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Filament activation and magnetic reconnection
Authors:Deng  Yuanyong  Lin  Yong  Schmieder  Brigitte  Engvold  OddbjØrn
Affiliation:(1) Beijing Astronomical Observatory, Chinese Academy of Sciences, 20 Datun Road, Chaoyang, 100012 Beijing, Peoples Republic of China;(2) Institute of Theoretical Astrophysics, University of Oslo, P.O.Box 1029, Blindern, N-0315 Oslo, Norway;(3) Observatoire de Paris, 5, Place Jules Janssen, F-92195 Meudon Cedex, France
Abstract:Solar Physics - A curved filament in a decaying active region (AR&;nbsp;8329) was observed on 9 September 1998 with a combination of several instruments. The main data base is a 4-hour long time...
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