Mark 5 – Status and Developments Alan Whitney MIT Haystack Observatory 14 May 2007 U.S. VLBI Technical Coordination Meeting NRAO Socorro, NM.

Slides:



Advertisements
Similar presentations
PRODUCT PRESENTATION QUANTUM2. EVOLIS QUANTUM, MODULAR SYSTEM FOR CENTRALIZED CARD PRODUCTION.
Advertisements

Mark 6 VLBI Data System Alan Whitney Roger Cappallo Chet Ruszczyk Jason SooHoo MIT Haystack Observatory 11 Oct nd International VLBI Technical Jeju,
StreamBlade SOE TM Initial StreamBlade TM Stream Offload Engine (SOE) Single Board Computer SOE-4-PCI Rev 1.2.
A new Network Concept for transporting and storing digital video…………
Arecibo Telescope Servo & Drive System Technical Meeting May 2004 VERTEX ANTENNENTECHNIK GmbH Arecibo Telescope Servo Drive System Ideas For Computer.
Integration of the Mk5B Playback System into the Mk4 Correlator Roger Cappallo MIT Haystack Observatory Concepcion
The Mark 5B VLBI Data System Alan Whitney Will Aldrich John Ball Kevin Dudevoir Brian Fanous Dan Smythe MIT Haystack Observatory 24 March 2006 EVN TOG.
The CVN Real Time Correlator Zhang Xiuzhong, Chen Zhong Shanghai Astronomical Observatory China 4th e-VLBI Workshop Sydney
Mark 5C VLBI Data System Alan Whitney MIT Haystack Observatory 16 June 2008 e-VLBI workshop Shanghai, China.
Mark 6: design and status update VLBI Technical Meeting MIT Haystack Observatory Roger Cappallo Alan Whitney Chet Ruszczyk.
28 August 2002Paul Dauncey1 Readout electronics for the CALICE ECAL and tile HCAL Paul Dauncey Imperial College, University of London, UK For the CALICE-UK.
Chapter 3 Chapter 3: Server Hardware. Chapter 3 Learning Objectives n Describe the base system requirements for Windows NT 4.0 Server n Explain how to.
DBBC3 Development - Digital Base-Band Converter 3
 A system consisting of a number of remote terminal units (or RTUs) collecting field data connected back to a master station via a communications system.
© 2009 IBM Corporation Statements of IBM future plans and directions are provided for information purposes only. Plans and direction are subject to change.
Current plan for e-VLBI demonstrations at iGrid2005 and SC2005 Yasuhiro Koyama *1, Tetsuro Kondo *1, Hiroshi Takeuchi *1, Moritaka Kimura, Masaki Hirabaru.
Ongoing e-VLBI Developments with K5 VLBI System Hiroshi Takeuchi, Tetsuro Kondo, Yasuhiro Koyama, and Moritaka Kimura Kashima Space Research Center/NICT.
Atacama Large Millimeter/submillimeter Array Expanded Very Large Array Robert C. Byrd Green Bank Telescope Very Long Baseline Array Spectrometer PDR John.
Electronic Transmission of Very- Long Baseline Interferometry Data National Internet2 day, March 18, 2004 David LapsleyAlan Whitney MIT Haystack Observatory,
E-VLBI Development at Haystack Observatory 5 th Annual e-VLBI Workshop Haystack Observatory 20 September 2006 Alan R. Whitney Kevin Dudevoir Chester Ruszczyk.
Goals of a New VLBI Data System Low cost Based primarily on unmodified COTS components Modular, easily upgradeable Robust operation, low maintenance.
Camera Link Communication Interface for Vision Applications J. Egri 6/7/05.
IDE Interface. Objectives In this chapter, you will -Learn about each of the ATA standards (ATA-1 through ATA-6) used in PCs -Identify the ATA connector.
2012 DiFX user’s meeting, Sydney, Australia USNO Software Correlator: Status Report Outline USNO/WACO Background USNO Prototype Software Correlator (UPSC)
1 Chapter Overview CD-ROM and DVD Drives Advanced Hard Disk Drives SCSI Drives.
Current LBA Developments Chris Phillips CSIRO ATNF 13/7/2005.
E-VLBI developments with the K5 VLBI system Koyama Yasuhiro *1, Kondo Tetsuro *1, Kimura Moritaka *1, Takeuchi Hiroshi *1, and Masaki Hirabaru *2 *1 Kashima.
Online Systems Status Review of requirements System configuration Current acquisitions Next steps... Upgrade Meeting 4-Sep-1997 Stu Fuess.
Developments for real-time software correlation e-VLBI Y. Koyama, T. Kondo, M. Kimura, M. Sekido, M. Hirabaru, and M. Harai Kashima Space Research Center,
Data Acquisition  From receivers to correlator  Data Acquisition System  Recorder  Station Unit – DAS2  Correlator  Key Features:  Digital, KISS.
DBBC Stutus Report November 2007 G. Tuccari, W. Alef, S. Buttaccio, G. Nicotra, M. Wunderlich.
DLS Digital Controller Tony Dobbing Head of Power Supplies Group.
