Delivered-To: igsmail@igscb.jpl.nasa.gov From: Jim Ray "(NGS" 301-713-2850 "x112)" Message-Id: <200412021353.IAA28167@ness.ngs.noaa.gov> Subject: [IGSMAIL-5059]: Reference System session at EGU2005 To: igsmail@igscb.jpl.nasa.gov, ivsmail@ivscc.gsfc.nasa.gov, slrmail@dgfi.badw-muenchen.de, dorismail@ensg.ign.fr Date: Thu, 2 Dec 2004 08:53:06 -0500 (EST) Content-Type: text/plain; charset=US-ASCII Content-Transfer-Encoding: 7bit Sender: owner-igsmail Precedence: bulk ****************************************************************************** IGS Electronic Mail 02 Dec 05:56:58 PST 2004 Message Number 5059 ****************************************************************************** Author: Jim Ray, Ernst Schrama, & Zuheir Altamimi EGU 2nd General Assembly -- Vienna, Austria, 25-29 April 2005 http://www.copernicus.org/EGU/ga/egu05/ Dear Colleagues, The 2nd General Assembly of the European Geosciences Union will be held in Vienna, Austria, 25-29 April 2005. We draw your attention in particular to session "G1 - Reference System Stability, Accuracy, and the Presence of Secular or Seasonal Signals", which is co-sponsored by Hydrological and Cryospheric Sciences. This session should provide a good opportunity to prepare for the new ITRF2004 realization, among other things. As geodetic applications in the Earth sciences advance in their capabilities and accuracy goals, the demands placed on the International Terrestrial Reference Frame (ITRF) increase also since this is the fundamental platform from which most large-scale measurements are made. The basic ITRF requirements concern: accuracy in terms of origin and scale; precision in terms of relative internal consistency of station positions and velocities; long-term stability of origin, scale, and orientation; universal and easy user access. ITRF is formed by a combination of different space geodetic techniques. Since no one technique possesses all the needed strengths, a major challenge is to detect and mitigate systematic errors from the individual techniques optimally. Stability is particularly important for such problems as reliable detection of e.g. sea-level change, which requires scale rate uncertainties <0.1 ppb/yr. It is difficult to objectively assess whether this level is actually being attained or not because there is minimal internal redundancy, especially for origin and scale. The presence of non-linear (non-tidal) variations in station motions complicates ITRF maintenance. On the one hand, these can provide valuable geophysical insights, for example into large-scale fluid mass movements or aspects of global change or post-seismic deformation. Full geophysical utilization requires separating complicating effects such as highly localized motions like subsidence, or effects caused by long wavelength GPS orbit errors, propagation correction errors, antenna model limitations, multipath and other environmental effects, etc. This session will focus on updating user requirements for the ITRF and examining its current capabilities and limitations. Any inputs that might aid in improving the next ITRF realization and studies of the ITRF accuracy or stability using independent methods are welcome. Important Dates: 07 January 2005: Deadline for support applications 21 January 2005: Deadline for receipt of abstracts 08 April 2005: Deadline for pre-registration & hotel booking Please consider submitting a paper to this symposium or contact us directly if you have any questions. Sincerely, Jim Ray, jimr@ngs.noaa.gov Geosciences Research Division, National Geodetic Survey Ernst Schrama, e.j.o.schrama@lr.tudelft.nl Department of Geodesy, Technical Univ. of Delft Zuheir Altamimi, altamimi@ensg.ign.fr ENSG/LAREG, Institut Geographique National