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      Magnetic confinement of the solar tachocline

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      Astronomy & Astrophysics
      EDP Sciences

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          Numerical simulations of stellar convective dynamos. I. the model and method

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            Three‐dimensional Spherical Simulations of Solar Convection. I. Differential Rotation and Pattern Evolution Achieved with Laminar and Turbulent States

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              Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars

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                Author and article information

                Journal
                Astronomy & Astrophysics
                A&A
                EDP Sciences
                0004-6361
                1432-0746
                October 2006
                September 12 2006
                October 2006
                : 457
                : 2
                : 665-674
                Article
                10.1051/0004-6361:20053908
                ccc55b40-dbe5-45a5-8121-3c5d35a22d5e
                © 2006
                History

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