deletions | additions       diff --git a/Magnetic Constraints.tex b/Magnetic Constraints.tex  index d1731d5..d7f2fbf 100644  --- a/Magnetic Constraints.tex  +++ b/Magnetic Constraints.tex 
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Above, we showed that incoming magneto-gravity waves will become trapped in the core if the magneto-gravity frequency $\omega_{\rm MG}$ exceeds the wave frequency $\omega$ at some point within the core. Magnetic trapping therefore require field strengths such that  \begin{equation}  v_A > \gtrsim  \frac{\omega^2}{2 \mu N k_\perp} \end{equation}  somewhere in the g-mode cavity. This requires field strengths to exceed a critical value:  \beqin{equation}