期刊
SOLAR PHYSICS
卷 251, 期 1-2, 页码 77-89出版社
SPRINGER
DOI: 10.1007/s11207-008-9232-6
关键词
helioseismology, direct modeling; interior, convection zone; oscillations, solar; velocity fields, interior; waves, acoustic, modes
We investigate the influence of large-scale meridional circulation on solar p modes by quasi-degenerate perturbation theory, as proposed by Lavely and Ritzwoller (Roy. Soc. Lond. Phil. Trans. Ser. A 339, 431, 1992). As an input flow we use various models of stationary meridional circulation obeying the continuity equation. This flow perturbs the eigenmodes of an equilibrium model of the Sun. We derive the signatures of the meridional circulation in the frequency multiplets of solar p modes. In most cases the meridional circulation leads to negative average frequency shifts of the multiplets. Further possibly observable effects are briefly discussed.
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