[IGSREPORT-5999] Wk 1006 GPS Earth Orientation

IERS IERS
Mon Apr 26 10:57:45 PDT 1999


******************************************************************************
IGS Electronic Report    Mon Apr 26 10:57:45 PDT 1999      Message Number 5999
******************************************************************************

Author: IERS Sub-bureau for Rapid Service and Predictions
Subject: Wk 1006 GPS Earth Orientation

Subject: Earth Orientation Contributions to IERS Bulletin A
Date: 22 Apr 99


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.    51287.64    24                .003                .017

SPbU Int.    51278.82    23                .005                .014

NEOS VLBI    51282.25     6   -.13   .04  -.004    .17   .04   .003

CSR SLR      51279.03    11   -.13  -.09  -.014*   .30   .33   .102*

TUD SLR      51282.00    10   -.52  -.17           .34   .45

IAA SLR      51288.00    30   -.04  -.12           .17   .23

MCC SLR      51282.00    30   -.10  -.11           .14   .17

UTX LLR      51237.27     9               -.064                .388

IGS Final    51278.50    30    .01   .01           .02   .03

IGS Rapid    51289.50    11    .02   .00           .05   .01

             51289.50     2                .006*               .004*

USNO GPS     51289.50    22                .001*               .015*

EMR GPS      51289.50    22                .005*               .045*

* 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          51284.5  30    .28   .09   2.87   .020    .09   .10    .18   .017

ESA          51278.5  30    .30   .16         -.033    .13   .16          .030

EMR          51278.5  30    .18   .22 -16.51   .017    .17   .17    .06   .031

GFZ          51285.5  30    .32   .00   -.15   .010    .08   .09    .33   .039

JPL          51278.5  30    .31   .05 -13.77   .004    .12   .11    .08   .028

NGS          51285.5  30    .44  -.08         -.039    .18   .17          .046

SIO          51278.5  30    .31   .14          .015    .11   .12          .029

USN (Rapid)  51289.5  30    .34   .11         -.019    .15   .16          .031

USNO GPS UT  51289.5  30                 .93                        .02

IGS Final    51278.5  30    .31   .08    .01  -.005    .06   .06    .02   .021

IGS Rapid    51289.5  30    .32   .09    .03   .001    .12   .12    .10   .023

* 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   51239.   30    .03   .05  -.009           .06   .10   .019

97C04        51289.   30   -.01   .10   .001           .09   .11   .022


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


[Mailed From: Dennis McCarthy <dmc at maia.usno.navy.mil>]



More information about the IGSREPORT mailing list