This paper reports on efforts to simulate wave propagation in the solar interior. Presented is work on extending a numerical code for constant entropy acoustic waves in the absence of magnetic fields to the case where magnetic fields are present. A set of linearized magnetohydrodynamic (MHD) perturbation equations has been derived and implemented.
@article{arxiv.0805.0333,
title = {Wave propagation in the magnetic sun},
author = {T. Hartlep and M. S. Miesch and N. N. Mansour},
journal= {arXiv preprint arXiv:0805.0333},
year = {2008}
}