<div class="csl-bib-body">
<div class="csl-entry">Schartner, M., Böhm, J., & Nothnagel, A. (2020). Optimal antenna locations of the VLBI Global Observing System for the estimation of Earth orientation parameters. <i>EARTH PLANETS AND SPACE</i>, <i>72</i>(87). https://doi.org/10.1186/s40623-020-01214-1</div>
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dc.identifier.issn
1880-5981
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dc.identifier.uri
http://hdl.handle.net/20.500.12708/141812
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dc.description.abstract
To support monitoring subtle effects in the Earth system such as a mean sea level rise of 3 mm/year, a next-gener-ation VLBI system, the VLBI Global Observing System (VGOS), has been developed and a new VGOS station network is being built. However, the geometry of the current VGOS network and its planned extension suffer from a lack of stations in the southern hemisphere. In this investigation, we identify optimal locations for additional VGOS radio telescopes with a new method based on bulk observing schedule generation and subsequent large-scale Monte-Carlo simulations. The location of the additional station is varied over 477 possible locations, homogeneously distrib-uted over land areas on the globe. For each antenna location, several schedules have been generated and simulated to minimize the effects of scheduling and the randomness of simulations. Thereby, it is possible to judge, in which regions an additional VGOS station would have the biggest impact on the precision of the estimated geodetic param-eters, in our case assessed by the repeatabilities of the estimated Earth orientation parameters (EOPs). To generate highly optimized schedules and to remove effects due to non-optimized scheduling, a total of 93 thousand schedules were iteratively generated, investigating over 300 billion scans and 2.4 trillion observations. Each schedule was further simulated 1000 times, leading to over 5 trillion simulated and analyzed observations. Although the optimum location of a future VLBI station depends on the EOP of interest and the geometry of the existing network, it is shown that the more the VGOS network grows, the more the lack of southern stations becomes prominent. The best location for an additional VGOS station for most EOP components and especially in the case of future VGOS networks would be the southern part of South America. It is further shown that the location of the additional antenna highly determines the expectable precision of the EOP estimates. For a 6-station network, the location of an additional seventh antenna can improve the precision of the EOP by a factor of 2.4 to 3.8. For an 18-station network, the location of an additional 19th station still improves the repeatability by a factor of 1.6. It is also found that adding a station at some locations will not improve the precision at all.
en
dc.language.iso
en
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dc.publisher
SPRINGER
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dc.relation.ispartof
EARTH PLANETS AND SPACE
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dc.subject
VieSched++
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dc.subject
Space and Planetary Science
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dc.subject
Geology
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dc.subject
VLBI Global Observing System (VGOS)
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dc.subject
Very Long Baseline Interferometry (VLBI)
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dc.subject
Global Geodetic Observing System (GGOS)
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dc.subject
Vienna VLBI and Satellite Software (VieVS)
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dc.title
Optimal antenna locations of the VLBI Global Observing System for the estimation of Earth orientation parameters
en
dc.type
Artikel
de
dc.type
Article
en
dc.type.category
Original Research Article
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tuw.container.volume
72
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tuw.container.issue
87
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tuw.journal.peerreviewed
true
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tuw.peerreviewed
true
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tuw.researchTopic.id
X1
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tuw.researchTopic.id
C5
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tuw.researchTopic.id
C4
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tuw.researchTopic.name
außerhalb der gesamtuniversitären Forschungsschwerpunkte