The IVS data input to ITRF2014

Axel Nothnagel Walter Alef Jun Amagai Per Helge Andersen 1 Tatiana Andreeva Thomas Artz Sabine Bachmann Christophe Barache 2 Alain Baudry 3 Erhard Bauernfeind Karen Baver Christopher Beaudoin Dirk Behrend A. Bellanger 4 Anton Berdnikov Per Bergman 5 Simone Bernhart Alessandra Bertarini Giuseppe Bianco Ewald Bielmaier David Boboltz Johannes Böhm Sigrid Böhm 6 Armin Boer Sergei Bolotin Mireille Bougeard 7 G. Bourda 4 Salvo Buttaccio Letizia Cannizzaro Roger Cappallo Brent Carlson 8 Merri Sue Carter 9 P. Charlot 4 Chenyu Chen Maozheng Chen 10 Jungho Cho 11 Thomas Clark 12 A. Collioud 4 Francisco Colomer Giuseppe Colucci 13 Ludwig Combrinck John Conway Brian Corey 14 Ronald Curtis 15 Reiner Dassing Maria Davis 16 Pablo De Vicente Alexey Diakov John Dickey 17 Irv Diegel Koichiro Doi Hermann Drewes Maurice Dube 18 Gunnar Elgered Gerald Engelhardt Mark Evangelista 19 Qingyuan Fan Leonid Fedotov Alan Fey Ricardo Figueroa 20, 21 Yoshihiro Fukuzaki Daniel Gambis Susana Garcia-Espada Ralph Gaume 22 Michael Gaylard Nicole Geiger John Gipson Frank Gomez Jesus Gomez-Gonzalez 23 David Gordon Ramesh Govind Vadim Gubanov Sergei Gulyaev Ruediger Haas David Hall Sebastian Halsig Roger Hammargren Hayo Hase Robert Heinkelmann Leif Helldner Cristian Herrera Ed Himwich Thomas Hobiger Christoph Holst Xiaoyu Hong Mareki Honma Xinyong Huang 24 Urs Hugentobler Ryuichi Ichikawa Andreas Iddink Johannes Ihde Gennadiy Ilijin Alexander Ipatov 25 Irina Ipatova Misao Ishihara D. V. Ivanov Chris Jacobs Takaaki Jike Karl-Ake Johansson 26 Heidi Johnson 27, 28 Kenneth Johnston 29 Hyunhee Ju Masao Karasawa Pierre Kaufmann Ryoji Kawabata Noriyuki Kawaguchi Eiji Kawai Michael Kaydanovsky Mikhail Kharinov Hideyuki Kobayashi Kensuke Kokado Tetsuro Kondo Edward Korkin Yasuhiro Koyama Hana Krasna Gerhard Kronschnabl Sergey Kurdubov Shinobu Kurihara Jiro Kuroda 30 Younghee Kwak Laura La Porta Ruth Labelle Doug Lamb Sébastien Lambert Line Langkaas Roberto Lanotte Alexey Lavrov 31 Karine Le Bail Judith Leek Bing Li Huihua Li Jinling Li Shiguang Liang 32 Michael Lindqvist Xiang Liu Michael Loesler Jim Long 33 Colin Lonsdale Jim Lovell Stephen Lowe Antonio Lucena Brian Luzum Chopo Ma 34 Jun Ma 35 Giuseppe Maccaferri Morito Machida 36 Dan Macmillan Matthias Madzak Zinovy Malkin 37 Seiji Manabe Franco Mantovani Vyacheslav Mardyshkin Dmitry Marshalov Geir Mathiassen Shigeru Matsuzaka Dennis Mccarthy 38 Alexey Melnikov 39 Andrey Michailov Natalia Miller Donald Mitchell 40 Julian Andres Mora-Diaz Arno Mueskens Yasuko Mukai 41 Mauro Nanni Tim Natusch Monia Negusini Alexander Neidhardt George Nicolson Arthur Niell 14 Pavel Nikitin Tobias, Nilsson Tong Ning 42 Takashi Nishikawa 43 Carey Noll 44 Kentarou Nozawa 45 Clement Ogaja Hongjong Oh Hans Olofsson 46 Per Erik Opseth Sandro Orfei Rosa Pacione 47 Katherine Pazamickas William Petrachenko 48 Lars Pettersson Pedro Pino 49 Lucia Plank Christian Ploetz Michael Poirier 7 Markku Poutanen 50 Zhihan Qian 51 Jonathan Quick Ismail Rahimov Jay Redmond 52, 53 Brett Reid John Reynolds Bernd Richter Maria Rioja Andres Romero-Wolf Chester Ruszczyk Alexander Salnikov Pierguido Sarti 54 Raimund Schatz 55, 56 Hans-Georg Scherneck Francesco Schiavone Ulrich Schreiber 57 Harald Schuh Walter Schwarz Cecilia Sciarretta Anthony Searle Mamoru Sekido Manuela Seitz Minghui Shao Kazuo Shibuya Fengchun Shu Moritz Sieber 58 Asmund Skjaeveland Elena Skurikhina Sergey Smolentsev 59 Dan Smythe Don Sousa 60 Ojars Sovers 17 Laura Stanford Carlo Stanghellini Alan Steppe Rich Strand Jing Sun Igor Surkis Kazuhiro Takashima Kazuhiro Takefuji Hiroshi Takiguchi Yoshiaki Tamura Tadashi Tanabe Emine Tanir 61 