High time resolution optical measurements in the magnetic zenith are c
ompared with European Incoherent Scatter (EISCAT) field-aligned measur
ements of electron density at 0.2-s resolution and with horizontal ele
ctric field measurements made at 278 km with resolution of 9 s. In one
event, 20 min after a spectacular amoral breakup, a system of narrow
and active are elements moved southward into the magnetic zenith, wher
e it remained for several minutes. During a 30-s interval of activity
in a narrow are element very close to the radar beam, the electric fie
ld vectors at 3-s resolution were found to be extremely large (up to 4
00 mV m(-1)) and to point toward the bright optical features in the ar
c, which moved along its length. It is proposed that the large electri
c fields are short-lived and are directly associated with the particle
precipitation that causes the bright features in auroral are elements
.