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Jim Fuller edited Magnetic_fields_can_provide_the__.tex
almost 9 years ago
Commit id: e570cff1ac6528116a45f0d23c6d42d0d9423a00
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\end{equation}
This field strength approximately corresponds to the point at which the Alfv\'en speed becomes larger than the radial group velocity of gravity waves.
Magneto-gravity waves become evanescent in regions where the radial magnetic field strength exceeds the critical value of equation \ref{eqn:Bc}. Low-frequency gravity waves cannot exist in these regions because magnetic tension overwhelms the buoyancy force, i.e., the stiff field lines cannot be bent by the placid gravity wave motion. {\bf
Magneto-gravity Dipole magneto-gravity waves are evanescent when $\omega < \omega_{\rm MG}$, where the magneto-gravity frequency $\omega_{\rm MG}$ is defined as}
\begin{equation}
\label{eqn:maggrav}
\omega_{\rm MG} = \bigg[ \frac{2}{\pi} \frac{B_r^2 N^2}{\rho r^2} \bigg]^{1/4} \, .
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