An Tao Claudio Tateyama Kamil Teke Cynthia Thomas Volkmar Thorandt Bruce Thornton Claudia Tierno Ros Oleg Titov Mike Titus Paolo Tomasi Vincenza Tornatore Corrado Trigilio Dmitriy Trofimov Masanori Tsutsumi 62 Gino Tuccari 63 Tasso Tzioumis Hideki Ujihara Dieter Ullrich Minttu Uunila Tiziana Venturi Francesco Vespe Veniamin Vityazev Alexandr Volvach Alexander Vytnov Guangli Wang 64 Jinqing Wang 65 Lingling Wang 66 Na Wang Shiqiang Wang Wenren Wei Stuart Weston Alan Whitney Reiner Wojdziak Yaroslav Yatskiv Wenjun Yang Shuhua Ye 67 Sangoh Yi 68 Aili Yusup Octavio Zapata Reinhard Zeitlhoefler Hua Zhang 69, 70 Ming Zhang 71 Xiuzhong Zhang Rongbing Zhao Weimin Zheng Ruixian Zhou 72 Nataliya Zubko
3 FORMATION STELLAIRE 2015
LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac], UB - Université de Bordeaux, INSU - CNRS - Institut national des sciences de l'Univers , CNRS - Centre National de la Recherche Scientifique
4 M2A 2015
LAB - Laboratoire d'Astrophysique de Bordeaux [Pessac]
8 Birkeland Centre for Space Science
Department of Physics and Technology [Bergen]
36 Department of Mathematics, University of Michigan
Department of Mathematics, University of Michigan
60 CEP/Paris
CEP - Centre Énergétique et Procédés
Abstract : Very Long Baseline Interferometry (VLBI) is a primary space-geodetic technique for determining precise coordinates on the Earth, for monitoring the variable Earth rotation and orientation with highest precision, and for deriving many other parameters of the Earth system. The International VLBI Service for Geodesy and Astrometry (IVS, http://ivscc.gsfc.nasa.gov/) is a service of the International Association of Geodesy (IAG) and the International Astronomical Union (IAU). The datasets published here are the results of individual Very Long Baseline Interferometry (VLBI) sessions in the form of normal equations in SINEX 2.0 format (http://www.iers.org/IERS/EN/Organization/AnalysisCoordinator/SinexFormat/sinex.html, the SINEX 2.0 description is attached as pdf) provided by IVS as the input for the next release of the International Terrestrial Reference System (ITRF): ITRF2014. This is a new version of the ITRF2008 release (Bockmann et al., 2009). For each session/ file, the normal equation systems contain elements for the coordinate components of all stations having participated in the respective session as well as for the Earth orientation parameters (x-pole, y-pole, UT1 and its time derivatives plus offset to the IAU2006 precession-nutation components dX, dY (https://www.iau.org/static/resolutions/IAU2006_Resol1.pdf). The terrestrial part is free of datum. The data sets are the result of a weighted combination of the input of several IVS Analysis Centers. The IVS contribution for ITRF2014 is described in Bachmann et al (2015), Schuh and Behrend (2012) provide a general overview on the VLBI method, details on the internal data handling can be found at Behrend (2013).
Type de document :
Autre publication
2015ivs.data..1N - GFZ Data Services, Helmoltz Centre, Potsdam, Germany. 2015, 〈10.5880/GFZ.1.1.2015.002〉
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https://hal.archives-ouvertes.fr/hal-01281368
Contributeur : Marie-Paule Pomies <>
Soumis le : mercredi 2 mars 2016 - 09:27:30
Dernière modification le : jeudi 21 mars 2019 - 14:43:22

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Axel Nothnagel, Walter Alef, Jun Amagai, Per Helge Andersen, Tatiana Andreeva, et al.. The IVS data input to ITRF2014. 2015ivs.data..1N - GFZ Data Services, Helmoltz Centre, Potsdam, Germany. 2015, 〈10.5880/GFZ.1.1.2015.002〉. 〈hal-01281368〉

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