Rosie Bolton1 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKADS Costing work: Spreadsheets to scalable designs Rosie Bolton Dominic.

Slides:



Advertisements
Similar presentations
SKA New Technology Demonstrator Ray Norris CSIRO Australia Telescope National Facility.
Advertisements

SKADSMTAvA A. van Ardenne SKADS Coördinator ASTRON, P.O. Box 2, 7990 AA Dwingeloo The Netherlands SKADS; The.
SKAMP Square Kilometre Array Molonglo Prototype. Supporting Institutions  University of Sydney  Argus Technologies  ATNF  ICT Centre.
Paul Alexander DS3 & DS3-T3 SKADS Review 2006 DS3 The Network and its Output Data Paul Alexander.
Schediwy: Advantages and Disadvantages of Sparse Aperture Arrays Fermilab: October 2009.
Comparison of SKA Survey Speeds John D. Bunton, CSIRO TIP Figures of Merit SKA survey bandwidth can be large e.g. HI for redshifts up to 4. Thus it is.
SKA South Africa Overview Thomas Kusel MeerKAT System Engineering Manager April 2011.
Paul Alexander, Peter Hall Design Issues and Implementation ChallengesAAVP 2010 Design issues and implementation challenges Paul Alexander and Peter Hall.
Netherlands Institute for Radio Astronomy 1 ASTRON is part of the Netherlands Organisation for Scientific Research (NWO) From LOFAR design to SKA1 System.
BDT Radio – 2b – CMV 2009/10/09 Basic Detection Techniques 2b (2009/10/09): Focal Plane Arrays Case study: WSRT System overview Receiver and.
March 2009LOFAR MKSP Update: SKA and PrepSKA Paul Alexander.
Cylindrical Reflector SKA Update
1 Introduction to OBIEE: Learning to Access, Navigate, and Find Data in the SWIFT Data Warehouse Lesson 8: Printing and Exporting an OBIEE Analysis This.
Dec 2010 AAVP Cambridge workshop AAVP AAVS1/2-low demonstrators Jan Geralt Bij de Vaate.
National Astronomy and Ionosphere Center © Germán Cortés M 2008 SKA TDP Antenna Optics By Germán Cortés M. Cornell University Ithaca NY 14853, USA National.
Name1 title 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Progress in Active Antenna Design and Developement - FIDA3 Timothy Finn FG-IGN
Name1 SKA(DS) System Design Aspects 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA(DS) System Design Aspects: building a system Laurens Bakker.
Chris Shenton1 DSP Technology Options 4 th SKADS Workshop, Lisbon, 2-3 October 2008 DSP Technology Options Matching The Technology Platform To The Instrument.
Microsoft Access Database software. What is a database? … a database is an organized collection of data. A collection of data of similar information compiled.
© 2003 Xilinx, Inc. All Rights Reserved Power Estimation.
AA-Low Technical Progress Meeting, October 2012, Medicina, Italy AAVS0 & AAVS0.5: System Design and Test Plan Nima Razavi-Ghods Eloy de Lera Acedo.
CONSULTANT: BETTY ZOU CSSCR WINTER 2010 Beginning ATLAS.ti 5.5.
DE&T (QuickVic) Reporting Software Overview Term
SKA AA-Low Station Configurations and Trade-off Analysis Nima Razavi-Ghods, Ahmed El-Makadema AAVP 2011, ASTRON, Dwingeloo Dec
Phased Array Feeds John O’Sullivan SKANZ 2012 CSIRO Astronomy and Space Science,
SKA Introduction Jan Geralt Bij de Vaate Andrew Faulkner, Andre Gunst, Peter Hall.
S. Montebugnoli 2 nd SKADS Workshop October 2007 Stelio Montebugnoli IRA - INAF- Italy.
Transition from SKADS to PrepSKA Richard Schilizzi Lisbon, 3 October 2008.
A New Method For Developing IBIS-AMI Models
Simulations of Beamforming Algorithms Stelio Montebugnoli, IRA-INAF, Medicina (BO), Italy, Giovanni Naldi, IRA-INAF, Medicina.
Philippe Picard1 System Design 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Aperture Arrays system design Front end RF combining: an efficient way to.
Widefield Astronomy and Technologies for the SKA November 2009 at Limelette, Belgium The SKA AA-lo array; E.M. simulation and design Eloy de Lera.
Andrew Faulkner1 Technology Readiness Levels 4 th SKADS Workshop, Lisbon Technology Readiness Levels TRLs Andrew Faulkner.
Andrew Faulkner1 SKADS and SKA 4 th SKADS Workshop, Lisbon SKADS and SKA Andrew Faulkner.
OARE Module 5A: Scopus (Elsevier). Table of Contents About Scopus (Elsevier) Using Scopus Search Page Results/Refine Search Pages Download, PDF, Export,
Paul Alexander & Jaap BregmanProcessing challenge SKADS Wide-field workshop SKA Data Flow and Processing – a key SKA design driver Paul Alexander and Jaap.
XNTD/SKAMP/LFD Correlator 4th RadioNet Engineering Forum Workshop Next Generation Correlators for Radio Astronomy and Geodesy June 2006, Groningen,
Casper Signal Processing Workshop 2009 SKA Signal Processing (Preliminary) Wallace Turner Domain Specialist for Signal Processing.
Rosie Bolton SKADS Workshop April 10th 2008 SKADS Costing work: beyond the benchmark scenario Rosie Bolton Paul Alexander, Andy Faulkner and SKADS Costing.
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"
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.
MeerKAT DBE Past Present Future Alan Langman 28 September 2009.
Mário Santos1 EoR / 21cm simulations 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Epoch of Reionization / 21cm simulations Mário Santos CENTRA - IST.
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.
Roshene McCool1 Phase Transfer & WANs 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Local Oscillator distribution over fibre Roshene McCool SPDO – Signal.
Paul Alexander 2 nd SKADS Workshop October 2007 SKA and SKADS Costing The Future Paul Alexander Andrew Faulkner, Rosie Bolton.
A System View on SKA Bandwidth Usage G.W. (Dion) Kant AAVP Dwingeloo, 14 December 2011.
Rosie Bolton 2 nd SKADS Workshop October 2007 SKADS System Design and Costing: Update and next steps Rosie Bolton University of Cambridge.
Update On The Square Kilometer Array World Space Congress October 15, 2002 Jill Tarter.
SKA1-low: Cost Considerations AAVP Meeting, ASTRON 14 December, 2011 Tim Colegate, Peter Hall (ICRAR/Curtin) Andre Gunst (SPDO/ASTRON)
Lesson 7: Using Mail Merge
Paul Alexander1 DS3 Deliverable Status 4 th SKADS Workshop, Lisbon, 2-3 October 2008 DS3 Deliverables Review.
EoR/Cosmic Dawn SWG Feedback on SKA1-Low Array Configuration Cath Trott Brad Greig, Leon Koopmans, Andrei Mesinger, Garrelt Mellema, Jonathan Pritchard.
Engineering Commissioning May 2016 SKA1 LOW – Assembly, Integration & Verification Adam MacLeod AIV Consortium Manager & ASKAP System Engineer.
Andrew Faulkner April 2016 STFC Industry Day: Low Frequency Aperture Array Andrew Faulkner Project Engineer.
Phased Array Feeds SKANZ 2012 John O’Sullivan
Signal Processing for Aperture Arrays
Capability reporting Francesco Schillirò INAF- OACT
OSKAR station simulator
Aperture Array Station Processing
InnovationQ Plus Quick Start Guide
Technical Foundations & Enabling Technologies – DS4
SKADS White Paper - Technologies -
DVA1 as Part of the Dish Verification Program (DVP) Washington, DC P
Aperture Array Simulations
CAD DESK PRIMAVERA PRESENTATION.
Presentation transcript:

