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DTSTART:19700308T020000
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DTSTART:19701101T020000
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BEGIN:VEVENT
DTSTAMP:20190719T085744Z
LOCATION:HG F 3
DTSTART;TZID=Europe/Stockholm:20190614T103000
DTEND;TZID=Europe/Stockholm:20190614T110000
UID:submissions.pasc-conference.org_PASC19_sess123_msa111@linklings.com
SUMMARY:The RAMSES Code, Next Generation
DESCRIPTION:Minisymposium\nComputer Science and Applied Mathematics, Physi
 cs, Solid Earth Dynamics\n\nThe RAMSES Code, Next Generation\n\nTeyssier, 
 Potter\n\nWe present our strategy to implement the next generation of the 
 RAMSES code, a community code with adaptive mesh refinement for astrophysi
 cal fluid flows. Our current prototype is based on a global multi-level Ca
 rtesian grid indexing scheme with a software cache. The MPI and OpenMP bac
 kend is hidden to the developer. We will discuss the present status of the
  prototype and elaborate on our strategy for the next step. An important p
 oint will be to allow for efficient use of accelerators, with an emphasis 
 on using higher order methods for MHD flows.
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