Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips ....Radio Interferometer Studies of Compact Astronomical Sources. The giant black holes in the centres of distant galaxies that are the topic of this study are used to set the reference frame for geodesy on the earth. Remote and exotic as they are, they have real-world applications such as improving the positions available from GPS receivers and measuring continental drift. The signal processing equipment being developed for this new telescope is based on FPGA (field programmable gate array) chips, that promise to revolutionize the data processing industry, from radar to cellular telephones to computer networks. The young scientists who are working on this project will go on to lead the commercial and industrial applications of this new technology.Read moreRead less
Linkage Infrastructure, Equipment And Facilities - Grant ID: LE0236393
Funder
Australian Research Council
Funding Amount
$175,000.00
Summary
A Gigabit per second Data Recording System for Geodesy and Astronomy. We plan to acquire a gigabit per second digital data recorder for geodesy and astronomy. We will develop a geodetic VLBI capability to provide independent confirmation of results from alternative techniques such as GPS and SLR and allow us to characterise and remove the systematic errors inherent in these systems. We will estimate motion at sites from the combination of VLBI, GPS, gravity and tide gauge data for geodynamic ef ....A Gigabit per second Data Recording System for Geodesy and Astronomy. We plan to acquire a gigabit per second digital data recorder for geodesy and astronomy. We will develop a geodetic VLBI capability to provide independent confirmation of results from alternative techniques such as GPS and SLR and allow us to characterise and remove the systematic errors inherent in these systems. We will estimate motion at sites from the combination of VLBI, GPS, gravity and tide gauge data for geodynamic effects, such as post-glacial rebound and tectonic motion and global mean sea level change.
We will increase the density of southern radio sources used to define the International Celestial Reference Frame and investigate their structure and evolution. We will make high time resolution observations of young pulsars to study the phenomena of pulsar glitches and aid in the understanding of neutron star interiors.Read moreRead less