[IGSREPORT-7246] Wk 1065 GPS Earth Orientation
Dennis McCarthy
dmc at maia.usno.navy.mil
Thu Jun 8 12:33:56 PDT 2000
******************************************************************************
IGS Electronic Report 08 Jun 12:33:41 PDT 2000 Message Number 7246
******************************************************************************
Author: IERS Sub-bureau for Rapid Service and Predictions
Subject: Earth Orientation Contributions to IERS Bulletin A
Date: 8 Jun 00
In this report, individual Earth orientation time series are compared
to the IERS Bulletin A combination. For further information, including
the raw time series, refer to http://maia.usno.navy.mil/bulletin-a.html.
The first table below shows some comparison results for those series
included in Bulletin A during the last 30 days. All data are aligned to
the system defined by ITRF94 and the current ICRF by removing a priori mean
bias, rate, annual and semiannual terms. (No corrections are applied to
the NEOS VLBI and the NEOS Intensives series for UT1-UTC.)
Units: milliseconds of arc for x, y; milliseconds of time for UT1-UTC
Contributor Latest # Mean Standard Deviation
Series Day (series-BullA)
x y UT1-UTC x y UT1-UTC
NEOS Int. 51700.68 21 -.004 .028
SPbU Int. 51698.85 19 -.012 .027
NEOS VLBI 51674.25 5 -.14 -.05 -.002 .22 .20 .005
IAA VLBI 51674.25 5 -.09 .06 .003 .13 .10 .004
CSR SLR 51698.61 11 .02 -.15 -.068* .66 .34 .188*
TUD SLR 51696.00 10 -.66 .03 .23 .27
IAA SLR 51701.00 30 .05 .01 .18 .19
MCC SLR 51695.00 30 .17 -.24 .15 .18
UTX LLR 51688.48 13 .300 .238
IGS Final 51684.50 30 .00 .00 .02 .04
IGS Rapid 51702.50 18 .00 .00 .04 .06
51702.50 2 -.009* .002*
USNO GPS 51702.50 30 .005* .015*
* All satellite techniques provide information on the rate of change of
Universal Time contaminated by effects due to unmodelled orbit node
motion. VLBI-based results have been used to minimize drifts in UT
estimates.
The following tables show comparisons for other related time series during
the last 30 days. All IGS series are final solutions except for the USNO
series. No a priori systematic corrections have been applied.
Units: milliseconds of arc for x, y; milliseconds of time for UT, LOD
IGS Latest # Mean Standard Deviation
Series Day (series-BullA)
x y UT* LOD* x y UT* LOD*
COD 51697.5 30 .03 .15 -7.56 .009 .06 .04 .04 .020
ESA 51691.5 30 -.04 .38 -.013 .06 .13 .022
EMR 51691.5 30 .10 .14 -23.94 .086 .11 .17 .59 .024
GFZ 51698.5 30 .03 .24 .01 -.006 .05 .09 .05 .023
JPL 51691.5 30 .10 .11 -18.96 .016 .07 .12 .13 .039
NGS 51694.5 30 .11 .24 -.026 .23 .14 .063
SIO 51677.5 30 .03 .16 .040 .06 .09 .016
USN (Rapid) 51702.5 30 .10 .13 -.022 .12 .17 .023
USNO GPS UT 51702.5 30 1.66 .03
IGS Final 51684.5 30 .02 .23 .00 .000 .04 .05 .01 .018
IGS Rapid 51702.5 30 .04 .22 .01 -.002 .08 .08 .06 .016
* All satellite techniques provide information on the rate of change of
Universal Time contaminated by effects due to unmodelled orbit node
motion. The UT results for COD and JPL are integrations of LOD estimates.
EMR estimates UT and LOD separately by applying a priori orbit constraints.
GFZ and IGS use VLBI-based results to minimize drifts in their UT estimates
and thus the standard deviations are not representative of the intrinsic
capabilities of GPS alone for monitoring UT variations. USNO estimates
UT using long-term models for orbit plane rotations.
IERS Central Bureau Series:
Series Latest # Mean Standard Deviation
Day (series-BullA)
x y UT1-UTC x y UT1-UTC
Bulletin B 51674. 30 .04 -.02 -.001 .04 .05 .031
97C04 51703. 30 .02 .02 -.012 .09 .06 .029
Plots of the residuals are available at http://maia.usno.navy.mil/plots.html.
------------------------------------------------------------------------------
The IERS Sub-bureau for Rapid Service and Prediction is an activity of the
National Earth Orientation Service and is performed by the Earth Orientation
Department at the U.S. Naval Observatory.
--
Dennis D. McCarthy dmc at maia.usno.navy.mil
Director, Directorate of Time phone: (202) 762-1837
U.S. Naval Observatory fax: (202) 762-1563
Washington, DC 20392-5420
More information about the IGSREPORT
mailing list