Update on LBA Technical Developments CASS Chris Phillips 11 October 2013.

Slides:



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

E-VLBI Progress with the LBA Chris Phillips, eVLBI Project Scientist November 2011.
Digital FX Correlator Nimish Sane Center for Solar-Terrestrial Research New Jersey Institute of Technology, Newark, NJ EOVSA Technical Design Meeting.
E-VLBI progress in the South Tasso Tzioumis ATNF, CSIRO September 2006 “Towards e-VLBI”  “e-VLBI”
Baseband Processing and SKA Simulations using Supercomputers: Enhancing Australia‘s radio astronomy facilities and its bid for the SKA Steven Tingay Swinburne.
East Coast Geodetic VLBI Workshop12011 Feb ~ 2.2 – 15 GHz Spanned RF Bandwidth OLD Phase Frequency (GHz) 142 Observing Frequency Bands.
David Hawkins Exascale Signal Processing for Millimeter-Wavelength Radio Interferometers David Hawkins
Prototype SKA Technologies at Molonglo: 3. Beamformer and Correlator J.D. Bunton Telecommunications and Industrial Physics, CSIRO. Australia. Correlator.
DBBC3 Development - Digital Base-Band Converter 3
Ninth Synthesis Imaging Summer School Socorro, June 15-22, 2004 Cross Correlators Walter Brisken.
Xcube Recorder Chris Phillips. X-cube Data Logger 100% COTS hardware recorder 16 Gbps capability – 32 Gbps possible – External replaceable storage modules.
Current LBA Developments Chris Phillips CSIRO ATNF 13/7/2005.
VLBI in Africa Michael Bietenholz Hartebeesthoek Radio Observatory.
Backend electronics for radioastronomy G. Comoretto.
ASKAP Signal Processing Overview DIFX Users and Developers Meeting
DBBC Stutus Report November 2007 G. Tuccari, W. Alef, S. Buttaccio, G. Nicotra, M. Wunderlich.
Mark Bowen Acting Theme Leader – Technologies for Radio Astronomy CSIRO Astronomy and Space Science 14 October 2010 Australia Telescope Users Committee.
LBA Calibrator Survey Chris Phillips eVLBI Project Scientist 23 July 2009.
A Low-Cost Phase Cal Monitor and RFI Spectrum Analyzer for VLBI2010 Mark-5 / Mark-6 using Cheap,COTS Software Defined Radio (SDR) Hardware & Software Gleaned.
 Computer memory is device that is used to store data or programs (sequences of instructions) on a temporary or permanent basis for use in an electronic.
Nov 1, 2011 RN - 1 Jet Propulsion Laboratory California Institute of Technology Implementation Issues and Choices for VLBI data Acquisition System in DSN.
David Cussans/Scott Mandry, NIKHEF, October 2008 TLU v0.2.
Polarization at IRAM Status and Plans S.Guilloteau Laboratoire d’Astrophysique de Bordeaux.
IVS-4th General Meeting, Concepción- Chile, Jan 2006 DBBC - A Flexible Platform for VLBI Data Process G. Tuccari, S. Buttaccio, G. Nicotra - Istituto di.
The ATNF Front End and Back End Groups Presented by Graeme Carrad Assistant Director – Engineering - October 2009 Australia Telescope Users Committee Technologies.
Eleventh Synthesis Imaging Workshop Socorro, June 10-17, 2008 THE VLBA SENSITIVITY UPGRADE Craig Walker, NRAO.
Correlator Growth Path EVLA Advisory Committee Meeting, March 19-20, 2009 Michael P. Rupen Project Scientist for WIDAR.
Nov 3, 2009 RN - 1 Jet Propulsion Laboratory California Institute of Technology Current Developments for VLBI Data Acquisition Equipment at JPL Robert.
GPU DAS CSIRO ASTRONOMY AND SPACE SCIENCE Chris Phillips 23 th October 2012.
Casper 2010Marc Torres Part 2: Building blocks for the next generation.
1 Advanced ATNF Correlators Dick Ferris AT Electronics Development Group May 2003.