The Mark 5B VLBI Data System Alan Whitney for the Mark 5 team MIT Haystack Observatory 20 September th e-VLBI Workshop Haystack Observatory.
VLBA Software Group Meeting RBDE Control via VSI-S Interface Miguel Guerra National Radio Astronomy Observatory (Socorro, NM) 2010 January 12.
XFEL The European X-Ray Laser Project X-Ray Free-Electron Laser Dariusz Makowski, Technical University of Łódź LLRF review, DESY, 3-4 December 2007 Advanced.
Trimble NetR8 GNSS Reference Receiver
Eleventh Synthesis Imaging Workshop Socorro, June 10-17, 2008 THE VLBA SENSITIVITY UPGRADE Craig Walker, NRAO.
E-VLBI: Creating a Global Radio Telescope via High-Speed Networks Alan R. Whitney MIT Haystack Observatory SLAC Data Management Workshop 17 March 2004.
Nov 3, 2009 RN - 1 Jet Propulsion Laboratory California Institute of Technology Current Developments for VLBI Data Acquisition Equipment at JPL Robert.
Long Term Transition Plan Gareth Hunt EVLA M&C PDR 2002 May 15.
DiFX New Features. Disk based file specification Improved specification of files to correlate Wild cards with time of scan name filtering? External reference.
Multimedia Devices Chapter 8. Multimedia Overview The term multimedia has different meanings for people because there are many types of multimedia devices.
VLBI_UDP An application for transferring VLBI data via UDP protocol Simon Casey e-VLBI meeting, Haystack 20 Sep 2006.
The Mark 5B VLBI Data System Alan Whitney MIT Haystack Observatory 10 Jan 2006 IVS General Meeting Concepion, Chile.
VLBA Implementation of the ROACH Digital Backend Jonathan Romney on behalf of the VLBA Upgrade development team NRAO / Socorro First International VLBI.
Demonstration of 16Gbps/station broadband-RF VLBI system Alan Whitney for the VLBI2010 development team MIT Haystack Observatory 22 October st Intl.
Correlator Options for 128T MWA Cambridge Meeting Roger Cappallo MIT Haystack Observatory
2005/7/131 Plans and Options for e-VLBI on the VLBA Jon Romney NRAO, Socorro 4 th e-VLBI Workshop 2005 July 13.
P08311: FPGA Based multi-purpose driver / data acquisition system Sponsor: Dr. Marcin Lukowiak Team MemberDisciplineRole Andrew FitzgeraldCEProject Manager/FPGA.
Mk5B DOM Phase-cal, State Statistics, and SU Capability Roger Cappallo, Brian Fanous Haystack eVLBI Conference
1 Conduant Mark5C VLBI Recording System 7 th US VLBI Technical Coordination Meeting Manufacturers of StreamStor ® real-time recording products
E-VLBI: A Brief Overview Alan R. Whitney MIT Haystack Observatory.
11 th April 2003L1 DCT Upgrade FDR – TSF SessionMarc Kelly University Of Bristol On behalf of the TSF team Firmware and Testing on the TSF Upgrade Marc.
ECGV Workshop, Haystack Observatory USNO Status Report: S/W Correlator & e-VLBI Dave Boboltz, Nicole Geiger, Alan Fey, Ralph Gaume, Kerry Kingham & Dave.
Software Requirements for the Testing of Prototype Correlator Sonja Vrcic Socorro, December 11, 2007.
ECE 456 Computer Architecture Lecture #9 – Input/Output Instructor: Dr. Honggang Wang Fall 2013.
Data-Acquisition and Transport – Looking Forward to 2010 and Beyond Definition of ‘Data-Acquisition and Transport’ Continuum of Transport Options Limitations.
Potential VLBI2010 Data System Alan Whitney MIT Haystack Observatory Mikael Taveniku XCube Systems 24 Feb 2011 East Coast VLBI meeting Haystack Observatory.
Secondary Storage – 1980’s 5 ¼” Floppy Drive – very low storage capacity maxing out at 1.2 Mb Mid-1980’s – 1990’s 3 ½” Floppy Drive – low storage.
Vanderbilt University Toshiba IR Test Apparatus Project Final Design Review Ahmad Nazri Fadzal Zamir Izam Nurfazlina Kamaruddin Wan Othman.
Broadband Interfacing eMerlin-JIVE (1-10Gbps) Onsala-Jodrell Bank (
A Wide-Band VLBI Digital Backend System Alan Whitney Shep Doeleman Brian Fanous Hans Hinteregger Alan Rogers MIT Haystack Observatory 10 Jan 2006 IVS General.
2007 / 5 / 141 VLBA Requirements, Plans & Status Jon Romney NRAO, Socorro Second US VLBI Technical Coordination Meeting Socorro 2007 / 5 / 14.
Future LBO Developments
e-VLBI: Creating a Global Radio Telescope via High-Speed Networks
Mark 5 / VLBA Correlator Topics
Haystack Geodesy Program and Technical Development
AMCOM Digital Archive Design Review - Week 3.
VLBA Correlator Interfaces for VSOP-2
SKAMP Square Kilometre Array Molonglo Prototype
Presentation transcript:

