Anomaly Conversion
Anomaly Conversion is a computational method in celestial mechanics that transforms orbital position information between different types of Keplerian anomalies—specifically, mean, eccentric, and true anomalies—by solving the underlying transcendental equations to enable consistent characterization of time-dependent orbital motion.
4
Publications
174
Citations
8
Authors
7
Institutions
Publications per year
2017–2026
2
4
1–4 of 4
8
1
h-index
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Research Institute of Geodesy, Topography and Cartography, Czechia
1 publications · 29 citations
1
h-index
1
h-index
1–5 of 8
7

University of Maryland, Baltimore
Baltimore, United States
1 h-index
1 publications
45 citations

Dalian Maritime University
Dalian, China
1 h-index
1 publications
45 citations
Research Institute of Geodesy, Topography and Cartography
Zdiby, Czechia
1 h-index
1 publications
29 citations
Collecte Localisation Satellites (France)
Ramonville-Saint-Agne, France
1 h-index
1 publications
29 citations

University of Baghdad
Baghdad, Iraq
1 h-index
2 publications
24 citations

University of British Columbia
Vancouver, Canada
1 h-index
1 publications
88 citations

Centre National d'Études Spatiales
Paris, France
1 h-index
1 publications
29 citations
1–7 of 7
1 publications · 12 citations
1
h-index
1 publications · 29 citations
1
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1 publications · 88 citations
1
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1 publications · 45 citations
1
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1–4