Narrow-banded emissions (f=130-260 Hz), registered on board the Aureol
-3 satellite for several years, were received at the auroral zone stat
ion Apatity. Comparison with the data of the magnetometer located also
in Apatity showed that the emissions were observed just before or at
the beginning of a magnetic disturbance. The connection of the observe
d emissions with auroral arcs confirms the generation of these emissio
ns by the electron beams. The properties of the considered narrow-band
ed ELF emissions can be used for the investigation of the electron acc
eleration region.