Mark 5 – Status and Developments Alan Whitney MIT Haystack Observatory 14 May 2007 U.S. VLBI Technical Coordination Meeting NRAO Socorro, NM

Mark 5 team Will Aldrich John Ball Peter Bolis Roger Cappallo Kevin Dudevoir Brian Fanous Dave Fields Dan Smythe Jason SooHoo Mike Titus Ken Wilson Alan Whitney Conduant Corp

Mark 5A Data Acquisition System (introduced 2002)

Main features of Mark 5A Data System Direct plug-compatible replacement for 64-track Mark4 or VLBA tape drives Record/Playback at rates up to 1024 Mbps Two independent ‘8-pack’ disk modules can be used in ‘ping-pong’ fashion for nearly continuous recording Records 8, 16, 32 or 64 tracks from Mark4 formatter (1024 Mbps max) or VLBA formatter (512 Mbps max)

Current Mark 5A Status ~150 Mark 5 systems deployed; >95% of tape systems have been replaced ~1300 Mark 5A ‘8-pack’ disk modules deployed (>2 PB of storage!); growing rapidly! 1 Gbps experiments are now routine for both geodesy and astronomy VLBA has converted to Mark 5; all VLBA stations have Mark 5A, but correlator is fitted with only enough to process VLBA stationS Correlator efficiency has improved by factor of ~2 over tape! Challenge –support of systems in field! –Mostly due to large variety of system configurations

Mark 5B Data System Features Full VSI-H compatibility Same chassis as Mark 5A; uses same disk modules; requires Mark 5B I/O card 1024 Mbps record/playback Eliminates need for external formatters, but requires sampler adapter for Mark 4/VLBA DASs to provide VSI-compatible output Station Unit capabilities for connection to Mark 4 correlators is designed into Mark 5B Extensive built-in phase-cal extraction and state counting on both data record and data playback Front-panel status display – 8 tri-color LEDs DIM and DOM capabilities are separate FPGA downloads FPGA is programmable via software Development support from Mark 5 development consortium – NASA, NRAO, USNO, MPI, BKG, EVN, KVN, JPL

VSI-H VSI-S VSI-E

Mark 5B Functional Block Diagram

Mark 4 Station Unit emulation Mark 4 Station Unit

Mark 5B I/O Board FPDPVSI OutputVSI Cntl/Mntr VSI Input 256MB memory PCI Connector

