M.P. RupenCorrelator Connectivity Scheme Review 31 July 2007 1 Correlator Specifications Michael P. Rupen.

Slides:



Advertisements
Similar presentations
E-VLBI down-under Tasso Tzioumis ATNF, CSIRO July 2005 Towards e-VLBI.
Advertisements

Thirteenth Synthesis Imaging Workshop 2012 May 29– June 5 Planning VLA Observations: Tutorial Michael P. Rupen NRAO/Socorro.
David Hawkins Exascale Signal Processing for Millimeter-Wavelength Radio Interferometers David Hawkins
RFI Subtraction with a reference horn… F. Briggs & M. Kesteven illustrations from Parkes Telescope… (Jon Bell et al.) origins in Int-Mit group at CSIRO.
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.
DBBC3 Development - Digital Base-Band Converter 3
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Cross Correlators Walter Brisken.
HIAPER Cloud Radar Transceiver Exciter Receiver Oscillators High-Powered Amplifier Calibration Exciter Receiver Oscillators High-Powered Amplifier Calibration.
Cross-correlators for Radio Astronomy
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.
Backend electronics for radioastronomy G. Comoretto.
Eleventh Synthesis Imaging Workshop Socorro, June 10-17, 2008 Cross Correlators & New Correlators Michael P. Rupen NRAO/Socorro.
EVLA Correlator P. Dewdney Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysics National Research Council Canada.
GBT Spectral Baselines – Tuesday, 11 March 2003 GBT Spectral Baseline Investigation Rick Fisher, Roger Norrod, Dana Balser (G. Watts, M. Stennes)
Digital Filters Mike Davis. Requirements Avoid non-linearity up to and through the analog to digital (A/D) converter Use enough bits to adequately represent.
1 of 20 Z. Nikolova, V. Poulkov, G. Iliev, G. Stoyanov NARROWBAND INTERFERENCE CANCELLATION IN MULTIBAND OFDM SYSTEMS Dept. of Telecommunications Technical.
From Idea to ALMA Project James Di Francesco Herzberg Institute of Astrophysics North American ALMA Science Center (thanks to Mike Rupen, Gianni Comoretto.
EVLA Early Science: Shared Risk Observing EVLA Advisory Committee Meeting, March 19-20, 2009 Claire Chandler Deputy AD for Science, NM Ops.
Technology and Functionality of the EVLA Correlator (Next Corr Workshop, June 27, 2006)
10 January 2006AAS EVLA Town Hall Meeting1 The EVLA: A North American Partnership The EVLA Project on the Web
Advances In Millimeter Wave Measurements Banded Differential and Pulse Measurements.
Introducing the EVLA NRAO Postdoctoral Symposium, 29 April-1 May 2009 Michael P. Rupen Project Scientist for WIDAR.
April 19, 2007 EVLA Update1 The EVLA Project An Update Rick Perley National Radio Astronomy Observatory.
1 SAGE Committee Meeting – December 19 & 20, 2008 National Radio Astronomy Observatory EVLA Goals, Progress, Status, and Projections Rick Perley Mark McKinnon.
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
EVLA Correlator P. Dewdney Dominion Radio Astrophysical Observatory Herzberg Institute of Astrophysics National Research Council Canada.
JVLA capabilities to be offered for semester 2013A Claire Chandler.
Casper 2010Marc Torres Part 2: Building blocks for the next generation.
Australian Astronomy MNRF Development of Monolithic Microwave Integrated Circuits (MMIC) ATCA Broadband Backend (CABB)
Adaptive Filters for RFI Mitigation in Radioastronomy
The Correlators ( Spectrometers ) Mopra Induction - May 2005.
Brent CarlsonEVLA System PDR (Correlator V2) December 4-5, Correlator.
Tenth Synthesis Imaging Summer School UNM, June 13-20, 2006 Cross Correlators Walter Brisken.
1 SAGE Committee Meeting – December 19 & 20, 2008 National Radio Astronomy Observatory Correlator Status and Growth of Capabilities Michael P. Rupen Project.
Rick Perley 2 Nov 2001 EVLA Correlator Conceptual Design Review 1 Science Drivers for the EVLA Correlator Rick Perley EVLA Project Scientist 2 Nov 2001.
M.P. RupenCorrelator Face-to-Face Meeting 31 Oct 2006 Output Formats Part II Michael P. Rupen.
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.
Rick PerleyEVLA Advisory Committee Meeting September 6-7, 2007 Some Illustrative Use Cases Rick Perley.
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.
M.P. RupenCorrelator Connectivity Scheme Review 31 July Scientific Impact Michael P. Rupen.
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.
JIVE UniBoard Correlator External Review
Surveying Cosmic Time with the WIDAR Correlator
Mark 5 / VLBA Correlator Topics
EVLA Availability - or - When Can I Use It?
JIVE UniBoard Correlator (JUC) Firmware
Correlator – Backend System Overview
EVLA Correlator New Connectivity Scheme Software Impact Sonja Vrcic
EVLA Status and Prospects
EVLA System PDR System Overview
Rick Perley National Radio Astronomy Observatory
Observational Astronomy
Observational Astronomy
Shared Risk Observing Claire Chandler EVLA SSS Review, June 5, 2009
Some Illustrative Use Cases
Prototype Correlator Testing
Shared Risk Science with the EVLA
Correlator Growth Path
VLA EXPANSION PROJECT Correlator Issues.
EVLA Advisory Panel Mtg. System Overview
Presentation transcript:

M.P. RupenCorrelator Connectivity Scheme Review 31 July Correlator Specifications Michael P. Rupen

M.P. RupenCorrelator Connectivity Scheme Review 31 July Principle Requirements 32 stations, scaleable in 8-station increments; up to 256 allowed 8 x 2 GHz “basebands”, each comprised of 16 tunable sub-bands 16,384 channels per max. BW 4 million channels per baseline, w/ recirculation High spectral dynamic range 1, 2, 3, 4, or 8-bit initial quantization; 4- or 7-bit after sub-band filter

M.P. RupenCorrelator Connectivity Scheme Review 31 July Sub-bands and recirculation Sub-band BW: 128, 64, 32 MHz, …, kHz Sub-bands in integer 128/64 MHz slots (but note baseband tuning) Seamless (cross-correlation) sub-band stitching Recirculation on 4 of 8 sub-band pairs Max. recirculation factor= 256 (?) Wideband recirculation

M.P. RupenCorrelator Connectivity Scheme Review 31 July Phased Array 1 GHz phased-VLA capability (8 sub- bands, 32 antennas)  Up to 16 GHz with more money  8-bits  4 sub-bands on 64 antennas  Can be fed back into WIDAR…  Simultaneous with “normal” same phase center

M.P. RupenCorrelator Connectivity Scheme Review 31 July VLBI VLBI-ready  Max. baseline 25,000 km  Ability to accept and produce VSI  Trade bandwidth for antennas (see later)  “Two correlators in one”: could correlator VLBA at the same time

M.P. RupenCorrelator Connectivity Scheme Review 31 July Auto-correlations etc. Auto-correlations Wideband 4x1024 channels (64-lag chunks every 10 msec) Sub-band as cross-corr’ns (up to 16,384 channels per antenna) Pre-filter Wideband state counts, auto-correlation (time-multiplexed) Post-filter, pre-requantizer Power (binned by noise tube ON/OFF) Post-requantizer Power Phase cals State counts Lag zero

M.P. RupenCorrelator Connectivity Scheme Review 31 July Pulsar Processing Pulsar processing  2 banks of 1000 bins each per baseline  Up to 65,536 bins per baseline in S/W  Bins as narrow as 200 microsec (all channels), or 15microsec with 64 channels/sub-band/baseline  Gating with one time+multi-gate generator per 2 GHz baseband  Can gate with different delays per sub-band Phased array output as previously described

M.P. RupenCorrelator Connectivity Scheme Review 31 July Dump time & data rate Min. dump time: 100 msec with all channels (set by CBE)  Absolute minimum ~60 microseconds Max. dump time: unlimited Correlator Backend (CBE) I/O  Input: 1.6 GB/s  Output: 25 MB/s  N.B. CBE limited by I/O, not by processing power

M.P. RupenCorrelator Connectivity Scheme Review 31 July Sub-arrays and low- bandwidth stations Sub-arrays  Unlimited for cross-correlations  4 phased-array sub-arrays with complete flexibility in antenna selection 16 GHz stations tradeable for 2x4 GHz (Nchan/4) or 4x1 GHz (Nchan/16)

M.P. RupenCorrelator Connectivity Scheme Review 31 July RFI Excision RFI excision  Sub-band power over-range detection & blanking  Post-corr’n cancellation (CBE)  Excision based on autocorr’ns

M.P. RupenCorrelator Connectivity Scheme Review 31 July Flexibility  Single or dual pol’n BB pairs  1, 2, or 4 polarizations/sub-band  Mixed high and low BW antennas  Each sub-band can be 4- or 7-bit  Recirculation available in 4 of 8 sub-band pairs  Each sub-band can have its own BW & (where applicable) recirculation factor FIR filters Radar mode: two kHz 8-bit sub-bands; wider BW with fewer bits