000101534 001__ 101534 000101534 005__ 20240122154814.0 000101534 0247_ $$2doi$$a10.1016/j.asr.2020.04.018 000101534 0248_ $$2sideral$$a117952 000101534 037__ $$aART-2021-117952 000101534 041__ $$aeng 000101534 100__ $$0(orcid)0000-0002-8507-4679$$aArnas, D. 000101534 245__ $$a4D Lattice Flower Constellations 000101534 260__ $$c2021 000101534 5060_ $$aAccess copy available to the general public$$fUnrestricted 000101534 5203_ $$a4D Lattice Flower Constellations is a new constellation design framework, based on the previous 2D and 3D Lattice theories of Flower Constellations, that focus on the generation of constellations whose satellites can have different semi-major axis and still present a constellation structure that is maintained during the dynamic of the system. This situation can arise when dealing with satellites with very different instruments, or when it is of interest to coordinate two different constellations. In that sense, 4D Lattice Flower Constellations constitutes the most general representation of the Flower Constellation formulation. In addition, the effects of the J2 perturbation are taken into account in order to generate distributions that maintain their initial design configuration under this perturbation for longer periods of time with a low fuel budget. Finally, examples of application are presented, showing the possibilities in satellite constellation design of this new approach. 000101534 536__ $$9info:eu-repo/grantAgreement/ES/DGA-FEDER/E24-17R$$9info:eu-repo/grantAgreement/ES/MINECO-FEDER/ESP2017-87113-R 000101534 540__ $$9info:eu-repo/semantics/openAccess$$aAll rights reserved$$uhttp://www.europeana.eu/rights/rr-f/ 000101534 590__ $$a2.611$$b2021 000101534 592__ $$a0.613$$b2021 000101534 594__ $$a4.7$$b2021 000101534 591__ $$aENGINEERING, AEROSPACE$$b10 / 34 = 0.294$$c2021$$dQ2$$eT1 000101534 593__ $$aAerospace Engineering$$c2021$$dQ2 000101534 591__ $$aGEOSCIENCES, MULTIDISCIPLINARY$$b120 / 202 = 0.594$$c2021$$dQ3$$eT2 000101534 593__ $$aAstronomy and Astrophysics$$c2021$$dQ2 000101534 591__ $$aMETEOROLOGY & ATMOSPHERIC SCIENCES$$b66 / 94 = 0.702$$c2021$$dQ3$$eT3 000101534 593__ $$aSpace and Planetary Science$$c2021$$dQ2 000101534 591__ $$aASTRONOMY & ASTROPHYSICS$$b35 / 69 = 0.507$$c2021$$dQ3$$eT2 000101534 593__ $$aGeophysics$$c2021$$dQ2 000101534 593__ $$aAtmospheric Science$$c2021$$dQ2 000101534 655_4 $$ainfo:eu-repo/semantics/article$$vinfo:eu-repo/semantics/acceptedVersion 000101534 700__ $$0(orcid)0000-0002-7620-4523$$aCasanova, D. 000101534 700__ $$0(orcid)0000-0003-4859-7224$$aTresaco, E. 000101534 773__ $$g67, 11 (2021), 683-3695$$pAdv. space res.$$tAdvances in Space Research$$x0273-1177 000101534 85641 $$uhttps://www.sciencedirect.com/science/article/pii/S0273117720302568?dgcid=coauthor$$zTexto completo de la revista 000101534 8564_ $$s406642$$uhttps://zaguan.unizar.es/record/101534/files/texto_completo.pdf$$yPostprint 000101534 8564_ $$s2391083$$uhttps://zaguan.unizar.es/record/101534/files/texto_completo.jpg?subformat=icon$$xicon$$yPostprint 000101534 909CO $$ooai:zaguan.unizar.es:101534$$particulos$$pdriver 000101534 951__ $$a2024-01-22-15:34:53 000101534 980__ $$aARTICLE