Polar patches are regions within the polar cap where the F-region elec
tron concentration and airglow emission at 630 nm are enhanced above a
background level. Previous observations have demonstrated that polar
patches can be readily identified in Polar Anglo-American Conjugate Ex
periment (PACE) data. Here PACE data and those from complementary inst
ruments are used to show that some polar patches form in the dayside c
usp within a few minutes of the simultaneous occurrence of a flow chan
nel event (short-lived plasma jets approximately 2 km s-1) and azimuth
al flow changes in the ionospheric convection pattern. The latter are
caused by variations of the y-component of the interplanetary magnetic
field. The physical processes by which these phenomena cause plasma e
nhancements and depletions in the vicinity of the dayside cusp and cle
ft are discussed. Subsequently, these features are transported into th
e polar cap where they continue to evolve. The spatial scale of patche
s when formed is usually 200-1000 km in longitude and 2-degrees-3-degr
ees wide in latitude. Their motion after formation and the velocity of
the plasma within the patches are the same, indicating that they are
drifting under the action of an electric field. Occasionally, patches
are observed to occur simultaneously in geomagnetic conjugate regions.
Since some of these observations are incompatible with the presently-
accepted model for patch formation involving the expansion of the high
latitude convection pattern entraining solar-produced plasma, further
modeling of the effects of energetic particle precipitation in the cu
sp, the consequences of flow channel events on the plasma concentratio
ns, and the time dependence of plasma convection as a result of interp
lanetary magnetic field By changes is strongly recommended. Such studi
es could be used to determine the relative importance of this new mech
anism compared with the existing theory for patch formation as a funct
ion of universal time and season.