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It is well known that for a typical halo orbit around L1 or L2 libration point in circular restricted three-body problem its monodromy matrix has eigenvalues of the following form: lambda1 >...
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Often in astrodynamics we need conducting a high order integration of orbits in higly pertubed dynamics (the n-body problem augmented by the solar radiation pressure, J2, atmosphere, low-thrust,...
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