This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical and technical details of WARK12M - the new IVS network station operated by the Institute for Radio Astronomy and Space Research (IRASR) of Auckland University of Technology (AUT). The details of the VLBI system installed in the station are outlined along with those of the collocated GNSS station. We report on the status of broadband connectivity and on the results of testing data transfer protocols; we investigate UDP protocols such as 'tsunami' and UDT and demonstrate that the UDT protocol is more efficient than 'tsunami' and 'ftp'. In general, the WARK12M IVS network station is fully equipped, connected and tested to start participating in...
During 2012 we participated in 40 IVS sessions. As in the previous four years, we used the majority ...
The 250-2500 km baseline vectors between radio telescopes located at Tidbinbilla (DSS43) near Canber...
The AuScope VLBI array was built with the purpose to improve the terrestrial (TRF) and celestial ref...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
The Institute for Radio Astronomy and Space Research (IRASR) of Auckland University of Technology (A...
The New Zealand 12-m antenna is scheduled to start participating in regular IVS VLBI sessions from t...
We report the results of a successful 7-hour 1.4 GHz Very Long Baseline Interferometry (VLBI) experi...
Very Long Baseline Interferometry (VLBI) is a space geodesy technique used to determine the Celestia...
The AUSTRAL observing program was started in 2011, performing geodetic and astrometric very long bas...
The AUSTRAL observing program was started in 2011, performing geodetic and astrometric very long bas...
Three 12-meter radio telescopes are being built in Australia (the AuScope project) and one in New Ze...
This report of the Technology Coordinator includes the following: 1) continued work to implement the...
During 2010 the Onsala Space Observatory contributed as an IVS Network Station to 27 VLBI sessions o...
The Tsukuba 32-m VLBI station is operated by the Geospatial Information Authority of Japan. This rep...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
During 2012 we participated in 40 IVS sessions. As in the previous four years, we used the majority ...
The 250-2500 km baseline vectors between radio telescopes located at Tidbinbilla (DSS43) near Canber...
The AuScope VLBI array was built with the purpose to improve the terrestrial (TRF) and celestial ref...
This report summarizes the geodetic VLBI activities in New Zealand in 2010. It provides geographical...
The Institute for Radio Astronomy and Space Research (IRASR) of Auckland University of Technology (A...
The New Zealand 12-m antenna is scheduled to start participating in regular IVS VLBI sessions from t...
We report the results of a successful 7-hour 1.4 GHz Very Long Baseline Interferometry (VLBI) experi...
Very Long Baseline Interferometry (VLBI) is a space geodesy technique used to determine the Celestia...
The AUSTRAL observing program was started in 2011, performing geodetic and astrometric very long bas...
The AUSTRAL observing program was started in 2011, performing geodetic and astrometric very long bas...
Three 12-meter radio telescopes are being built in Australia (the AuScope project) and one in New Ze...
This report of the Technology Coordinator includes the following: 1) continued work to implement the...
During 2010 the Onsala Space Observatory contributed as an IVS Network Station to 27 VLBI sessions o...
The Tsukuba 32-m VLBI station is operated by the Geospatial Information Authority of Japan. This rep...
The activities related to geodetic VLBI performed at the IVS AC PMD during 2017 and 2018 w...
During 2012 we participated in 40 IVS sessions. As in the previous four years, we used the majority ...
The 250-2500 km baseline vectors between radio telescopes located at Tidbinbilla (DSS43) near Canber...
The AuScope VLBI array was built with the purpose to improve the terrestrial (TRF) and celestial ref...