MHD Star Formation in a Protostellar Cloud#
Domain: Consider a 3D computational domain representing a protostellar cloud.
Finite Element Mesh: Use a tetrahedral or hexahedral mesh for the 3D domain.
Boundary Conditions:
Inflow boundary conditions representing the infall of material.
Outflow conditions at the outer boundary.
Initial Conditions:
Set up an initial density and temperature distribution.
Include a small seed magnetic field perturbation.