\label{fig:DipoleTime}
Wave leakage time scale as a function of $\nu_{\rm max}$ for a $1.6 \, M_\odot$ stellar model. The leakage timescale has been calculated by solving the linearized wave equations (Eqn. \ref{eqn:tleak2}), and by approximating it using Eqn. \ref{eqn:tleak}, evaluating the transmission coefficient $T$ via Eqn. \ref{eqn:integral2} or \ref{eqn:integral}.