e-VLBI progress in the South “Towards e-VLBI” “e-VLBI” Tasso Tzioumis ATNF, CSIRO September 2006 Outline • Overview - details in other presentations/posters • Current LBA systems/developments – – – – Tapes - phasing out DAS - digital filters Disks - LBADR Software Correlators • Network developments • “Real” e-VLBI tests • Plans & the Future LBA x NTD x New Norcia Long baseline Array (LBA) • Telescopes in Australia – ATNF, U.Tasmania, NASA - “core” Oz VLBI network • • + South Africa + Telescopes in Asia Pacific region – Japan, China, Hawaii, VLBA,… Asia Pacific Telescope (APT) (VSOP support) • • Open network (EVN model of operations) http://www.atnf.csiro.au/vlbi • (+ Tests with NZ - fringes ok - no large antenna) LBA -S2 tape system • Canadian S2 VCR-based recorder – 8 VCR recorders 128 Mbps max data rates – S2 maintenance issues (no external support) • 7-station S2 LBA correlator at ATNF Sydney – XF architecture (ATCA correlator design) – Difficult to upgrade correlator • The main production-VLBI system for > 12 years • 2005 workshop: Phase-out S2 within ~3-4 years? • 2006 workshop: Decommission S2 in 2006-7!! • Move to disk-systems + software correlation – Correlation contracted to Swinburne - 1 October 2006 LBA - DAS • DAS: Based on Digital Filters (> 10 years old!) – – – – – – – 2 input IFs @ 64 MHz BW (2 pols or 2 frequencies) Sampling (10 bits) + Digital filters (ideal passbands) Bands: 64MHz 125 KHz S2 mode: 2 x 16 MHz ( 128 Mbps to match S2) Huygens mode: 4 x 16 MHz (256 Mbps) Maximum: 2 x 64 MHz (512 Mbps) - tested in 2006 Multibit mode: 2 x 16 MHz x 8(10) bits 1 Gbps • Interference excision? • ATNF stations: 2 DAS units – 512 Mbps for Huygens (8 x 16 MHz) – 1 Gbps by 4 x 64 MHz channels - developed & tested in 2006 • Remains the main DAS for LBA system(s) – BUT no more units available!! • Move to new VLBI dBBC units? (Haystack) - timescales? LBADR - Disk recorders • (See C. Phillips poster for details) • PCEVN-Metsahovi VSI interface system – VSIC (ECL-LVDS) & VSIB(computer) – Connects to LBA DAS – All LBA antennas equipped • COTS computers – New Tyan “Thunder K8WE” motherboards (2005) • Multiple PCI bus systems • Internal disks; IDE removable disks; X-RAID on fibre channel • (Replaced test systems on Dell 1600SC servers) • Apple Xserve hardware RAID systems (7 TB) Software correlators • See poster by S. Tingay & A. Deller • FX software correlator(s) • Swinburne Supercomputer – 300 Dell computers in cluster – Real time correlation (“normal” modes) - 30-50 nodes • Smaller clusters at telescopes – (Parkes: 32 nodes; ATCA: 16 nodes) • Cray XD-1 supercomputer in WA + FPGAs – Under development • Very versatile & robust (can run on most systems) • Only correlators in Australia for disk systems! “Real-time” fringe testing • Disk-systems – Can run parallel to S2 VCRs (S2 C2 output port) – Short segment (~0.1s) data or use full recorded data – Transfer to Swinburne - (slow) ftp or fast links • Correlate and post on web – Start correlating immediately (not all data needed) – Fringe in a few secs; web post within minutes • Semi-automatic operation • Routine for all LBA observations – Setup fringe tests for all observations – http://pentane.ssi.swin.edu.au/~cphillip/ Increased LBA reliability and robustness Network connectivity -1 • See talk by Shaun Amy • AARNet3 Regional Network • Fibre tails to ATNF antennas in 2005-6 – – – – $2M project, funded by CSIRO corporate Fibre “tails” owned by CSIRO “e-vlbi” tests in March 2006 - Official