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This paper extends the Hamiltonian structure-preserving control from two-imensional formation flying to three-dimensioanal case, and handles two new topology types that have not been studied in the literature: saddle × saddle × center and complex saddle × complex saddle × center. These topology types exist in the low-energy lunar halo transfer trajectory, which can represent the time-varing and complicated dynamics in the vast Earth-Moon space region.

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This page is a summary of: Hamiltonian Structure-Based Formation Flight Control Along Low-Energy Transfer Trajectory, Journal of Guidance Control and Dynamics, March 2021, American Institute of Aeronautics and Astronautics (AIAA),
DOI: 10.2514/1.g005294.
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