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Coordinator: M.L.Khodachenko ( IWF-ÖAW, Graz, Austria )

JRA 3 // WP 24 European Modelling & Data Analysis Facility (EMDAF) development of a distributed computational and data analysis service for the European planetary science. Coordinator: M.L.Khodachenko ( IWF-ÖAW, Graz, Austria ) Deputy: S. Miller ( UCL, London, UK )

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Coordinator: M.L.Khodachenko ( IWF-ÖAW, Graz, Austria )

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  1. JRA 3 // WP 24European Modelling & Data AnalysisFacility (EMDAF) development of a distributed computational and data analysis service for the European planetary science Coordinator: M.L.Khodachenko (IWF-ÖAW, Graz, Austria) Deputy: S. Miller (UCL, London, UK) Task Leaders: R. Stöckler, F. Topf (IWF-ÖAW, Graz, Austria) EC Grant agreement n° 228319

  2. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at Involvement of computing power & resource Need of specific knowledge & qualifications ● Motivation for proposing JRA-3 / EMDAF : Data analysis & modeling – two basic components of scientific research Two aspects of modeling: -- Theoretical modelling --Numerical modelling / simulation Variety of numerical models and data analysis algorithms is available now at the European planetary science community Each Numerical Code or Software is associated with a certain team or group of teamsKnow-how(i. e. local nature) - Development of software - Support of operation - Application to particular problems

  3. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at Development / operation of complex advanced software tools requires professional expertiseand full enga- gement of the staff Specialization of teams in particular kinds of M & DA software       The need to provide conditions under whichdevelopment and applicatopn of numerical toolsfor observational data analysis and modeling are performed in closeinterrelation & coordinationbetween software developers and scientific research teams ● Motivation for proposing JRA-3 / EMDAF :  Other research groupsdealt with theoretical and applied planetary science problems may need application of advanced DA & M methods in their study.Potential users  Engagement intodevelopment of advanced & complex software not always can be easy combined with the efficient scientific research Distributed and Coordinated Interdisciplinary Facility for Planetary Computational Modelling and Data Analysis a new type of Research Infrastructure (RI)

  4. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at ● Main Strategic Goal : Creation of a distributed and coordinated RI, based on the existing in Europe computational modelling and data analysis centres, which will provide the scientific community with the dedicated services in the fields of their computational & data analysis expertise. To produce astep change in the infrastructureof European activities in planetary modelling and data analysis; To support European planetary space missionsand ground-based observationswith reliable models and data analysis tools; To support European Planetary Science modellingand data analysiswith reliable algorithms and high-performance computing techniques; To bring together European computing and planetary scienceresearch groups into a distributed European infrastructure ● Objectives :

  5. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at EMDAF will providea setdemonstrators and opera- tional testsof interconnected Computational Modelling & multi-disciplinary Data Analysisservice in key areas of European Planetary Science. ● Matter of work : EMDAF will: Develop web-based tools for planetary scientists to communicate with modelling and data analysis experts; Produce anInteractive Catalogueof planetary models & data analysis tools; Develop aDistributed Numerical Modelling Laboratory, to allow scientists to specify inputs for models to be run “on demand”, includingcoordinated, interconnected, multi-disciplinary simulations; Develop aDistributed Data Analysis Laboratorywith services “on demand”; Enable the codes involved with the DNML and DDAL to run onHPC facilities, in cooperation with the European HPC Grid DEISA-2; Perform furtherelaboration of data analysis and modelling methodsfor their coodinated use by the scientific community. • Space weather, incl. magnetospheric & atmospheric aspects; • Mars in time & space; • Environment of airless bodies, Mercury & Moon; • Comets

  6. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at Task#1: Management of EMDAF (JRA3) Task#3: DNML Task#4: DDAL Task#5: HPC resources and standatds Task#2: ICPM&DAT ● Structure of the activity:Tasks / Sub-divisions Task#1 Coordination and Management Task#2 Interactive Catalogue of Planetary Models & Data Analysis Tools (ICPM&DAT) Task#3 Distributed Numerical Modelling Laboratory (DNML) Task#4 Distributed Data Analysis Laboratory (DDAL) Task#5 Enabling High Performance & Grid Computing Architec- tures, Codes Standardization

