EGEE NA4 Lofar Lofar Information System Design OmegaCEN

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Presentation transcript:

EGEE NA4 Lofar Lofar Information System Design OmegaCEN Kapteyn Institute TARGET- Computing Center University Groningen Orsay, 10 June 2008 Fokke Dijkstra (most slides by Edwin Valentijn) EGEE: Lofar

LOFAR in short Large distributed radio telescope Two main bands In NL 2008: initial roll out 20 stations In NL 2009: 18 central (24 Gbps) + 18 remote (2 Gbps) phased array antenna stations each ~4 soccerfields size Full scale aperture synthesis array, extends 100 km Two main bands High Band ~ 7,500 tiles 120 – 240 MHz Low Band ~ 7,500 dipoles 20 – 80 MHz Fibre network, Software Correlator Run as a broad common-user observatory Making the transition now from “project” to “observatory” EGEE: Lofar

E-LOFAR Participants • GLOW: -- Effelsberg station delivered -- Garching, Potsdam, Tautenburg stations ordered --Jülich station federal funding proposal submitted • LOFAR-UK: – Chilbolton, Cambridge, Jodrell, Edinburgh – 1 station funded, site to be chosen --3 more stations • Sweden: – Onsala station funded + Poland, Italy, Austria, Bulgaria, Ireland, France EGEE: Lofar

Wires in the field EGEE: Lofar

Station based processing Input data rate: ~ 460 Gbps Output data rate: ~ 2 Gbps Processing capacity: ~ 1.5 Tmul/s Storage capacity: 96 Gbyte Receiver Filter Beamformer Buffer 10 GbE 1 GbE Used for 1 beam & station cross correlation EGEE: Lofar

Lofar: Data Stream EGEE: Lofar The streams from each station are processed in CIT, Blue Gene/L is a core element of the processing and the data compressed and archived is stored in the Long Tern Archive. The Long Term Archive will increase up to 4TB each year and the target – the Lofar Information System has to store data and supply users with the data as well as provide the data storage for data reprocessing. The Astro-WISE is an informational system which provides both data storage and data reprocessing for wide field astronomical instruments. The Astro-WISE is an ideal prototype for the Lofar Information System which must be transferred and adopted to Lofar requests. The main problemis that Astro-WISE works with TB of data – up to 100 TB and we need to make possible to store and operates PB instead of TB. EGEE: Lofar

Lofar Storage EGEE: Lofar

LoWISE design EGEE: Lofar

LoWise- concepts All Tier 1s on an equal footing Centrally operated GPFS distributed filesystem File retrieval Db viewer (web) Prompt (db query) Pathname – data server gLite – Grid ftp Single distributed db- with all Meta and source data Valid --Quality -- ready for publication flags Visibility of data Owner –Project –Archive --EURO-VO Authentication / Assigned resources AstroWISE Oracle system EGEE: Lofar

Processing - options Tier 0 – CP Tier 1 – re-processing Tier 2 Local clusters EGEE GRID Tier 2 On Tier 1 Local anarchy EGEE: Lofar

AstroWISE-Up EGEE: Lofar

VST - Virtual Survey Telescope EURO-VO: GRID and VO

TARGET diagram Extreme data lineage! EGEE: Lofar

Astro-WISE: Services EGEE: Lofar Astro-WISE interfaces includes CLI, dbviewer, external interfaces, target processor. EGEE: Lofar

Astro-WISE: Grid Computing The target procesor interface allow the user to reprocess data from the beginning. Here you can see the selection of the computing element which will be used for the processing. selection of Target in Astro-Wise storage element defined a priori EGEE computing EGEE: Lofar

LoWise and Euro-VO EGEE: Lofar

NA4 areas of work Improve integration with EGEE Authentication Use of Grid certificates through whole chain Portable client tools Computing Portability of software (Python) Coherent and fast execution of subtasks Storage SRM interfaces to Lofar archive StoRM ? EGEE: Lofar