Calculation of Solar P-mode Oscillation Frequency Splittings Based on a Two-dimensional Solar Model

Abstract

We compute the p-mode oscillation frequencies and frequency splittings that arise in a two-dimensional model of the Sun that contains toroidal magnetic fields in its interior.

4 pages, 3 figures, in proceedings of GONG2008/SOHO XXI: Solar-stellar dynamos as revealed by helio- and asteroseismology, August 11-15, 2008 - Boulder, Colorado