MeerKAT DBE Past Present Future Alan Langman 28 September 2009.

Slides:



Advertisements
Similar presentations
1 National Radio Astronomy Observatory The EVLA -- Status, Future Rick Perley National Radio Astronomy Observatory.
Advertisements

SKA New Technology Demonstrator Ray Norris CSIRO Australia Telescope National Facility.
The Karoo Array Telescope Adrian Tiplady v1.0, v1.1, v2.0, v2.1 …
SKAMP Square Kilometre Array Molonglo Prototype. Supporting Institutions  University of Sydney  Argus Technologies  ATNF  ICT Centre.
// RF Transceiver Design Condensed course for 3TU students Peter Baltus Eindhoven University of Technology Department of Electrical Engineering
SADC HPC Workshop, 2 Dec 2013, Cape Town
Antennas for MeerKAT March TDP AWG, 13-14/3/08, San Francisco MeerKAT Semantics K.A.T. = Karoo Array Telescope –KAT is Afrikaans for cat –MeerKAT:
Digital FX Correlator Nimish Sane Center for Solar-Terrestrial Research New Jersey Institute of Technology, Newark, NJ EOVSA Technical Design Meeting.
AAVS receiver Federico Perini AAVP December, ASTRON, Dwingeloo.
All things DBE… Francois Kapp Sub-system Manager: DBE On behalf of the DBE team present and past... S Rajan, E Bauermeister, A.
SKA South Africa Overview Thomas Kusel MeerKAT System Engineering Manager April 2011.
Probing the field of Radio Astronomy with the SKA and the Hartebeesthoek Radio Observatory: An Engineer’s perspective Sunelle Otto Hartebeesthoek Radio.
SKAMP - the Molonglo SKA Demonstrator M.J. Kesteven CSIRO ATNF, T. J. Adams, D. Campbell-Wilson, A.J. Green E.M. Sadler University of Sydney, J.D. Bunton,
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array DBE Implementation.
Advances in Plasma Astrophysics, Giardini-Naxos, 6-10 Sept D Modeling of Solar Flaring Loops New Interactive Solar Flare Modeling and Advanced Radio.
BDT Radio – 2b – CMV 2009/10/09 Basic Detection Techniques 2b (2009/10/09): Focal Plane Arrays Case study: WSRT System overview Receiver and.
Polar Loop Transmitter T. Sowlati, D. Rozenblit, R. Pullela, M. Damgaard, E. McCarthy, D. Koh, D. Ripley, F. Balteanu, I. Gheorghe.
Prototype SKA Technologies at Molonglo: 3. Beamformer and Correlator J.D. Bunton Telecommunications and Industrial Physics, CSIRO. Australia. Correlator.
Signal Processing for Aperture Arrays. AAVS1 256 antenna elements distributed over –4 stations –64 elements each.
National Astronomy and Ionosphere Center © Germán Cortés M 2008 SKA TDP Antenna Optics By Germán Cortés M. Cornell University Ithaca NY 14853, USA National.
What’s Going on in Canada?
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Digital Signal Processing.
HIAPER Cloud Radar Transceiver Exciter Receiver Oscillators High-Powered Amplifier Calibration Exciter Receiver Oscillators High-Powered Amplifier Calibration.
SKA-Japan Industry Forum [SKA-Japan Workshop 2010] EMC & Microwave Systems November 05, 2010.
VLBI in Africa Michael Bietenholz Hartebeesthoek Radio Observatory.
Highly Scalable Packetised correlators Jason Manley CASPER workshop 2009.
GNSS Receiver - Software Radio Concept František Vejražka Czech Technical University in Prague Faculty of Electrical Engineering.
SKA Introduction Jan Geralt Bij de Vaate Andrew Faulkner, Andre Gunst, Peter Hall.
Road to MeerKAT KAT-7 DBE Alan Langman. meerKAT Overview Objectives of meerKAT Location Location Location MeerKAT Engineering Specification Prototypes.
An African VLBI network of radio telescopes as an SKA precursor Michael Gaylard Hartebeesthoek Radio Astronomy Observatory (HartRAO) P. O. Box 443, Krugersdorp.
Rosie Bolton1 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKADS Costing work: Spreadsheets to scalable designs Rosie Bolton Dominic.
CRISP & SKA WP19 Status. Overview Staffing SKA Preconstruction phase Tiered Data Delivery Infrastructure Prototype deployment.