Mark 5B Status Mark 5B fully tested and operational Mark 5B DIM software is complete except for phase-cal extraction Direct connection to Mark 4 correlator is operational at Haystack; has proven to be extremely reliable and repeatable ~15 Mark 5B I/O boards have been distributed to Mark 5 development consortia members Mark 5B system and Mark 5A→Mark 5B upgrade now available from Conduant Corp (already ~30 delivered) Mark 5B system is in routine use at Westford Mark 5B support on correlators –Haystack supports Mark 5B (including phase-cal/state-count) –MPI and USNO in process of upgrading to support Mark 5B –JIVE correlator has committed to Mark 5B upgrade, but schedule unknown; will use Mark 5A+ in meantime –NRAO will use Mark 5A+ for forseeable future

Reasons to adopt Mark 5B Eliminate need for expensive external formatters; particularly important for new stations or stations without existing Mark 4 or VLBA formatters With a 14-BBC Mark4 or VLBA4 system, up to 1792 Mbps can be recorded with two parallel Mark 5B systems; current 14-BBC systems can only generate a maximum of 1024 Mbps of formatted data Extensive phase-cal extraction and state counting capabilities for better diagnostics and better system calibration Replace unreliable Station Units on Mark 4 correlators; SU capability is built into Mark 5B Stepping stone to Mark 5B+ (2Gbps)

Mark 5A/B Compatibility Problem: Mark 5A cannot playback Mark 5B recordings  how can Mark 5B recordings be processed on correlators that support onlyly Mark 5A? Solution: Mark 5A+ (upgraded FPGA code for Mark 5A) Upgraded Mark 5A (“Mark 5A+”) can play: -All Mark 5A recordings -All Mark 5B recordings, playback is in VLBA-track-format Mark 5A+ design complete and tested Mark 5A+ not compatible with 2Gbps recording from Mark 5B+ Bottom line: Mark 4/VLBA correlator with only Mark 5A units can process data from both Mark 5A and Mark 5B units during transition period to Mark 5B.

Mark 5B+ (2048Mbps) Conduant has introduced an upgraded StreamStor (dubbed “Amazon”) that supports up to ~3 Gbps on FPDP2 interface, which supports FPDP clock at 64 MHz Mark 5B I/O card has been designed and tested to support input VSI-H clock rate of 64MHz, as well as FPDP2 compatibility, to support max recording rate of 2048 Mbps Can record to one disk module at 2Gbps; plan to support recording across 2 disk modules (16 disks) for improved robustness in face of slow disks Playback is limited to 1024 Mbps Compatibility: Mark 5B+ recordings compatible with playback on Mark 5B and Mark 5A+ (except 2048Mbps) Mark 5B+ is operational and has been used in a number of experiments with DBEs Mark 5B+ is available from Conduant Corp as system or upgrade

How to upgrade a station from Mark 5A to Mark 5B Purchase Mark 5B upgrade kit (includes front-panel LED status panel and rear-panel I/O adapter) Options to create VSI-H data source: 1.Modify Mark 4 formatter to “VSI4 Sampler Adapter” –Two VSI-H outputs; 1792Mbps total –Cost ~$2K (board and new rear panel from Haystack) –Pretty much irreversible 2.Acquire Digital Back End unit 3.Acquire VSI-C adapter to VLBA samplers 4.Acquire Japanese VSI-H sampler unit

How to upgrade a Mark 4 correlator to support Mark 5B recordings Option 1 1.Purchase Mark 5B upgrade kit (includes front-panel LED status panel and rear-panel I/O adapter) 2.Procure Correlator Interface Unit from Haystack, plus upgraded Serial-Link boards from MPI (if necessary) 3.Discard Mark 5 Station Unit 4.Upgrade correlator software (significant work) 5.Advantage: Supports Mark 5B+ recording at 2048Mbps Option 2 1.Upgrade Mark 5A units Mark 5A+ (FPGA code upgrade) 2.Upgrade correlator software to support Mark 5A+ (minor upgrade)

