Baseline Vector Repeatability at the Sub-Millimeter Level Enabled by Radio Interferometer Phase Delays of Intra-Site Baselines

dc.contributorAalto-yliopistofi
dc.contributorAalto Universityen
dc.contributor.authorXu, Ming H.en_US
dc.contributor.authorSavolainen, Tuomasen_US
dc.contributor.authorBolotin, Sergeien_US
dc.contributor.authorBernhart, Simoneen_US
dc.contributor.authorPlötz, Christianen_US
dc.contributor.authorHaas, Rüdigeren_US
dc.contributor.authorVarenius, Eskilen_US
dc.contributor.authorWang, Guanglien_US
dc.contributor.authorMcCallum, Jamieen_US
dc.contributor.authorHeinkelmann, Roberten_US
dc.contributor.authorLunz, Susanneen_US
dc.contributor.authorSchuh, Haralden_US
dc.contributor.authorZubko, Nataliyaen_US
dc.contributor.authorKareinen, Nikoen_US
dc.contributor.departmentDepartment of Electronics and Nanoengineeringen
dc.contributor.departmentMetsähovi Radio Observatoryen
dc.contributor.groupauthorAnne Lähteenmäki Groupen
dc.contributor.organizationNASA Goddard Space Flight Centeren_US
dc.contributor.organizationReichert GmbHen_US
dc.contributor.organizationFederal Agency for Cartography and Geodesyen_US
dc.contributor.organizationChalmers University of Technologyen_US
dc.contributor.organizationCAS - Shanghai Astronomical Observatoryen_US
dc.contributor.organizationUniversity of Tasmaniaen_US
dc.contributor.organizationHelmholtz Centre Potsdam - German Research Centre for Geosciencesen_US
dc.contributor.organizationTechnical University of Berlinen_US
dc.contributor.organizationNational Land Survey of Finlanden_US
dc.date.accessioned2023-04-19T06:04:45Z
dc.date.available2023-04-19T06:04:45Z
dc.date.issued2023-03en_US
dc.descriptionFunding Information: We would like to thank Arthur Niell very much for the comments during the reviews. The results reported in this paper used the data coordinated by the International VLBI Service (IVS) and its international self‐funded member organizations. We are grateful to the IVS stations at Hartebeesthoek (South Africa Radio Astronomical Observatory), Ishioka (Geospatial Information Authority of Japan), Kokee Park (U.S. Naval Observatory and NASA GSFC, USA), Ny‐Ålesund (Norwegian Mapping Authority, Norway), Onsala (Onsala Space Observatory, Chalmers University of Technology, Sweden), Shanghai (Shanghai Astronomical Observatory, China), Wettzell (Bundesamt für Kartographie und Geodäsie and Technische Universität München, Germany), and Yebes (Instituto Geográfico Nacional, Spain), to the staff at the Bonn Correlator, the Washington Correlator, the Onsala Observatory Correlator, and the MIT Haystack Observatory correlator for performing the correlations and the fringe fitting of the data, to the NASA GSFC VLBI group and the BKG VLBI group for doing the geodetic solutions, and to the IVS Data Centers at BKG (Leipzig, Germany), Observatoire de Paris (France), and NASA CDDIS (Greenbelt, MD, USA) for the central data holdings. This research has made use of the Generic Mapping Tools package, the pgplot library, and the SAO/NASA Astrophysics Data System. The work was supported by the Academy of Finland project No. 315721. Open Access funding enabled and organized by Projekt DEAL. Funding Information: We would like to thank Arthur Niell very much for the comments during the reviews. The results reported in this paper used the data coordinated by the International VLBI Service (IVS) and its international self-funded member organizations. We are grateful to the IVS stations at Hartebeesthoek (South Africa Radio Astronomical Observatory), Ishioka (Geospatial Information Authority of Japan), Kokee Park (U.S. Naval Observatory and NASA GSFC, USA), Ny-Ålesund (Norwegian Mapping Authority, Norway), Onsala (Onsala Space Observatory, Chalmers University of Technology, Sweden), Shanghai (Shanghai Astronomical Observatory, China), Wettzell (Bundesamt für Kartographie und Geodäsie and Technische Universität München, Germany), and Yebes (Instituto Geográfico Nacional, Spain), to the staff at the Bonn Correlator, the Washington Correlator, the Onsala Observatory Correlator, and the MIT Haystack Observatory correlator for performing the correlations and the fringe fitting of the data, to the NASA GSFC VLBI group and the BKG VLBI group for doing the geodetic solutions, and to the IVS Data Centers at BKG (Leipzig, Germany), Observatoire de Paris (France), and NASA CDDIS (Greenbelt, MD, USA) for the central data holdings. This research has made use of the Generic Mapping Tools package, the pgplot library, and the SAO/NASA Astrophysics Data System. The work was supported by the Academy of Finland project No. 315721. Open Access funding enabled and organized by Projekt DEAL. Publisher Copyright: © 2023. The Authors.
