Abstract
CONT17 is an observation campaign of continuous Very Long Baseline Interferometry (VLBI) sessions for a period of 15 days, carried out by the International VLBI Service for Geodesy and Astrometry (IVS). This campaign represents an interesting opportunity for the inter-comparison of space geodetic techniques given that they share the same observability conditions in co-located sites. In this work, VLBI estimates of Earth orientation parameters (EOP), station coordinates and troposphere—zenith total delays (ZTD) and gradients—are compared to those estimated by means of Global Navigation Satellite Systems (GNSS) observations. We considered solutions from different software packages and processing techniques for this analysis, including all the available IVS and IGS (International GNSS Service) solutions and two VLBI series obtained by the authors. This extensive analysis provides a representative view of the inter-technique differences under the same observation conditions. We considered in the analysis the two VLBI legacy S/X networks that took part in the CONT17 campaign. We found that the EOP WRMS with respect to IGS final products is similar to previous CONT campaigns, even using global VLBI solutions that assimilate the data from both CONT17 legacy-1 and legacy-2 networks. Repeatabilities of estimated VLBI antenna coordinates of the legacy-1 network have a similar behaviour than GNSS-based repeatabilities in east and north components and slightly worse in up component whereas the repeatabilities of the legacy-2 network are smaller than legacy-1 network and similar to the IGS combined solution. Finally, troposphere inter-technique differences in terms of ZTD and gradients also show a similar agreement to different sources of GNSS-based troposphere estimates.
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Data Availability Statement
The datasets analysed in this study are freely available at IVS and IGS servers. VLBI series estimated by the authors and results of the analysis carried out can be made available by the corresponding author on request.
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Acknowledgements
We are grateful to all parties that contributed to the success of the CONT17 campaign, in particular to the IVS Coordinating Center at NASA Goddard Space Flight Center (GSFC) for taking the bulk of the organizational load, to the GSFC VLBI group for preparing the legacy S/X observing schedules and MIT Haystack Observatory for the VGOS observing schedules, to the IVS observing stations at Badary and Zelenchukskaya (both Institute for Applied Astronomy, IAA, St. Petersburg, Russia), Fortaleza (Rádio Observatório Espacial do Nordeste, ROEN; Center of Radio Astronomy and Astrophysics, Engineering School, Mackenzie Presbyterian University, Sao Paulo and Brazilian Instituto Nacional de Pesquisas Espaciais, INPE, Brazil), GGAO (MIT Haystack Observatory and NASA GSFC, USA), Hartebeesthoek (Hartebeesthoek Radio Astronomy Observatory, National Research Foundation, South Africa), the AuScope stations of Hobart, Katherine and Yarragadee (Geoscience Australia, University of Tasmania), Ishioka (Geospatial Information Authority of Japan), Kashima (National Institute of Information and Communications Technology, Japan), Kokee Park (U.S. Naval Observatory and NASA GSFC, USA), Matera (Agencia Spatiale Italiana, Italy), Medicina (Istituto di Radioastronomia, Italy), Ny Ålesund (Kartverket, Norway), Onsala (Onsala Space Observatory, Chalmers University of Technology, Sweden), Seshan (Shanghai Astronomical Observatory, China), Warkworth (Auckland University of Technology, New Zealand), Westford (MIT Haystack Observatory), Wettzell (Bundesamt für Kartographie und Geodäsie and Technische Universität München, Germany) and Yebes (Instituto Geográfico Nacional, Spain) plus the Very Long Baseline Array (VLBA) stations of the Long Baseline Observatory (LBO) for carrying out the observations under the US Naval Observatory’s time allocation, to the staff at the MPIfR/BKG Correlator Center, the VLBA Correlator at Socorro and the MIT Haystack Observatory Correlator for performing the correlations and the fringe fitting of the data, and to the IVS Data Centers at BKG (Leipzig, Germany), Observatoire de Paris (France) and NASA CDDIS (Greenbelt, MD, USA) for the central data holds. We wish to also thank the hard work of IGS contributors for providing high-quality data and products and the very valuable feedback provided by the three anonymous reviewers of this paper.
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VP designed the study, collected IVS and IGS series, performed the different comparisons and wrote the manuscript. EA and YGE participated in the analysis of VLBI series using VieVS and Where software packages. SGE provided support and reviewed the manuscript. All authors provided critical feedback and helped to shape the research and the manuscript.
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Puente, V., Azcue, E., Gomez-Espada, Y. et al. Comparison of common VLBI and GNSS estimates in CONT17 campaign. J Geod 95, 120 (2021). https://doi.org/10.1007/s00190-021-01565-x
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DOI: https://doi.org/10.1007/s00190-021-01565-x