Rosie Bolton1 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKADS Costing work: Spreadsheets to scalable designs Rosie Bolton Dominic Ford Gabriel Grigorescu Paul Alexander Tim Colegate

Rosie Bolton2 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Talk outline Design and Costing: Second document –Latest SKADS costing figures –Identifying cost-scaling parameters Time line: moving to the new tool and handing over to the System design group. The SKA Functional Simulator Costing tool –Introduction –Example telescope design –GUI development Demonstration of the Costing tool.

Rosie Bolton3 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Outline Configuration: Memo 100 Follow concentration based on the SKA Draft specification: DishAA-hiAA-lo <1Km 20%30%~15% <5Km50%66%50% <180Km75%100%100% <3000Km100% AAs only out to 180km, frequency bands 70MHz-450MHz and 300MHz- 1,000MHz. AA bandwidth up to full range – set by data transfer spec Dishes all correlated, not beam-formed in Stations. 800MHz-10GHz. B/W 4GHz 5 spiral arms, with –3 to 3,000km, 2 only to 180km (saves trenching cost but configuration studies must verify / challenge this) Station Core ~5km dia Central Processing Facility Not to scale! 180km Dishes AA-hi AA-lo

Rosie Bolton4 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA cost breakdown: total €1.5Bn No: Infrastructure Roads, buildings No: Development costs NREs, tooling No: Software development costs No: Running costs No: Project management costs No: Contingency (but we do have an uncertainty estimate)

Rosie Bolton5 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Cost / design dependencies Collector costs Data transport CorrelatorBack end computing Trenching AA Field of View  Sensitivity ( ) T sys ( ) AA Station size  ( ) Dish size ( ) Bandwidth  AA top frequency  Layout 

Rosie Bolton6 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Cost / design dependencies Collector costs Data transport CorrelatorBack end computing Trenching AA Field of View  Sensitivity ( ) T sys ( ) AA Station size  ( ) Dish size ( ) Bandwidth  AA top frequency  Layout  For the Aperture arrays, with the FoV made up of multiple station beams, the data rate is directly proportional to the required FoV (if it is larger than the station beam size). Larger FoV => more processing to make maps

