Abstract
This paper is concerned with convective and absolute instabilities in the boundary-layer
flow over the outer surface of a sphere rotating in an otherwise still fluid. Viscous
and streamline-curvature effects are included and the analysis is conducted between
latitudes of 10° and 80° from the axis of rotation. Both convective and absolute
instabilities are found at each latitude within specific parameter spaces. The results of
the convective instability analysis show that a crossflow instability mode is the most
dangerous below θ = 66°. Above this latitude a streamline-curvature mode is found
to be the most dangerous, which coincides with the appearance of reverse flow in the
radial component of the mean flow. At low latitudes the disturbances are considered
to be stationary, but at higher latitudes they are taken to rotate at 76% of the sphere
surface speed, as observed in experimental studies. Our predictions of the Reynolds
number and vortex angle at the onset of convective instability are consistent with
existing experimental measurements. Results are also presented that suggest that the
occurrence of the slowly rotating vortices is associated with the dominance of the
streamline-curvature mode at θ = 66°. The local Reynolds number at the predicted
onset of absolute instability matches experimental data well for the onset of turbulence
at θ = 30°; beyond this latitude the discrepancy increases but remains relatively small
below θ = 70°. It is suggested that this absolute instability may cause the onset of
transition below θ = 70°. Close to the pole the predictions of each stability analysis
are seen to approach those of existing rotating disk investigations.
Publisher
Cambridge University Press (CUP)
Subject
Mechanical Engineering,Mechanics of Materials,Condensed Matter Physics
Cited by
54 articles.
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