Astronomy and Astrophysics – Astronomy
Scientific paper
Feb 1993
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993azh....70..226k&link_type=abstract
Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 70, no. 1, p. 226-229.
Astronomy and Astrophysics
Astronomy
Earth-Moon System, Satellite Perturbation, Solar Planetary Interactions, Trigonometric Functions, Chebyshev Approximation, Satellite Orbits, Time Dependence
Scientific paper
A new method of calculating the lunar-solar perturbations in the motion of artificial earth satellites is suggested. It is based on a representation of the perturbations in the elements of the satellite's intermediate orbit by short partial sums of trigonometric series. The coefficients of the series are functions of time which are expanded into Chebyshev series at short intervals (up to 4 d). This form of perturbations significantly saves computer time and memory.
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