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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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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