A theoretical study of the transition of a three-dimensional boundary
layer on a sphere rotating in still fluid is carried out by a linear s
tability analysis. A set of perturbation equations governing the insta
bility of the flow field is derived assuming the perturbations to be c
onsisting of spiral vortices. It is shown that the critical Reynolds n
umbers obtained in the present analytical study are close to those obs
erved in experiments. It has been found that the streamline-curvature
instability appears in the rotating sphere flow. It is also shown that
the cross-flow instability is dominant near the poles of a sphere, wh
ile the streamline-curvature instability overtakes near the equator.