000101166 001__ 101166
000101166 005__ 20240206150120.0
000101166 0247_ $$2doi$$a10.1007/s10569-020-09958-4
000101166 0248_ $$2sideral$$a117887
000101166 037__ $$aART-2020-117887
000101166 041__ $$aeng
000101166 100__ $$0(orcid)0000-0002-8507-4679$$aArnas Martínez, David$$uUniversidad de Zaragoza
000101166 245__ $$aNominal definition of satellite constellations under the Earth gravitational potential
000101166 260__ $$c2020
000101166 5060_ $$aAccess copy available to the general public$$fUnrestricted
000101166 5203_ $$aThis work focuses on the definition of satellite constellations whose secular relative distributions are invariant under the perturbation produced by the Earth gravitational potential. This is done by defining the satellite distribution directly in the Earth-Centered–Earth-Fixed frame of reference and using the along-track time distances between satellites to define the satellite constellation configuration. In addition, in order to expand the possibilities of application of this design methodology, a general transformation between the formulations of Flower Constellations, Walker Constellations, and a relative to Earth formulation based on along-track and cross-track distances between satellites is obtained. This allows not only for a relation between these formulations, but also for the obtainment of the relative to Earth distribution of such constellations. Finally, an example of application of these methodologies is presented for a low Earth orbit.
000101166 536__ $$9info:eu-repo/grantAgreement/ES/DGA-FEDER/E24-17R$$9info:eu-repo/grantAgreement/ES/MINECO-AEI-FEDER/ESP2017-87113-R
000101166 540__ $$9info:eu-repo/semantics/openAccess$$aAll rights reserved$$uhttp://www.europeana.eu/rights/rr-f/
000101166 590__ $$a1.664$$b2020
000101166 591__ $$aMATHEMATICS, INTERDISCIPLINARY APPLICATIONS$$b70 / 108 = 0.648$$c2020$$dQ3$$eT2
000101166 591__ $$aASTRONOMY & ASTROPHYSICS$$b45 / 68 = 0.662$$c2020$$dQ3$$eT3
000101166 592__ $$a0.714$$b2020
000101166 593__ $$aApplied Mathematics$$c2020$$dQ2
000101166 593__ $$aAstronomy and Astrophysics$$c2020$$dQ2
000101166 593__ $$aSpace and Planetary Science$$c2020$$dQ2
000101166 593__ $$aMathematical Physics$$c2020$$dQ2
000101166 593__ $$aModeling and Simulation$$c2020$$dQ2
000101166 593__ $$aComputational Mathematics$$c2020$$dQ2
000101166 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/acceptedVersion
000101166 700__ $$0(orcid)0000-0002-7620-4523$$aCasanova Ortega, Daniel
000101166 7102_ $$12006$$2200$$aUniversidad de Zaragoza$$bDpto. Matemáticas$$cÁrea Didáctica Matemática
000101166 773__ $$g132, 3 (2020), 19 [20 pp.]$$pCelest. mech. dyn. astron.$$tCelestial Mechanics and Dynamical Astronomy$$x0923-2958
000101166 8564_ $$s478015$$uhttps://zaguan.unizar.es/record/101166/files/texto_completo.pdf$$yPostprint
000101166 8564_ $$s1216781$$uhttps://zaguan.unizar.es/record/101166/files/texto_completo.jpg?subformat=icon$$xicon$$yPostprint
000101166 909CO $$ooai:zaguan.unizar.es:101166$$particulos$$pdriver
000101166 951__ $$a2024-02-06-14:55:53
000101166 980__ $$aARTICLE