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authorallen <allen@c78560ca-4b45-4335-b268-5f3340f3cb52>1999-09-24 09:06:10 +0000
committerallen <allen@c78560ca-4b45-4335-b268-5f3340f3cb52>1999-09-24 09:06:10 +0000
commit99240a432530b3d9be2028b9320a302cb196cc57 (patch)
treeccf6154e5810b16f358125c54ee0d947bd0d74eb /doc
parente249568b916c3a2c2dee2ed25bf3de2c5c1c5f32 (diff)
The very beginning of the CartGrid3D doc
git-svn-id: http://svn.cactuscode.org/arrangements/CactusBase/CartGrid3D/trunk@57 c78560ca-4b45-4335-b268-5f3340f3cb52
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+\documentclass{article}
+\begin{document}
+
+\title{CartGrid3D}
+\author{Gabrielle Allen, Gerd Lanfermann}
+\date{1999}
+\maketitle
+
+\abstract{Cartesian coordinates and symmetries for 3D grids}
+
+\section{Purpose}
+
+Allows you to set up coordinates on a 3D Cartesian grid in a
+flexible manner. Different grid domains (e.g. octant) can
+be chosen to allow you to exploit any symmetry in your
+problem. Routines for registering symmetries of grid functions
+and applying symmetry conditions across the coordinate axes
+are provided.
+
+\section{Comments}
+
+\subsection{Coordinates}
+
+The Cartesian coordinates supplied by this thorn are
+grid functions with the standard names {\tt x}, {\tt y}, and
+{\tt z}. To use these coordinates you need to {\tt inherit}
+from {\tt grid}. The coordinates are
+registered with the flesh using the same names "x", "y"
+and "z". In addition a grid function {\tt r} (registered as
+"r") is provided, containing the radius from the origin.
+
+
+
+% Automatically created from the ccl files by using gmake thorndoc
+\include{interface}
+\include{param}
+\include{schedule}
+
+\end{document}