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Jim Fuller edited figures/DipoleTime/caption.tex
almost 9 years ago
Commit id: 4e5c308e51b55097ebbaa23a49f036c5f873700a
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\label{fig:DipoleTime}
{\bf Wave leakage time scale as a function of $\nu_{\rm
max}$}. max}$ for a $1.6 \, M_\odot$ stellar model.}. The leakage timescale has been calculated by solving the linearized wave equations (equation \ref{eqn:tleak2}), and by approximating it using equation \ref{eqn:tleak}, evaluating the transmission coefficient $T$ via equation \ref{eqn:integral2} or \ref{eqn:integral}.