Relative Motion Dynamics
Relative Motion Dynamics is a mathematical model that describes the time-varying positional and orientational relationships between orbiting spacecraft in formation, distinguished by its incorporation of perturbed orbital mechanics and frame-dependent kinematic equations to characterize their coupled translational and rotational motions.
1.2K
Publications
64K
Citations
3.1K
Authors
960
Institutions
Publications per year
2017–2026
205
Parents
1.2K
Sea-floor spreading and continental drift
Xavier Le Pichon · Journal of Geophysical Research Atmospheres · 1968 · 1.5K citations
Present-Day Crustal Deformation in China Constrained by Global Positioning System Measurements
Qi Wang, Peizhen Zhang, Jeffrey T. Freymueller et al. · Science · 2001 · 1.2K citations
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Stanford University
Stanford, United States
18 h-index
39 publications
3.2K citations

Beihang University
Beijing, China
15 h-index
49 publications
1.4K citations
Technion – Israel Institute of Technology
Haifa, Israel
15 h-index
29 publications
1.6K citations

Harbin Institute of Technology
Harbin, China
15 h-index
64 publications
1.8K citations
Massachusetts Institute of Technology
Cambridge, United States
15 h-index
45 publications
5K citations
Tsinghua University
Beijing, China
14 h-index
34 publications
990 citations

Centre National de la Recherche Scientifique
Paris, France
14 h-index
36 publications
1.9K citations

Chinese Academy of Sciences
Beijing, China
13 h-index
45 publications
1.6K citations
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87 publications · 5.5K citations
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PRL · 29 publications · 2.5K citations
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PRA · 20 publications · 789 citations
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17 publications · 682 citations
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14 publications · 807 citations
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