IAG-IASPEI 2017

Presentation information

Oral

IAG Symposia » G01. Reference frames

[G01-1] International terrestrial reference frame

Wed. Aug 2, 2017 8:30 AM - 10:00 AM Room 502 (Kobe International Conference Center 5F, Room 502)

Chairs: Geoffrey Blewitt (University of Nevada, Reno) , Johannes Boehm (Technische Universität Wien)

9:45 AM - 10:00 AM

[G01-1-06] The status of DORIS in light of ITRF2014

Frank Lemoine1, Laurent Soudarin2, Guilhem Moreaux2, Hugues Capdeville2, Jean-Michel Lemoine3, Pascale Ferrage3, Jerome Saunier4, Denise Dettmering5, Marek Ziebart6, Pascal Willis4,7, Patrick Michael1 (1.NASA Goddard Space Flight Center, Greenbelt, Maryland, U.S.A., 2.Collecte Localisation Satellite, Ramonville Saint Agne, FRANCE, 3.Centre National D'Etudes Spatiales, Toulouse, FRANCE, 4.Institut National de l'information Geographique et forestiere, Saint-Mande, FRANCE, 5.DGFI, Technical University of Munich, Munich , GERMANY, 6.University College London, London, UNITED KINGDOM, 7.Institut de Physique du Globe de Paris, UMR 7154, Gravimetrie et Geodesie Spatiale, Universite Paris Diderot, Paris, FRANCE)

The Doppler Orbitography and Radiopositioning Integrated by Satellite (DORIS) is one of the four techniques of Space Geodesy that contributes to the International Terrestrial Reference Frame. It consists of a network of 55-60 beacons distributed nearly homogeneously around the Earth's surface, as well as a satellite segment including up to six receiving satellites in Low Earth Orbit. Recently the DORIS community reprocessed more than 22 years of data in order to develop the DORIS technique contribution to the ITRF2014 realization of the International Terrestrial Reference Frame (ITRF). Six analysis centers implemented a series of improvements in both measurement and force modeling in order to develop their contributions. The IDS Combination Center prepared the technique contribution which revealed that recent data since the launch of Jason-2 have an intrinsic positioning uncertainty 9, 7, 8 mm respectively in the North, East and Up components, and yield a standard deviation in the polar motion differences with IERS C04 of 245 (Px) and 235 (Py) microseconds.

We discuss in this paper the continuing improvements in the DORIS technique since the completion of ITRF2014. These include the efforts to process a rawer form of the DORIS observable in the RINEX format, the development of a routine combination of DORIS coordinates for application to precise orbit determination DPOD2014, and a preliminary assessment of the contributions of Sentinel-3A and Jason-3 to the DORIS weekly solutions. We also review the performance of the “C" generation of Starec beacons, whose phase centers are defined to +/- 1 mm, and whose development and deployment was initiated in light of the work done by the IDS for ITRF2014.