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Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations

This paper deals with the analysis of local Love and Shida numbers (parameters h(2) and l(2)) values of the Australian Yarragadee and Mount Stromlo satellite laser ranging (SLR) stations. The research was conducted based on data from the Medium Earth Orbit (MEO) satellites, LAGEOS-1 and LAGEOS-2, an...

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Autores principales: Jagoda, Marcin, Rutkowska, Miłosława, Lejba, Paweł, Katzer, Jacek, Obuchovski, Romuald, Šlikas, Dominykas
Formato: Online Artículo Texto
Lenguaje:English
Publicado: MDPI 2020
Materias:
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7730351/
https://www.ncbi.nlm.nih.gov/pubmed/33266091
http://dx.doi.org/10.3390/s20236851
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author Jagoda, Marcin
Rutkowska, Miłosława
Lejba, Paweł
Katzer, Jacek
Obuchovski, Romuald
Šlikas, Dominykas
author_facet Jagoda, Marcin
Rutkowska, Miłosława
Lejba, Paweł
Katzer, Jacek
Obuchovski, Romuald
Šlikas, Dominykas
author_sort Jagoda, Marcin
collection PubMed
description This paper deals with the analysis of local Love and Shida numbers (parameters h(2) and l(2)) values of the Australian Yarragadee and Mount Stromlo satellite laser ranging (SLR) stations. The research was conducted based on data from the Medium Earth Orbit (MEO) satellites, LAGEOS-1 and LAGEOS-2, and Low Earth Orbit (LEO) satellites, STELLA and STARLETTE. Data from a 60-month time interval, from 01.01.2014 to 01.01.2019, was used. In the first research stage, the Love and Shida numbers values were determined separately from observations of each satellite; the obtained values of h(2), l(2) exhibit a high degree of compliance, and the differences do not exceed formal error values. At this stage, we found that it was not possible to determine l(2) from the data of STELLA and STARLETTE. In the second research stage, we combined the satellite observations of MEO (LAGEOS-1+LAGEOS-2) and LEO (STELLA+STARLETTE) and redefined the h(2), l(2) parameters. The final values were adopted, and further analyses were made based on the values obtained from the combined observations. For the Yarragadee station, local h(2) = 0.5756 ± 0.0005 and l(2) = 0.0751 ± 0.0002 values were obtained from LAGEOS-1 + LAGEOS-2 and h(2) = 0.5742 ± 0.0015 were obtained from STELLA+STARLETTE data. For the Mount Stromlo station, we obtained the local h(2) = 0.5601 ± 0.0006 and l(2) = 0.0637 ± 0.0003 values from LAGEOS-1+LAGEOS-2 and h(2) = 0.5618 ± 0.0017 from STELLA + STARLETTE. We found discrepancies between the local parameters determined for the Yarragadee and Mount Stromlo stations and the commonly used values of the h(2), l(2) parameters averaged for the whole Earth (so-called global nominal parameters). The sequential equalization method was used for the analysis, which allowed to determine the minimum time interval necessary to obtain stable h(2), l(2) values. It turned out to be about 50 months. Additionally, we investigated the impact of the use of local values of the Love/Shida numbers on the determination of the Yarragadee and Mount Stromlo station coordinates. We proposed to determine the stations (X, Y, Z) coordinates in International Terrestrial Reference Frame 2014 (ITRF2014) in two computational versions: using global nominal h(2), l(2) values and local h(2), l(2) values calculated during this research. We found that the use of the local values of the h(2), l(2) parameters in the process of determining the stations coordinates influences the result.
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spelling pubmed-77303512020-12-12 Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations Jagoda, Marcin Rutkowska, Miłosława Lejba, Paweł Katzer, Jacek Obuchovski, Romuald Šlikas, Dominykas Sensors (Basel) Article This paper deals with the analysis of local Love and Shida numbers (parameters h(2) and l(2)) values of the Australian Yarragadee and Mount Stromlo satellite laser ranging (SLR) stations. The research was conducted based on data from the Medium Earth Orbit (MEO) satellites, LAGEOS-1 and LAGEOS-2, and Low Earth Orbit (LEO) satellites, STELLA and STARLETTE. Data from a 60-month time interval, from 01.01.2014 to 01.01.2019, was used. In the first research stage, the Love and Shida numbers values were determined separately from observations of each satellite; the obtained values of h(2), l(2) exhibit a high degree of compliance, and the differences do not exceed formal error values. At this stage, we found that it was not possible to determine l(2) from the data of STELLA and STARLETTE. In the second research stage, we combined the satellite observations of MEO (LAGEOS-1+LAGEOS-2) and LEO (STELLA+STARLETTE) and redefined the h(2), l(2) parameters. The final values were adopted, and further analyses were made based on the values obtained from the combined observations. For the Yarragadee station, local h(2) = 0.5756 ± 0.0005 and l(2) = 0.0751 ± 0.0002 values were obtained from LAGEOS-1 + LAGEOS-2 and h(2) = 0.5742 ± 0.0015 were obtained from STELLA+STARLETTE data. For the Mount Stromlo station, we obtained the local h(2) = 0.5601 ± 0.0006 and l(2) = 0.0637 ± 0.0003 values from LAGEOS-1+LAGEOS-2 and h(2) = 0.5618 ± 0.0017 from STELLA + STARLETTE. We found discrepancies between the local parameters determined for the Yarragadee and Mount Stromlo stations and the commonly used values of the h(2), l(2) parameters averaged for the whole Earth (so-called global nominal parameters). The sequential equalization method was used for the analysis, which allowed to determine the minimum time interval necessary to obtain stable h(2), l(2) values. It turned out to be about 50 months. Additionally, we investigated the impact of the use of local values of the Love/Shida numbers on the determination of the Yarragadee and Mount Stromlo station coordinates. We proposed to determine the stations (X, Y, Z) coordinates in International Terrestrial Reference Frame 2014 (ITRF2014) in two computational versions: using global nominal h(2), l(2) values and local h(2), l(2) values calculated during this research. We found that the use of the local values of the h(2), l(2) parameters in the process of determining the stations coordinates influences the result. MDPI 2020-11-30 /pmc/articles/PMC7730351/ /pubmed/33266091 http://dx.doi.org/10.3390/s20236851 Text en © 2020 by the authors. Licensee MDPI, Basel, Switzerland. This article is an open access article distributed under the terms and conditions of the Creative Commons Attribution (CC BY) license (http://creativecommons.org/licenses/by/4.0/).
spellingShingle Article
Jagoda, Marcin
Rutkowska, Miłosława
Lejba, Paweł
Katzer, Jacek
Obuchovski, Romuald
Šlikas, Dominykas
Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title_full Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title_fullStr Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title_full_unstemmed Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title_short Satellite Laser Ranging for Retrieval of the Local Values of the Love h(2) and Shida l(2) Numbers for the Australian ILRS Stations
title_sort satellite laser ranging for retrieval of the local values of the love h(2) and shida l(2) numbers for the australian ilrs stations
topic Article
url https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7730351/
https://www.ncbi.nlm.nih.gov/pubmed/33266091
http://dx.doi.org/10.3390/s20236851
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