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Helioseismology has taught us a great deal about the stratification and kinematics of the solar interior, sufficient for us to embark upon dynamical studies more detailed than have been possible before.
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2003
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P.H. Diamond, S.-I. Itoh, K. Itoh, L.J. Silvers, β \beta -Plane Mhd Turbulence and Dissipation in the Solar Tachocline, in The Solar Tachocline
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S. Basu, W.J. Chaplin, Y. Elsworth, R. New, A.M. Serenelli, Fresh Insights on the Structure of the Solar Core. Astrophys. J. 699
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B.M. Byington, N.H. Brummell, J.M. Stone, D.O. Gough, Stoked nondynamos: sustaining field in magnetically non-closed systems. New J. Phys. 16
2014
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2015
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S. Hanasoge, M.S. Miesch, M. Roth, J. Schou, M. Schüssler, M.J. Thompson, Solar dynamics, rotation, convection and overshoot. Space Sci. Rev. (2015). doi:10.1007/s11214-015
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J. Toomre, M.J. Thompson, Prospects and Challenges for Helioseismology, in this volume
2015
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H.M. Antia, S. Basu, Revisiting the Solar Tachocline: Average Properties and Temporal Variations. Astrophys. J. Lett. 735
2041
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