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Matteo Cantiello edited figures/visibility_mosser_suppressed_band/caption.tex
about 9 years ago
Commit id: 6a0dbb08bd6f80482f360a85ab02798d0f33f9c2
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Replace this text Visibility $V^2$ of $\ell=1$ modes as function of $\nu_{max}$. The star symbols represent data from \citet{Mosser_2011} rescaled by 1.54, the expected average visibility of $\ell=1$ modes \citep{Ballot_2011}. The theoretical band shows the visibility of dipole modes suppressed by the magnetic greenhouse effect in a $1.6\mso$ star, as predicted by Eq.~\ref{eqn:vis}. Suppressed dipoles (orange stars) are identified following the same criteria as in \citet{Mosser_2011}. The visibility of the suppressed dipoles in KIC 8561221 \cite{Garc_a_2014} and KIC 9073950 is also shown (diamond and circle symbols, respectively). Here we used values for $\tau_{\rm ac}$ in the range [5, 20] d, consistent with
your caption \cite{Dupret_2009}.
