The PLUTO Code for Adaptive Mesh Computations in Astrophysical Fluid Dynamics

We present a description of the adaptive mesh refinement (AMR) implementation of the PLUTO code for solving the equations of classical and special relativistic magnetohydrodynamics (MHD and RMHD). The current release exploits, in addition to the static grid version of the code, the distributed infra...

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Bibliographic Details
Published in:	The Astrophysical journal. Supplement series Vol. 198; no. 1; pp. 7 - 31
Main Authors:	Mignone, A, Zanni, C, Tzeferacos, P, van Straalen, B, Colella, P, Bodo, G
Format:	Journal Article
Language:	English
Published:	United States IOP Publishing 01.01.2012
Subjects:	ANISOTROPY ASTROPHYSICS ASTROPHYSICS, COSMOLOGY AND ASTRONOMY BENCHMARKS CALCULATION METHODS Computational fluid dynamics Corners DAMPING Dissipation ERRORS Infrastructure INTERPOLATION MAGNETIC FIELDS MAGNETOHYDRODYNAMICS Mathematical analysis P CODES RELATIVISTIC RANGE SOURCE TERMS THERMAL CONDUCTION VISCOSITY
ISSN:	0067-0049, 1538-4365
Online Access:	Get full text
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