The nonaxisymmetric linear stability of spherical Couette flow is inve
stigated numerically when the ratio of gap width to inner sphere radiu
s (R(2) - R(1))/R(1) = 0.5. The basic flow becomes unstable at Re-c =
1245 and the associated azimuthal wave number is n(c) = 5, which agree
s remarkably well with the experimental results by Egbers and Rath [Ac
ta Mech. 81, 3 (1990)]. The marginal mode is oscillatory and has a dis
tinctive wavy structure around the equator and spirals extended in eac
h hemisphere. Sufficiently large spatial resolution is found to be req
uired in order to avoid serious underestimation of the critical Reynol
ds number. (C) 1997 American Institute of Physics.