Asymptotic g modes: Evidence for a rapid rotation of the solar core

@article{Fossat2017AsymptoticGM,
  title={Asymptotic g modes: Evidence for a rapid rotation of the solar core},
  author={E. Fossat and P. Boumier and T. Corbard and J. Provost and D. Salabert and F. Schmider and A. Gabriel and G. Grec and C. Renaud and J. Robillot and T. Roca-Cort'es and S. Turck-chi{\`e}ze and R. Ulrich and M. L. U. C. D. Azur and Cnrs and Laboratoire Lagrange and France. and I. D. Spatiale and U. Paris-sud and Laboratoire Aim Paris-Saclay and CEADRF-CNRS-Univ. Paris Diderot - IRFUSAp and Lab and D. D. Astrof'isica and U. L. Laguna and Spain. and I. A. D. Canarias and D. Physics and A. Department and U. Angeles and U.S.A. and Lphea Laboratory and O. Observatory and Cadi Ayyad University Fssm and Morocco.},
  journal={arXiv: Solar and Stellar Astrophysics},
  year={2017}
}
We present the identification of very low frequency g modes in the asymptotic regime and two important parameters that have long been waited for: the core rotation rate, and the asymptotic equidistant period spacing of these g modes. The GOLF instrument on board the SOHO space observatory has provided two decades of full-disk helioseismic data. In the present study, we search for possible collective frequency modulations that are produced by periodic changes in the deep solar structure. Such… Expand
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