Abstract

Self-similar, magnetohydrodynamic (MHD) solutions are developed for a cold planar wall next to a hot plasma with an embedded magnetic field parallel to the wall, including the relevant electro-thermal terms. Velikovich et al., [1] studied the Nernst effect in the induction equation for such a problem under the assumption that the ratio of thermal to magnetic pressure $(\beta)$ was large. Other electro-thermal processes, such as Ettingshausen, Joule heating, and Nernst-thermal heating vary inversely with $\beta$ . To study all these we have extended the self-similar formulation to allow for an arbitrary $\beta$ . The self-similar ansatz requires constant total pressure, thermal plus magnetic. Four self-similar solutions are presented with the same density and temperature boundary conditions: two of high $\beta$ and two of low $\beta,$ and for each of these with and without electro-thermal terms. At high $\beta$ only the N ernst term $i$ n the induction equation affects the solution. At low $\beta$ The Ettingshausen term is larger than thermal conduction at the wall, and the thermal N ernst term is negative. The results are proposed as verification tests for advanced, multi-physics, MHD codes. An example calculation is presented from a 1D MHD simulation code that allows for total pressure changes through the momentum equation. Comparison with the self-similar solution for one case shows that the simulation results approach the self-similar solution.

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