start June 2006! Legal contract problems!! • 2 x 1 Gbps connectivity – 1 operating now; 2nd circuit to be connected • 10 Gbps (x multiple wavelengths) backbone • Good international connectivity AARNet3 Regional Network Network connectivity -2 • Swinburne: 1 Gbps link(s) constructed – Operation delayed by legal problems!! (again) – (10 Gbps link from Parkes?) – Enables software correlator connectivity • Hobart: Fibre links funded and in construction (2006) – 1 Gbps - telescope ---> University – 10 Gbps to AARNet – (BUT Bass-link limited to ~0.5 Gbps?) • WA Connectivity (Cray @ UWA) – CeNTIE: 3 x 1 Gbps BUT closes in 2006! – AARNet3 links planned – Impact on x-NTD? • (Tidbinbilla - NASA: 2 Mbps commercial links First Oz real “e-VLBI” • • • • • • • + Date: 24 August 2006 Antenna: Parkes, Mopra, ATCA Data rate: 128 Mbps (per station) Bandwidth: 2x16 MHz (per station) Processor: Dual AMD server (ie only 2 CPUs) No disk buffering --> “e-VLBI” Time: 10minutes • 1-bas test Parkes-ATCA at 256 Mbps/station Plans - Near term • Transition production VLBI to disk systems + software correlation (2006-7) – Investigate remote-disk recording – Acquire ~$0.5M of disks • Extensive “real” e-VLBI tests – To Swinburne cluster correlator (in 2006) – To JIVE correlator under EXPReS (2006-7) • Data disk formatting issues (LBA - Mk5a) - VSI-E?? – Tests to Haystack/Japan/Global - VSI-E?? • DAS replacement? Special “e-VLBI” Instrument? • Parkes-Mopra- Narrabri – 1 Gbps links installed – 1 Gbps data from 2 x DAS systems – Software correlation (Parkes or ATCA cluster) Real-time VLBI instrument at 1 Gbps – Cf PTI instrument (Parkes -Tid @ 10 MHz BW) • Very popular with non-VLBI specialists – Fast detection observations/surveys – May operate in parallel with disk recording • E.g. correlate 2nd 512 Mbps stream from ATNF antennas Plans - Longer term • CABB - Broadband upgrade of ATCA – 4 Gsamples x (8) bits 32 Gbps streams – 4 IFs per antenna; 8 antennas – Digital Polyphase filters -- > CABB Correlator • ATCA operation in 2007-8 – VLBI capability designed-in (2008?) • Need for VLBI operation: – n x 10 Gbps connections to ATCA (Narrabri) – Broadbanding of Rx systems (Mopra, Parkes) • Narrabri polyphase filters? – Broadband and Fast links from non-ATNF antennas Multiple 10 Gbps inputs & e-VLBI A Wideband Upgrade for the Australia Telescope Compact Array Luneburg Lens Phased Array Luneburg Lens Phased Array 6 * 22m antenna AT Compact Array Basic Configuration Simple Zoom x 0(m) x 1(m) x ρ (m) xM-1(m) X0(m) po(m) 0 p1(m) 1 pρ(m) ρ p M-1(m) M-1 xn FPGA hardware may be completely reprogrammed to produce many different filterbank configurations, as different observations may require. X1(m) M-Point DFT via FFT FFT FIR FFT Multiple Zoom (>2 possible) Xk(m) XM-1(m) DMUX A 2GHz bandwidth polyphase digital filterbank with 4096 channels ... RF, IF and Baseband Signal Path FIR Filterbank Fringe Rotators Correlator s ... will fit into four XC2V6000 FPGAs Filterbank Architecture Compound Zoom Summary • S2 tape LBA system to be decommissioned 2006-7 • LBADR - disk recorder developed • Software correlation - “real time” speeds – Very versatile, robust and portable • LBA transition: disk recording + software correlation • Digital DAS - need to augment/replace • 1 Gbps links to ATNF antennas operating – Links to correlator and other telescopes in construction • First “real” e-VLBI tests successful • Plans for eVLBI instrument (Pks-Mop-Nar) • Future: 10 Gbps links + CABB correlator