Analysis of analytical attitude propagators for spin-stabilized satellites

Bibliographic Details
Main Author: Zanardi, M. C.
Publication Date: 2018
Other Authors: Celestino, C. C., Borderes Motta, G. [UNESP], Franca, E. M., Garcia, R. V.
Format: Article
Language: eng
Source: Repositório Institucional da UNESP
Download full: http://dx.doi.org/10.1007/s40314-018-0644-0
http://hdl.handle.net/11449/184260
Summary: In this paper, analytical attitude propagators for spin-stabilized satellites are analyzed. For this purpose, external torques are introduced in the motion equations such as solar radiation pressure torque, aerodynamic torque, gravity gradient torque, and magnetic residual and eddy current torques. For the magnetic torques, it used both the dipole and quadripole Earth's magnetic field models. The obtained analytical solution is applied and compared with actual data for Brazilian data collection satellites SCD1 and SCD2. The results, when a daily data update is applied, based on the INPE-Brazilian Institute for Space Research supplied data, show a good agreement of all involved parameters with the actual deviations in the parameter values within the precision required for the satellite mission. This permits to conclude that the used theory is suitable for the studied problem. Thus, the propagators presented in this work can be applied to predict the rotational motion of spin-stabilized artificial satellites, particularly for SCD1 and SCD2 satellites over the considered time period.
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spelling Analysis of analytical attitude propagators for spin-stabilized satellitesAnalytical propagatorsSpin-stabilized satellitesEnvironmental torquesIn this paper, analytical attitude propagators for spin-stabilized satellites are analyzed. For this purpose, external torques are introduced in the motion equations such as solar radiation pressure torque, aerodynamic torque, gravity gradient torque, and magnetic residual and eddy current torques. For the magnetic torques, it used both the dipole and quadripole Earth's magnetic field models. The obtained analytical solution is applied and compared with actual data for Brazilian data collection satellites SCD1 and SCD2. The results, when a daily data update is applied, based on the INPE-Brazilian Institute for Space Research supplied data, show a good agreement of all involved parameters with the actual deviations in the parameter values within the precision required for the satellite mission. This permits to conclude that the used theory is suitable for the studied problem. Thus, the propagators presented in this work can be applied to predict the rotational motion of spin-stabilized artificial satellites, particularly for SCD1 and SCD2 satellites over the considered time period.Coordenação de Aperfeiçoamento de Pessoal de Nível Superior (CAPES)Conselho Nacional de Desenvolvimento Científico e Tecnológico (CNPq)Fed Univ ABC, Ave Estados 5001, BR-09210580 Santo Andre, SP, BrazilSao Paulo State Univ, Ave Dr Ariberto Pereia da Cunha 333, BR-12516410 Guaratingueta, SP, BrazilUniv Sao Paulo, EEL, Est Municipal Campinho S-N, BR-12602810 Lorena, SP, BrazilSao Paulo State Univ, Ave Dr Ariberto Pereia da Cunha 333, BR-12516410 Guaratingueta, SP, BrazilCNPq: 421672/2016-1SpringerFed Univ ABCUniversidade Estadual Paulista (Unesp)Universidade de São Paulo (USP)Zanardi, M. C.Celestino, C. C.Borderes Motta, G. [UNESP]Franca, E. M.Garcia, R. V.2019-10-04T11:56:19Z2019-10-04T11:56:19Z2018-12-01info:eu-repo/semantics/publishedVersioninfo:eu-repo/semantics/article96-109http://dx.doi.org/10.1007/s40314-018-0644-0Computational & Applied Mathematics. Heidelberg: Springer Heidelberg, v. 37, p. 96-109, 2018.0101-8205http://hdl.handle.net/11449/18426010.1007/s40314-018-0644-0WOS:000455228900009Web of Sciencereponame:Repositório Institucional da UNESPinstname:Universidade Estadual Paulista (UNESP)instacron:UNESPengComputational & Applied Mathematicsinfo:eu-repo/semantics/openAccess2021-10-23T19:02:20Zoai:repositorio.unesp.br:11449/184260Repositório InstitucionalPUBhttp://repositorio.unesp.br/oai/requestopendoar:29462021-10-23T19:02:20Repositório Institucional da UNESP - Universidade Estadual Paulista (UNESP)false
dc.title.none.fl_str_mv Analysis of analytical attitude propagators for spin-stabilized satellites
title Analysis of analytical attitude propagators for spin-stabilized satellites
spellingShingle Analysis of analytical attitude propagators for spin-stabilized satellites
Zanardi, M. C.
