/*********************************************************************************** Copyright 2006 Charles F. Gammie, Jonathan C. McKinney, Scott C. Noble, Gabor Toth, and Luca Del Zanna HARM version 1.0 (released May 1, 2006) This file is part of HARM. HARM is a program that solves hyperbolic partial differential equations in conservative form using high-resolution shock-capturing techniques. This version of HARM has been configured to solve the relativistic magnetohydrodynamic equations of motion on a stationary black hole spacetime in Kerr-Schild coordinates to evolve an accretion disk model. You are morally obligated to cite the following two papers in his/her scientific literature that results from use of any part of HARM: [1] Gammie, C. F., McKinney, J. C., \& Toth, G.\ 2003, Astrophysical Journal, 589, 444. [2] Noble, S. C., Gammie, C. F., McKinney, J. C., \& Del Zanna, L. \ 2006, Astrophysical Journal, 641, 626. Further, we strongly encourage you to obtain the latest version of HARM directly from our distribution website: http://rainman.astro.uiuc.edu/codelib/ HARM is free software; you can redistribute it and/or modify it under the terms of the GNU General Public License as published by the Free Software Foundation; either version 2 of the License, or (at your option) any later version. HARM is distributed in the hope that it will be useful, but WITHOUT ANY WARRANTY; without even the implied warranty of MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the GNU General Public License for more details. You should have received a copy of the GNU General Public License along with HARM; if not, write to the Free Software Foundation, Inc., 51 Franklin St, Fifth Floor, Boston, MA 02110-1301 USA ***********************************************************************************/