Directory: ${PENCIL_HOME}/samples/corona SVN Id: $Id$ Maintainer: Philippe Bourdin <pc/bourdin[dot]ch> Matthias Rheinhardt <mreinhardt/nordita[dot]org> Jörn Warnecke <joern[dot]warnecke/gmail[dot]com> Sven Bingert <sven[dot]bingert/gwdg[dot]de> Vartika Pandey <vartika[dot]pandey/uni-graz[dot]at> Added: 12-Oct-2006 Status: succeeds # One of [succeeds|failing since <date>|obsolete| ...] Recommended resolution: 128x128x128 (nu=eta=10 Mm km/s) Comments: The initial magnetic field distribution is derived from a magnetogram. On the lower boundary there is time-dependent forcing. Heat conduction is here uniform (iheatcond='K-const'). This example uses SI units, a non-uniform mesh in the z direction, References: Gudiksen, B. V., and Nordlund, Å.: 2005, ``An Ab Initio Approach to the Solar Coronal Heating Problem,'' Astrophys. J. 618, 1020-1030