Lunisolar gravitational perturbations in the motion of an Earth's satellite with large orbit eccentricity.

Details Lunisolar gravitational perturbations in the motion of an Earth's satellite with large orbit eccentricity. Lunisolar gravitational perturbations in the motion of an Earth's satellite with large orbit eccentricity.

Apr 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999kosis..37..156v&link_type=abstract

Kosmicheskie Issledovaniia, Tom 37, No. 2, p. 156 - 162

Physics

Artificial Satellites: Perturbation Theory, Artificial Satellites: Motions

Scientific paper

The authors present an analytical theory of the lunisolar gravitational
perturbations. The theory is developed for Earth-orbital artificial
satellites with large orbit eccentricity and is based on rapidly
convergent series in multiples of the elliptic anomaly.

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