Vector electric field measurements from the San Marco D satellite are
utilized to investigate the bifurcation of ionospheric plasma depletio
ns (sometimes called ''bubbles'') associated with nightside equatorial
spread F. These depletions are identified by enhanced upward ExB conv
ection in depleted plasma density channels in the nighttime equatorial
ionosphere. The in situ determination of the bifurcation process is b
ased on de electric field measurements of the bipolar variation in the
zonal flow, westward and eastward, as the eastbound satellite crosses
isolated signatures of updrafting plasma depletion regions. We also p
resent data in which more complicated regions of zonal velocity variat
ions appear as the possible result of multiple bifurcations of updraft
ing equatorial plasma bubbles.