Rosie Bolton7 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Cost / design dependencies Collector costs Data transport CorrelatorBack end computing Trenching AA Field of View  Sensitivity ( ) T sys ( ) AA Station size  ( ) Dish size ( ) Bandwidth  AA top frequency  Layout  In combination, the sensitivity requirements and the system temperature determine how much “stuff” we need, affecting everything. 10% reduction in collecting area / Tsys across the SKA would save ~€140 Million NPV (no correlator scaling for Dishes – will be non-linear with dish number)

Rosie Bolton8 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Cost / design dependencies Collector costs Data transport CorrelatorBack end computing Trenching AA Field of View  Sensitivity ( ) T sys ( ) AA Station size  ( ) Dish size ( ) Bandwidth  AA top frequency  Layout  Make AA-hi Stations larger and more sensitive Have proportionally fewer stations to reach sensitivity Station beams are proportionally smaller: need more to fill FoV Station data rate goes up proportionally to area Total data rate transported to correlator is unchanged Fewer stations: fewer correlations – cheaper correlator

Rosie Bolton9 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Cost / design dependencies Collector costs Data transport CorrelatorBack end computing Trenching AA Field of View  Sensitivity ( ) T sys ( ) AA Station size  ( ) Dish size ( ) Bandwidth  AA top frequency  Layout  Same data rate, factor of ~6 difference in price

Rosie Bolton10 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Design and Costing: 2 Second Design and Costing document is to be delivered imminently –Includes updated SKA design, in line with SKA Memo 100 –Latest SKADS costs –Scaling relationships for overall costs

Rosie Bolton11 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 The SKA Costing tool Concept of “Design Blocks” was introduced in SKADS for D&C 1: Hierarchical Telescope designs made up of discrete blocks and components. SKACost tool was developed by the ISPO (Peter Hall, Aaron Chippendale and Tim Colegate) SKADS costing based on Excel spreadsheet The new SKA costing tool combines the best of these approaches –Advanced cost modelling and uncertainty handling –Plug-and-play telescope designs –GUI for easy browsing and editing

Rosie Bolton12 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 A: Tool with Example telescope design in database is made available B: Users download tool and database containing Design Blocks and components C: Users learn to use the tool by playing with example design blocks D: “Experts” study the relevant example design blocks create their own, improved, design blocks and / or components E: Code Checks: design blocks and components created by users are checked for functionality by the costing team F: SPDO Verification: New design blocks and components have calculations and cost estimates (with proof) checked by SPDO Design block development cycle

Rosie Bolton13 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 A: Tool with Example telescope design in database is made available B: Users download tool and database containing Design Blocks and components C: Users learn to use the tool by playing with example design blocks D: “Experts” study the relevant example design blocks create their own, improved, design blocks and / or components E: Code Checks: design blocks and components created by users are checked for functionality by the costing team F: SPDO Verification: New design blocks and components have calculations and cost estimates (with proof) checked by SPDO Design block development cycle In development now: available to selected people ~end Oct 08 End Oct 08 Early November 08 Mid November 08 Submit to costing team Mid Dec 08 Submit to SPDO Spring 09 Need full SKADS costs by ~Feb 09 SKADS Internal verification

Rosie Bolton14 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 Example telescope design Dishes and feeds in core and in outer array 2400 dishes Dishes and feeds in core and in outer array 2400 dishes AA-lo array antennas AA Station 85 Stations, 1 AA-lo, 1 AA-hi “array” in each AA Station 85 Stations, 1 AA-lo, 1 AA-hi “array” in each Digital Signal Transport Central processing and correlator SKA First stage Analogue beam-former First stage digital beam-forming Station beam-former Analogue data transport Mechanical infrastructure AA-hi array antennas AA-hi Local digital data transport Mechanical Infrastructure Analogue data transport Digital data transport First stage digital beamforning AA-lo AA Collectors AA-hi core 165 AA-hi “arrays” AA-hi core 165 AA-hi “arrays” AA-lo core 165 AA-lo “arrays” AA-lo core 165 AA-lo “arrays” Processing boxes Infrastructure and Trenching

Rosie Bolton15 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Open the GUI and choose a telescope design file from the repository…

Rosie Bolton16 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Browse available design blocks, view author information

Rosie Bolton17 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Set specific build options for the top level design block that you wish to build

Rosie Bolton18 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI

Rosie Bolton19 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Get cost and power outputs

Rosie Bolton20 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 List contents of build, including all sub-design blocks and components SKA Costing Tool GUI

Rosie Bolton21 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Display the hierarchy interactively

Rosie Bolton22 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Investigate cost / power breakdown by querying built design blocks

Rosie Bolton23 SKADS Costing work 4 th SKADS Workshop, Lisbon, 2-3 October 2008 SKA Costing Tool GUI Time for a quick demonstration…