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Paper: Modelling Astrophysical Turbulent Convection
Monograph: 6, Twenty Years of ADASS
Page: 23
Authors:
Abstract: Numerical simulations of highly turbulent flows in astrophysics benefit greatly from recent advances in high performance computing. Yet such three-dimensional modelling raises major problems in capturing, moving, and analyzing the resulting massive data sets necessary to sample the evolving intricate dynamics. Thus archiving, networking, and visualization are as essential as the actual act of computing when it comes to real scientific progress.
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