Technology and Functionality of the EVLA Correlator (Next Corr Workshop, June 27, 2006)

Slides:



Advertisements
Similar presentations
Maciej Gołaszewski Tutor: Tadeusz Sondej, PhD Design and implementation of softcore dual processor system on single chip FPGA Design and implementation.
Advertisements

Digital RF Stabilization System Based on MicroTCA Technology - Libera LLRF Robert Černe May 2010, RT10, Lisboa
David Hawkins Exascale Signal Processing for Millimeter-Wavelength Radio Interferometers David Hawkins
DATA TRANSMISSION SYSTEM MIKE REVNELL. OUTLINE Top level specifications Basic architecture Fiber plant DTS module Digitizers Formatter Deformatter Transition.
Prototype SKA Technologies at Molonglo: 3. Beamformer and Correlator J.D. Bunton Telecommunications and Industrial Physics, CSIRO. Australia. Correlator.
Programmable logic and FPGA
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Cross Correlators Walter Brisken.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Digital Signal Processing.
The ALMA Correlator Gianni Comoretto, J.C. Webber, A. Baudry, C.M. Broadwell, R. P. Escoffier, J.H. Greenberg, R.R. Treacy, P. Cais, B Quertier, P. Camino,
Programmer’s Guide to the EVLA Correlator B. Carlson EVLA Correlator S/W F2F Apr. 3-4, 2006.
The Prototype Correlator Sonja Vrcic Socorro, 5. December, 2006.
ASKAP Signal Processing Overview DIFX Users and Developers Meeting
Electronics for PS and LHC transformers Grzegorz Kasprowicz Supervisor: David Belohrad AB-BDI-PI Technical student report.
Technical Benefits and Difficulties B. Carlson July 31, 2007.
EVLA Early Science: Shared Risk Observing EVLA Advisory Committee Meeting, March 19-20, 2009 Claire Chandler Deputy AD for Science, NM Ops.
Systems Integration and Testing EVLA Advisory Committee Meeting, March 19-20, 2009 Jim Jackson Systems Engineer.
DLS Digital Controller Tony Dobbing Head of Power Supplies Group.
FPGA-based Dedispersion for Fast Transient Search John Dickey 23 Nov 2005 Orange, NSW.
IVS-4th General Meeting, Concepción- Chile, Jan 2006 DBBC - A Flexible Platform for VLBI Data Process G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di.
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
JVLA capabilities to be offered for semester 2013A Claire Chandler.
© ASTRON On the Fly LOFAR Station Correlator André W. Gunst.
Australian Astronomy MNRF Development of Monolithic Microwave Integrated Circuits (MMIC) ATCA Broadband Backend (CABB)
EVLA Correlator Prototype and OTS Testing B. Carlson EVLA Correlator S/W F2F Apr 3-4, 2006.
EVLA Corr Racks/Cables etc. B. Carlson EVLA Correlator F2F Meeting Dec , 2007.
An FX software correlator for VLBI Adam Deller Swinburne University Australia Telescope National Facility (ATNF)
The Correlators ( Spectrometers ) Mopra Induction - May 2005.
Lecture 12: Reconfigurable Systems II October 20, 2004 ECE 697F Reconfigurable Computing Lecture 12 Reconfigurable Systems II: Exploring Programmable Systems.
Brent CarlsonEVLA System PDR (Correlator V2) December 4-5, Correlator.
1 SAGE Committee Meeting – December 19 & 20, 2008 National Radio Astronomy Observatory Correlator Status and Growth of Capabilities Michael P. Rupen Project.
Station Board Testing EVLA Correlator S/W F2F 3-4 April 2006 D. Fort.
18-19 July, 2002Correlator Backend System OverviewTom Morgan 1 Correlator Backend System Overview Tom Morgan, NRAO.
Configuration Mapper Sonja Vrcic Socorro,
VLBA Implementation of the ROACH Digital Backend Jonathan Romney on behalf of the VLBA Upgrade development team NRAO / Socorro First International VLBI.
A real-time software backend for the GMRT : towards hybrid backends CASPER meeting Capetown 30th September 2009 Collaborators : Jayanta Roy (NCRA) Yashwant.
New Technologies for Future VLBI Correlators B. Carlson High Res. Astronomy, June 8-12, 2003 Socorro NM.
Philippe Picard 2 nd SKADS Workshop October 2007 Station Processing Philippe Picard Observatoire de Paris Meudon, 11th October 2007.
ATCA GPU Correlator Strawman Design ASTRONOMY AND SPACE SCIENCE Chris Phillips | LBA Lead Scientist 17 November 2015.
Overview of New Connectivity Scheme for the EVLA Correlator B. Carlson July 31, 2007.
M.P. RupenEVLA Advisory Committee Meeting September 6-7, Correlator Test Plan Michael P. Rupen.
XLV INTERNATIONAL WINTER MEETING ON NUCLEAR PHYSICS Tiago Pérez II Physikalisches Institut For the PANDA collaboration FPGA Compute node for the PANDA.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Correlator Specifications Michael P. Rupen.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Scientific Impact Michael P. Rupen.
Raw Status Update Chips & Fabrics James Psota M.I.T. Computer Architecture Workshop 9/19/03.
Software Requirements for the Testing of Prototype Correlator Sonja Vrcic Socorro, December 11, 2007.
Master Correlator Control Computer (MCCC) Requirements & Status Sonja Vrcic Socorro, December 12, 2007.
M.P. Rupen, Synthesis Imaging Summer School, 18 June Cross Correlators Michael P. Rupen NRAO/Socorro.
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA Correlator.
SAGE meeting Socorro, May 22-23, 2007 WIDAR Correlator Overview Michael P. Rupen Project Scientist for WIDAR & Software.
FP7 Uniboard project Digital Receiver G. Comoretto, A. Russo, G. Tuccari, A Baudry, P. Camino, B. Quertier Dwingeloo, February 27, 2009.
WIDAR Correlator Options and Potential Craig Walker NRAO Socorro U.S. VLBI Technical Coordination Meeting May 14-15, 2007.
Software Overview Sonja Vrcic
Mark 5 / VLBA Correlator Topics
The UniBoard Generic Hardware for Radio Astronomy Signal Processing
EVLA Availability - or - When Can I Use It?
EVLA Advisory Committee Meeting System Status
EVLA NSF Mid-Project Review System / Antenna Status
EVLA Correlator F2F Meeting Dec , 2007
EVLA NSF Mid-Project Review System / Antenna Status
EVLA Correlator New Connectivity Scheme Software Impact Sonja Vrcic
EVLA System PDR System Overview
Rick Perley National Radio Astronomy Observatory
Shared Risk Observing Claire Chandler EVLA SSS Review, June 5, 2009
EVLA Advisory Committee Meeting System Status
Prototype Correlator Testing
The Uniboard  FPGA Processing for Astronomy
Correlator Growth Path
VLA EXPANSION PROJECT Correlator Issues.
EVLA Advisory Panel Mtg. System Overview
Programmable logic and FPGA
Presentation transcript:

