We use results from a coupled thermosphere-ionosphere-plasmasphere mod
el to illustrate a new mechanism for the formation of a large-scale po
lar cap patch of ionization arising from a rapid polar cap expansion.
The patch, having an ion density at the F2 peak twice that of the back
ground plasma, is isolated within the polar cap by a depletion due to
rapid flows in the cusp region. Such depletions caused by rapid flows
are generally ascribed to increases in the temperature dependent rates
of plasma loss reactions due to ion frictional heating. In this paper
, we demonstrate, however, that the depletion at the F peak is caused
primarily by large upward (field aligned) plasma flows. These flows al
so give rise to an increase in the height of the F peak in the deplete
d region. The morphology of the patch in the F region is subsequently
modulated by the return flow of plasma down previously depleted flux t
ubes as they convect across the polar cap, So that the enhancement dec
reases rapidly in both magnitude and spatial extent. Time histories fo
r the plasma density profiles above the EISCAT Svalbard radar and the
optical observatory at Eureka are presented as examples of what ground
-based observers might be expected to measure under these circumstance
s.