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hal.structure.identifierMax-Planck-Institut für Radioastronomie [MPIFR]
hal.structure.identifierNVI, Inc.
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorBEHREND, J.
hal.structure.identifierinstitut de geodesie et geophysique de Vienne [INSTITUT DE GEODESIE ET GEOPHYSIQUE]
dc.contributor.authorBOEHM, J.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
dc.contributor.authorCHARLOT, P.
hal.structure.identifierNVI, Inc.
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorCLARK, T.
hal.structure.identifierMIT Haystack Observatory
dc.contributor.authorCOREY, B.
hal.structure.identifierNVI, Inc.
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorGIPSON, J.
hal.structure.identifierOnsala Space Observatory [OSO]
dc.contributor.authorHAAS, R.
hal.structure.identifierKashima Space Technology Center
dc.contributor.authorKOYAMA, Y.
hal.structure.identifierNVI, Inc.
hal.structure.identifierNASA Goddard Space Flight Center [GSFC]
dc.contributor.authorMACMILLAN, D.
hal.structure.identifierPulkovo Observatory
dc.contributor.authorMALKIN, Z.
hal.structure.identifierMIT Haystack Observatory
dc.contributor.authorNIELL, A.
hal.structure.identifierOnsala Space Observatory [OSO]
dc.contributor.authorNILSSON, T.
hal.structure.identifierGeodetic Survey Division
dc.contributor.authorPETRACHENKO, B.
hal.structure.identifierMIT Haystack Observatory
dc.contributor.authorROGERS, A.
hal.structure.identifierIstituto di Radioastronomia di Noto
dc.contributor.authorTUCCARI, G.
hal.structure.identifierinstitut de geodesie et geophysique de Vienne [INSTITUT DE GEODESIE ET GEOPHYSIQUE]
dc.contributor.authorWRESNIK, J.
dc.date.issued2008
dc.description.abstractEnFrom October 2003 to September 2005, the International VLBI Service for Geodesy and Astrometry (IVS) examined current and future requirements for geodetic VLBI, including all components from antennas to analysis. IVS Working Group 3 ‘VLBI 2010', which was tasked with this effort, concluded with recommendations for a new generation of VLBI systems. These recommendations were based on the goals of achieving 1 mm measurement accuracy on global baselines, performing continuous measurements for time series of station positions and Earth orientation parameters, and reaching a turnaround time from measurement to initial geodetic results of less than 24 hours. To realize these recommendations and goals, along with the need for low cost of construction and operation, requires a complete examination of all aspects of geodetic VLBI including equipment, processes, and observational strategies. Hence, in October 2005, the IVS VLBI2010 Committee (V2C) commenced work on defining the VLBI2010 system specifications. In this paper we give a summary of the recent progress of the VLBI2010 project.
dc.language.isoen
dc.publisherSpringer Verlag
dc.title.enRecent Progress in the VLBI2010 Development
dc.typeArticle de revue
dc.identifier.doi10.1007/978-3-540-85426-5_96
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Cosmologie et astrophysique extra-galactique [astro-ph.CO]
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]
bordeaux.journalIAG Symposia series
bordeaux.page833-840
bordeaux.volume133
bordeaux.issuePart 5
bordeaux.peerReviewedoui
hal.identifierhal-00299737
hal.version1
hal.popularnon
hal.audienceInternationale
dc.subject.itgeodetic VLBI
dc.subject.itnext generation VLBI2010
dc.subject.itIVS
dc.subject.itMonte Carlo simulations
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00299737v1
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