[IGSMAIL-1384] CODE Changes of June 30, 1996
Markus
Markus
Thu Jul 11 23:55:04 PDT 1996
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IGS Electronic Mail Thu Jul 11 23:55:04 PDT 1996 Message Number 1384
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Author: Markus Rothacher, Tim Springer
Subject: CODE Changes of June 30, 1996
Dear Colleagues,
starting with day 182, 1996 (June 30, 1996, start of GPS week 860) the CODE
Analysis Center of the IGS has changed its processing strategy in several ways.
The changes produced in the CODE results by some of these modifications
(e.g. the change from ITRF93 to ITRF94) could be obtained
by recomputing the daily solutions (transformations of the normal equations),
whereas the impact of other changes (e.g. the orbit model changes and subdaily
ERP model) cannot be assessed so easily and a reprocessing going back to the
observations would be necessary.
Below we list the changes adopted and the effects they will have on the
CODE products:
1) The coordinate system has been changed from ITRF93 to ITRF94. According
to the IGS processing standards again 13 sites are fixed in the routine
analysis to define the reference frame. All the solutions since July 19,
1993 (day of year 200, 1993) were recomputed using the ITRF94 reference
frame to provide as long a time series of ERPs as possible to the IERS.
The comparison of these new solutions with the solutions referring to the
ITRF93 shows
Offset (1993.0) Drift (1993.0)
X-pole 0.27 +- 0.01 mas 0.20 +- 0.003 mas/year
Y-pole 0.68 +- 0.01 mas 0.25 +- 0.010 mas/year
For the epoch 1996.5 the offsets between the two series are 0.97 mas and
1.55 mas in the x- and y-component, respectively.
Some more details are given below.
2) Several modifications concern the orbit modeling:
- Change of the Love Number k2 from 0.285 to 0.030
- Change from GEMT3 to the JGM3 earth potential field
- Improved model for the solid earth tides (earth potential, see IERS
Standards 1995, draft of chapter 6)
- General relativity term introduced (see IERS Standards 1992, p.123)
These changes have an influence mainly on the orbits and the UT1-UTC drift.
The UT1-UTC drift in our series will change by about 0.010 to
0.015 msec/day starting June 30, 1996, in the sense that the
difference between our UT1-UTC series and the IERS products will be
smaller.
3) Subdaily pole model: the model by Ray for the correction of the subdaily
pole and UT1-UTC variations has been adopted. It changes the daily
ERP values by up to about 0.1 mas. The UT1-UTC drift is also slightly
changed. The ERP values we supply to the IERS and to the global data
centers do not contain the contribution of the subdaily model (i.e. the
ERP values submitted are linear function of time over one day and do not
vary with diurnal and semi-diurnal periods).
4) A new set of antenna phase center variations is in use starting
June 30, 1996 (GPS week 860, day of year 181). Because the Dorne Margolin
antennas -- making up most of the antennas in the global IGS network --
were left unchanged the effect of this change on the ERP series is
expected to be marginal. First tests didn't show any significant
rotations or any significant scaling of the coordinate system. The sites
equipped with Trimble antennas change by a few millimeters in
horizontal position and about 1 cm in height (compared to the results
with the phase center corrections we were using for almost 4 years).
The AC questionnaire will be updated according to the new strategy and sent
to the IGSCB as soon as possible.
We hope to serve you with this information and remain
with best regards,
Markus Rothacher
Tim Springer
CODE Analysis Center
PS: Below you find some additional information about the changes in our
products (orbits, coordinates and ERPs) based on the reprocessing of two
days with our OLD and NEW strategy (day 181 and 182 of the year 1996):
CODE product changes due to ALL changes (not only ITRF93-94 switch)
===================================================================
DX DY DZ RX RY RZ SCALE RMS
(mm) (mm) (mm) (mas) (mas) (mas) (ppb) (mm)
ORB 181 NEW-OLD 5 1 1 -1.57 -1.07 -0.89 0.2 14.8
ORB 182 NEW-OLD 7 1 1 -1.47 -1.01 -0.89 0.2 17.8
CRD 181 NEW-OLD 13 2 5 -1.4 -1.0 -0.7 -0.1 8.4
CRD 182 NEW-OLD 16 -0 6 -1.4 -0.9 -0.8 0.0 9.1
ERP 181 NEW-OLD 1.26 1.62 -
ERP 182 NEW-OLD 0.95 1.49 -
--------------------------------------------------------------------------------
Dr. Markus Rothacher Phone : ++41-31-631-8591
Astronomical Institute Fax : ++41-31-631-3869
University of Berne E-mail : rothacher at aiub.unibe.ch
Sidlerstrasse 5 AFTP : ftp ubeclu.unibe.ch (130.92.6.11)
CH-3012 Bern cd aiub$ftp after login
Switzerland WWW : http://ubeclu.unibe.ch/aiub/
[Mailed From: MARKUS ROTHACHER <ROTHACHER at aiub.unibe.ch>]
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