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Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination

The deviation of Universal Time from atomic time, expressed as UT1−UTC, reflects the irregularities of the Earth rotation speed and is key to precise geodetic applications which depend on the transformation between celestial and terrestrial reference frames. A rapidly varying quantity such as UT1−UT...

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Autores principales: Böhm, Sigrid, Böhm, Johannes, Gruber, Jakob, Kern, Lisa, McCallum, Jamie, McCallum, Lucia, McCarthy, Tiege, Quick, Jonathan, Schartner, Matthias
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9334372/
https://www.ncbi.nlm.nih.gov/pubmed/35915663
http://dx.doi.org/10.1186/s40623-022-01671-w
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author Böhm, Sigrid
Böhm, Johannes
Gruber, Jakob
Kern, Lisa
McCallum, Jamie
McCallum, Lucia
McCarthy, Tiege
Quick, Jonathan
Schartner, Matthias
author_facet Böhm, Sigrid
Böhm, Johannes
Gruber, Jakob
Kern, Lisa
McCallum, Jamie
McCallum, Lucia
McCarthy, Tiege
Quick, Jonathan
Schartner, Matthias
author_sort Böhm, Sigrid
collection PubMed
description The deviation of Universal Time from atomic time, expressed as UT1−UTC, reflects the irregularities of the Earth rotation speed and is key to precise geodetic applications which depend on the transformation between celestial and terrestrial reference frames. A rapidly varying quantity such as UT1−UTC demands observation scenarios enabling fast delivery of good results. These criteria are currently met only by the Very Long Baseline Interferometry (VLBI) Intensive sessions. Due to stringent requirements of a fast UT1−UTC turnaround, the observations are limited to a few baselines and a duration of one hour. Hence, the estimation of UT1−UTC from Intensives is liable to constraints and prone to errors introduced by inaccurate a priori information. One aspect in this context is that the regularly operated Intensive VLBI sessions organised by the International VLBI Service for Geodesy and Astrometry solely use stations in the northern hemisphere. Any potential systematic errors due to this northern hemisphere dominated geometry are so far unknown. Besides the general need for stimulating global geodetic measurements with southern observatories, this served as a powerful motivation to launch the SI (Southern Intensive) program in 2020. The SI sessions are observed using three VLBI antennas in the southern hemisphere: Ht (South Africa), Hb (Tasmania) and Yg (Western Australia). On the basis of UT1−UTC results from 53 sessions observed throughout 2020 and 2021, we demonstrate the competitiveness of the SI with routinely operated Intensive sessions in terms of operations and UT1−UTC accuracy. The UT1−UTC values of the SI reach an average agreement of 32 µs in terms of weighted standard deviation when compared with the conventional Intensives results of five independent analysis centers and of 27 µs compared with the 14C04 series. The mean scatter of all solutions of the considered northern hemisphere Intensives with respect to C04 is at a comparable level of 29 µs. The quality of the results is only slightly degraded if just the baseline HtHb is evaluated. In combination with the e-transfer capabilities from Ht to Hb, this facilitates continuation of the SI by ensuring rapid service UT1−UTC provision. GRAPHICAL ABSTRACT: [Image: see text]
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spelling pubmed-93343722022-07-30 Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination Böhm, Sigrid Böhm, Johannes Gruber, Jakob Kern, Lisa McCallum, Jamie McCallum, Lucia McCarthy, Tiege Quick, Jonathan Schartner, Matthias Earth Planets Space Full Paper The deviation of Universal Time from atomic time, expressed as UT1−UTC, reflects the irregularities of the Earth rotation speed and is key to precise geodetic applications which depend on the transformation between celestial and terrestrial reference frames. A rapidly varying quantity such as UT1−UTC demands observation scenarios enabling fast delivery of good results. These criteria are currently met only by the Very Long Baseline Interferometry (VLBI) Intensive sessions. Due to stringent requirements of a fast UT1−UTC turnaround, the observations are limited to a few baselines and a duration of one hour. Hence, the estimation of UT1−UTC from Intensives is liable to constraints and prone to errors introduced by inaccurate a priori information. One aspect in this context is that the regularly operated Intensive VLBI sessions organised by the International VLBI Service for Geodesy and Astrometry solely use stations in the northern hemisphere. Any potential systematic errors due to this northern hemisphere dominated geometry are so far unknown. Besides the general need for stimulating global geodetic measurements with southern observatories, this served as a powerful motivation to launch the SI (Southern Intensive) program in 2020. The SI sessions are observed using three VLBI antennas in the southern hemisphere: Ht (South Africa), Hb (Tasmania) and Yg (Western Australia). On the basis of UT1−UTC results from 53 sessions observed throughout 2020 and 2021, we demonstrate the competitiveness of the SI with routinely operated Intensive sessions in terms of operations and UT1−UTC accuracy. The UT1−UTC values of the SI reach an average agreement of 32 µs in terms of weighted standard deviation when compared with the conventional Intensives results of five independent analysis centers and of 27 µs compared with the 14C04 series. The mean scatter of all solutions of the considered northern hemisphere Intensives with respect to C04 is at a comparable level of 29 µs. The quality of the results is only slightly degraded if just the baseline HtHb is evaluated. In combination with the e-transfer capabilities from Ht to Hb, this facilitates continuation of the SI by ensuring rapid service UT1−UTC provision. GRAPHICAL ABSTRACT: [Image: see text] Springer Berlin Heidelberg 2022-07-28 2022 /pmc/articles/PMC9334372/ /pubmed/35915663 http://dx.doi.org/10.1186/s40623-022-01671-w Text en © The Author(s) 2022 https://creativecommons.org/licenses/by/4.0/Open AccessThis article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article's Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article's Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4.0/ (https://creativecommons.org/licenses/by/4.0/) .
spellingShingle Full Paper
Böhm, Sigrid
Böhm, Johannes
Gruber, Jakob
Kern, Lisa
McCallum, Jamie
McCallum, Lucia
McCarthy, Tiege
Quick, Jonathan
Schartner, Matthias
Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title_full Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title_fullStr Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title_full_unstemmed Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title_short Probing a southern hemisphere VLBI Intensive baseline configuration for UT1 determination
title_sort probing a southern hemisphere vlbi intensive baseline configuration for ut1 determination
topic Full Paper
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9334372/
https://www.ncbi.nlm.nih.gov/pubmed/35915663
http://dx.doi.org/10.1186/s40623-022-01671-w
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