Mean Anomaly
Mean Anomaly is a time-dependent angular parameter in celestial mechanics that, within the formalism of Keplerian motion, represents the angle a body would have swept out if it moved with constant angular velocity along a circular orbit with the same orbital period as the actual elliptical orbit.
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218
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131
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2017–2026
18
103
Solution of the problem of artificial satellite theory without drag
Dirk Brouwer · The Astronomical Journal · 1959 · 857 citations
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NSF National Center for Atmospheric Research, United States
3 publications · 181 citations
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Centre National de la Recherche Scientifique
Paris, France
4 h-index
9 publications
551 citations
Nanjing University
Nanjing, China
3 h-index
4 publications
81 citations
GFZ Helmholtz Centre for Geosciences
Potsdam, Germany
2 h-index
3 publications
81 citations
École Polytechnique
Palaiseau, France
2 h-index
2 publications
179 citations

Western University
London, Canada
2 h-index
5 publications
391 citations

Tohoku University
Sendai, Japan
2 h-index
4 publications
162 citations
University of Colorado Boulder
Boulder, United States
2 h-index
5 publications
809 citations
The Ohio State University
Columbus, United States
2 h-index
2 publications
135 citations
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AJ · 11 publications · 1.2K citations
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10 publications · 215 citations
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JGR · 9 publications · 858 citations
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6 publications · 508 citations
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5 publications · 534 citations
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