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International Earth Rotation and Reference Systems Service
Glossary
The following terms are related to the IERS and to Earth rotation and reference systems in general.
Additions will follow, proposals are welcome.
T eph (Teph)
independent time argument of JPL ephemerides (Standish, A&A, 336, 381, 1998) that is, for practical purposes, the same as Barycentric Dynamical Time (TDB). TDB is related to Barycentric Coordinate Time (TCB) by
TDB = TCB - LB × (JDTCB - T0) × 86400 + TDB0, where T0 = 2443144.5003725, and
LB = 1.550519768 × 10-8 and TDB0 = -6.55 × 10-5 s
are defining constants. [IAU 2006 Resolution B3]
origin of longitude in the Intermediate Terrestrial Reference System. It is the non-rotating origin in the ITRS that is recommended by the IAU 2000 Resolution B1.8, where it was designated Terrestrial Ephemeris Origin. The name Terrestrial Intermediate Origin was adopted by IAU 2006 Resolution B2. The TIO was originally set at the ITRF origin of longitude and throughout 1900-2100 stays within 0.1 mas of the ITRF zero meridian.
a geocentric reference system defined by the intermediate equator of the CIP and the TIO (IAU 2006 Resolution B2). It is related to the ITRS by polar motion and s′ (see TIO locator). It is related to the Celestial Intermediate Reference System by a rotation of ERA around the CIP, which defines the common z-axis of the two systems. Since the acronym for this system is close to another acronym (namely ITRS), it is suggested that wherever possible the complete name be used.
TT is conventionally realized by TT = TAI + 32.184 s (although in fact TAI and TT are independent time scales, and different implementations of TT may differ by a few tens of microseconds.)