Mark 5C (under development) Amazon StreamStor board with new 10GigE daughter board (no separate I/O board – unlike Mark 5A/B/B+) Will accept single-stream 10 Gigabit Ethernet (OSI Layer 2) 4096 Mbps max data rate to two standard Mark 5 disk modules Record-only through SS 10GigE interface 10GigE packet specification will be VSI-E subset –Will support an arbitrary # of channels (i.e. not constrained to 2**n like current VSI-E, Mark 5A/B) –Will require extension of VSI-E specification Data format on SS disk currently under design –A Mark 5B compatibility mode will be supported (i.e. 2**n channels; will be readable on Mark 5B) Playback will be through host computer –Natural for software correlators Prototype expected by ~early 2008

Generalized 10GigE Data Distribution Concept + + Channelized Ethernet packets

Mark 5A/B/B+/C System Comparisons Mk5AMk5BMk5B+Mk5C (under development) Data Interface Emulates Mk4/VLBA tape transport VSI-H (64MHz max clock rate) 10 GigE (OSI Layer 2) Max data rate1024 Mbps 2048 Mbps4096 Mbps Record modes8, 16, 32, 64 “tracks” 1,2,4,8,16,32 bitstreams Same as Mk5B ─ DisksMk5 “8-pack”Same ChassisMk5Same I/O cardMk5AMk5B None SS cardXF2 Amazon I/O-SS intfModified FPDPFPDPFPDP2 (clocks on both edges) 10GigE Direct to Amazon Max playback rate 1024 Mbps (to VSI-H) ~4Gbps (to host) Playback Compatibility Mk5A (to VSI-H) Mk5A+ (to VSI-H) Mk5B Mk5A+ (except 2Gbps) ─

Mark 5 Upgrade Costs Target Existing Mk5AMk5B (requires VSI-H data source) Mk5B+Mk5C (not yet available; rough estimates) 0Unavailable$20.8K~$22.3K$20-25K Mk5A-~$3.5K (Mk5B I/O) ~$13K (Amazon plus Mk5B I/O) Est. $12-14K (Amazon plus 10GigE DB) Mk5B--~$9.6K (Amazon) Est. $12-14K (Amazon plus 10GigE DB) Mk5B+-- - Est. $2-4K (10GigE DB) Note: Costs do not include cost of creating data source

Disk-Media Status Hard disk price vs capacity/performance continues to drop -Now below ~$0.50/GB and continue to drop (Mark 4/VLBA tape is ~$2.00/GB) 400 GB disks are commonly used – Two 8-packs of 400GB disks comparable to ~13 VLBA/Mark 4 tapes 750 GB disks now available – Two 8-packs of 750GB disks comparable to ~24 VLBA/Mark 4 tapes; ~26 1 Gbps unattended!

Tape vs. Disc Price Comparison

Disk-Media Reliability Based on statistics collected at Haystack, average disk drive failure rate is ~0.5% per year Failure rate of Hitachi 250GB was higher than average, but now believed stabilized Disk reliability at high altitudes (Mauna Kea summit) was investigated prior to UVLBI experiment; only Hitachi 250GB disks passed.

Disk-Media Reliability Based on statistics collected at Haystack, average disk drive failure rate is ~0.5% per year Failure rate of Hitachi 250GB has been higher than average Conduant has qualified drives from Maxtor, WD and Seagate 400GB – Seagate 250GB – Western Digital RAID Edition (high-reliability) 250GB – Maxtor Maxline III (high-reliability) Conduant is shipping these disks in assembled Mark 5 disk modules Disk reliability at high altitudes is under investigation

Mark 5 file access Conduant working on upgrade to allow Mark 5 scans to be accessed as standard Linux files Probably will be read-only (similar to CD-ROM) Will be targeted at upgraded Mark 5 data-directory structure Convenient for e-VLBI and software correlators Availability ~end 2007

SATA disk module Now available from Conduant Interchangeable with PATA disk module New mechanical design allows very easy access to insert/remove individual disks; increased module stiffness for better mechanical stability SATA Drive Connectors PATA Module connector

Summary Transition from tape to disk is nearly complete at nearly all stations and correlators Mark 5B is ready for prime time; in routine use at Westford antenna Upgrading to Mark 5B is not necessary at all stations, but may be advantageous; will be required for use with DBE Mark 5B+ (2 Gbps) is also operational and has been used extensively for astronomy observations Mark 5C (4 Gbps) is currently under development to support industry- standard 10GigE interface

Questions?