A Comparison of Solar p ‐Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions - Archive ouverte HAL Access content directly
Journal Articles The Astrophysical Journal Year : 2002

A Comparison of Solar p ‐Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions

J. Christensen‐dalsgaard
  • Function : Author
F. Hill
  • Function : Author
R. Komm
  • Function : Author
R. Larsen
  • Function : Author
M. Rabello‐soares
  • Function : Author
M. Thompson
  • Function : Author
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hal-02896051 , version 1 (10-07-2020)

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J. Schou, R. Howe, S. Basu, J. Christensen‐dalsgaard, T. Corbard, et al.. A Comparison of Solar p ‐Mode Parameters from the Michelson Doppler Imager and the Global Oscillation Network Group: Splitting Coefficients and Rotation Inversions. The Astrophysical Journal, 2002, 567 (2), pp.1234-1249. ⟨10.1086/338665⟩. ⟨hal-02896051⟩
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