Precession-Nutation Estimates from Optical Astrometry 1899.7-1992.0 and Comparison with VLBI Results
Abstract
The most recent solution of Earth Orientation Parameters (EOP) from the observations made by optical astrometry from 1899.7 to 1992.0 at 33 observatories is used to estimate the corrections of the present International Astronomical Union (IAU) model of precession-nutation. Since the resolution of the solution is about 5 days, only the terms with periods of 14 days and longer are considered. The results are compared with Very Long Baseline Interferometry-based corrections of the standard precession-nutation model, and the differences are discussed.
Document Details
- Document Type
- Technical Report
- Publication Date
- Mar 01, 2000
- Accession Number
- ADA436097
Entities
People
- Cyril Ron
- Jan Vondrak
Organizations
- Czech Academy of Sciences