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The asymptotic spectrum of gravity modes as a function of the solar structure: Standard solar model

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Abstract

Some results are given on the properties of the second-order asymptotic expression of the periods of low-degree gravity modes and on their rotational splitting. These could be of some help for the detection of these modes in the signal.

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Authors and Affiliations

  1. Département Cassini, CNRS and Observatoire de la Cote d'Azur, Nice, France

    G. Berthomieu & J. Provost

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  1. G. Berthomieu
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  2. J. Provost
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Berthomieu, G., Provost, J. The asymptotic spectrum of gravity modes as a function of the solar structure: Standard solar model. Sol Phys 133, 127–138 (1991). https://doi.org/10.1007/BF00149833

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  • DOI: https://doi.org/10.1007/BF00149833

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