Spatial palaeomagnetic field data associated with the Matuyama-Brunhes reve
rsal reveal a global pattern of virtual geomagnetic poles (VGPs) so distinc
t that inferences about the temporal nature, and, possibly, the energetics
of the dynamo process, can be drawn. Specifically, what is observed are two
pairs of low- and mid-latitude VGP concentrations mirrored about the Equat
or. Yet, while the path of the virtual pole associated with any given site
must pass through the Equator at least once during the polarity transition,
remarkably few data record the actual crossing. We propose that early in t
he reversal process a transitional state was reached within the dynamo and
held for a considerable time; only much later was it possible for field cha
nges to take place whereby VGPs crossed the Equator into the Northern Hemis
phere. Thus, a barrier to reversal may exist, related, perhaps, to the stat
e of magnetic Aux emerging from the solid inner core. Regardless, these pal
aeomagnetic data suggest that when this apparent barrier was successfully s
urmounted, field directions at sites about the globe rotated quickly in suc
h a manner that the associated VGPs transited the Equator at minimum rates
of speed approaching 1 deg yr(-1). The contention that the Matuyama-Brunhes
reversal was dominated by quasi-stationary transitional field states of lo
w harmonic order is supported by the data; however, the stage of rapid VGP
movement needs to be associated with a predominantly driving dynamo process
.