*Youhei SASAKI1, Shin-ichi TAKEHIRO2
(1.Department of Mathematics, Kyoto University, 2.Research Institute for Mathematical Sciences, Kyoto University)
Keywords:Earth's outer core, Mercury's outer core, Dynamo, Alfven waves
Numerical experiments of magneto-hydrodynamic dynamo in a rotating spherical shell with a strongly stable outer layer are performed. Although the estimated values of penetration thickness of the disturbances into the stable layer proposed by Takehiro and Lister (2001) for non-magnetic cases are sufficiently small compared with the thickness of the stable layer, it is observed that vortical fluid motions and toroidal magnetic field disturbances deeply penetrate into the stable layer. These magneto-hydrodynamic disturbances in the stable layer can be interpreted as the Alfven waves whose fluid motions are restricted in the horizontal directions. The proposed theoretical expression of propagation distance
of the Alfven waves suggests that the numerically obtained fields permit the complete propagation of the Alfven waves across the stable layer.