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Jim Fuller edited section_Segue_to_RGs_maybe__.tex
almost 9 years ago
Commit id: a616437a70f671de5207b620c842f8acea578db9
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%[REF Bedding2011/Stello2013/Mosser2014]
and to measure radial differential rotation \citep{Beck_2011,Mosser_2012}.
This fortune arises because %[through resonance coupling where]
each acoustic non-radial envelope mode
couple couples to multiple gravity
modes in the
core core, forming several
observable mixed modes %observable at the surface,
with frequencies
observable in the vicinity of the acoustic mode \citep{Beck_2011}.
This coupling is strongest for dipole modes making them the most useful
probes of the core \citep{Dupret_2009}. %[REF Unno/Dupret?].