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LOCATION:HG F 3
DTSTART;TZID=Europe/Stockholm:20190614T133000
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UID:submissions.pasc-conference.org_PASC19_sess146@linklings.com
SUMMARY:MS48 - Adaptive Mesh Refinement in the Era of Platform Heterogenei
 ty, Part II of II
DESCRIPTION:Minisymposium\nComputer Science and Applied Mathematics, Physi
 cs\n\nRearchitecting FLASH for Exascale\n\nO'Neal, Dubey, Weide, Chawdhary
 \n\nFLASH is a highly-configurable multiphysics code that allows users to 
 run a large class of simulations involving fluid flow and to leverage adap
 tive mesh refinement to achieve their goals.  FLASH has already under
 gone four major revisions and is presently being updated and rearchitected
  to meet...\n\n---------------------\nGeneral Discussion About Addressing 
 Heterogeneity in AMR\n\nDubey\n\nThe final presentation slot in the minisy
 mposium will be used for a general discussion on techniques for managing p
 latform heterogeneity in AMR based applications. There are two objectives 
 of this exercise. The first is to give opportunity to the members of the a
 udience to share their approaches and...\n\n---------------------\nAsynchr
 onous AMR and  Runtime Systems\n\nBerzins\n\nThe uintah software has adopt
 ed an asynchronous task based approach since 2011 or so. Both traditional 
 and amr for globally connected radiation problems are supported. In this w
 ork the advantages and challenges of an asynchronous approach are consider
 ed. The outcome of this is that a combination of ...\n\n------------------
 ---\nEnzo-E, an Array-of-Octrees AMR Cosmology Code for the Exascale Era\n
 \nNorman, Bordner\n\nEnzo-E is an evolution of the Enzo-P/Cello astrophysi
 cal simulation framework targeting exascale architectures. Enzo-E implemen
 ts the Enzo community code’s rich suite of physics solvers on an ext
 reme scale AMR software framework called Cello developed concurrently. Cel
 lo implements array-of-oc...\n
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