Technology and Functionality of the EVLA Correlator (Next Corr Workshop, June 27, 2006)

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Outline EVLA project overview. Correlator capabilities. Correlator architecture. Technology. Schedule.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 EVLA Project Overview NRAO: –Upgrade VLA from the current ~100 MHz BW to 16 GHz (8 GHz/pol’n). –New receivers: 1-50 GHz contiguous frequency coverage. –Replace waveguide system with digital fiber system. –3-bit (8x2 GHz) and 8-bit (4x1 GHz) sampling. New correlator (NRC Canada).

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Correlator Capabilities 16 GHz/antenna (8 GHz/poln). 32-antenna system…expandable. Can tradeoff BW for #ants and #beams; can proc multiple narrow (<1 GHz) bands; VLBI ready. 3/8-bit ADC (at antenna), 4/7-bit re-quantization and correlation…more bits/less BW possible. All digital +/-1/32 sample delay tracking; 0.26 sec delay range. 3-level phase rotation in correlator chip: sub-sample delay, LO offset removal, earth-rotation phase, bias/birdie/aliasing de-correlation.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Correlator Capabilities 16k channels/baseline wideband; up to 4 Mchannels/baseline narrowband with “recirculation”. Up to 144 tunable multi-stage digital filters per antenna…’slot’ restrictions in 1 st stage of filter. Use filter logic for sub-band multi-beaming and/or narrowband delay. ~60 dB spectral dynamic range. “WIDAR” technique (hybrid).

