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Impact of end of EMI+EGI-SA3

Impact of end of EMI+EGI-SA3. April 2013: EMI project finishes EGI-Inspire-SA3 finishes (mainly CERN affected) EGI-Inspire continues until April 2014 EGI.eu continues indefinitely Impact on WLCG & CERN IT. Impact in IT.

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Impact of end of EMI+EGI-SA3

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  1. Impact of end of EMI+EGI-SA3 • April 2013: • EMI project finishes • EGI-Inspire-SA3 finishes (mainly CERN affected) • EGI-Inspire continues until April 2014 • EGI.eu continues indefinitely • Impact on WLCG & CERN IT

  2. IT POW

  3. IT POW

  4. IT POW

  5. Impact in IT • Significant reduction in staff in ES and GT groups (~33% and ~45% reduction resp.) • No prospect of additional equivalent funding in the near future • Re-prioritisation of functions is unavoidable

  6. Evolution of functions • CERN has some ongoing commitments to EGI.eu and NGIs • Esp since we expect EGI to support WLCG • These are in-line with what we need for LHC • Must focus remaining effort where can have the most impact • Better in areas that benefit >1 experiment; • Less “labelled” staff (dedicated to experiments) • EMI: • Complex infrastructure used by EMI no longer required • Middleware support process under active discussion with partners • IT responsible for DM m/w + info system – must be maintained

  7. What IT must do • WLCG operations, service coordination, support • Consolidate related efforts (daily ops, integration, deployment, problem follow-up etc) • Broader than just CERN – encourage other labs to participate • Common solutions • Set of activities benefitting several experiments. Coordinates experiment work as well as IT-driven work. Experiments see this as strategic for the future; beneficial for long term sustainability • Grid monitoring • Must be consolidated (SAM/Dashboards). Infrastructure becoming more common (also with AI mon); focus on commonalities, less on experiment-specifics • Grid swdev+support • WLCG DM tools (FTS, DPM/LFC, Coral/COOL, etc), information system; Simplification of build, packaging, etc.  open source community processes; (See WLCG doc)

  8. What can no longer be supported • Support for Ganga core • Agreed with Ganga collaboration • POOL • Now only used by ATLAS; they assume responsibility • Activities where no interest from experiments: • Gridview, SE-catalog sync, … will be stopped • Experiment-specific customisations of (e.g. dashboards, SAM tests) • Move to experiment teams • Previous level of dedicated expert support to experiments unsustainable • Understood by ATLAS/CMS; issue for LHCb and ALICE • Some reduction in this effort already – but…

  9. Notes • There is no simple definition of "common solutions" - actually this can be part of many different activities, but a coordination of this is required, as well as available effort to work on priority projects • Support for middleware: • Proposal for methodology under discussion (document) with EMI and EGI as well as within WLCG • Relies on on-going commitments from m/w development partners • Encouraging broader community involvement and support where possible (e.g. WLCG Operations, middleware such as DPM, …)

  10. Potential for future projects • Only in 2014 at the earliest • Must be broader than just HEP • Must involve industrial partners (public-private partnerships) • Continued development of grids will not be feasible projects • And: • We must have commitments across the board this time – not IT alone

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