Abstract
A noncanonical Hamiltonian formulation of the Coulomb formation dynamics is used to develop necessary conditions for static Coulomb formations with constant charges. With a static or frozen formation the satellites perform non-Keplerian orbits and maintain constant relative position vectors. As seen by an observer following the center of mass motion, the spacecraft formation would appear to behave equivalently to a rigid body in orbit. Previous research has demonstrated the existence of such static Coulomb formations analytically by employing symmetry simplifying assumptions with linearized relative motion dynamics, or by using numerical genetic search algorithms. These static solutions are used as reference geometries and charges for feedback law developments. This paper presents nonlinear static formation conditions for the circularly restricted problem. Hamiltonian formulations have been used to study equilibrium conditions of rigid bodies in orbit. Analogous techniques are employed to study necessary conditions to achieve a static Coulomb formation. Analytical results using the full and truncated formation gravity potential function are presented. Numerical results illustrate convergence performance improvements of an evolutionary search algorithm where the presented necessary conditions are enforced.
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Schaub, H., Hall, C.D. & Berryman, J. Necessary conditions for circularly-restricted static coulomb formations. J of Astronaut Sci 54, 525–541 (2006). https://doi.org/10.1007/BF03256504
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DOI: https://doi.org/10.1007/BF03256504