dc.contributorNational Institute for Space Research
dc.contributorUniversidade Estadual Paulista (Unesp)
dc.date.accessioned2018-12-11T16:50:37Z
dc.date.available2018-12-11T16:50:37Z
dc.date.created2018-12-11T16:50:37Z
dc.date.issued2017-10-25
dc.identifierJournal of Physics: Conference Series, v. 911, n. 1, 2017.
dc.identifier1742-6596
dc.identifier1742-6588
dc.identifierhttp://hdl.handle.net/11449/170396
dc.identifier10.1088/1742-6596/911/1/012013
dc.identifier2-s2.0-85034624638
dc.identifier2-s2.0-85034624638.pdf
dc.description.abstractThis paper presents a study about the tetrahedral layout of four satellites in a way that every half-orbital period this set groups together while flying in formation. The formation is calculated analyzing the problem from a geometrical perspective and disposed by precisely adjusting the orbital parameters of each satellite. The dynamic modelling considers the orbital motion equations. The results are analyzed, compared and discussed. A detection algorithm is used as flag to signal the regular tetrahedron's exact moments of occurrence. To do so, the volume calculated during the simulation is compared to the real volume, based on the initial conditions of the exact moment of formation and respecting a tolerance. This tolerance value is stablished arbitrarily depending on the mission and the formation's geometrical parameters. The simulations will run on a computational environment.
dc.languageeng
dc.relationJournal of Physics: Conference Series
dc.relation0,241
dc.relation0,241
dc.rightsAcesso aberto
dc.sourceScopus
dc.titleRelative Positioning Evaluation of a Tetrahedral Flight Formation's Satellites
dc.typeActas de congresos


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