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dc.contributor.authorLópez Ortí, José Antonio
dc.contributor.authorAgost Gómez, Vicente
dc.contributor.authorBarreda Rochera, Miguel
dc.date.accessioned2022-10-13T14:20:53Z
dc.date.available2022-10-13T14:20:53Z
dc.date.issued2022-07-20
dc.identifier.citationLópez Ortí JA, Agost Gómez V, Barreda Rochera M. CMMSE: Study of a newsymmetric anomaly in the elliptic, hyperbolic, and parabolic Keplerian motion.Math Meth Appl Sci. 2022;1-14.doi:10.1002/mma.8586ca_CA
dc.identifier.issn0170-4214
dc.identifier.issn1099-1476
dc.identifier.urihttp://hdl.handle.net/10234/200362
dc.description.abstractIn the present work, we define a new anomaly, Ψ, termed semifocal anomaly. It is determined by the mean between the true anomaly, f', and the antifocal anomaly, f'; Fukushima defined f' as the angle between the periapsis and the secondary around the empty focus. In this first part of the paper, we take an approach to the study of the semifocal anomaly in the hyperbolic motion and in the limit case corresponding to the parabolic movement. From here, we find a relation between the semifocal anomaly and the true anomaly that holds independently of the movement type. We focus on the study of the two-body problem when this new anomaly is used as the temporal variable. In the second part, we show the use of this anomaly—combined with numerical integration methods—to improve integration errors in one revolution. Finally, we analyze the errors committed in the integration process—depending on several values of the eccentricity—for the elliptic, parabolic, and hyperbolic cases in the apsidal region.ca_CA
dc.description.sponsorShipFunding for open access charge: CRUE-Universitat Jaume I
dc.format.extent14 p.ca_CA
dc.format.mimetypeapplication/pdfca_CA
dc.language.isoengca_CA
dc.publisherJohn Wiley & Sons, Ltdca_CA
dc.relationProceso de mejora de catálogos celestes previos al ICRF3 y GAIA, con objeto de enlazar los sistemas HCRF-ICRF2-GCRFca_CA
dc.relation.isPartOfMathematical Methods in the Applied Sciences (2022)ca_CA
dc.rightsThis is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made. © 2022 The Authors. Mathematical Methods in the Applied Sciences published by John Wiley & Sons, Ltd.ca_CA
dc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/4.0/ca_CA
dc.subjectcelestial mechanicsca_CA
dc.subjectcomputational algebraca_CA
dc.subjectorbital motionca_CA
dc.subjectordinary differential equationsca_CA
dc.subject70F15ca_CA
dc.subject70F05ca_CA
dc.subject70H09ca_CA
dc.subject74H10ca_CA
dc.subject74H15ca_CA
dc.titleCMMSE: Study of a new symmetric anomaly in the elliptic, hyperbolic, and parabolic Keplerian motionca_CA
dc.typeinfo:eu-repo/semantics/articleca_CA
dc.identifier.doihttps://doi.org/10.1002/mma.8586
dc.rights.accessRightsinfo:eu-repo/semantics/openAccessca_CA
dc.type.versioninfo:eu-repo/semantics/publishedVersionca_CA
project.funder.nameUniversitat Jaume Ica_CA
oaire.awardNumber16I358.01/1ca_CA


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This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium,
provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made.
© 2022 The Authors. Mathematical Methods in the Applied Sciences published by John Wiley & Sons, Ltd.
Excepto si se señala otra cosa, la licencia del ítem se describe como: This is an open access article under the terms of the Creative Commons Attribution-NonCommercial-NoDerivs License, which permits use and distribution in any medium, provided the original work is properly cited, the use is non-commercial and no modifications or adaptations are made. © 2022 The Authors. Mathematical Methods in the Applied Sciences published by John Wiley & Sons, Ltd.