dc.description.abstractWe report the results of position ties for short baselines at eight geodetic sites based on phase delays that are extracted from global geodetic very-long-baseline interferometry (VLBI) observations rather than dedicated short-baseline experiments. An analysis of phase delay observables at X band from two antennas at the Geodetic Observatory Wettzell, Germany, extracted from 107 global 24-hr VLBI sessions since 2019 yields weighted root-mean-square scatters about the mean baseline vector of 0.3, 0.3, and 0.8 mm in the east, north, and up directions, respectively. Position ties are also obtained for other short baselines between legacy antennas and nearby, newly built antennas. They are critical for maintaining a consistent continuation of the realization of the terrestrial reference frame, especially when including the new VGOS network. The phase delays of the baseline WETTZ13N–WETTZELL enable an investigation of sources of error at the sub-millimeter level. We found that a systematic variation of larger than 1 mm can be introduced to the Up estimates of this baseline vector when atmospheric delays were estimated. Although the sub-millimeter repeatability has been achieved for the baseline vector WETTZ13N–WETTZELL, we conclude that long term monitoring should be conducted for more short baselines to assess the instrumental effects, in particular the systematic differences between phase delays and group delays, and to find common solutions for reducing them. This will be an important step toward the goal of global geodesy at the 1 mm level.en
dc.description.versionPeer revieweden
dc.format.mimetypeapplication/pdfen_US
dc.identifier.citationXu, M H, Savolainen, T, Bolotin, S, Bernhart, S, Plötz, C, Haas, R, Varenius, E, Wang, G, McCallum, J, Heinkelmann, R, Lunz, S, Schuh, H, Zubko, N & Kareinen, N 2023, 'Baseline Vector Repeatability at the Sub-Millimeter Level Enabled by Radio Interferometer Phase Delays of Intra-Site Baselines', Journal of Geophysical Research: Solid Earth, vol. 128, no. 3, e2022JB025198. https://doi.org/10.1029/2022JB025198en
dc.identifier.doi10.1029/2022JB025198en_US
dc.identifier.issn2169-9313
dc.identifier.issn2169-9356
dc.identifier.otherPURE UUID: 12792d9f-ef8a-43a7-80b7-76fb8029f1f8en_US
dc.identifier.otherPURE ITEMURL: https://research.aalto.fi/en/publications/12792d9f-ef8a-43a7-80b7-76fb8029f1f8en_US
dc.identifier.otherPURE FILEURL: https://research.aalto.fi/files/105623060/JGR_Solid_Earth_2023_Xu_Baseline_Vector_Repeatability_at_the_Sub_Millimeter_Level_Enabled_by_Radio_Interferometer.pdf
dc.identifier.urihttps://aaltodoc.aalto.fi/handle/123456789/120435
dc.identifier.urnURN:NBN:fi:aalto-202304192751
dc.language.isoenen
dc.publisherWiley
dc.relation.fundinginfoWe would like to thank Arthur Niell very much for the comments during the reviews. The results reported in this paper used the data coordinated by the International VLBI Service (IVS) and its international self‐funded member organizations. We are grateful to the IVS stations at Hartebeesthoek (South Africa Radio Astronomical Observatory), Ishioka (Geospatial Information Authority of Japan), Kokee Park (U.S. Naval Observatory and NASA GSFC, USA), Ny‐Ålesund (Norwegian Mapping Authority, Norway), Onsala (Onsala Space Observatory, Chalmers University of Technology, Sweden), Shanghai (Shanghai Astronomical Observatory, China), Wettzell (Bundesamt für Kartographie und Geodäsie and Technische Universität München, Germany), and Yebes (Instituto Geográfico Nacional, Spain), to the staff at the Bonn Correlator, the Washington Correlator, the Onsala Observatory Correlator, and the MIT Haystack Observatory correlator for performing the correlations and the fringe fitting of the data, to the NASA GSFC VLBI group and the BKG VLBI group for doing the geodetic solutions, and to the IVS Data Centers at BKG (Leipzig, Germany), Observatoire de Paris (France), and NASA CDDIS (Greenbelt, MD, USA) for the central data holdings. This research has made use of the Generic Mapping Tools package, the pgplot library, and the SAO/NASA Astrophysics Data System. The work was supported by the Academy of Finland project No. 315721. Open Access funding enabled and organized by Projekt DEAL. We would like to thank Arthur Niell very much for the comments during the reviews. The results reported in this paper used the data coordinated by the International VLBI Service (IVS) and its international self-funded member organizations. We are grateful to the IVS stations at Hartebeesthoek (South Africa Radio Astronomical Observatory), Ishioka (Geospatial Information Authority of Japan), Kokee Park (U.S. Naval Observatory and NASA GSFC, USA), Ny-Ålesund (Norwegian Mapping Authority, Norway), Onsala (Onsala Space Observatory, Chalmers University of Technology, Sweden), Shanghai (Shanghai Astronomical Observatory, China), Wettzell (Bundesamt für Kartographie und Geodäsie and Technische Universität München, Germany), and Yebes (Instituto Geográfico Nacional, Spain), to the staff at the Bonn Correlator, the Washington Correlator, the Onsala Observatory Correlator, and the MIT Haystack Observatory correlator for performing the correlations and the fringe fitting of the data, to the NASA GSFC VLBI group and the BKG VLBI group for doing the geodetic solutions, and to the IVS Data Centers at BKG (Leipzig, Germany), Observatoire de Paris (France), and NASA CDDIS (Greenbelt, MD, USA) for the central data holdings. This research has made use of the Generic Mapping Tools package, the pgplot library, and the SAO/NASA Astrophysics Data System. The work was supported by the Academy of Finland project No. 315721. Open Access funding enabled and organized by Projekt DEAL.
dc.relation.ispartofseriesJournal of Geophysical Research: Solid Earthen
dc.relation.ispartofseriesVolume 128, issue 3en
dc.rightsopenAccessen
dc.subject.keywordgeodetic VLBIen_US
dc.subject.keywordGGOSen_US
dc.subject.keywordITRFen_US
dc.subject.keywordphase delaysen_US
dc.subject.keywordreference framesen_US
dc.subject.keywordVGOSen_US
dc.titleBaseline Vector Repeatability at the Sub-Millimeter Level Enabled by Radio Interferometer Phase Delays of Intra-Site Baselinesen
dc.typeA1 Alkuperäisartikkeli tieteellisessä aikakauslehdessäfi
dc.type.versionpublishedVersion

Files