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dc.contributor.authorLópez Ortí, José Antonio
dc.contributor.authorAgost Gómez, Vicente
dc.contributor.authorBarreda Rochera, Miguel
dc.date.accessioned2022-10-27T17:49:09Z
dc.date.available2022-10-27T17:49:09Z
dc.date.issued2022
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.urihttp://hdl.handle.net/10234/200625
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 antifo-cal anomaly,𝑓′; Fukushima defined𝑓′as the angle between the periapsis andthe secondary around the empty focus. In this first part of the paper, we takean approach to the study of the semifocal anomaly in the hyperbolic motionand in the limit case corresponding to the parabolic movement. From here, wefind a relation between the semifocal anomaly and the true anomaly that holdsindependently of the movement type. We focus on the study of the two-bodyproblem when this new anomaly is used as the temporal variable. In the secondpart, we show the use of this anomaly—combined with numerical integrationmethods—to improve integration errors in one revolution. Finally, we analyzethe errors committed in the integration process—depending on several values ofthe eccentricity—for the elliptic, parabolic, and hyperbolic cases in the apsidalregion.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.publisherWileyca_CA
dc.relation.isPartOfMathematical Methods in the Applied Sciences, 2022;1-14.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 equationca_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.nameUniversity Jaume I of Castellónca_CA
oaire.awardNumber16I358.01/1ca_CA


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