Precession Modelling
Precession Modelling is a theoretical framework within astronomical surveying that systematically characterizes the gradual, periodic reorientation of the Earth's rotational axis in space due to gravitational torques from the Sun and Moon, distinguishing it from other geodetic or celestial reference frame corrections by specifically accounting for the long-term, cyclical shift in the equatorial and ecliptic coordinate systems.
92
Publications
5.3K
Citations
190
Authors
139
Institutions
Publications per year
2017–2026
22
Parents
92
1–5 of 92
190
7
h-index
6
h-index
3
h-index
3
h-index
3
h-index
1–5 of 190
139

Centre National de la Recherche Scientifique
Paris, France
10 h-index
17 publications
774 citations
Systèmes de Référence Temps-Espace
Paris, France
9 h-index
16 publications
745 citations

Observatoire de Paris
Paris, France
6 h-index
10 publications
558 citations

Rutherford Appleton Laboratory
Didcot, United Kingdom
5 h-index
5 publications
316 citations
Jet Propulsion Laboratory
Pasadena, United States
5 h-index
7 publications
346 citations
California Institute of Technology
Pasadena, United States
5 h-index
8 publications
915 citations
Massachusetts Institute of Technology
Cambridge, United States
4 h-index
4 publications
596 citations

University of Madras
Chennai, India
3 h-index
3 publications
549 citations
1–8 of 139
11 publications · 440 citations
11
h-index
9 publications · 351 citations
9
h-index
PRD · 7 publications · 500 citations
7
h-index
AJ · 6 publications · 245 citations
6
h-index
5 publications · 148 citations
5
h-index
1–5