Observations of coronal mass ejections (CMEs) by the Large Angle Spectromet
ric Coronagraph (LASCO) on the Solar and Heliospheric Observatory (SOHO) sh
ow a significant fraction with circular intensity patterns. In the past, th
ese would have been called "disconnection" events, but we suggest that thes
e are evidence of CMEs containing helical magnetic flux ropes that are ofte
n central to many theoretical models of CMEs and have been observed in magn
etic clouds near 1 AU. Three examples are examined in detail with the LASCO
and Extreme-Ultraviolet Imaging Telescope (EIT) data sets, which provide o
bservations from their initiation through 30 R..