Thermal and dynamical structures of the Convective motions in a rotating fluid annulus, heated internally by passing an a.c, current through the fluid, are studied experimentally.
The effects of internal heating are seen in the following results.
1) The measurements of the rate of radial heat transport to the inner wall and the drift angular velocity of the vortex disturbances show that they depend on the rotation rate Ωin a similar way, with the minimum at a certain rotation rate Ω
m.
2) The distributions of the zonal mean temperature show that, when Ω>Ω
m, the region nearby the mean radius of the fluid layer becomes warmer than the inner and outer regions at the same height.
3) The mean zonal flow of the wave motion for Ω>Ωm, as well as the axisymmetric zonal flows, has the distribution of the vertical component of vorticity with negative values over a wide region at the top-surface.
4) The amplitudes of the temperature and pressure deviations increase with Ω and, near Ωm, the inclination of the axes of the temperature deviation from the vertical direction becomes least and the most active outward heat transport due to the vortex disturbances takes place.
The analysis shows that the fundamental structures of the vortex disturbances developing in the internally heated system are the same as those of the baroclinic waves analyzed by Matsuwo et al. (1976, 1977) in the wall-heated system. Therefore, the indication by Hide and Mason (1970), namely, that the principal characteristics of the flow (in the rotating fluid annulus) are fairly insensitive to the radial dependence of heating and cooling, is supported from the view-point of structure analysis.
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