[IGSREPORT-0653] EMR Analysis Report (Week #726)
Geodetic
Geodetic
Tue Dec 14 13:20:36 PST 1993
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IGS Electronic Report Tue Dec 14 13:20:36 PST 1993 Message Number 0653
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Author: Geodetic Survey of Canada
Subject: EMR Analysis Report (Week #726)
Subject: EMR Analysis Report (week 726)
(Dec 05 - Dec 11,93)
Our analysis utilizes the JPL GIPSY/OASIS II (UNIX) software system
and data from all (up to 7) Canadian stations augmented by up to 12, globally
distributed, core stations (see Table 1 for the list of stations).
This effort is a part of a joint pilot project called
"Active Control System" and involves the Geodetic Survey Division (GSD),
SMRSS; the Geophysics Division and Pacific Geoscience Centre of the
Geological Survey of Canada, all three institutions are part of the
Department of Energy, Mines & Resources (EMR).
Table 1 : Station Summary (also indicated are day no. for which a
particular station is not included in the daily solution, either due to
being down or data being late).
STATION IGS code MISSING DAY NO. 1993
Albert Head, CAN ALBH
Algonquin, CAN ALGO*
Fairbanks FAIR*
Goldstone GOLD*
Hartebeesthoek HART*
Holberg,CAN HOLB
Kokee Park KOKB
Madrid MADR*
McMurdo MCMU 343 to 345
Pamatai PAMA 344, 345
Penticton, CAN DRAO
Santiago SANT*
St. Johns, CAN STJO
Canbera TIDB*
Tromsoe TROM*
Wettzell WETT*
Yarragadee YAR1*
Yellowknife, CAN YELL* 342
* indicates constrained stations, remaining are solved for (50m apriori sig.)
SOLUTION CHARACTERISTICS
Reference frame and orientation:
Nominally ITRF91, at epoch 1992.5 is realized by constraining up to 12
of the above stations at the IGS coordinates (see IGS message #90).
Orientation is realized through the above coordinates and, once a week,
the fixed DUT1 values from the current NEOS/IERS (Bull. A).
Constants and models:
- no change, see the IGS mess. #101 for details.
Estimation strategies:
- no change, see the IGS mess. #101 for details - , except for the estimation
of DUT1, stochastic orbit modeling, new weighting of L3,P3,
see IGS mess. #130.
ALGO was used as time reference.
Aposteriori variance factors typically are between 0.5 and 1.0 (noise
about 3mm and 200mm for phase and smoothed pseudorange observations, resp.).
PRODUCTS GENERATED:
The following products are generated and uploaded into CDDIS @ NASA/GSFC
EMR07260-6.SP3 GPS ephem. files for days 0-6, week #726 in sp3 format
EMR07267.ERP pole x,y and DUT1 solutions for week #726
EMR07267.SUM name of this text summary file
REMARKS on EMR's products:
1. ALGO hydrogen maser used as a time reference. In the sp3 EPH file sat.
epochs with no reference (e.g. ALGO not observing a satellite) have a value
of 99999. microseconds.
ALGO clock error & drift were about -1450 ns (49326) & -14 ns/day w.r.t.
GPS time.
2. Starting with the week #720 we are assigning nominal sigma codes of 8(256mm)
for all the orbits passing our quality analysis. For errors larger than 1.5m
we are assigning sigmas of abs(error)/4, expressed by the binary
exponent in the sp3 header.
3. Only 50% or less data for PRN13 (GPS9) for all days during this week.
4. PRN12 (GPS10) was deleted from orbit processing on Dec. 07 (day341) due
to modelling problems.
5. Starting with the week #726, the name of the ephemeris file will end with
".sp3" instead of ".eph".
6. Note: additional infomation added to the erp file.
# of stations # of fix stations # of satellites
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