Lunisolar resonances revisited
From MaRDI portal
Publication:5960104
DOI10.1023/A:1013363221377zbMath1043.70009OpenAlexW4240067022MaRDI QIDQ5960104
Publication date: 11 April 2002
Published in: Celestial Mechanics and Dynamical Astronomy (Search for Journal in Brave)
Full work available at URL: https://doi.org/10.1023/a:1013363221377
Related Items (11)
Dynamical taxonomy of the coupled solar radiation pressure and oblateness problem and analytical deorbiting configurations ⋮ The dynamical structure of the MEO region: long-term stability, chaos, and transport ⋮ Proper elements for space debris ⋮ Bifurcation of Lunisolar Secular Resonances for Space Debris Orbits ⋮ Analytical development of the lunisolar disturbing function and the critical inclination secular resonance ⋮ Resonant dynamics of medium Earth orbits: space debris issues ⋮ Nekhoroshev estimates for the orbital stability of Earth's satellites ⋮ To the substantiation of a numerical-analytical method for revealing secular resonances ⋮ Phase space description of the dynamics due to the coupled effect of the planetary oblateness and the solar radiation pressure perturbations ⋮ On the predictability and robustness of Galileo disposal orbits ⋮ A deep dive into the \(2g+h\) resonance: separatrices, manifolds and phase space structure of navigation satellites
This page was built for publication: Lunisolar resonances revisited
