pith. sign in

arxiv: 1112.4482 · v1 · pith:3GLUKBU6new · submitted 2011-12-19 · 🌌 astro-ph.IM · astro-ph.CO

High-Performance Astrophysical Simulations and Analysis with Python

classification 🌌 astro-ph.IM astro-ph.CO
keywords astrophysicaldataanalysispythonvisualizationgeneratedhigh-performancemechanisms
0
0 comments X
read the original abstract

The usage of the high-level scripting language Python has enabled new mechanisms for data interrogation, discovery and visualization of scientific data. We present yt, an open source, community-developed astrophysical analysis and visualization toolkit for data generated by high-performance computing (HPC) simulations of astrophysical phenomena. Through a separation of responsibilities in the underlying Python code, yt allows data generated by incompatible, and sometimes even directly competing, astrophysical simulation platforms to be analyzed in a consistent manner, focusing on physically relevant quantities rather than quantities native to astrophysical simulation codes. We present on its mechanisms for data access, capabilities for MPI-parallel analysis, and its implementation as an in situ analysis and visualization tool.

This paper has not been read by Pith yet.

discussion (0)

Sign in with ORCID, Apple, or X to comment. Anyone can read and Pith papers without signing in.