Polarimetric Solid State Radar Design for CASA Student Test Bed
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
Next Generation Digital Back-ends at the GMRT Yashwant Gupta Yashwant Gupta National Centre for Radio Astrophysics Pune India CASPER meeting Cambridge.
JVLA capabilities to be offered for semester 2013A Claire Chandler.
2 nd convergence workshop: introduction R. T. Schilizzi Penticton 22 July 2004.
Phase and Gain stability of optical fibre link used in MeerKAT Author : Roufurd Julie Supervised by : Prof Michael Inggs SKA HCD bursary conference Dec.
SKA System Design Kobus Cloete 9 December 2010 AAVP Workshop "Exploring the Universe with the world's largest radio telescope"
CASPER Packetised correlators Jason Manley CASPER workshop 2009.
Integrated receivers for mid-band SKA Suzy Jackson Engineer, Australia Telescope National Facility SKADS FP6 Meeting – Chateau de Limelette – 4-6 November,
Andrew Faulkner 2 nd SKADS Workshop October 2007 SKADS Benchmark Scenario Andrew Faulkner.
Australian Astronomy MNRF Development of Monolithic Microwave Integrated Circuits (MMIC) ATCA Broadband Backend (CABB)
S.Montebugnoli BEST 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Stelio Montebugnoli IRA -INAF- Bologna –Italy- SKADS 4th -Lisbon- Oct 2-3, 2008.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Phased Array Feed Development.
Jason Manley, Aaron Parsons, Don Backer, Henry Chen, Terry Filiba, David MacMahon, Peter McMahon, Arash Parsa, Andrew Siemion, Dan Werthimer, Mel Wright.
Large Area Surveys - I Large area surveys can answer fundamental questions about the distribution of gas in galaxy clusters, how gas cycles in and out.
A Modular K-Band Focal Plane Array for the Green Bank Telescope Matt Morgan National Radio Astronomy Observatory 9/28/2007.
VLBI2010 Phase Calibration Signal Generator and Broadband Considerations Christopher Beaudoin Research Engineer MIT Haystack Observatory.
Australian SKA Pathfinder (ASKAP) David R DeBoer ATNF Assistant Director ASKAP Theme Leader 06 November 2007.
Summary of the Paris SKA Meeting 4-8 September 2006 R. T. Schilizzi.
Andrew Faulkner1 DS4 Deliverables 4 th SKADS Workshop, Lisbon DS4 Deliverables Andrew Faulkner.
Review of developments in Australasia and mainland Asia Steven Tingay Swinburne University of Technology Next Generation correlator meeting, JIVE 27 -
A real-time software backend for the GMRT : towards hybrid backends CASPER meeting Capetown 30th September 2009 Collaborators : Jayanta Roy (NCRA) Yashwant.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Correlator Specifications Michael P. Rupen.
Netherlands Institute for Radio Astronomy 1 APERTIF beamformer and correlator requirements Laurens Bakker.
SAGE meeting Socorro, May 22-23, 2007 WIDAR Correlator Overview Michael P. Rupen Project Scientist for WIDAR & Software.
Netherlands Institute for Radio Astronomy 1 ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) Square Kilometer Array Low Central.
Medichats 14 October 2008 ADC bit number and input power needed, in new radio-astronomical applications View of the Medicina Radiotelescopes - Italy Eng.
Mid Frequency Aperture Arrays
EVLA Availability - or - When Can I Use It?
Modern Interferometric Arrays
Multifunctional Digital Backend (MDBE) for "Quasar" VLBI-network
Phased Array Feeds Wim van Cappellen
Lessons from CASPER Correlators at GMRT
5 Gsps ADC Developement and Future Collaboration
Rick Perley National Radio Astronomy Observatory
Analysis of Adaptive Array Algorithm Performance for Satellite Interference Cancellation in Radio Astronomy Lisha Li, Brian D. Jeffs, Andrew Poulsen, and.
Correlator Growth Path
KFPA CDR R. Norrod Feb 27, 2008.
Presentation transcript:

MeerKAT DBE Past Present Future Alan Langman 28 September 2009

Overview Objectives of MeerKAT MeerKAT Phase XDM KAT-7 –ROACH/katADC –Fringe Finder MeerKAT Conclusions 2

