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Optimal VLBI baseline geometry for UT1-UTC Intensive observations

One of the main tasks of Very Long Baseline Interferometry (VLBI) is the rapid determination of the highly variable Earth’s rotation expressed through the difference between Universal Time UT1 and Coordinated Universal Time UTC (dUT1). For this reason, dedicated one hour, single baseline sessions, c...

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Autores principales: Schartner, Matthias, Kern, Lisa, Nothnagel, Axel, Böhm, Johannes, Soja, Benedikt
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2021
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8550500/
https://www.ncbi.nlm.nih.gov/pubmed/34720450
http://dx.doi.org/10.1007/s00190-021-01530-8
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author Schartner, Matthias
Kern, Lisa
Nothnagel, Axel
Böhm, Johannes
Soja, Benedikt
author_facet Schartner, Matthias
Kern, Lisa
Nothnagel, Axel
Böhm, Johannes
Soja, Benedikt
author_sort Schartner, Matthias
collection PubMed
description One of the main tasks of Very Long Baseline Interferometry (VLBI) is the rapid determination of the highly variable Earth’s rotation expressed through the difference between Universal Time UT1 and Coordinated Universal Time UTC (dUT1). For this reason, dedicated one hour, single baseline sessions, called “Intensives”, are observed on a daily basis. Thus far, the optimal geometry of Intensive sessions was understood to include a long east–west extension of the baseline to ensure a dUT1 estimation with highest accuracy. In this publication, we prove that long east–west baselines are the best choice only for certain lengths and orientations. In this respect, optimal orientations may even require significant inclination of the baseline with respect to the equatorial plane. The basis of these findings is a simulation study with subsequent investigations in the partial derivatives of the observed group delays [Formula: see text] with respect to dUT1 [Formula: see text] . Almost 3000 baselines between artificial stations located on a regular [Formula: see text] degree grid are investigated to derive a global and generally valid picture about the best length and orientation of Intensive baselines. Our results reveal that especially equatorial baselines or baselines with a center close to the equatorial plane are not suited for Intensives although they provide a good east–west extension. This is explained by the narrow right ascension band of visible sources and the resulting lack of variety in the partial derivatives. Moreover, it is shown that north–south baselines are also capable of determining dUT1 with reasonable accuracy, given that the baseline orientation is significantly different from the Earth rotation axis. However, great care must be taken to provide accurate polar motion a priori information for these baselines. Finally, we provide a better metric to assess the suitability of Intensive baselines based on the effective spread of [Formula: see text] .
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spelling pubmed-85505002021-10-29 Optimal VLBI baseline geometry for UT1-UTC Intensive observations Schartner, Matthias Kern, Lisa Nothnagel, Axel Böhm, Johannes Soja, Benedikt J Geod Original Article One of the main tasks of Very Long Baseline Interferometry (VLBI) is the rapid determination of the highly variable Earth’s rotation expressed through the difference between Universal Time UT1 and Coordinated Universal Time UTC (dUT1). For this reason, dedicated one hour, single baseline sessions, called “Intensives”, are observed on a daily basis. Thus far, the optimal geometry of Intensive sessions was understood to include a long east–west extension of the baseline to ensure a dUT1 estimation with highest accuracy. In this publication, we prove that long east–west baselines are the best choice only for certain lengths and orientations. In this respect, optimal orientations may even require significant inclination of the baseline with respect to the equatorial plane. The basis of these findings is a simulation study with subsequent investigations in the partial derivatives of the observed group delays [Formula: see text] with respect to dUT1 [Formula: see text] . Almost 3000 baselines between artificial stations located on a regular [Formula: see text] degree grid are investigated to derive a global and generally valid picture about the best length and orientation of Intensive baselines. Our results reveal that especially equatorial baselines or baselines with a center close to the equatorial plane are not suited for Intensives although they provide a good east–west extension. This is explained by the narrow right ascension band of visible sources and the resulting lack of variety in the partial derivatives. Moreover, it is shown that north–south baselines are also capable of determining dUT1 with reasonable accuracy, given that the baseline orientation is significantly different from the Earth rotation axis. However, great care must be taken to provide accurate polar motion a priori information for these baselines. Finally, we provide a better metric to assess the suitability of Intensive baselines based on the effective spread of [Formula: see text] . Springer Berlin Heidelberg 2021-06-19 2021 /pmc/articles/PMC8550500/ /pubmed/34720450 http://dx.doi.org/10.1007/s00190-021-01530-8 Text en © The Author(s) 2021 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 Original Article
Schartner, Matthias
Kern, Lisa
Nothnagel, Axel
Böhm, Johannes
Soja, Benedikt
Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title_full Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title_fullStr Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title_full_unstemmed Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title_short Optimal VLBI baseline geometry for UT1-UTC Intensive observations
title_sort optimal vlbi baseline geometry for ut1-utc intensive observations
topic Original Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC8550500/
https://www.ncbi.nlm.nih.gov/pubmed/34720450
http://dx.doi.org/10.1007/s00190-021-01530-8
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