The quest for the solar g modes

@article{Appourchaux2010TheQF,
  title={The quest for the solar g modes},
  author={Thierry Appourchaux and K'evin Belkacem and A-M. Broomhall and William J. Chaplin and Douglas O. Gough and G{\"u}nter Houdek and Janine Provost and Fr'ed'eric Baudin and Patrick Boumier and Yvonne P. Elsworth and R. A. Garcı́a and Bo Nyborg Andersen and Wolfgang Finsterle and Claus Fr{\"o}hlich and Alan H. Gabriel and G{\'e}rard Grec and Antonio J. Jimenez and Alexander G. Kosovichev and Takashi Sekii and Thierry Toutain and S. Turck-chi{\`e}ze},
  journal={The Astronomy and Astrophysics Review},
  year={2010},
  volume={18},
  pages={197-277}
}
Solar gravity modes (or g modes)—oscillations of the solar interior on which buoyancy acts as the restoring force—have the potential to provide unprecedented inference on the structure and dynamics of the solar core, inference that is not possible with the well-observed acoustic modes (or p modes). The relative high amplitude of the g-mode eigenfunctions in the core and the evanesence of the modes in the convection zone make the modes particularly sensitive to the physical and dynamical… Expand
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