Directory:
    ${PENCIL_HOME}/samples/supernova-driven-turbulence/ferriere-hs-magnetic/
SVN Id:
    $Id: README 13067 2010-01-25 07:08:53Z f.a.gent@ncl.ac.uk $
Maintainer:
    Frederick Gent <fred.gent.ncl/gmail[dot]com>
Added:
    22-Jan-2010
Status:
    has been working in this form since 22-Jan-2010
Recommended resolution:
    at least 52x52x200
Comments:
    galactic gravity profile derived from Katia Ferriere review
    initial density(z) profile chosen to approximate
    isothermal hydrostatic equilibrium
    weak azimuthal seed field (peak 1.7724e-8 Gauss)
    proportional to gas density
    includes radiative cooling, uv heating