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\subsection{Local Analysis} \subsection{Magneto-Gravity Waves}  The properties of magnetohydrodynamic waves in red giant cores can be understood using a local (WKB) analysis for high wavenumbers ${\bf k}$, in which $k r \gg 1$ and $k H \gg 1$ (where $H$ is a pressure scale height). We show below the WKB limit is always a good approximation in our stellar models.