作者: Katsuhiko Yamada , Masaya Kimura , Takeya Shima , Shoji Yoshikawa
DOI: 10.2514/1.53926
关键词: Perturbation (astronomy) 、 Physics 、 Orbital elements 、 Classical mechanics 、 Relative motion 、 Numerical integration 、 State-transition matrix 、 Elliptic orbit 、 Osculating circle 、 Computer simulation
摘要: A state transition matrix for formation flying in eccentric orbits is considered this paper. The relative motion of the obeys Tschauner–Hempel equations, which are extended presence a J2 perturbation. Furthermore, transitionmatrix equations J2, and it demonstrated that becomes solution equations. Because only uses osculating orbital elements initial does not use mean elements, an analytical treatment possible. When first-order term errors sometimes become large compared with distancemultiplied by time range longer thanone orbit period.Amethod to suppress numerically also proposed.