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Contribution of high-degree frequency splittings to the inversion of the solar rotation rate

  • Part V Inverse Problems of Solar Oscillations
  • Conference paper
  • First Online:
Progress of Seismology of the Sun and Stars

Part of the book series: Lecture Notes in Physics ((LNP,volume 367))

Abstract

We present the contribution of high degree rotational splittings to the inversion of the internal rotation rate around the equator. The extention of the input data set to l of 500, allow us to improve the resolution of the solution mainly in the outermost 15% of the solar radius. The rotational profile obtained in the regions below the surface leads to an attractive picture that could reconcile different non-seismic estimates of the “surface” rotation rate.

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Author information

Authors and Affiliations

  1. University of California, 90024, Los Angeles, CA, USA

    Sylvain G. Korzennik & Roger K. Ulrich

  2. University “La Sapienza”, Rome, Italy

    Alessandro Cacciani

  3. University of Southern California, 90089, Los Angeles, CA, USA

    Edward J. Rhodes Jr.

  4. Jet Propulsion Laboratory, California Institute of Technology, 91109, Pasadena, CA, USA

    Edward J. Rhodes Jr.

Authors
  1. Sylvain G. Korzennik
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  2. Alessandro Cacciani
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  3. Edward J. Rhodes Jr.
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  4. Roger K. Ulrich
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Editor information

Y. Osaki H. Shibahashi

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© 1990 Springer-Verlag

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Korzennik, S.G., Cacciani, A., Rhodes, E.J., Ulrich, R.K. (1990). Contribution of high-degree frequency splittings to the inversion of the solar rotation rate. In: Osaki, Y., Shibahashi, H. (eds) Progress of Seismology of the Sun and Stars. Lecture Notes in Physics, vol 367. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-53091-6_99

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  • DOI: https://doi.org/10.1007/3-540-53091-6_99

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-53091-6

  • Online ISBN: 978-3-540-46645-1

  • eBook Packages: Springer Book Archive

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