The Progress Report for KVN Construction Seog-Tae Han and KVN staffs Korea Astronomy and Space Science Institute March18 th 2009.
Australian Astronomy MNRF Development of Monolithic Microwave Integrated Circuits (MMIC) ATCA Broadband Backend (CABB)
DiFX Performance Testing Chris Phillips eVLBI Project Scientist 25 June 2009.
An FX software correlator for VLBI Adam Deller Swinburne University Australia Telescope National Facility (ATNF)
Future FONT BPM Processors C.Perry 25 June Types of Processor Two types of processor: a) present mixer type b) baseband type Both will be made because:
Jason Manley, Aaron Parsons, Don Backer, Henry Chen, Terry Filiba, David MacMahon, Peter McMahon, Arash Parsa, Andrew Siemion, Dan Werthimer, Mel Wright.
Adaptive Filters for RFI Mitigation in Radioastronomy
The Correlators ( Spectrometers ) Mopra Induction - May 2005.
Brent CarlsonEVLA System PDR (Correlator V2) December 4-5, Correlator.
DiFX New Features. Disk based file specification Improved specification of files to correlate Wild cards with time of scan name filtering? External reference.
Australia Telescope Users Committee Technologies Report - Oct 2008.
VLBA Implementation of the ROACH Digital Backend Jonathan Romney on behalf of the VLBA Upgrade development team NRAO / Socorro First International VLBI.
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.
Giga-bit Geodesy e-VLBI at 22GHz Hiroshi Takaba Gifu University, Japan.
Philippe Picard1EMBRACE station processing SKADS Conference, Limelette, 4-6 November 2009 EMBRACE station processing P. Picard Station de Radioastronomie.
Demonstration of 16Gbps/station broadband-RF VLBI system Alan Whitney for the VLBI2010 development team MIT Haystack Observatory 22 October st Intl.
Collaborative Research Projects in Australia: Radio Astronomy Dr. Greg Wickham (AARNet) Dr Tasso Tzioumis Dr Shaun Amy Dr Chris Phillips (CSIRO ATNF) Global.
ATCA GPU Correlator Strawman Design ASTRONOMY AND SPACE SCIENCE Chris Phillips | LBA Lead Scientist 17 November 2015.
Integration and commissioning of the Pile-Up VETO.
1 Advanced ATNF Correlators Dick Ferris AT Electronics Group.
Atacama Large Millimeter/submillimeter Array Karl G. Jansky Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array ALMA Correlator.
Institute of Applied Astronomy Third International VLBI Technology Workshop, Groningen/Dwingeloo, Netherlands, November 10-13, 2014 Current State of Russian.
VLBI Developments in Australia ASTRONOMY AND SPACE SCIENCE Chris Phillips| LBA Lead Scientist 11 November 2014.
Title FABRIC Progress - Mark, Huib etc. T. Charles Yun Project Manager EXPReS/JIVE.
VGOS GPU Based Software Correlator Design Igor Surkis, Voytsekh Ken, Vladimir Mishin, Nadezhda Mishina, Yana Kurdubova, Violet Shantyr, Vladimir Zimovsky.
WIDAR Correlator Options and Potential Craig Walker NRAO Socorro U.S. VLBI Technical Coordination Meeting May 14-15, 2007.
Future LBO Developments
JIVE UniBoard Correlator External Review
Correlators ( Backend System )
Mark 5 / VLBA Correlator Topics
Chris Phillips.
Concepts for a Next-Generation VLBA
The Development of Broadband VLBI Technologies in SHAO
Testing Multibit Encoding Schemes
EVLA Advisory Committee Meeting System Status
17/04/2019 Future VLBI systems Tasso Tzioumis| Facilities Program Director– Technologies for Radio Astronomy CSIRO Astronomy and Space Science IVTW.
EVLA Advisory Panel Mtg. System Overview
SKAMP Square Kilometre Array Molonglo Prototype
Presentation transcript:

