This submodule defines an equilibrium in Cartesian geometry with a stratified equilibrium profile, representing a solar magnetic atmosphere. The equilibrium is isothermal with a constant magnetic field. The scale height is given by The geometry is fixed to Cartesian, boundaries can be overridden using the parfile.
This equilibrium is taken from Nye, A., & Thomas, J. (1976). Solar magneto-atmospheric waves. I. An exact solution for a horizontal magnetic field. The Astrophysical Journal, 204. 573-581.
Default values are given by
and can all be changed in the parfile.
This equilibrium has no regression test yet!