A new bi-parametric family of temporal transformations to improve the integration algorithms in the study of the orbital motion

DOI10.1016/J.CAM.2016.01.057zbMath1381.70027OpenAlexW2276212217MaRDI QIDQ507919

José Antonio López Ortí, Vicente Agost-Gómez, Miguel Barreda-Rochera

Publication date: 9 February 2017

Published in: Journal of Computational and Applied Mathematics (Search for Journal in Brave)

Full work available at URL: http://hdl.handle.net/10234/159569

zbMATH Keywords

ordinary differential equationscelestial mechanicscomputational algebra

Mathematics Subject Classification ID

Two-body problems (70F05) Celestial mechanics (70F15) Orbital mechanics (70M20) (n)-body problems (70F10)

Related Items (1)

Corrigendum to: ``A new bi-parametric family of temporal transformations to improve the integration algorithms in the study of the orbital motion

Cites Work

• Unnamed Item
• An improved algorithm to develop semi-analytical planetary theories using Sundman generalized variables
• Length of arc as independent argument for highly eccentric orbits
• A study about the integration of the elliptical orbital motion based on a special one-parametric family of anomalies
• Expansions of elliptic motion based on elliptic function theory
• Note on Lagrange's inversion formula
• Accurate computation of highly eccentric satellite orbits
• The intermediate anomaly

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