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Analytical attitude prediction of spin stabilized spacecrafts perturbed by magnetic residual torque

dc.contributor.authorZanardi, M. C.
dc.contributor.authorQuirelli, IMP
dc.contributor.authorKuga, H. K.
dc.contributor.institutionUniversidade Estadual Paulista (Unesp)
dc.contributor.institutionInstituto Nacional de Pesquisas Espaciais (INPE)
dc.date.accessioned2014-05-20T13:27:57Z
dc.date.available2014-05-20T13:27:57Z
dc.date.issued2005-01-01
dc.description.abstractAn analytical approach for spin-stabilized spacecraft attitude prediction is presented for the influence of the residual magnetic torques. Assuming an inclined dipole model for the Earth's magnetic field, an analytical averaging method is applied to obtain the mean residual torque every orbital period. The orbit mean anomaly is utilized to compute the average components of residual torque in the spacecraft body frame reference system. The theory is developed for time variations in the orbital elements, and non-circular orbits, giving rise to many curvature integrals. It is observed that the residual magnetic torque does not have component along the spin axis. The inclusion of this torque on the rotational motion differential equations of a spin stabilized spacecraft yields conditions to derive an analytical solution. The solution shows that residual torque does not affect the spin velocity magnitude, contributing only for the precession and the drift of the spin axis of the spacecraft. (c) 2005 COSPAR. Published by Elsevier Ltd. All rights reserved.en
dc.description.affiliationUNESP, FEG, Dept Math, Grp Orbital Dynam & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.description.affiliationBrazilian Inst Space Res, INPE, BR-12221970 Sao Jose Dos Campos, SP, Brazil
dc.description.affiliationUnespUNESP, FEG, Dept Math, Grp Orbital Dynam & Planetol, BR-12516410 Guaratingueta, SP, Brazil
dc.format.extent460-465
dc.identifierhttp://dx.doi.org/10.1016/j.asr.2005.07.020
dc.identifier.citationSatellite Dynamics In the Era of Intredisciplinary Space Geodesy. Oxford: Elsevier B.V. Ltd, v. 36, n. 3, p. 460-465, 2005.
dc.identifier.doi10.1016/j.asr.2005.07.020
dc.identifier.issn0273-1177
dc.identifier.urihttp://hdl.handle.net/11449/9269
dc.identifier.wosWOS:000235247800019
dc.language.isoeng
dc.publisherElsevier B.V.
dc.relation.ispartofSatellite Dynamics In the Era of Intredisciplinary Space Geodesy
dc.relation.ispartofjcr1.529
dc.relation.ispartofsjr0,569
dc.rights.accessRightsAcesso restrito
dc.sourceWeb of Science
dc.subjectattitude propagationpt
dc.subjectspin stabilized satellitept
dc.subjectresidual magnetic torquept
dc.subjectgeomagnetic fieldpt
dc.titleAnalytical attitude prediction of spin stabilized spacecrafts perturbed by magnetic residual torqueen
dc.typeArtigo
dcterms.licensehttp://www.elsevier.com/about/open-access/open-access-policies/article-posting-policy
dcterms.rightsHolderElsevier B.V.
dspace.entity.typePublication
unesp.campusUniversidade Estadual Paulista (UNESP), Faculdade de Engenharia, Guaratinguetápt
unesp.departmentMatemática - FEGpt

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