The Oporto radiospectrograph and the Nancay radioheliograph recorded a radi
o event on November 6, 1997, closely related in time with a flare on Nation
al Oceanic and Atmospheric Administration (NOAA) active region 8100. At the
beginning: of the event the radio sources are located on a rather small vo
lume in the vicinity of the flare site. In a timescale df only a few minute
s the radio emission sites spread over a large volume in the corona, coveri
ng a range of 100 degrees in heliolatitude. During the period of the radio
event the Large Angle and Spectrometric Coronagraph (LASCO) on board the So
lar and Heliospheric Observatory (SOHO) observed an extremely fast coronal
mass ejection (CME), with a velocity around 2000 km s(-1) This CME presents
the particularity of having a fast lateral expansion, giving it a shape re
miniscent of a "coat hanger." There is a very good association between the
latitudinal extent and time development of the CME seen by LASCO and the ra
dio sources recorded by the radio instruments.