Update on LBA Technical Developments CASS Chris Phillips 11 October 2013

Linear to Circular conversion

Linear Polarizations While VLBI standard is to use circular polarizations, linear polarizations are “better”: Easier to make wideband receivers Better separation between polarizations Need to convert linear to circular for compatibility with other antennas and calibration and analysis software RF and IF hybrids typically narrow band VLBI TECHNOLOGY KOREA - Chris Phillips 3 |

Digital Polarization Conversion Digital polarization conversion can overcome wideband problem Has worked very well with ATCA for 20 years Conceptually easy: Align amplitude, phase and delay between two polarizations Rotate phase of one polarization by 90 degrees Simply add and subtract two linear polarizations Essentially same as hybrids Ideally added to VLBI DAS firmware but never implemented VLBI TECHNOLOGY KOREA - Chris Phillips 4 |

L2C in DiFX Can we do circular conversion within DIFX Very “cheap” to do conversion after FFT in correlator Biggest DIFX change is to get calibration values into correlator Side benefit is polarization dependent delay offset VLBI TECHNOLOGY KOREA - Chris Phillips 5 |

VLBI TECHNOLOGY KOREA - Chris Phillips 6 | FFT Xmult Amplitude & Phase Correction Amplitude & Phase Correction Add and subtract FFT Xmult

Status One session at ASKAP, new receiver installed with linear rather than circular polarizations (no hybrid) ASKAP no noisecal to aid calibration Also very good isolation between polarizations Need to use VLBI cross correlations for calibration Delays well calibrated but problem getting phase difference Seeking help to work out calibration problem VLBI TECHNOLOGY KOREA - Chris Phillips 7 |

Xcube Wideband VLBI Backend

X-cube Data Logger 100% COTS hardware recorder Proprietary software 16 Gbps capability External replaceable storage modules –Up to 32 TB packs Management of slow or broken disks Standard file-systems

Back View of Chassis © 2010 XCube R&D Ethernet (2 x 10Gb/s) SAS Disk Cables (16 x 300MB/s) Self Contained Disk Pack Cooling and Power

Xcube Internals “Mix and Match” approach to plug in devices 1 or 2 dual 10 Gbps Ethernet –Intel SPP+ Optical module needed Can support up to 4 disk modules GPU for number crunching Other options available –However may run out of slots…. VLBI TECHNOLOGY KOREA - Chris Phillips 11 |

Xcube tests Seems to run fine up to around 8 Gbps/diskpack (as advertised) Basic Ethernet recorder, similar to Mark5C However this is NOT a feature Records full Ethernet frame – allows post recording filtering Simple easy to use control program Can control remotely via XML messages Does not allow simultaneous recording and reading Have not started using for operations yet VLBI TECHNOLOGY KOREA - Chris Phillips 12 |

Data access Data cannot be accessed directly Cannot directly use standard transfer software such as ftp, gridftp, tsunami-udp etc Supplied with easy to use library to read data from diskpack Can copy “raw” files and decode on a different system Easy to write code to copy off disk Time filtering etc available not tested VLBI TECHNOLOGY KOREA - Chris Phillips 13 |

Xcube sampler 4 Channel 1 Gsample/sec 4x512 MHz IFs For each IF 16 channel polyphase filterbank 32 MHz channels, complex “double sideband” sampling Re-quantization to 2 bit 8 Gbps VLBI VLBI TECHNOLOGY KOREA - Chris Phillips 14 |

Xcube Issues Only 8 or 4 Gbps modes No channel sub-selection Clumsy quantization threshold setting No automatic gain adjustment No total power monitoring No eVLBI option Initial firmware version had synchronization issues… Fixed now and “zero baseline” fringes to existing LBA DAS VLBI TECHNOLOGY KOREA - Chris Phillips 15 |

VLBI TECHNOLOGY KOREA - Chris Phillips 16 |

Next Steps Working with Xcube to transition to “production” suitable operation Probably combination of Firmware and software changes Roll out at Parkes and ASKAP Mopra when satisfied system is usable ATCA Xcube recorder All digital system VLBI TECHNOLOGY KOREA - Chris Phillips 17 |

ATCA CABB ATCA correlator is now 2x2 GHz (dual pol) 32 Gbps 2 bit capable 10 Gbps (x16) Ethernet output available Engineer assigned to implement 10 GbE output of tied array But wrong clock on board…. Requires “full board” heat sink to be removed from every board VLBI TECHNOLOGY KOREA - Chris Phillips 18 |

Oz eVLBI No major changes recently 1 Gbps between ATNF observatories 1 Gbps shared routed to elsewhere 10 Gbps routed connection “soon” 40 Gbps test circuit between Parkes and ATCA 10 Gbps upgrade to observatories cheap but no funding and VLBI only user VLBI TECHNOLOGY KOREA - Chris Phillips 19 |

AARnet4 80x100 Gbps from Adelaide to ASKAP (MRO) 80x100 Gbps wavelengths on East coast by middle x40 Gbps Sydney to USA Upgraded to 100 Gbps VLBI TECHNOLOGY KOREA - Chris Phillips 20 |

Mopra Mopra operational again after fires which devastated control room Equipment room survived with relatively little damage VLBI TECHNOLOGY KOREA - Chris Phillips 21 |

Astronomy and Space Science Chris Phillips t wwww.csiro.au/atnf ASTRONOMY AND SPACE SCIENCE Thank you