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Solar-B Global DataGrid 21st September 2006 UK e-Science All Hands Meeting 2006 RAL Tim Folkes Jens Jensen Matthew Wild Elizabeth Auden MSSL Elizabeth Auden Paul Lamb Matthew Whillock Len Culhane 21 September 2006 e-Science AHM 2006 Overview The Solar-B mission will be launched tomorrow, Friday 22 September 2006, from the Uchinoura Space Center in Japan. Mission duration: 3 years nominal, +10 years lifetime expected Scientists and software engineers at MSSL and RAL have designed the Solar-B global data grid to provide mission data to solar research communities in the UK and abroad. • • • • • Solar-B science objectives Data transfer and processing Data storage User access to data Data security Elizabeth Auden 21 September 2006 e-Science AHM 2006 Solar-B Mission Overview EIS - MSSL/NRL EUV Imaging Spectrometer SOT - ISAS/NAOJ Solar Optical Telescope XRT - SAO/ISAS X-ray Telescope FPP - Lockheed/NAOJ Focal Plane Package Elizabeth Auden 21 September 2006 e-Science AHM 2006 Solar-B Science Key Science Questions 1. How is the solar corona heated? Are active regions heated in a different way to the quiet Sun? 2. What causes solar flares and coronal mass ejections? 3. How is energy transferred in the quiet Sun? How are solar magnetic fields affected? Solar events like flares and coronal mass ejections can have a profound affect on the Earth’s magnetosphere. A geomagnetic storm in 1989 triggered a blackout of the Hydro Quebec power system. Elizabeth Auden 21 September 2006 e-Science AHM 2006 Transfer of Solar-B Data to ADS Data Migration Facility Manages NFS area ISAS Japan Satellite data LL data ADS RAL LL data processing LL HL data MSSL HL Solar-B data transferred via GridFTP from ISAS and MSSL to an NFS mounted disk at ADS. Elizabeth Auden 21 September 2006 • Produced by SGI • User transparent file migration • Licence for 500Tbytes storage • Backend: STK SL8500 – 10,000 tape slots – STK 9940B drives (200GB 30MB/sec) – STK T10000 drives (500GB 120MB/sec) e-Science AHM 2006 ADS Data Storage The DMF monitors the Solar-B NFS area and removes disk copies of data to keep free space at required level. ADS Interface NFS DMF STK SL8500 robot Hardware • Based on Altix 350 • Numaflex architecture • 40 Tbytes raid disk Network • Local server: 1Gbit network • Part of 10Gbit back-bone • Coming soon: SJ5 10Gbit link Elizabeth Auden Tape Small Larger files fileshave haveprimary primarycopy on copy disk. onhave (Speeds tape.secondary up All files read/writes.) copy on tape. These are periodically moved to the Firesafe firesafe. 21 September 2006 e-Science AHM 2006 User Access to Solar-B Data Instrument Data SOT: Solar Optical Telescope Magnetic field images Optical images Magnetic field velocity measurements DMF XRT: X-Ray Telescope X-ray coronal images EIS: EUV Imaging Spectrometer Coronal line strengths and profiles Plasma diagnostics Files via URLs and DMF system at RAL’s UKSSDC Users access data as URLs through the AstroGrid workbench, STAP web services, browsers, or wget. Elizabeth Auden 21 September 2006 e-Science AHM 2006 Accessing Solar-B data through AstroGrid AstroGrid workbench INPUT: ADQL queries AstroGrid DSA OUTPUT: FITS keywords, URLs DSA: DataSet Access ADQL to SQL AstroGrid HelioScope, STAP enabled tools AstroGRID PLASTIC tools, Solar-B website, wget, browser Elizabeth Auden INPUT: start / stop dates OUTPUT: URLs AstroGrid STAP service MySQL FITS keywords, Data URLs STAP: Simple Time Access Protocol INPUT: URLs OUTPUT: Solar-B files 21 September 2006 ADS Web-visible file system e-Science AHM 2006 AstroGrid User Components AstroGrid workbench: STAP service access through HelioScope, DSA access through the Task Launcher. Task Launcher: locate DSAs, submit ADQL queries Workbench: http://www2.astrogrid.org/desktop/index STAP: Simple Time Access Protocol http://personalpages.manchester.ac.uk/staff/s.dalla/astrogrid/strap.html DSA: DataSet Access http://www.astrogrid.org/maven/docs/HEAD/pal/index.html ADQL: Astronomical Data Query Language HelioScope: solar data results from STAP services. Elizabeth Auden http://www.ivoa.net/Documents/latest/ADQL.html 21 September 2006 e-Science AHM 2006 Mission Data Flow Elizabeth Auden 21 September 2006 e-Science AHM 2006 Solar-B Studies / Observation Planning • • • Study Proposal – All study proposals are tested on the Flight Spare model before acceptance into the master Study Database – The Study Database contains information about the science (target, pointing, rationale) as well as meta-data (author, joint ops id, etc) Database Distribution – This is done using the automatic Solarsoft update mechanism through Goddard Space Flight Centre Daily Planning – Performed at ISAS using the Study Database – Studies are entered into the Timeline (As-planned) Database Elizabeth Auden 21 September 2006 e-Science AHM 2006 FITS File Reformatting • • Fits Reformatting (1) – Level-0 performed at ISAS – Accesses As-Planned Database – Populates As-Run Database – Transfers files to ADS and ISAS web system – Accesses other instruments’ Fits files and transfers them to the ADS for storage Fits Reformatting (2) – EIS Level-0 Fits files are used to generate Level-2 Fits files at MSSL – Updates the data catalogue – Transfers Level-2 Fits files back to the ADS Elizabeth Auden 21 September 2006 e-Science AHM 2006 Data Security GRIDFTP • Secure transfers GridFTP used for file transfers • 3rd party transfers • Good performance ADS (RAL) • Certificates from UK eScience CA and AIST (Japan) GridFTP GridFTP ADS (RAL) HTTP USERS STORAGE • 10 TB per year ADS (RAL) • 30 TB over nominal 3 year duration of mission GridFTP GridFTP: Clients / hosts authenticate with X509 certificates Elizabeth Auden 21 September 2006 e-Science AHM 2006 Conclusions • Solar-B launch tomorrow. 22 September 2006 • Data transferred via GridFTP to ADS at RAL • ADS facility uses DMF to manage files on disk and tape • Data searchable through AstroGrid DSA and STAP web service • Solar community accesses data through AstroGrid workbench, HelioScope or a web browser LINKS: AstroGrid: http://www.astrogrid.org Solar-B countdown: http://www.mssl.ucl.ac.uk/www_solar/ Questions? Elizabeth Auden 21 September 2006 e-Science AHM 2006