Effects of boundary layers on magnetic field behavior in an MHD dynamo model

F. Takahashi, J. S. Katayama, M. Matsushima, Y. Honkura

研究成果: ジャーナルへの寄稿学術誌査読

12 被引用数 (Scopus)

抄録

Numerical simulations of three-dimensional self-consistent MHD dynamos in a rotating spherical shell are performed to examine the structures of the velocity and the magnetic fields and the mechanism of magnetic field generation. Emphasis is put on an important role of the boundary layer which arises for the no-slip boundary condition. The most important is precise computation in the boundary layers, in which the number of grid points must be large enough to ensure spatial resolution there. The result of computation shows that the dipole field is dominant and that the magnetic field is concentrated in the convection columns. Such results are the same as those derived from our previous study for the stress-free boundary condition. A marked difference is the strong toroidal magnetic field generated by strong shear flow inside the boundary layers. Also the effect of magnetic diffusion is strong and more significant than that of magnetic induction near the spherical surfaces. This suggests that the so-called frozen-flux hypothesis, which has usually been used to estimate core surface flows, does not necessarily hold for the cases in which significant boundary layers appear.

本文言語英語
ページ(範囲)149-161
ページ数13
ジャーナルPhysics of the Earth and Planetary Interiors
128
1-4
DOI
出版ステータス出版済み - 2001
外部発表はい

!!!All Science Journal Classification (ASJC) codes

  • 天文学と天体物理学
  • 地球物理学
  • 物理学および天文学(その他)
  • 宇宙惑星科学

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