Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure

Detalhes bibliográficos
Autor(a) principal: Moraes, Rodolpho Vilhena De [UNESP]
Data de Publicação: 2008
Outros Autores: Raimundo, Paula Cristiane P., Kuga, Helio K.
Tipo de documento: Artigo de conferência
Idioma: eng
Título da fonte: Repositório Institucional da UNESP
Texto Completo: http://hdl.handle.net/11449/231859
Resumo: The main target here is to determine the orbit of an artificial satellite, using signals of the GPS constellation and least squares algorithms implemented through sequential Givens rotations as a method of estimation, with the aim of improving the performance of the orbit estimation process and, at the same time, minimizing the computational procedure cost. Geopotential perturbations up to high order and direct solar radiation pressure were taken into account. It was also considered the position of the GPS antenna on the satellite body that, lately, consists of the influence of the satellite attitude motion in the orbit determination process. An application has been done, using real data from the Topex/Poseidon satellite, whose ephemeris is available at Internet. The best accuracy obtained in position was smaller than 5 meters for short period (2 hours) and smaller than 28 meters for long period (24 hours) orbit determination. In both cases, the perturbations mentioned before were taken into consideration and the analysis occurred without selective availability on the signals measurements.
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spelling Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressureThe main target here is to determine the orbit of an artificial satellite, using signals of the GPS constellation and least squares algorithms implemented through sequential Givens rotations as a method of estimation, with the aim of improving the performance of the orbit estimation process and, at the same time, minimizing the computational procedure cost. Geopotential perturbations up to high order and direct solar radiation pressure were taken into account. It was also considered the position of the GPS antenna on the satellite body that, lately, consists of the influence of the satellite attitude motion in the orbit determination process. An application has been done, using real data from the Topex/Poseidon satellite, whose ephemeris is available at Internet. The best accuracy obtained in position was smaller than 5 meters for short period (2 hours) and smaller than 28 meters for long period (24 hours) orbit determination. In both cases, the perturbations mentioned before were taken into consideration and the analysis occurred without selective availability on the signals measurements.UNESP, Guaratingueta - SPINPE - Sao Jose dos Campos, SPUNESP, Guaratingueta - SPUniversidade Estadual Paulista (UNESP)INPE - Sao Jose dos CamposMoraes, Rodolpho Vilhena De [UNESP]Raimundo, Paula Cristiane P.Kuga, Helio K.2022-04-29T08:47:50Z2022-04-29T08:47:50Z2008-12-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/conferenceObject923-933Advances in the Astronautical Sciences, v. 130 PART 1, p. 923-933.0065-3438http://hdl.handle.net/11449/2318592-s2.0-60349098949Scopusreponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengAdvances in the Astronautical Sciencesinfo:eu-repo/semantics/openAccess2022-04-29T08:47:50Zoai:repositorio.unesp.br:11449/231859Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462022-04-29T08:47:50Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
title Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
spellingShingle Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
Moraes, Rodolpho Vilhena De [UNESP]
title_short Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
title_full Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
title_fullStr Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
title_full_unstemmed Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
title_sort Orbit determination using gps including perturbations due to geopotential coefficients of high degree and order and solar radiation pressure
author Moraes, Rodolpho Vilhena De [UNESP]
author_facet Moraes, Rodolpho Vilhena De [UNESP]
Raimundo, Paula Cristiane P.
Kuga, Helio K.
author_role author
author2 Raimundo, Paula Cristiane P.
Kuga, Helio K.
author2_role author
author
dc.contributor.none.fl_str_mv Universidade Estadual Paulista (UNESP)
INPE - Sao Jose dos Campos
dc.contributor.author.fl_str_mv Moraes, Rodolpho Vilhena De [UNESP]
Raimundo, Paula Cristiane P.
Kuga, Helio K.
description The main target here is to determine the orbit of an artificial satellite, using signals of the GPS constellation and least squares algorithms implemented through sequential Givens rotations as a method of estimation, with the aim of improving the performance of the orbit estimation process and, at the same time, minimizing the computational procedure cost. Geopotential perturbations up to high order and direct solar radiation pressure were taken into account. It was also considered the position of the GPS antenna on the satellite body that, lately, consists of the influence of the satellite attitude motion in the orbit determination process. An application has been done, using real data from the Topex/Poseidon satellite, whose ephemeris is available at Internet. The best accuracy obtained in position was smaller than 5 meters for short period (2 hours) and smaller than 28 meters for long period (24 hours) orbit determination. In both cases, the perturbations mentioned before were taken into consideration and the analysis occurred without selective availability on the signals measurements.
publishDate 2008
dc.date.none.fl_str_mv 2008-12-01
2022-04-29T08:47:50Z
2022-04-29T08:47:50Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/conferenceObject
format conferenceObject
status_str publishedVersion
dc.identifier.uri.fl_str_mv Advances in the Astronautical Sciences, v. 130 PART 1, p. 923-933.
0065-3438
http://hdl.handle.net/11449/231859
2-s2.0-60349098949
identifier_str_mv Advances in the Astronautical Sciences, v. 130 PART 1, p. 923-933.
0065-3438
2-s2.0-60349098949
url http://hdl.handle.net/11449/231859
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Advances in the Astronautical Sciences
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eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 923-933
dc.source.none.fl_str_mv Scopus
reponame:Repositório Institucional da UNESP
instname:Universidade Estadual Paulista (UNESP)
instacron:UNESP
instname_str Universidade Estadual Paulista (UNESP)
instacron_str UNESP
institution UNESP
reponame_str Repositório Institucional da UNESP
collection Repositório Institucional da UNESP
repository.name.fl_str_mv Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)
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