A 1, 2 and 3 dimensional Smoothed Particle Hydrodynamics (SPH) simulation code. This is my "development" code, used to develop new SPH algorithms. Contains implementations of nearly algorithm I have published for SPH, but not particularly optimised, nor parallel, but good for exploring how SPH works and trying out new ideas on a wide range of test problems for compressible hydrodynamics and magnetohydrodynamics, mostly in the context of astrophysics.
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NDSPMHD: A Smoothed Particle (Magneto)Hydrodynamics code for (astrophysical)
fluid dynamics simulations in 1, 2 and 3 spatial dimensions.
(c) 2002-2015 Daniel Price
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THIS CODE IS DISTRIBUTED UNDER THE TERMS OF THE GNU GENERAL PUBLIC LICENCE
(see LICENSE file for details)
Please note that I am able to provide only limited support for this code.
[email protected], May 2015
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The code is written in Fortran 90/95
by Daniel Price, [email protected]
The source code is organised into the following directories:
src -- source code for NDSPMHD
docs -- contains documentation for NDSPMHD
scripts -- various scripts for manipulating data/running multiple jobs
see the INSTALL file for installation instructions
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All documentation that exists for this code is now on the web page:
http://users.monash.edu.au/~dprice/ndspmhd/
I no longer maintain separate documentation in the code directories
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