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CMMSE: Study of a new symmetric anomaly in the elliptic, hyperbolic, and parabolic Keplerian motion
dc.contributor.author | López Ortí, José Antonio | |
dc.contributor.author | Agost Gómez, Vicente | |
dc.contributor.author | Barreda Rochera, Miguel | |
dc.date.accessioned | 2022-10-13T14:20:53Z | |
dc.date.available | 2022-10-13T14:20:53Z | |
dc.date.issued | 2022-07-20 | |
dc.identifier.citation | López 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.8586 | ca_CA |
dc.identifier.issn | 0170-4214 | |
dc.identifier.issn | 1099-1476 | |
dc.identifier.uri | http://hdl.handle.net/10234/200362 | |
dc.description.abstract | In 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.sponsorShip | Funding for open access charge: CRUE-Universitat Jaume I | |
dc.format.extent | 14 p. | ca_CA |
dc.format.mimetype | application/pdf | ca_CA |
dc.language.iso | eng | ca_CA |
dc.publisher | John Wiley & Sons, Ltd | ca_CA |
dc.relation | Proceso de mejora de catálogos celestes previos al ICRF3 y GAIA, con objeto de enlazar los sistemas HCRF-ICRF2-GCRF | ca_CA |
dc.relation.isPartOf | Mathematical Methods in the Applied Sciences (2022) | ca_CA |
dc.rights | 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. | ca_CA |
dc.rights.uri | http://creativecommons.org/licenses/by-nc-nd/4.0/ | ca_CA |
dc.subject | celestial mechanics | ca_CA |
dc.subject | computational algebra | ca_CA |
dc.subject | orbital motion | ca_CA |
dc.subject | ordinary differential equations | ca_CA |
dc.subject | 70F15 | ca_CA |
dc.subject | 70F05 | ca_CA |
dc.subject | 70H09 | ca_CA |
dc.subject | 74H10 | ca_CA |
dc.subject | 74H15 | ca_CA |
dc.title | CMMSE: Study of a new symmetric anomaly in the elliptic, hyperbolic, and parabolic Keplerian motion | ca_CA |
dc.type | info:eu-repo/semantics/article | ca_CA |
dc.identifier.doi | https://doi.org/10.1002/mma.8586 | |
dc.rights.accessRights | info:eu-repo/semantics/openAccess | ca_CA |
dc.type.version | info:eu-repo/semantics/publishedVersion | ca_CA |
project.funder.name | Universitat Jaume I | ca_CA |
oaire.awardNumber | 16I358.01/1 | ca_CA |
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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.