (DEG) (AMIN)
-------- ---- ----------------- ------- --- -------- -------- ------



WFPC2 AP17 Controlled Exposures in SA325P00

Start Time Duration(sec) End Time(approx) SCAP
--------------------------------------------------------------------
2005.328:11:01:16.721 400.0 2005.328:11:07:56.721 CNTROL
2005.328:12:26:16.722 400.0 2005.328:12:32:56.722 CNTROL
2005.328:12:38:16.722 400.0 2005.328:12:44:56.722 CNTROL
2005.328:14:02:16.722 400.0 2005.328:14:08:56.722 CNTROL
2005.329:01:16:16.722 700.0 2005.329:01:27:56.722 CNTROL
2005.329:01:30:16.722 700.0 2005.329:01:41:56.722 CNTROL
2005.329:01:45:16.722 400.0 2005.329:01:51:56.722 CNTROL
2005.329:01:54:16.722 400.0 2005.329:02:00:56.722 CNTROL
2005.330:09:11:16.724 200.0 2005.330:09:14:36.724 CLOCKSON
2005.330:09:21:16.724 200.0 2005.330:09:24:36.724 CLOCKSON
2005.330:10:41:16.724 200.0 2005.330:10:44:36.724 CLOCKSON
2005.330:10:51:16.724 200.0 2005.330:10:54:36.724 CLOCKSON
2005.330:11:01:16.724 160.0 2005.330:11:03:56.724 CLOCKSON