Expressions to implement the IAU 2000 definition of UT1

被引:15
作者
Capitaine, N
Wallace, PT
McCarthy, DD
机构
[1] CNRS, Observ Paris, SYRTE, UMR8630, F-75014 Paris, France
[2] Rutherford Appleton Lab, HM Naut Almanac Off, Space Sci & Technol Dept, CLRC, Didcot OX11 0QX, Oxon, England
[3] USN Observ, Washington, DC 20392 USA
关键词
astrometry; reference systems; ephemerides; time;
D O I
10.1051/0004-6361:20030817
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
This paper provides expressions to be used to implement the new definition of UT1 corresponding to the IAU 2000 resolutions either in the new (CEO-based) or classical (equinox-based) transformations between the International Terrestrial Reference System ( ITRS) and the Geocentric Celestial Reference System (GCRS). The new expression for Greenwich Sidereal Time (GST) has to be in agreement at the microarcsecond level, for one century, with the IAU 2000 expressions for the Earth Rotation Angle ( ERA) and for the quantity s positioning the Celestial Ephemeris Origin (CEO) on the equator of the CIP. The computations of the new expressions using the IAU 2000 precession-nutation model are performed in such a manner as to ensure that there is no discontinuity in UT1 on 1 January 2003 and that there is equivalence of the classical and new transformations between the ITRS and GCRS relative to the rotation about the axis of the CIP when these expressions are used. The equinox offset that is considered in the computations refers to the dynamical mean equinox of J2000.0. The resulting expressions have been included in the IERS Conventions 2000.
引用
收藏
页码:1135 / 1149
页数:15
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