Expressions for IAU 2000 precession quantities
By N. Capitaine, Patrick T. Wallace, J. Chapront. 2003
212 citations recorded by the source corpus.
Subfields: Astronomy and Astrophysics, Geophysics, Oceanography
View Paper: https://www.semanticscholar.org/paper/0be95145eef11e5bf43100d37a9d0c15590134e4
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In Astronomy and Astrophysics
- E. Pitjeva
- A. Fienga
- William M. Folkner
- O. Paris
- C. I. O. Technology.
- France.
- Jet propulsion Laboratory
- Pasadena
In Geophysics
In Oceanography
- A. Fienga
- William M. Folkner
- Toshio Fukushima
- S. Lambert
- N. Capitaine
- Robert Heinkelmann
- C. Bizouard
- Lorenzo Iorio
Citations in the corpus
- The third realization of the International Celestial Reference Frame by very long baseline interferometry (2020, methodology): “Modeling of the Earth’s spin axis was achieved using the MHB nutation (Mathews et al. 2002) and P03 precession (Capitaine et al. 2003; Hilton et al. 2006), further designated as IAU 2000A nutation and IAU 2006 precession after adoption of these models by the IAU.”
- The IAU 2009 system of astronomical constants: the report of the IAU working group on numerical standards for Fundamental Astronomy (2011, methodology): “This value is taken from the P03 precession model of Capitaine et al. (2003) and was adopted in IAU 2006 Resolution B1.”
- The IERS EOP 14C04 solution for Earth orientation parameters consistent with ITRF 2014 (2019, background): “The interaction of the Sun and the Moon with the Earth’s equatorial bulge produces the precession–nutation, modeled to a very good accuracy (Mathews et al. 2002; Capitaine et al. 2003).”