A Three Function Variational Principle for Stationary Non-Barotropic Magnetohydrodynamics

Asher Yahalom

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arXiv · 2109.03817

A Three Function Variational Principle for Stationary Non-Barotropic Magnetohydrodynamics

Asher Yahalom

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Abstract

Variational principles for magnetohydrodynamics (MHD) were in\-troduced by previous authors both in Lagrangian and Eulerian form. In this paper we introduce simpler Eulerian variational principles from which all the relevant equations of non-barotropic stationary magnetohydrodynamics can be derived for certain field topologies. The variational principle is given in terms of three independent functions for stationary non-barotropic flows. This is a smaller number of variables than the eight variables which appear in the standard equations of non-barotropic magnetohydrodynamics which are the magnetic field $\vec B$ the velocity field $\vec v$, the entropy $s$ and the density $\rho$. We further investigate the case in the flow along magnetic lines is not ideal.

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Asher Yahalom. 2021-08-10. A Three Function Variational Principle for Stationary Non-Barotropic Magnetohydrodynamics. https://arxiv.org/abs/2109.03817

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