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RESEARCH PRODUCT
3-Dimensional Hydrodynamic Interaction of a Supernova Remnant Shock with an Isolated Cloud
Fabio RealeSalvatore OrlandoGiovanni Peressubject
Shock waveSupernovabusiness.industryComputer scienceInterstellar cloudCloud computingHydrodynamic codeShock (mechanics)Flash (photography)SupernovaSettore FIS/05 - Astronomia E AstrofisicaShock waveHydrodynamic interactionScalabilityAerospace engineeringbusinessSupernova remnantInterstellar clouddescription
We report on a computational key-project in astrophysics. The project is aimed at studying the interaction of a supernova shock wave with interstellar clouds. We describe the numerical code used, namely FLASH, a multi-dimensional astrophysical hydrodynamics code for parallel computers developed at the FLASH center (The University of Chicago); our team collaborates with, and contributes to, the FLASH project. We discuss the resources required for the whole project, the I/O management, the performance and the scalability of the code on IBM/Sp4 at CINECA. Finally, we present a selection of results. © 2005 IEEE.
year | journal | country | edition | language |
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2006-10-11 | Seventh International Workshop on Computer Architecture for Machine Perception (CAMP'05) |