Abstract
The perturbations of artificial satellite are derived here by a new method, somewhat similar to that of Poisson.
The novel feature of the method is that the right-hand member f(t;x) of the differential equations need not be developed in series, as it is done in the von Zeipel and other methods.
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Cui, DX. A method for computation of perturbations. Celestial Mechanics 32, 1–13 (1984). https://doi.org/10.1007/BF01358400
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DOI: https://doi.org/10.1007/BF01358400