Very Long Baseline Interferometry (VLBI) plays a unique and fundamental role in the maintenance of the global (terrestrial and celestial) reference frames, which are required for precise positioning in many research areas such as the understanding and monitoring of global changes, and for space missions. The International VLBI Service for Geodesy and Astrometry (IVS) coordinates the global VLBI components and resources on an international basis. The service is tasked by the International Association of Geodesy (IAG) and International Astronomical Union (IAU) to provide products for the realization of the Celestial Reference Frame (CRF) through the positions of quasars, to deliver products for the maintenance of the terrestrial reference frame (TRF), such as station positions and their changes with time, and to generate products describing the rotation and orientation of the Earth. In particular, VLBI uniquely provides direct observations of nutation parameters and of the time difference UT1-UTC. This paper summarizes the evolution and current status of the IVS. It points out the activities to improve further on the product quality to meet future service requirements.
[1]
Zuheir Altamimi,et al.
Global geodetic observing system-considerations for the geodetic network infrastructure
,
2006
.
[2]
Thomas A. Clark,et al.
Measurement of horizontal motions in Alaska using very long baseline interferometry
,
1990
.
[3]
John W. Dawson,et al.
Indirect approach to invariant point determination for SLR and VLBI systems: an assessment
,
2007
.
[4]
Dirk Behrend,et al.
International VLBI Service for Geodesy and Astrometry 2004 Annual Report
,
2005
.
[5]
Karen D. Baver,et al.
International VLBI Service for Geodesy and Astrometry: 2000 General Meeting Proceedings
,
2000
.
[6]
Harald Schuh,et al.
Modeling thermal deformation of VLBI antennas with a new temperature model
,
2007
.
[7]
Axel Nothnagel,et al.
The contribution of Very Long Baseline Interferometry to ITRF2005
,
2007
.