Differential Rotation and Dynamics of the Solar Interior

@article{Thompson1996DifferentialRA,
  title={Differential Rotation and Dynamics of the Solar Interior},
  author={Michael J. Thompson and J. Toomre and E. R. Anderson and H. M. Antia and Gabrielle Berthomieu and D. Burtonclay and Shashikumar M. Chitre and J. Christensen-Dalsgaard and Thierry Corbard and Marc L. Derosa and Christopher R. Genovese and Douglas O. Gough and Deborah A. Haber and J. W. Harvey and Frank Hill and Roger T. Howe and Sylvain Gereon Korzennik and Alexander G. Kosovichev and John Leibacher and Frank P Pijpers and Janine Provost and Edward J. Rhodes and Jesper Schou and Takashi Sekii and Philip B. Stark and P. R. Wilson},
  journal={Science},
  year={1996},
  volume={272},
  pages={1300 - 1305}
}
Splitting of the sun's global oscillation frequencies by large-scale flows can be used to investigate how rotation varies with radius and latitude within the solar interior. The nearly uninterrupted observations by the Global Oscillation Network Group (GONG) yield oscillation power spectra with high duty cycles and high signal-to-noise ratios. Frequency splittings derived from GONG observations confirm that the variation of rotation rate with latitude seen at the surface carries through much of… Expand

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