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Seventh International Workshop on Computer Architecture for Machine Perception (CAMP'05)
3-Dimensional Hydrodynamic Interaction of a Supernova Remnant Shock with an Isolated Cloud
Palermo, Italy
July 04-July 06
ISBN: 0-7695-2255-6
Salvatore Orlando, INAF - Osservatorio Astronomico di Palermo
Giovanni Peres, Universit? degli Studi di Palermo
Fabio Reale, Universit? degli Studi di Palermo
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.
Citation:
Salvatore Orlando, Giovanni Peres, Fabio Reale, "3-Dimensional Hydrodynamic Interaction of a Supernova Remnant Shock with an Isolated Cloud," camp, pp.135-140, Seventh International Workshop on Computer Architecture for Machine Perception (CAMP'05), 2005
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