  7. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at ● Organizational principles & management :  Each of 5 Working Tasks of JRA-3 / EMDAF has 2 responsible leaders and a team (group of scientists / labs);  Coordination of EMDAF, as a distributed RI, will be performed by the Board of Experts (leaders of Tasks);  To reach its goals on establishing dedicated modelling and data analysis services, JRA3 / EMDAF will develop and provide: - Specialized user services within particular Tasks; Flexible schedules - Topic oriented tutorial teams + communication - Broad advertising of the available services  Collaboration of many laboratories and individual scientists will be ensured by 1) Joint authorship of papers and the inclusion into mission teams; 2) strict & clear copy right policy; 3) Reimbursement of compu- tational service and software R&D work on a sub-contract basis;  Cooperation with other activities in EUROPLANET (NA1, NA2, JRA-IDIS).

  8. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at 0 12 24 36 48 Web page T1 Coordination T2 Interactive Catalog T3 Distributed Num.Modeling Lab. T4 Distributed Data Analysis Lab. Enabling HPC & Codes Stand. T5 Annual reports T1 Delivery to IDIS ● Work package time line: Milestones and Deliverables M24.1.1 M24.3.1 M24.1.3 M24.4.2 M24.1.3 D24.1.3 D24.1.3 M24.1.1 D24.3.1 D24.4.2 M24.1.2 M24.4.1 M24.5.1 M24.3.2 M24.5.2 D24.1.2 D24.4.1 D24.5.1 D24.3.2 M24.2.2 M24.4.2 M24.2.1 D24.2.2 D24.4.2 D24.2.1 M24.5.3 D24.5.2

  9. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at ● Tasks, staff effort, coordinating institutes :(total95.5)

  10. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at ● JRA-3/EMDAF Team : Coordinator : Maxim L. Khodachenko (IWF, Austria) Deputy-coordinator :Steve Miller (UCL, UK) • Task1: Task-leader: Robert Stöckler (IWF, Austria) • Deputy: Nick Achilleos (UCL, UK) • Co-leader: Florian Topf (IWF, Austria) • Task2:Task-leader: Florian Topf (IWF, Austria) • Deputy: Jean Lilensten (CNRS/LPG, France) • Co-leaders: Daniel Heynderickx (DHConsultancy, Belgium) • Robert Stöckler (IWF, Austria) • Task3: Task-leader: Patrick Guio (UCL, UK) • Deputy: Esa Kallio (FMI, Finland) • Co-leader: Anatoly Petrukovich (IKI, Russia) • Task4:Task-leader: Albert Kislyakov (NNSU, Russia) • Deputy: Ondrej Santolik (IAP, Czech Rep.) • Task5: Task-leader: Claudio Gheller (CINECA, Italy) • Deputy: Maxim L. Khodachenko (IWF, Austria) • Co-leaders: Esa Kallio; Walter Schmidt (FMI, Finland) • Florian Topf; Robert Stöckler (IWF, Austria)

  11. Existing Interdisciplinary Cooperations in JRA3/EMDAF Distributed Data Analysis Laboratory: - Application of Wigner-Ville (WV) and Sliding Window Fourier (SWF) transform methods in planetary sciences - Combination with Wavelet analysis methods Saturnian Physics ♦SKR impulsive modulation burst ♦Variation of 10.77 h impulsive modulation of SKR

  12. Existing Interdisciplinary Cooperations in JRA3/EMDAF Distributed Numerical Modelling Laboratory : - Simulators of solar/stellar wind interactions with planetary obstacles (MHD, Hybrid, Kinetic codes) - Global system reconstruction and conceptual modeling of complex natural phenomena in planetary physics; Neuron networks modeling ♦ Magnetosphere compression by solar/stellar wind and surface material spattering Mercury Physics & Space weather Ordinary SW: n = 72 cm-3 VSW = 430 km/s BzSW = 10 nT Extreme events (CMEs): n = 72 cm-3 VSW = 860 km/s BzSW = 10 nT

  13. JRA-3 / EMDAFhttp://europlanet-jra3.oeaw.ac.at ● European/International Perspectives: EMDAFwithin EUROPLANET FP7 will gain and foster the syner- gies of coordinatedandcoherentuse of available computational modelling and data analysis RIs (computational resources and services, data bases). It will serve as a prototype of a new kind ofpan-European inter-national Research Infrastructurewhich will provide the scientific community with the dedicated services in the field of computa-tional modelling and data analysis.

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