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Correlator Capabilities High-speed pulsar phase binning; 2000 bins/product, min ~15 usec bin width. High-speed dumping. 1 Gbps Ethernet/board standard. Up to 10 Gbps/board. 25 Mbytes/sec to archive. All digital phased output…1 GHz…expandable to full BW. Unlimited sub-arrays. Multiple VSI I/O. Configurable for virtually any radio telescope configuration…including auto- correlation. Uses VLBI standard frequencies (256 MHz…). Can incorporate VLBA into “excess” correlator capacity.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Correlator Architecture Station Board: –6U Fiber receiver mezzanine card (NRAO). –Cross-bar switch FPGA. –Delay module mezzanine card (+/-0.5 samples delay). –Wideband autocorrelator. –Multi-stage digital filters (1 FPGA per sub-band). Cross-bar switch and sub-and multi-beaming delay memory. 4 stages…128 MHz…31.25 kHz BW out. Power measurements for sub-band stitching. Real-time RFI blanking per sub-band. CPU-settable scaling factors/re-quantization for max sensitivity/dynamic range. State counts, lag-0 power, phase-cal. Narrowband sub-sample delay with 16-step FIR interpolation. –Cross-bar switch and mux to 1 Gbps for data transport to Baseline Board.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Correlator Architecture Fanout Board: –Dual 1-8 fanout of signals (4-wafer ‘stack’, 1 sub-band, all basebands, one antenna) for baseline rack signal distribution. Baseline Board: –8x8 matrix of corr chips fed by 8 ‘X’ and 8 ’Y’ FPGAs (recirculation, phase generation, 7-bit handling, cross-bar). –Corr chip: 2048 c-lags, in c-lag “cells”. Full 4-bit multiply, no trunc,  sec int. Cells can be concatenated. –Dedicated LTA FPGA +256 Mbit RAM for each corr chip; high- speed phase binning and recirculation. –Output 1 Gbps Ethernet via FPGA. –Can set corr chip and board for autocorr mode: 64 independent 2048 channel, 128 MHz autocorrelations. –Can process up to 32 stations (1024 correlations), 128 MHz, 1 poln product, at 64 channels/baseline.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Technology Use Xilinx Virtex-IV, and Altera Stratix II/GX/Cyclone FPGAs. Standard cell correlator chip, 4 million gate, 0.13  m. PD~3.7 W 256 MHz, 1 V. Use ‘Accel’ point-of-load reg to minimize power, track chip speed with time. BGA packages throughout, some gull-wing memories/drivers.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Technology 8 different boards in total: Station Board, Baseline Board: 12U x 400 mm, 28 layer, ” trace-’n- space, 0.125” thick. Phasing Board: ~6U x 160 mm(?). Fanout Board: 6U x 100 mm, with re-sync Stratix II FPGA. Common Backplane/midplane (3U x 25 mm); signal I/O, power, ID…used everywhere…no monolithic backplanes. HM 2.0 mm straight-thru. All press- fit. Delay module (~5”x3.5”)mezzanine card: FPGA+DDR SDRAMs PC/104+ COTS CPU + PCMC card. RPMIB (very simple; diodes, optos) for rack/fan power monitor and control

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Technology 1 Gbps station-baseline data transport on high-density Meritec 2 mm hardmetric cable assemblies. Make correlator highly configurable for various correlator configurations (e.g. e- MERLIN). Use Altera’s 1 Gbps mux/demux with dynamic phase alignment…built into Stratix chips. About 500 rack-to-rack cables, 2500 intra-rack cables (<1 m) in EVLA correlator. All cables plug into 3U x 25mm Common Backplane.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Baseline Board (12Ux400 mm) PCB-back

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Baseline Board PCB-front

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Thermal vias “pocket” for corr chip heatsink

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Technology Use central -48 VDC COTS power supply, DC-DC supplies on each board. Provides battery backup (5 min req). 24, 24” racks (2.5’ x 3’ x 7’), each one holding up to 16 large boards in two crates, and Fanout Boards in 6U crate. All hot-swappable, including fans. On-line detection of communications errors, temps, voltages…remote shutdown/power cycle of any board through central PXI chassis/CPU.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Thermal mock- up test rack

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Technology Software: –Embedded PC/104+ COTS CPU on each large board. Cheap, fast, easily available, easily replaceable, many vendors. –RT Linux…”Unix-style” device drivers. –System…board…chip-level GUIs for initial testing. Useful during operations for continued debugging, low-level access. –MCCC—central host computer maps high-level requests from EVLA M&C to embedded processors, via XML messages. –CPCC—central power control computer. –Backend—array of COTS PCs connected to Baseline Boards via commercial GigE switches.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Schedule Slipped about 1.5 yrs from original 2001 schedule…various reasons. 10 proto corr chips arrived June 20/06. Baseline Board…probably August/06…some PCB fab problems have delayed delivery. Station Board…signed-off design for fab quotation…probably get assembled board late September/06. Depending on how well testing goes: –1 st prototype corrs at VLA/Jodrell Bank…mid ’07. –Full production mid Full installation early –Turn off old correlator end of 2009.

Next Gen Corr Workshop: EVLA Correlator—Carlson June 27, 2006 Summary Response Type of correlations: all Output req: spectral + continuum Special processing req: tunable sub-bands, high spec res, pulsar, 4/7-bit corr, RFI blanking/robust; RFI excision in backend CPUs eventually; possible RT RFI cancel. Input BW + digitization: 8x2GHz 3-bit; 4x1GHz 8-bit; dedicated fiber I/F on mezzanine card; Other BW/digitization supported; VSI I/O. #spec channels at max BW: 16k, increases by 2X with each decrease in BW by ½. #baselines correlated: 528 baselines, 163,840 cross-corrs Integration times: min ~15 usec with binning. 11 msec standard…scalable with backend and O/P link; unlimited max. Dynamic range: ~60 dB spectral. Scale: large, near limits of technology but not “bleading edge”. Technology: FPGAs, custom hardware, 1 ASIC, COTS CPUs/network, standard form factor. Scalability: unlimited but high flexibility not necessarily best approach for ‘large N’. 4X baselines possible with new ASIC, same architecture. Flexibility: high: BW/Nant/Nchan/Nbeam/Nbits; RT, nRT VLBI, auto, connected element, integration/dumping independent of system timing. Architecture: “WIDAR” (hybrid XF). RFI mitigation: Nbits, RT blanking, high dynamic range.