[IGSREPORT-327] EMR Jan93 Orbit Test Report
Jan
Jan
Sat Jun 12 12:04:45 PDT 1993
***********************************************************************
IGS Electronic Report 12-JUN-1993 12:04:45 Message Number 327
***********************************************************************
From: Jan Kouba
Subj: EMR Jan93 Orbit Test Report
---------------------------------
Subject: EMR Reanalysis of the GPS week 680-681
(Jan. 17 to Jan. 30, 1993)
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 project called
"Active Control System" in Canada 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* 018
McMurdo MCMU 017 to 023 ; 26 to 30
Pamatai PAMA
Penticton, CAN DRAO 024, 029, 030
Santiago SANT*
St. Johns, CAN STJO
Canbera TIDB*
Tromsoe TROM*
Wettzell WETT*
Yarragadee YAR1* 017 to 020
Yellowknife, CAN YELL*
* indicates fixed stations, remaining are solved for (50m apriori sig.)
SOLUTION CHARACTERISTICS
Reference frame and orientation:
Nominally ITRF91, at epoch 1993.06 is realized by fixing the 12
stations at the IGS (SSC(IERS) 93 C 02) coordinates (see IGS message #236)
Orientation is realized through the above coordinates and, by fixing the DUT1
value on Jan 17, 93 obtained from the final values of the IERS Bull.B
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 were generated and uploaded into AIUB astronomy/igscomp
EMR06800-6.EPH GPS ephem. for week # 680 in sp3 format & in ITRF91
EMR06810-6.EPH GPS ephem. for week # 681 in sp3 format & in ITRF91
EMR06800-6.EPHJ2000 GPS ephem. for week # 680 in sp3 format & in J2000
EMR06810-6.EPHJ2000 GPS ephem. for week # 681 in sp3 format & in J2000
EMR06817.ERP pole x,y and DUT1 solutions for weeks # 680, 681
EMR06817.SUM name of this text 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 -600 ns (49004) and -50 ns/day
w.r.t. GPS time.
2. Modelling problems with PRN11 on Jan17/93. Errors up to 9m! (About 20% and
50% of the usual amount of data was observed and used for this satellite
on Jan 17 and 18, respectively)
3. Due to data problems Penticton was excluded from processing on Jan 24, 29
30 and MCMU on Jan 26-30, respectively.
4. The J2000 ephemeris is based on the final IERS Bull.B EOP series;
The ITRF91 ephemeris (*.eph) is based on the EOP sol. in the emr06817.erp
file above.
5. DUT1 estimation initialized only once (on Jan 17) and solved for on all
subsequent days.
More information about the IGSREPORT
mailing list