Collaborative Research Projects in Australia: Radio Astronomy Dr. Greg Wickham (AARNet) Dr Tasso Tzioumis Dr Shaun Amy Dr Chris Phillips (CSIRO ATNF) Global Collaborations / APAN 28 th August 2007
Radio Interferometry Telescopes focus on a source Closest telescope has delay introduced Data streams fed into correlator Fringes are calculated: Provides information on structure and position of radio source Telescopes focused at different sources – no fringes
Building an Image Telescopes maintain focus on source for a period of time As the earth rotates more data is collected Data fed into correlator Similar in concept to “time lapse photograph” Final image is interpolated
Visibility of Sources
eVLBI Strategy Now 1024 Mbps/telescope - 2 x 1Gbps N x 1Gbps to correlators: Swinburne / Curtin --> 10 Gbps circuits? International: JIVE (n x 1 Gbps); USA; Asia 3 years: CABB correlator at Narrabri Min: 2 x 10 Gbps (8Gbps) / telescope N x 10 Gbps into Narrabri
eVLBI Strategy 5 years: ASKAP N x 10 Gbps per telescope to Correlators New NSW site (Fowler’s Gap) Connections to and in WA & NZ 10 years: SKA Candidates are Australia and South Africa Extreme bandwidth required (up to Tbps)
eVLBI – Strategy in Motion Huygens Transfer VLBI EXPReS milestone in the progress towards SKA. International collaborations are extremely important Strategic to be involved In Australia eVLBI is ~ 10% of the ATNF observations How is this going to evolve is not clear yet And as ASKAP and the SKA come along, there will be bigger sectors of the community involved
VLBI - Huygens Space Probe
EXPReS Data Path: Telescopes to Marsfield Marsfield to AARNet AARNet to Jive Trial: June 3 x 256Mbit/sec streams Using routed network Full Test: October 3 x 512Mbit/sec streams Using circuits Parkes
EXPReS: Trial 3 x 256 Mbit / sec Combined at Marsfield Temporary 1G connection to AARNet Routed connection back to JIVE “Relatively Simple”
Final Experiment 3 x 512Mbit/sec Direct patched in Sydney Not to Scale!
Square Kilometer Array
Thank You!