The unified ideal model of mean motion resonance of artificial satellites due to geopotential perturbations
Author:
Publisher
Springer Science and Business Media LLC
Subject
General Physics and Astronomy
Link
http://link.springer.com/content/pdf/10.1007/s11433-013-5022-8.pdf
Reference22 articles.
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2. Jupp A H. A solution of the ideal resonance problem for the case of libration. Astron J, 1969, 74: 35–43
3. Garfinkel B. Global solution of the ideal resonance problem. Celest Mech, 1973, 8: 207–212
4. Henrard J, Wauthier P. A geometric approach to the ideal resonance problem. Celest Mech, 1988, 44: 227–238
5. Erdi B, Kovacs J. A fourth-order solution of the ideal resonace problem. Celest Mech Dyn Astron, 1993, 56: 221–230
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1. On the lunar node resonance of the orbital plane evolution of the Earth’s satellite orbits;Advances in Space Research;2018-06
2. Long term evolution of Molniya orbit under the effect of Earth’s non-spherical gravitational perturbation;Advances in Space Research;2014-07
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