Observations of suprathermal electron conics in an interplanetary coronal mass ejection

Solar wind suprathermal electron velocity distributions measured by the SWE PAM experiment aboard ACE were studied to determine the internal magnetic s tructure of the coronal mass ejection (CME) that passed 1 AU on 4-5 Februar y, 1998. Pitch-angle distributions range from symmetric counter-streaming t o complex distributions that include conics. Identification of suprathermal electron conics in interplanetary CMEs (ICMEs) is reported here for the fi rst time. The origin of these conics is highly uncertain. We suggest, howev er, that the conics may originate in transient electron heating associated with magnetic reconnection within the magnetic legs of the CMEs. Such recon nection generates large, complex magnetic loops that have enhanced anti-sol ar electric fields at their solar edge to maintain charge neutrality. This field must be sufficiently strong to bind electrons with high pitch angles to the bottom of the loops as they propagate away from the Sun.