Research Project
Grant-in-Aid for Young Scientists (B)
Numerical model for MHD in rotating sphericall shells is developed. Linear stability analysis of compressible % thermal convection in rotating spherical shells using this numerical model is performed with the anelastic approximation. At large compressibility, the location of convection column is close to the outer boundary, and the convective motion occurs are near the outer boundary. This feature is highly depends radical thermal diffusivity. Numerical experiments of magneto-hydrodynamic dynamo in a rotating spherical shell with a strongly stable outer layer are performed. 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.
All 2017 2016 2015 2014 2013
All Journal Article (7 results) (of which Int'l Joint Research: 1 results, Peer Reviewed: 7 results, Open Access: 1 results) Presentation (22 results) (of which Invited: 3 results)
Physics of the Earth and Planetary Interiors
Volume: - Pages: 258-264
10.1016/j.pepi.2017.03.001
Geochemistry, Geophysics, Geosystem
Volume: 電子出版 Issue: 5 Pages: 1586-1607
10.1002/2015gc006159
Geophysical Journal International
Volume: 197 Issue: 1 Pages: 119-134
10.1093/gji/ggt518
Volume: 196 Issue: 2 Pages: 712-723
10.1093/gji/ggt425
Progress in Physics of the Sun and Stars
Volume: 479 Pages: 285-294
Phys. Earth Planet. Inter.
Volume: 223 Pages: 55-61
10.1016/j.pepi.2013.07.003
ながれ
Volume: 32 Pages: 469-472