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The Australian mixed-mode observing program

Global geodetic VLBI is upgrading to its next-generation observing system, VGOS. This upgrade has turned out to be a process over multiple years, until VGOS reaches its full capabilities with the envisaged continuous observations. Until then, for the Australian stations, the upgrade means ceasing th...

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Autores principales: McCallum, Lucia, Chin Chuan, Lim, Krásná, Hana, McCallum, Jamie, Böhm, Johannes, McCarthy, Tiege, Gruber, Jakob, Schartner, Matthias, Quick, Jonathan, Rogers, Axl
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Springer Berlin Heidelberg 2022
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9515051/
https://www.ncbi.nlm.nih.gov/pubmed/36188100
http://dx.doi.org/10.1007/s00190-022-01657-2
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author McCallum, Lucia
Chin Chuan, Lim
Krásná, Hana
McCallum, Jamie
Böhm, Johannes
McCarthy, Tiege
Gruber, Jakob
Schartner, Matthias
Quick, Jonathan
Rogers, Axl
author_facet McCallum, Lucia
Chin Chuan, Lim
Krásná, Hana
McCallum, Jamie
Böhm, Johannes
McCarthy, Tiege
Gruber, Jakob
Schartner, Matthias
Quick, Jonathan
Rogers, Axl
author_sort McCallum, Lucia
collection PubMed
description Global geodetic VLBI is upgrading to its next-generation observing system, VGOS. This upgrade has turned out to be a process over multiple years, until VGOS reaches its full capabilities with the envisaged continuous observations. Until then, for the Australian stations, the upgrade means ceasing their legacy S/X observations, leaving a large gap in the global network as well as in the station time series. The Australian mixed-mode observing program is a series of sessions where the VGOS stations in Hobart and Katherine observe legacy S/X VLBI together with other stations in the region. This paper describes the technical details of these observations and their processing strategies and discusses their suitability for geodetic results by comparison with those of standard legacy S/X sessions. The presented mixed-mode sessions allow a continuation of the station time series, a benefit for the stations themselves as well as for future realisations of the terrestrial and celestial reference frames. A novel mode of observing is introduced and tested. The results are promising and it is suggested for acceptance into standard legacy S/X IVS observations, overcoming current gaps in the network due to VGOS upgrades and preventing a worsening of global results otherwise.
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spelling pubmed-95150512022-09-29 The Australian mixed-mode observing program McCallum, Lucia Chin Chuan, Lim Krásná, Hana McCallum, Jamie Böhm, Johannes McCarthy, Tiege Gruber, Jakob Schartner, Matthias Quick, Jonathan Rogers, Axl J Geod Original Article Global geodetic VLBI is upgrading to its next-generation observing system, VGOS. This upgrade has turned out to be a process over multiple years, until VGOS reaches its full capabilities with the envisaged continuous observations. Until then, for the Australian stations, the upgrade means ceasing their legacy S/X observations, leaving a large gap in the global network as well as in the station time series. The Australian mixed-mode observing program is a series of sessions where the VGOS stations in Hobart and Katherine observe legacy S/X VLBI together with other stations in the region. This paper describes the technical details of these observations and their processing strategies and discusses their suitability for geodetic results by comparison with those of standard legacy S/X sessions. The presented mixed-mode sessions allow a continuation of the station time series, a benefit for the stations themselves as well as for future realisations of the terrestrial and celestial reference frames. A novel mode of observing is introduced and tested. The results are promising and it is suggested for acceptance into standard legacy S/X IVS observations, overcoming current gaps in the network due to VGOS upgrades and preventing a worsening of global results otherwise. Springer Berlin Heidelberg 2022-09-27 2022 /pmc/articles/PMC9515051/ /pubmed/36188100 http://dx.doi.org/10.1007/s00190-022-01657-2 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 Original Article
McCallum, Lucia
Chin Chuan, Lim
Krásná, Hana
McCallum, Jamie
Böhm, Johannes
McCarthy, Tiege
Gruber, Jakob
Schartner, Matthias
Quick, Jonathan
Rogers, Axl
The Australian mixed-mode observing program
title The Australian mixed-mode observing program
title_full The Australian mixed-mode observing program
title_fullStr The Australian mixed-mode observing program
title_full_unstemmed The Australian mixed-mode observing program
title_short The Australian mixed-mode observing program
title_sort australian mixed-mode observing program
topic Original Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC9515051/
https://www.ncbi.nlm.nih.gov/pubmed/36188100
http://dx.doi.org/10.1007/s00190-022-01657-2
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