HR: 1330h
AN: SP23B-03    [Abstracts]
TI: Converging motions of solar flare ribbons
AU: Ji, H
EM: jihs@bbso.njit.edu
AF: Purple Mountain Observatory, Weat Beijing Rd 2, Nanjing, 210008 China
AU: * Wang, H
EM: haimin@flare.njit.edu
AF: Big Bear Solar Observatory, 40386 North SHore Ln, Big Bear City, CA 92314 United States
AB: We present a number of examples of solar flares, in which conjugate ribbons move toward each other during the impulsive phase. Meanwhile, HXR coronal sources move down. Normal separation motions occur only after the impulsive phase. This phenomena may pose a new topic to flare reconnection theory.
DE: 7524 Magnetic fields
SC: Solar Physics Division - AAS [SP]
MN: 2005 Joint Assembly