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The AUSTRAL VLBI observing program
L Plank1, J E J Lovell1, J N McCallum1
11University of Tasmania, Private Bag 37, Hobart, 7001 Australia.
The AUSTRAL observing program improved geodetic and astrometric very long baseline interferometry (VLBI) results by a factor of two. This enhancement was achieved through optimized scheduling, increased observations, and automated operations for better reference frames and Earth orientation parameters.
Area of Science:
- Geodesy and Astrometry
- Radio Astronomy
- Earth Science
Background:
- The AUSTRAL observing program initiated in 2011 utilizes new Australian AuScope VLBI antennas.
- It incorporates international antennas from New Zealand and South Africa to form a southern hemisphere array.
- These antennas are designed for next-generation VLBI, enabling higher data rates and more frequent observations than standard International VLBI Service (IVS) sessions.
Purpose of the Study:
- To describe the continuous development of AUSTRAL sessions.
- To highlight improvements in baseline length repeatabilities.
- To assess the contribution of AUSTRAL sessions to geodetic and astrometric products.
Main Methods:
- Implementing advanced scheduling strategies and increasing the number of observations.
- Focusing on automated operation and efficient data logistics.
- Performing 151 AUSTRAL sessions and comparing results with IVS sessions.
Main Results:
- Achieved a factor of two improvement in baseline length repeatabilities since the program's inception.
- Demonstrated the significant contribution of AUSTRAL sessions to VLBI end-products.
- Showcased the suitability of AUSTRAL data for determining baselines, station coordinates, source coordinates, and Earth orientation parameters.
Conclusions:
- The AUSTRAL program has successfully enhanced the precision of geodetic and astrometric measurements.
- Optimized observing strategies and increased data volume are key to these improvements.
- AUSTRAL sessions are a vital component for establishing accurate terrestrial and celestial reference frames and Earth orientation parameters.
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