[IGSREPORT-467] EMR Analysis Report (711)
Jan
Jan
Tue Aug 31 15:44:54 PDT 1993
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IGS Electronic Report 31-AUG-1993 15:44:54 Message Number 467
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From: Jan Kouba
Subj: EMR Analysis Report (711)
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(Aug 22 - Aug 28,93)
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 235
Algonquin, CAN ALGO*
Fairbanks FAIR*
Goldstone GOLD*
Hartebeesthoek HART* 240
Holberg,CAN HOLB
Kokee Park KOKB
Madrid MADR*
McMurdo MCMU*
Pamatai PAMA 234 to 240
Penticton, CAN DRAO 235
Santiago SANT*
St. Johns, CAN STJO 235
Canbera TIDB*
Tromsoe TROM*
Wettzell WETT*
Yarragadee YAR1*
Yellowknife, CAN YELL*
* 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
EMR07110-6.EPH GPS ephem. files for days 0-6, week # 711 in sp3 format
EMR07117.ERP pole x,y and DUT1 solutions for week # 711
EMR07117.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 -440 ns (49221) & -26 ns/day w.r.t.
GPS time.
2. Starting with the week #709 we are including orbit sigma estimates in
the sp3 header format (lines 8 to 12), conforming to the sp3 convention
(see NOAA Technical Report NOS 133 NGS 46), i.e. the binary exponent
of sigma in mm. For the orbits passing our quality analysis we are
assigning 9, which, in the sp3 convention, translates into 2**9=512mm
sigmas. For errors larger than 2.5 we are assigning sigmas of
abs(error)/4 , again expressed by the binary exponent. In this way we
feel that problematic satellites indentification is easier and that
a range of errors formerly reported in our summary files can be recovered
as well.
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