Directory:
    ${PENCIL_HOME}/samples/spherical-convection-kramers/
SVN Id:
    $Id$
Maintainer:
    Petri Käpylä <pkaepyl/uni-goettingen[dot]de>
    Jörn Warnecke <joern[dot]warnecke/gmail[dot]com>
Added:
    08-May-2020
Status:
    Introduced in May 2020
Recommended resolution:
    144x432x216 (nu = eta = chi_t1 = 2.5e-5)
Comments:
    Spherical convection with Kramers heat conductivity with enhanced 
    fixed-in-space K-profile near the surface to carry the flux through
    the surface.
References:
    Käpylä, P. J., Gent, F. A., Olspert, N., Käpylä M. J. & Brandenburg A.: 
    2020, ``Sensitivity to luminosity, centrifugal force, and boundary 
    conditions in spherical shell convection,'' Geophys. Astrophys. Fluid. 
    Dyn, 114, 8

    Käpylä P. J., Viviani, M., Käpylä M. J., Brandenburg A. & Spada, F.:
    2019, ``Effects of a subadiabatic layer on convection and dynamos in 
    spherical wedge simulations,'' Geophys. Astrophys. Fluid. Dyn, 113, 149