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A study of VLB 2010 potential for source structure corrections

hal.structure.identifierGeodetic Survey Division
dc.contributor.authorPETRACHENKO, W. T.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCHARLOT, P.
hal.structure.identifierLaboratoire d'astrodynamique, d'astrophysique et d'aéronomie de bordeaux [L3AB]
hal.structure.identifierObservatoire aquitain des sciences de l'univers [OASU]
hal.structure.identifierLaboratoire d'Astrophysique de Bordeaux [Pessac] [LAB]
dc.contributor.authorCOLLIOUD, A.
dc.contributor.authorHOBIGER, T.
hal.structure.identifierMIT Haystack Observatory
dc.contributor.authorNIELL, A.
dc.date.issued2008
dc.date.conference2007-09-17
dc.description.abstractEnIn October 2003, the International VLBI Service for Geodesy and Astrometry (IVS) in- stalled Working Group 3 ‘VLBI2010' to examine current and future requirements for geodetic/astrometric VLBI including all components from antennas to analysis, and to create recommendations for a new gen- eration of VLBI systems. Some important recommendations include: the use of larger networks; the use of smaller faster slewing antennas; the use of very high data rates; and, the use of multiple (e.g. 4) widely spaced bands to resolve RF phase ambiguities. When taken together, these recommendations result in a many-fold increase in the number of observations per session. UV coverage improves to the point where precise VLBI images of the ICRF sources can be constructed on a daily basis directly from the geodetic observations, therefore enabling source structure corrections to be calculated. Simulations are currently underway to evaluate the potential of this approach.
dc.language.isoen
dc.source.title2008jsrs.meet...48P - Proceedings of the "Journées Systèmes de Référence Spatio-temporels 2007". Observatoire de Paris, 17-19 September 2007. Editor: Nicole Capitaine. ISBN: 978-2-901057-59-8
dc.title.enA study of VLB 2010 potential for source structure corrections
dc.typeCommunication dans un congrès
dc.subject.halPlanète et Univers [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
dc.subject.halPhysique [physics]/Astrophysique [astro-ph]/Planétologie et astrophysique de la terre [astro-ph.EP]
bordeaux.page48
bordeaux.countryFR
bordeaux.title.proceeding2008jsrs.meet...48P - Proceedings of the "Journées Systèmes de Référence Spatio-temporels 2007". Observatoire de Paris, 17-19 September 2007. Editor: Nicole Capitaine. ISBN: 978-2-901057-59-8
bordeaux.conference.cityParis
bordeaux.peerReviewedoui
hal.identifierhal-00402698
hal.version1
hal.invitednon
hal.proceedingsoui
hal.conference.end2007-09-19
hal.popularnon
hal.audienceInternationale
hal.origin.linkhttps://hal.archives-ouvertes.fr//hal-00402698v1
bordeaux.COinSctx_ver=Z39.88-2004&rft_val_fmt=info:ofi/fmt:kev:mtx:journal&rft.btitle=2008jsrs.meet...48P%20-%20Proceedings%20of%20the%20%22Journ%C3%A9es%20Syst%C3%A8mes%20de%20R%C3%A9f%C3%A9rence%20Spatio-temporels%202007%22.%20Observatoire%20de%20Paris,&rft.date=2008&rft.spage=48&rft.epage=48&rft.au=PETRACHENKO,%20W.%20T.&CHARLOT,%20P.&COLLIOUD,%20A.&HOBIGER,%20T.&NIELL,%20A.&rft.genre=unknown


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