A numerical investigation is presented of the effects of a strongly te
mperature-dependent viscosity on the radial structure, horizontal plan
form, and heat transfer characteristics of a thermally convecting, inf
inite Prandtl number, Boussinesq fluid in a spherical shell. Basal and
mixed-mode heating are considered wherein viscosity varies with tempe
rature according to a linearized Arrhenius theology. Three-dimensional
, fully nonlinear calculations are performed and compared to the predi
ctions of linear theory. For basal heating, three convective regimes (
mobile lid, sluggish lid, and stagnant lid) are observed in accord wit
h theoretical and numerical studies in cartesian geometry. Solutions s
tarred with similar initial conditions and comparable convective vigor
result in distinct horizontal planforms which correspond to these thr
ee regimes. In the mobile-lid regime, planforms with moderate horizont
al length scales are characterized by linear downwelling sheets and qu
asi-cylindrical upwelling plumes. Sluggish-lid flow assumes a much lon
ger wavelength with linear bands of upwelling plumes and large cylindr
ical downflows. Stagnant-lid flow is characterized by very small-scale
flow patterns with upwelling plumes embedded in a network of cold, st
iff fluid. Mobile-lid and sluggish-lid regimes are also observed in th
e mixed-mode heating calculations with changes in horizontal length sc
ales similar to those in the basally-heated cases.