Objectives of MeerKAT Build a world class radio telescope (up to 80 dishes) Choose a frequency range that is likely to have high science impact. Commission a 7 dish system from end of 2010, engineering risk mitigation and do some early science. Train a new generation of scientists and engineers who are capable to participate in large international projects, such as the SKA. Provide an excellent facility for local and international scientists. Implement mission-driven innovation to mobilise industry, academia and research fraternity. SKA pathfinder (precursor) 3

Definitions 4

KAT element MeerKAT 5

SKA-SA: MeerKAT Phases XDM (Done) Single Antenna HARTRAO (PED) KAT7 (7 antennas Karoo) Fringe Finder Phase 1 KAT7 Optimization/Learning?? MeerKAT (80 Antennas Karoo)

eXperimental DeMonstrator 7

Requirements Initially FPA/Multiple Feed (7 feeds) Spectrometer –256MHz bandwidth –2K channels –Minimum 100us dump time Radiometer Histogram 8

XDM: Plan A 9 ATX12 Power Relax Component Placement Focus gateware and firmware on XDM Requirements

XDM: Plan B

First Casper Solution 11

XDM Results 08/27/08

meerKAT-7 13

Key Requirements Input signal –72->328MHz, -27dBm (max 0dBm), NF=40dB Correlator/Beamformer – a) 1 band with total bandwidth >= 256MHz covering the whole input frequency range, with equi-spaced channels of at least 1 MHz bandwidth each –(b) 1 (goal 2 or 4) bands with total bandwidth >= 3.5 MHz selected from anywhere in the input frequency range, with equi- spaced channels of <= 10.7 kHz bandwidth each –(c) 1 (goal 2 or 4) bands with total bandwidth >= 580 kHz selected from anywhere in the input frequency range, with equi- spaced channels of <= 530 Hz bandwidth each 14

KAT-7 Block Diagram 15

Key Component ROACH 16

katADC (production) 17

katADC Prelim results 18

Mechanical Enclosure 19

Detailed Design 20

Key Component ROACH 21

Production (always fun) 22

Stress testing tool chain 23 Million channels, 512MHz BW, Single ROACH

Fringe Finder -Risk Mitigation Fringe Finder (same base specs as KAT- 7) – End of 2009 Single baseline dual polarized correlator Quad baseline single polarization correlator. 100ms dump time. 24

Physical Solution 25

FF Signal Flow 26

Yet another PoCo 27

Towards KAT-7 (Casper Collab) 28

MeerKAT Key Specs 29 MetricKAT-7MeerKAT Pre-SAC MeerKAT Post-SAC F low 1.2 GHz700 MHz580 MHz F high 1.95 GHz10 GHz15 GHz A e /T sys 16 m 2 /K200 m 2 /K DR imag 30 dB60 dB DR spec 30 dB50 dB Xpol-20 dB-25 dB BW256 MHz1 024 MHz (2 048 MHz) MHz (4 096 MHz) N chan ? T int <1 s0.1 ms

MeerKAT Phasing KAT Phase Phase Phase Phase F low 1.2 GHz0.9 GHz 8 GHz 0.9 GHz 8 GHz 0.58 GHz 8 GHz F high 1.95 GHz1.75 GHz 14.5 GHz 1.75 GHz 14.5 GHz 2.5 GHz 14.5 GHz BW RF 256 MHz850 MHz2 GHz 4 GHz ADC800 MSa/s5 GSa/s 10 GSa/s BW DIG 256 MHz850 MHz2 GHz 4 GHz B min 20 m B max 200 m10 km 50 km 30

MeerKAT Phasing KAT Phase F low 1.2 GHz0.9 GHz F high 1.95 GHz1.75 GHz BW RF 256 MHz850 MHz ADC800 MSa/s5 GSa/s BW DIG 256 MHz850 MHz B min 20 m B max 200 m10 km 31

Block Diagram 32

Key Challenges Digitization – Feed, Back Dish, Pedestal or correlator room Distributed correlator architecture Timing and synchronization Array Process/Backend Processor 33

Conclusions Road to MeerKAT XDM KAT-7 ROACH development Fringe Finder Risk Mitigation MeerKAT challenge 34

Questions?