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

Authors

190

  1. NC
    N. Capitaine

    Centre National de la Recherche Scientifique, France

    7 publications · 376 citations

    7

    h-index

  2. PT
    P. T. Wallace

    Rutherford Appleton Laboratory, United Kingdom

    6 publications · 347 citations

    6

    h-index

  3. FO
    F. Ohme

    Max Planck Institute for Gravitational Physics, Germany

    3 publications · 664 citations

    3

    h-index

  4. MH
    Mark Hannam

    Cardiff University, United Kingdom

    3 publications · 717 citations

    3

    h-index

  5. JC
    J. Chapront

    Centre National de la Recherche Scientifique, France

    3 publications · 251 citations

    3

    h-index

1–5 of 190

Venues

  1. Astronomy and Astrophysics

    11 publications · 440 citations

    11

    h-index

  2. 9

    h-index

  3. Physical review. D/Physical review. D.

    PRD · 7 publications · 500 citations

    7

    h-index

  4. The Astronomical Journal

    AJ · 6 publications · 245 citations

    6

    h-index

  5. Celestial Mechanics and Dynamical Astronomy

    5 publications · 148 citations

    5

    h-index

1–5