Meridian-plane elevation scans with the Millstone Hill incoherent scat
ter radar provide evidence of a strong perturbation of the coupled mid
-latitude magnetosphere-ionosphere system during the early phases of t
he November 4, 1993 magnetic storm. A narrow ionospheric trough formed
at L=3.5 in the pre-midnight sector, immediately poleward of the Mill
stone Hill site. The most pronounced radar signature of the developing
activity was a brief (20 min) uplifting of the F region plasma equato
rward of the trough, such that the peak altitude increased with distan
ce away from the trough. A similar signature had been observed during
storm onset on March 20, 1990, and in that event a pronounced topside
ionospheric depletion developed in the region far equatorward of the m
id-latitude trough and was observed by the radar and the DMSP F9 satel
lite. During the November 4, 1993 event, the DMSP F10 satellite observ
ed narrow magnetically conjugate regions of plasma density depletion a
nd strong horizontal and upward plasma velocity(> 1500 m/s) at L=1.5 a
t the time of the uplifting of the mid-latitude F region observed by t
he radar. These observations were confined to longitudes near the Sout
h Atlantic magnetic anomaly and, in the Nov 1993 case, the perturbatio
n was coincident with the peak of the precipitating particle fluxes as
sociated with inner-belt losses at the anomaly. Both the uplifting of
the ionospheric F layer and the triggering of topside density perturba
tions can be explained in terms of an eastward electric field imposed
on the mid and low-latitude ionosphere during the initial stages of th
e geomagnetic storm. The low-latitude ionospheric perturbations in the
se events were similar to supersonic equatorial bubbles, triggered by
the destabilizing effects of the upward ExB drift associated with the
eastward electric field.