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Prof. Andrew Soward16/02/2011, 11:00The onset of instability of a Boussinesq fluid within a rapidly rotating spherical shell is considered, when a thin unstable layer lies adjacent to the inner sphere boundary, radius r_i . This layer, which is of radial extent O(ε^2 r_i ), sits beneath the remaining (stably stratified) fluid. The variable stratification is effected by a combination of differential heating between the...Go to contribution page
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Dr Petri Käpylä (University of Helsinki)16/02/2011, 11:30The results for the α-effect as a function of rotation rate are consistent with earlier numerical studies, i.e. increasing magnitude as rotation increases and approximately cos θ latitude profile for moderate rotation. Turbulent diffusivity, η_t, is proportional to the square of the turbulent vertical velocity in all cases. Whereas ηt decreases approximately inversely proportional to...Go to contribution page
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Dr Gustavo Guerrero16/02/2011, 12:00One of the existing hypothesis on sunspot formation is the buoyant emergence of magnetic flux tubes created by the strong radial shear at the tachocline. In this scenario, the magnetic field has to exceed a threshold value before it becomes buoyant and emerges through the convection zone up to the surface. However, several physical constrains are required to be fulfilled for this model...Go to contribution page
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