The ion drift meter on the polar orbiting DMSP F-10 spacecraft observe
d bubble-like features near the magnetic equator that have remarkably
continuous transitions in ion concentration (N(i)) and drift velocity,
where there is a high positive correlation between upward velocity an
d decreased N(i). This is in marked contrast to the virtually disconti
nuous transitions that are characteristics of most bubbles. We conclud
e that these new features were probably observed on the bottomside of
the F-layer at DMSP altitudes (750 - 850 km), much higher than normall
y accepted values. These observations were made during Feb.-Mar.-Apr.
of 1991, when N(i) exceeded 10(6) cm-3 on nearly every equator crossin
g.