[IGSREPORT-443] EMR Analysis Report (709)
Jan
Jan
Fri Aug 20 09:41:58 PDT 1993
***********************************************************************
IGS Electronic Report 20-AUG-1993 09:41:58 Message Number 443
***********************************************************************
From: Jan Kouba
Subj: EMR Analysis Report (709)
-------------------------------
(Aug 08 - Aug 14,93)
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* 220, 221, 224 to 226
Pamatai PAMA 220 to 226
Penticton, CAN DRAO
Santiago SANT*
St. Johns, CAN STJO
Canbera TIDB*
Tromsoe TROM* 221
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
EMR07090-6.EPH GPS ephem. files for days 0-6, week # 709 in sp3 format
EMR07097.ERP pole x,y and DUT1 solutions for week # 709
EMR07097.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 -110 ns (49207) & -20 ns/day w.r.t.
GPS time.
2. Starting this week (709) we have included 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.
3. AS was on for PRN 18 on Aug 10 (day222), all observations for PRN 18
were downweighted, no DUT1 estimation on this day.
4. PRN26 was removed from the orbit processing on Aug 12 (day224) due to
maintainance/orbit repositioning
--
Jan Kouba
Geodetic Survey of Canada
Ottawa, Ontario, Canada
Internet: kouba at geod.emr.ca
More information about the IGSREPORT
mailing list