Orbital Propagation
Orbital Propagation is a computational method in astrodynamics that determines the future trajectory of a celestial or artificial body under gravitational forces by solving the equations of motion derived from conic section orbits.
83
Publications
2.5K
Citations
170
Authors
90
Institutions
Publications per year
2017–2026
21
Parents
83
1–5 of 83
170
4
h-index
4
h-index
2
h-index
2
h-index
2
h-index
1–5 of 170
90

University of Pisa
Pisa, Italy
7 h-index
13 publications
226 citations

Universidad Politécnica de Madrid
Madrid, Spain
3 h-index
6 publications
114 citations
Mitchell Institute
Portland, United States
3 h-index
5 publications
129 citations

Universidad de La Rioja
Logroño, Spain
3 h-index
7 publications
171 citations
Jet Propulsion Laboratory
Pasadena, United States
3 h-index
2 publications
54 citations

Keio University
Tokyo, Japan
2 h-index
4 publications
239 citations

Imperial College London
London, United Kingdom
2 h-index
3 publications
50 citations

University of Cologne
Cologne, Germany
2 h-index
7 publications
390 citations
1–8 of 90
12 publications · 601 citations
12
h-index
6 publications · 195 citations
7
h-index
5 publications · 71 citations
5
h-index
5 publications · 211 citations
5
h-index
3 publications · 52 citations
3
h-index
1–5