Simultaneous observations by EISCAT and the Kilpisjarvi all-sky camera
revealed the presence of a band of enhanced electric field on one sid
e only of an auroral arc. Both the arc and the enhanced electric field
drifted equatorward at a velocity close to the prevailing convection
velocity. The same drift speed was indicated by EISCAT measurements of
ion-frictional heating: this descended in height as the magnetic fiel
d lines carrying the enhanced electric field cut across the EISCAT bea
m.