An Analytical Study of the Structure of Two-Dimensional Magnetostatic Equilibria in the Presence of Gravity

T. Amari, J.J. Aly
1989 International Astronomical Union Colloquium  
In order to understand how prominences are supported in the solar corona, we have recently developed several 2D models describing x-invariant equilibrium configurations of a plasma occupying a half-space {z > 0} and submitted to a magnetic field then of the form(1)
doi:10.1017/s0252921100154326 fatcat:tiflekmh2fg5rmfpjnfnh6wlmy