VH-1, implementation of piecewise parabolic method <author>Numerical Astrophysics Group, University of Virginia Institute of Theoretical Astrophysics <version> <abstract> VH-1 is an implementation of the piecewise parabolic method (PPM) of Colella and Woodward. <contact>Greg Lindahl / lindahl@pbm.com <keywords>piecewise parabolic method (PPM); Lagrangian Remap; hydrodynamics; application program <category>application <publication-date> <environment> <method>piecewise parabolic method (PPM) <application>compressible non-turbulent hydrodynamics, astrophysics, ideal gas computations, convection <comments> The version that we distribute is a subset of everything we've done with the code. It does include 1D, 2D, 3D, 1D self-gravity, shock flattening, spherical and cylindrical geometries, and angular momentum. It does not include artificial viscosity, 2D or 3D self-gravity, multiple fluids, a variable gamma equation of state, or radiative heating or cooling. A large number of test case initializations are included. We highly recommend that you be familiar with numerical hydrodynamics before you attempt to use VH-1, or that you plan on spending a large amount of time learning hydro before you believe anything. </urc>

http://www.pbm.com/~lindahl/VH-1.html VH-1, implementation of piecewise parabolic method <author>Numerical Astrophysics Group, University of Virginia Institute of Theoretical Astrophysics <version> <abstract> VH-1 is an implementation of the piecewise parabolic method (PPM) of Colella and Woodward. <contact>Greg Lindahl / lindahl@pbm.com <keywords>piecewise parabolic method (PPM); Lagrangian Remap; hydrodynamics; application program <category>application <publication-date> <environment> <method>piecewise parabolic method (PPM) <application>compressible non-turbulent hydrodynamics, astrophysics, ideal gas computations, convection <comments> The version that we distribute is a subset of everything we've done with the code. It does include 1D, 2D, 3D, 1D self-gravity, shock flattening, spherical and cylindrical geometries, and angular momentum. It does not include artificial viscosity, 2D or 3D self-gravity, multiple fluids, a variable gamma equation of state, or radiative heating or cooling. A large number of test case initializations are included. We highly recommend that you be familiar with numerical hydrodynamics before you attempt to use VH-1, or that you plan on spending a large amount of time learning hydro before you believe anything. </urc>