Computer Science
Scientific paper
May 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987kosis..25..339v&link_type=abstract
Kosmicheskie Issledovaniia (ISSN 0023-4206), vol. 25, May-June 1987, p. 339-355.
Computer Science
High Altitude, Orbit Calculation, Orbit Perturbation, Satellite Orbits, Solar Activity Effects, Temporal Distribution, Axes Of Rotation, Equations Of Motion, Lunar Effects
Scientific paper
Vashkoviak's (1986) numerical-analytical method is used to investigate the evolution of satellite orbits with semimajor axes of l00,000-200,000 km for time periods of 5-10 years. The results obtained with this method are compared with results of the numerical integration of rigorous equations of satellite motion with allowance for lunar and solar perturbation effects. The range of eccentricities and inclinations is determined for a 10-year period for initial almost-circular orbits with semimajor axes of 125,000 and 160,000 km.
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