Analytical propagators
Spin-stabilized satellites
Environmental torques
title_short Analysis of analytical attitude propagators for spin-stabilized satellites
title_full Analysis of analytical attitude propagators for spin-stabilized satellites
title_fullStr Analysis of analytical attitude propagators for spin-stabilized satellites
title_full_unstemmed Analysis of analytical attitude propagators for spin-stabilized satellites
title_sort Analysis of analytical attitude propagators for spin-stabilized satellites
author Zanardi, M. C.
author_facet Zanardi, M. C.
Celestino, C. C.
Borderes Motta, G. [UNESP]
Franca, E. M.
Garcia, R. V.
author_role author
author2 Celestino, C. C.
Borderes Motta, G. [UNESP]
Franca, E. M.
Garcia, R. V.
author2_role author
author
author
author
dc.contributor.none.fl_str_mv Fed Univ ABC
Universidade Estadual Paulista (Unesp)
Universidade de São Paulo (USP)
dc.contributor.author.fl_str_mv Zanardi, M. C.
Celestino, C. C.
Borderes Motta, G. [UNESP]
Franca, E. M.
Garcia, R. V.
dc.subject.por.fl_str_mv Analytical propagators
Spin-stabilized satellites
Environmental torques
topic Analytical propagators
Spin-stabilized satellites
Environmental torques
description In this paper, analytical attitude propagators for spin-stabilized satellites are analyzed. For this purpose, external torques are introduced in the motion equations such as solar radiation pressure torque, aerodynamic torque, gravity gradient torque, and magnetic residual and eddy current torques. For the magnetic torques, it used both the dipole and quadripole Earth's magnetic field models. The obtained analytical solution is applied and compared with actual data for Brazilian data collection satellites SCD1 and SCD2. The results, when a daily data update is applied, based on the INPE-Brazilian Institute for Space Research supplied data, show a good agreement of all involved parameters with the actual deviations in the parameter values within the precision required for the satellite mission. This permits to conclude that the used theory is suitable for the studied problem. Thus, the propagators presented in this work can be applied to predict the rotational motion of spin-stabilized artificial satellites, particularly for SCD1 and SCD2 satellites over the considered time period.
publishDate 2018
dc.date.none.fl_str_mv 2018-12-01
2019-10-04T11:56:19Z
2019-10-04T11:56:19Z
dc.type.status.fl_str_mv info:eu-repo/semantics/publishedVersion
dc.type.driver.fl_str_mv info:eu-repo/semantics/article
format article
status_str publishedVersion
dc.identifier.uri.fl_str_mv http://dx.doi.org/10.1007/s40314-018-0644-0
Computational & Applied Mathematics. Heidelberg: Springer Heidelberg, v. 37, p. 96-109, 2018.
0101-8205
http://hdl.handle.net/11449/184260
10.1007/s40314-018-0644-0
WOS:000455228900009
url http://dx.doi.org/10.1007/s40314-018-0644-0
http://hdl.handle.net/11449/184260
identifier_str_mv Computational & Applied Mathematics. Heidelberg: Springer Heidelberg, v. 37, p. 96-109, 2018.
0101-8205
10.1007/s40314-018-0644-0
WOS:000455228900009
dc.language.iso.fl_str_mv eng
language eng
dc.relation.none.fl_str_mv Computational & Applied Mathematics
dc.rights.driver.fl_str_mv info:eu-repo/semantics/openAccess
eu_rights_str_mv openAccess
dc.format.none.fl_str_mv 96-109
dc.publisher.none.fl_str_mv Springer
publisher.none.fl_str_mv Springer
dc.source.none.fl_str_mv Web of Science
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)
repository.mail.fl_str_mv
_version_ 1799965092600610816